A simple model to interpret the ultraviolet, optical and infrared emission from galaxies

Abstract

We present a simple, largely empirical but physically motivated model to interpret the mid- and far-infrared spectral energy distributions of galaxies consistently with the emission at ultraviolet, optical and near-infrared wavelengths. Our model relies on an existing angle-averaged prescription to compute the absorption of starlight by dust in stellar birth clouds and in the ambient ISM in galaxies. We compute the spectral energy distribution of the power reradiated by dust in stellar birth clouds as the sum of three components: a component of PAHs; a mid-IR continuum characterising the emission from hot grains; and a component of warm grains in thermal equilibrium with adjustable temperature. In the ambient ISM, we fix for simplicity the relative proportions of these three components to reproduce the spectral shape of diffuse cirrus emission in the Milky Way, and we include a component of cold grains in thermal equilibrium with adjustable temperature. Our model can be used to derive statistical constraints on the star formation histories and dust contents of large samples of galaxies using UV, optical and IR observations. We illustrate this by deriving median-likelihood estimates of the star formation rates, stellar masses, effective dust optical depths, dust masses, and relative strengths of different dust components of 66 well-studied nearby star- forming galaxies from the Spitzer Infrared Nearby Galaxy Survey (SINGS). From this analysis, we conclude that the mid- and far-IR colours of galaxies correlate strongly with the specific star formation rate, as well as with other galaxy-wide quantities connected to this parameter. Our model can be straightforwardly applied to interpret UV, optical and IR spectral energy distributions from any galaxy sample. [abridged]

27 pages, 15 figures, accepted for publication in MNRAS. Full-resolution figures available from ftp://ftp.iap.fr/pub/from_users/dacunha/fullres_figures

References in corpus (56)

• Stellar population synthesis at the resolution of 2003
• Galactic Stellar and Substellar Initial Mass Function
• The physical properties of star forming galaxies in the low redshift universe
• The Spitzer Space Telescope Mission
• The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission
• Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era
• A Simple Model for the Absorption of Starlight by Dust in Galaxies
• UV Star Formation Rates in the Local Universe
• Infrared Emission from Interstellar Dust. II. The Diffuse Interstellar Medium
• SINGS: The SIRTF Nearby Galaxies Survey
• The ages and metallicities of galaxies in the local universe
• Dust Absorption And The Ultraviolet Luminosity Density At z \approx 3 As Calibrated By Local Starburst Galaxies
• Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample
• Interpreting the Cosmic Infrared Background: Constraints on the Evolution of the Dust Enshrouded Star Formation Rate
• The Mid-Infrared Spectrum of Star-Forming Galaxies: Global Properties of PAH Emission
• The Infrared Spectral Energy Distribution of Normal Star-Forming Galaxies: Calibration at Far-Infrared and Submillimeter Wavelengths
• SCUBA: A common-user submillimetre camera operating on the James Clerk Maxwell Telescope
• The GALEX Ultraviolet Atlas of Nearby Galaxies
• Absolute Calibration of the Infrared Array Camera on the Spitzer Space Telescope
• The SCUBA Local Universe Galaxy Survey I: First Measurements of the Submillimetre Luminosity and Dust Mass Functions
• Evolution of asymptotic giant branch stars I. Updated synthetic TP-AGB models and their basic calibration
• The Mid-IR Properties of Starburst Galaxies from Spitzer-IRS Spectroscopy
• The Bulk of the Cosmic Infrared Background Resolved by ISOCAM
• An Ultraviolet-to-Radio Broadband Spectral Atlas of Nearby Galaxies
• The SCUBA Local Universe Galaxy Survey II. 450 micron data - evidence for cold dust in bright IRAS Galaxies
• The Hubble Deep Field North SCUBA Super-map IV - Characterizing submillimetre galaxies using deep Spitzer imaging
• Modelling the infrared galaxy evolution using a phenomenological approach
• An Integrated Spectrophotometric Survey of Nearby Star-Forming Galaxies
• Variations of the Mid-IR Aromatic Features Inside and Among Galaxies
• PAHs contribution to the infrared output energy of the Universe at z~2
• Star formation history and dust attenuation in galaxies drawn from ultraviolet surveys
• Infrared Spectral Energy Distributions of Nearby Galaxies
• The K-band luminosity function at z=1: a powerful constraint on galaxy formation theory
• Detection and Characterization of Cold Interstellar Dust and PAH Emission from COBE Observations
• FAR-INFRARED SPECTRAL OBSERVATIONS OF THE GALAXY BY COBE
• Towards a resolution of the discrepancy between different estimators of star formation rate
• A Long-Wavelength View on Galaxy Evolution from Deep Surveys by the Infrared Space Observatory
• Modelling the spectral energy distribution of galaxies. III. Attenuation of stellar light in spiral galaxies
• Bursty stellar populations and obscured AGN in galaxy bulges
• Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: I. The role of ISM pressure & the Molecular Cloud Dissipation Timescale
• The aromatic infrared bands as seen by ISO-SWS: probing the PAH model
• The DIRTY Model. I. Monte Carlo Radiative Transfer Through Dust
• Infrared Emission of Normal Galaxies from 2.5 to 12 Microns: ISO Spectra, Near-Infrared Continuum and Mid-Infrared Emission Features
• A Comparison of Independent Star Formation Diagnostics for a UV-Selected Sample of Nearby Galaxies
• The Mid-Infrared Spectra of Normal Galaxies
• Spitzer/IRAC and ISOCAM/CVF insights on the origin of the Near to Mid-IR Galactic diffuse emission
• Modeling the spectral energy distribution of galaxies. II. Disk opacity and star formation in 5 edge-on spirals
• Nebular Abundances of Nearby Southern Dwarf Galaxies
• The DIRTY Model II: Self-Consistent Treatment of Dust Heating and Emission in a 3-D Radiative Transfer Code
• Mid-Infrared Observations of Normal Star-Forming Galaxies: The Infrared Space Observatory Key Project Sample
• Dust-Induced Systematic Errors in UV-Derived Star Formation Rates
• Mid infrared properties of distant infrared luminous galaxies
• An atlas of mid-infrared dust emission in spiral galaxies
• Infrared Spectral Energy Distributions of z~0.7 Star-Forming Galaxies

Cited by in corpus (960)

• CIGALE: a python Code Investigating GALaxy Emission
• Analysis of galaxy SEDs from far-UV to far-IR with CIGALE: Studying a SINGS test sample
• Modeling the Panchromatic Spectral Energy Distributions of Galaxies
• Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
• Dusty Star-Forming Galaxies at High Redshift
• Stellar Population Inference with Prospector
• Dust-Corrected Star Formation Rates of Galaxies. I. Combinations of H-alpha and Infrared Tracers
• Dust Attenuation Curves in the Local Universe: Demographics and New Laws for Star-forming Galaxies and High-redshift Analogs
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• Resolved stellar mass maps of galaxies. I: method and implications for global mass estimates
• Semi-analytic modeling of the EBL and consequences for extragalactic gamma-ray spectra
• Deriving Physical Properties from Broadband Photometry with Prospector: Description of the Model and a Demonstration of its Accuracy Using 129 Galaxies in the Local Universe
• The SAMI Galaxy Survey: instrument specification and target selection
• An ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling
• The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4
• The Detection of a Population of Submillimeter-Bright, Strongly-Lensed Galaxies
• GALEX-SDSS-WISE Legacy Catalog (GSWLC): Star Formation Rates, Stellar Masses and Dust Attenuations of 700,000 Low-redshift Galaxies
• Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
• A Two-Parameter Model for the Infrared/Submillimeter/Radio Spectral Energy Distributions of Galaxies and AGN
• On the effect of the Cosmic Microwave Background in high-redshift (sub-)millimeter observations
• A dusty, normal galaxy in the epoch of reionization
• Evidence for Ubiquitous Collimated Galactic-Scale Outflows along the Star-Forming Sequence at z~0.5
• Fitting the integrated Spectral Energy Distributions of Galaxies
• A Budget and Accounting of Metals at z~0: Results from the COS-Halos Survey
• The Main Sequence of star-forming galaxies across cosmic times
• Dust in the reionization era: ALMA observations of a $z$=8.38 Galaxy
• Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation
• Sub-millimeter galaxies as progenitors of compact quiescent galaxies
• A z=0 Multi-wavelength Galaxy Synthesis I: A WISE and GALEX Atlas of Local Galaxies
• A Fast Radio Burst Host Galaxy
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass
• An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies
• How to measure galaxy star-formation histories I: Parametric models
• Reconstructing the stellar mass distributions of galaxies using S4G IRAC 3.6 and 4.5 micron images: II. The conversion from light to mass
• The Dust Attenuation Law in Galaxies
• Stellar Masses and SFRs for 1M Galaxies from SDSS and WISE
• Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3
• Deep Spitzer 24mic COSMOS imaging -- I. The evolution of luminous dusty galaxies - Confronting the models
• Spectroscopic detection of CIV in a galaxy at z=7.045: Implications for the ionizing spectra of reionization-era galaxies
• Radial distribution of stars, gas and dust in SINGS galaxies. II. Derived dust properties
• Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations
• Herschel-ATLAS: Rapid evolution of dust in galaxies in the last 5 billion years
• An Older, More Quiescent Universe from Panchromatic SED Fitting of the 3D-HST Survey
• An Atlas of Galaxy Spectral Energy Distributions from the Ultraviolet to the Mid-Infrared
• The dust content of galaxies from z = 0 to z = 9
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description
• The Interstellar dust properties of nearby galaxies
• Galaxy And Mass Assembly (GAMA): Mid-Infrared Properties and Empirical Relations from $WISE$
• Timing the starburst-AGN connection
• Empirical determination of the shape of dust attenuation curves in star-forming galaxies
• A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios
• Ultraviolet Emission Lines in Young Low Mass Galaxies at z~2: Physical Properties and Implications for Studies at z>7
• Rotation in [CII]-emitting gas in two galaxies at a redshift of 6.8
• GAMA/G10-COSMOS/3D-HST: The 0<z<5 cosmic star-formation history, stellar- and dust-mass densities
• The dust scaling relations of the Herschel Reference Survey
• Dust temperature and mid-to-total infrared color distributions for star-forming galaxies at 0<z<4
• The LoTSS view of radio AGN in the local Universe. The most massive galaxies are always switched on
• Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors
• VLA-COSMOS 3GHz Large Project: The infrared-radio correlation of star-forming galaxies and AGN to $z\lesssim 6$
• High-redshift star formation in the ALMA era
• Encoding the infrared excess (IRX) in the NUVrK color diagram for star-forming galaxies
• The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6
• Post-starburst galaxies: more than just an interesting curiosity
• The VLA-COSMOS 3 GHz Large Project: Multiwavelength counterparts and the composition of the faint radio population
• Spectroscopic detections of CIII]1909 at z~6-7: A new probe of early star forming galaxies and cosmic reionisation
• GOODS-Herschel:dust attenuation properties of UV selected high redshift galaxies
• Tracing the cosmic growth of super massive black holes to z ~ 3 with Herschel
• Modelling the spectral energy distribution of galaxies. V. The dust and PAH emission SEDs of disk galaxies
• Dust Spectral Energy Distributions of Nearby Galaxies: an Insight from the Herschel Reference Survey
• Herschel-ATLAS: a binary HyLIRG pinpointing a cluster of starbursting proto-ellipticals
• LOFAR/H-ATLAS: The low-frequency radio luminosity - star-formation rate relation
• Herschel-ATLAS Galaxy Counts and High Redshift Luminosity Functions: The Formation of Massive Early Type Galaxies
• Panchromatic spectral energy distributions of Herschel sources
• CANDELS+3D-HST: compact SFGs at z~2-3, the progenitors of the first quiescent galaxies
• The VLA-COSMOS 3~GHz Large Project: AGN and host-galaxy properties out to z$\lesssim$6
• New insight into the relation between star formation activity and dust content in galaxies
• The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques
• How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting
• Linking dust emission to fundamental properties in galaxies: The low-metallicity picture
• Fast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8
• A massive, distant proto-cluster at z=2.47 caught in a phase of rapid formation?
• Radio-loud AGN in the first LoTSS data release: The lifetimes and environmental impact of jet-driven sources
• The Emission by Dust and Stars of Nearby Galaxies in the Herschel KINGFISH Survey
• The Direct Detection of Cool, Metal-Enriched Gas Accretion onto Galaxies at z ~ 0.5
• Galaxy And Mass Assembly (GAMA): Accurate Panchromatic Photometry from Optical Priors using LAMBDAR
• The VLA-COSMOS 3 GHz Large Project: The cosmic star formation history since z~5
• The ALMA Spectroscopic Survey in the HUDF: CO luminosity functions and the molecular gas content of galaxies through cosmic history
• The Radio Spectral Energy Distribution and Star Formation Rate Calibration in Galaxies
• Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget
• ProSpect: Generating Spectral Energy Distributions with Complex Star Formation and Metallicity Histories
• Investigations of dust heating in M81, M83, and NGC 2403 with the Herschel Space Observatory
• ALMA spectroscopic survey in the Hubble Ultra Deep Field: Continuum number counts, resolved 1.2-mm extragalactic background, and properties of the faintest dusty star forming galaxies
• SN 2015bn: a detailed multi-wavelength view of a nearby superluminous supernova
• Photometric Redshift with Bayesian Priors on Physical Properties of Galaxies
• Herschel-ATLAS: Multi-wavelength SEDs and physical properties of 250 micron-selected galaxies at z < 0.5
• The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z=1.5-10 UV-selected Galaxies and the Implied High-Redshift Star Formation History
• Outside-in Shrinking of the Star-forming Disk of Dwarf Irregular Galaxies
• The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3
• The evolution of post-starburst galaxies from z=2 to z= 0.5
• Insights into the content and spatial distribution of dust from the integrated spectral properties of galaxies
• ALMA reveals potential evidence for spiral arms, bars, and rings in high-redshift submillimeter galaxies
• Non-parametric Star Formation History Reconstruction with Gaussian Processes I: Counting Major Episodes of Star Formation
• GAMA/H-ATLAS: A meta-analysis of SFR indicators - comprehensive measures of the SFR-M* relation and Cosmic Star Formation History at z < 0.4
• On the dust temperatures of high redshift galaxies
• Calibrating Star Formation in WISE using Total Infrared Luminosity
• Mid-IR Luminosities and UV/Optical Star Formation Rates at z<1.4
• An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: Spectroscopic redshifts
• The heating of dust by old stellar populations in the Bulge of M31
• The total infrared luminosity may significantly overestimate the star formation rate of recently quenched galaxies
• A New Census of the 0.2< z <3.0 Universe, Part II: The Star-Forming Sequence
• The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS-UDS
• The Ubiquity of Coeval Starbursts in Massive Galaxy Cluster Progenitors
• Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function to $z=0.1$ from the r-band selected equatorial regions
• A New Census of the 0.2 < z < 3.0 Universe, Part I: The Stellar Mass Function
• Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): II. Cold Molecular Gas Evolution out to Redshift 6
• The Brightest Galaxies in the Dark Ages: Galaxies' Dust Continuum Emission During the Reionization Era
• Confronting theoretical models with the observed evolution of the galaxy population out to z=4
• Effect of galaxy mergers on star formation rates
• Relative merits of different types of rest-frame optical observations to constrain galaxy physical parameters
• Dusty galaxies in the Epoch of Reionization: simulations
• The REBELS ALMA Survey: cosmic dust temperature evolution out to z $\sim$ 7
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Source catalogue and properties
• DustPedia: Multiwavelength Photometry and Imagery of 875 Nearby Galaxies in 42 Ultraviolet--Microwave Bands
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Molecular gas reservoirs in high-redshift galaxies
• The main sequence of star forming galaxies I. The local relation and its bending
• Metal-enriched, sub-kiloparsec gas clumps in the circumgalactic medium of a faint z = 2.5 galaxy
• AGNfitter: A Bayesian MCMC approach to fitting spectral energy distributions of AGN
• A spectroscopic search for AGN activity in the reionization era
• Should we believe the results of UV-mm galaxy SED modelling?
• The Nature of Extreme Emission Line Galaxies at z=1-2: Kinematics and Metallicities from Near-Infrared Spectroscopy
• The ALMA Spectroscopic Survey in the HUDF: CO Excitation and Atomic Carbon in Star-Forming Galaxies at $z=1-3$
• The dust budget crisis in high-redshift submillimetre galaxies
• Deep Extragalactic VIsible Legacy Survey (DEVILS): SED Fitting in the D10-COSMOS Field and the Evolution of the Stellar Mass Function and SFR-$M_{\star }$ relation
• H-ATLAS/GAMA: Dusty early-type galaxies and passive spirals
• A Critical Look at the Mass-Metallicity-SFR Relation in the Local Universe. I. An Improved Analysis Framework and Confounding Systematics
• What Determines the Incidence and Extent of MgII Absorbing Gas Around Galaxies?
• The MUSE Hubble Ultra Deep Field surveys: Data release II
• The SAMI Galaxy Survey: Spatially Resolving the Main Sequence of Star Formation
• Old and young stellar populations in DustPedia galaxies and their role in dust heating
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). A precise measurement of the galaxy stellar mass function and the abundance of massive galaxies at redshifts 0.5<z<1.3
• The host galaxy and late-time evolution of the Super-Luminous Supernova PTF12dam
• HELP: modelling the spectral energy distributions of Herschel detected galaxies in the ELAIS N1 field
• Characterizing the UV-to-NIR shape of the dust attenuation curve of IR luminous galaxies up to z$\sim$2
• Stellar mass-to-light ratios from galaxy spectra: how accurate can they be?
• The Herschel Dwarf Galaxy Survey: II. Physical conditions, origin of [CII] emission, and porosity of the multiphase low-metallicity ISM
• Comprehensive comparison of models for spectral energy distributions from 0.1 micron to 1 mm of nearby star-forming galaxies
• A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy
• On Detecting Halo Assembly Bias with Galaxy Populations
• Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium
• Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies
• BAT AGN Spectroscopic Survey - XI. The Covering Factor of Dust and Gas in Swift/BAT Active Galactic Nuclei
• Discovery of a Multiply-Lensed Submillimeter Galaxy in Early HerMES Herschel/SPIRE Data
• Gas Fraction and Depletion Time of Massive Star Forming Galaxies at z~3.2: No Change in Global Star Formation Process out to z>3
• Alma Twenty-six Arcmin^2 Survey Of Goods-s At One-millimeter (asagao): Source Catalog And Number Counts
• Jekyll & Hyde: quiescence and extreme obscuration in a pair of massive galaxies 1.5 Gyr after the Big Bang
• Large scale outflows from z ~ 0.7 starburst galaxies identified via ultra-strong MgII quasar absorption lines
• An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies
• The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large Area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array
• Galaxy And Mass Assembly (GAMA): A forensic SED reconstruction of the cosmic star formation history and metallicity evolution by galaxy type
• A gravitationally unstable gas disk of a starburst galaxy 12 billion years ago
• The VIMOS Ultra Deep Survey: Emerging from the Dark, a Massive Proto-Cluster at z~4.57
• The quenching of the star formation activity in cluster galaxies
• The evolution of the cold interstellar medium in galaxies following a starburst
• Dust and star-formation properties of a complete sample of local galaxies drawn from the Planck Early Release Compact Source Catalogue
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$ VI: Redshift and emission-line catalog and basic properties of star-forming galaxies
• Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): I. Robust ALMA Continuum Photometry Catalogs and Stellar Mass and Star Formation Properties for ~700 Galaxies at z=0.5-6
• Hot dust in Panchromatic SED Fitting: Identification of AGN and improved galaxy properties
• Dust attenuation in disk-dominated galaxies: evidence for the 2175A dust feature
• The LOFAR Two-metre Sky Survey Deep fields: The star formation rate - radio luminosity relation at low frequencies
• Spatially resolved stellar, dust and gas properties of the post-interacting Whirlpool Galaxy system
• Complexity in the light curves and spectra of slow-evolving superluminous supernovae
• Determining the stellar masses of submillimetre galaxies: the critical importance of star formation histories
• A merger in the dusty, $z=7.5$ galaxy A1689-zD1?
• From light to baryonic mass: the effect of the stellar mass-to-light ratio on the Baryonic Tully-Fisher relation
• Detailed dust modelling in the L-Galaxies semi-analytic model of galaxy formation
• Exploring the physical properties of local star-forming ULIRGs from the ultraviolet to the infrared
• From the far-ultraviolet to the far-infrared -- galaxy emission at $0\le z\le 10$ in the Shark semi-analytic model
• An Observed Link between Active Galactic Nuclei and Violent Disk Instabilities in High-Redshift Galaxies
• The Herschel-ATLAS: The dust energy balance in the edge-on spiral galaxy UGC 4754
• Measures of galaxy dust and gas mass with Herschel photometry and prospects for ALMA
• Dust and gas in luminous proto-cluster galaxies at z=4.05: the case for different cosmic dust evolution in normal and starburst galaxies
• An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2 COSMOS field
• How dead are dead galaxies? Mid-Infrared fluxes of quiescent galaxies at redshift 0.3 < z < 2.5: implications for star formation rates and dust heating
• Compton Thick AGN in the XMM-COSMOS survey
• The LOFAR Two-metre Sky Survey Deep Fields Data Release 1: V. Survey description, source classifications and host galaxy properties
• Properties of z~3-6 Lyman break galaxies. II. Testing star formation histories and the SFR-mass relation with ALMA and near-IR spectroscopy
• Intra Cluster Light properties in the CLASH-VLT cluster MACS J1206.2-0847
• A Massive Galaxy in its Core Formation Phase Three Billion Years After the Big Bang
• Galaxy and Mass Assembly (GAMA): Morphological transformation of galaxies across the green valley
• Using dust, gas and stellar mass selected samples to probe dust sources and sinks in low metallicity galaxies
• Mapping the average AGN accretion rate in the SFR-M* plane for Herschel selected galaxies at 0<z<2.5
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• The SAMI Galaxy Survey: extraplanar gas, galactic winds, and their association with star formation history
• CIGALEMC: Galaxy Parameter Estimation using a Markov Chain Monte Carlo Approach with Cigale
• On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
• The origins of post-starburst galaxies at z<0.05
• The host galaxy of the super-luminous SN 2010gx and limits on explosive nickel-56 production
• Dust, CO and [CI]: Cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time
• CLASH-VLT: Environment-driven evolution of galaxies in the z=0.209 cluster Abell 209
• Starburst to quiescent from HST/ALMA: Stars and dust unveil minor mergers in submillimeter galaxies at $z\sim 4.5$
• Photometric redshifts for the next generation of deep radio continuum surveys - I: Template fitting
• Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the last 10 Gyr
• The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the molecular gas in CO-selected galaxies
• ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using [CI] and CO
• Physical Characterization of an Unlensed Dusty Star-Forming Galaxy at $z=5.85$
• ZFIRE: A KECK/MOSFIRE Spectroscopic Survey of Galaxies in Rich Environments at z~2
• On the interdependence of galaxy morphology, star formation, and environment in massive galaxies in the nearby Universe
• A new method for classifying galaxy SEDs from multi-wavelength photometry
• AGN Selection and Demographics in GOODS-S/HUDF from X-ray to Radio
• Ultraviolet to infrared emission of z>1 galaxies: Can we derive reliable star formation rates and stellar masses?
• Relationship between star formation rate and black hole accretion at z=2: The different contributions in quiescent, normal and starburst galaxies
• Accurate dust temperature determination in a $z=7.13$ galaxy
• Cold dust and stellar emissions in dust-rich galaxies observed with ALMA: a challenge for SED-fitting techniques
• The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm continuum number counts
• Mid-InfraRed Outburst in Nearby Galaxies (MIRONG) I: Sample Selection and Characterization
• Galaxy And Mass Assembly: The 1.4GHz SFR indicator, SFR-M* relation and predictions for ASKAP-GAMA
• The X-SHOOTER Lyman-$\alpha$ survey at z=2 (XLS-z2) I: What makes a galaxy a Lyman-$\alpha$ emitter?
• Fitting Analysis using Differential Evolution Optimization (FADO): Spectral population synthesis through genetic optimization under self-consistency boundary conditions
• The evolving relation between star-formation rate and stellar mass in the VIDEO Survey since $z=3$
• Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
• Dynamical signatures of a LCDM-halo and the distribution of the baryons in M33
• The MUSE Extremely Deep Field: the Cosmic Web in Emission at High Redshift
• Insights into formation scenarios of massive Early-Type galaxies from spatially resolved stellar population analysis in CALIFA
• Measurements of CO redshifts with Z-Spec for lensed submillimeter galaxies discovered in the H-ATLAS survey
• $\text{Herschel}$-ATLAS:The connection between star formation and AGN activity in radio-loud and radio-quiet active galaxies
• HerMES: The Rest-Frame UV Emission and A Lensing Model for the z=6.34 Luminous Dusty Starburst Galaxy HFLS3
• MAGPHYS+photo-z: Constraining the Physical Properties of Galaxies with Unknown Redshifts
• Mapping Obscuration to Reionization with ALMA (MORA): 2mm Efficiently Selects the Highest-Redshift Obscured Galaxies
• A Survey of the Molecular ISM Properties of Nearby Galaxies using the Herschel FTS
• An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling
• First gas-phase metallicity gradients of $0.1\lesssim z\lesssim 0.8$ galaxies with MUSE
• Estimating gas masses and dust-to-gas ratios from optical spectroscopy
• Fade to grey: systematic variation of the galaxy attenuation curves with galaxy properties in EAGLE
• The superluminous supernova PS1-11ap: bridging the gap between low and high redshift
• An ALMA survey of the S2CLS UDS field: Optically invisible submillimetre galaxies
• Illuminating the dark side of cosmic star formation two billion years after the Big Bang
• Dust attenuation in z $\sim$ 1 galaxies from Herschel and 3D-HST H$\alpha$ measurements
• The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to $z\sim 3$
• The Absence of [CII] 158$\mu$m Emission in Spectroscopically-Confirmed Galaxies at $z>8$
• ALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole at z=4.75
• Dust attenuation and Halpha emission in a sample of galaxies observed with Herschel at $0.6<z<1.6$
• Herschel-ATLAS: Properties of dusty massive galaxies at low and high redshifts
• The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 micron surface brightness ratios
• Strong FUV fields drive the [CII]/FIR deficit in z~3 dusty, star-forming galaxies
• GAMA/G10-COSMOS/3D-HST: Evolution of the galaxy stellar mass function over 12.5Gyrs
• Population synthesis modelling of luminous infrared galaxies at intermediate redshift
• Star formation and nuclear activity in luminous infrared galaxies: An infrared through radio review
• Shocked POststarburst Galaxy Survey II: The Molecular Gas Content and Properties of a Subset of SPOGs
• Spectral energy distributions of an AKARI-SDSS-GALEX sample of galaxies
• The Galaxy End Sequence
• Calibration of ultraviolet, mid-infrared and radio star formation rate indicators
• Molecular and atomic gas in dust lane early-type galaxies - I: Low star-formation efficiencies in minor merger remnants
• Simultaneous Modeling of the Stellar and Dust Emission in Distant Galaxies: Implications for Star Formation Rate Measurements
• Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-z Universe
• The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The nature of the faintest dusty star-forming galaxies
• Updated 34-Band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies
• A molecular line scan in the Hubble Deep Field North
• Infrared Selection of Obscured Active Galactic Nuclei in the COSMOS Field
• Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2
• Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
• Deep CO(1-0) Observations of z=1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation Efficiencies
• Physical properties and evolution of (Sub-)millimeter selected galaxies in the galaxy formation simulation Shark
• The origin of dust in galaxies across cosmic time
• Accretion mode versus radio morphology in the LOFAR Deep Fields
• Physical properties of z>4 submillimeter galaxies in the COSMOS field
• Near-Infrared MOSFIRE Spectra of Dusty Star-Forming Galaxies at 0.2<z<4
• The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy
• The fraction of bolometric luminosity absorbed by dust in DustPedia galaxies
• ALMA 26 Arcmin${}^2$ Survey of GOODS-S at One-millimeter (ASAGAO): Average Morphology of High-$z$ Dusty Star-Forming Galaxies is an Exponential-Disk ($n\simeq 1$)
• Galaxy And Mass Assembly (GAMA): growing up in a bad neighbourhood - how do low-mass galaxies become passive?
• Herschel-ATLAS: The Surprising Diversity of Dust-Selected Galaxies in the Local Submillimetre Universe
• CLASH-VLT: The stellar mass function and stellar mass density profile of the z=0.44 cluster of galaxies MACS J1206.2-0847
• The Nature of H$\beta +$[O{\sc iii}] and [O{\sc ii}] emitters to $z\sim 5$ with HiZELS: stellar mass functions and the evolution of EWs
• Infrared spectral energy distribution decomposition of WISE-selected, hyperluminous hot dust-obscured galaxies
• The evolution of superluminous supernova LSQ14mo and its interacting host galaxy system
• ALMA view of a massive spheroid progenitor: a compact rotating core of molecular gas in an AGN host at z=2.226
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• The Dust Attenuation of Star-forming Galaxies at $z\sim 3$ and Beyond: New Insights from ALMA Observations
• Global Star Formation Rates and Dust Emission Over the Galaxy Interaction Sequence
• PHANGS-HST: Star Cluster Spectral Energy Distribution Fitting with CIGALE
• Sub-kiloparsec Imaging of Cool Molecular Gas in Two Strongly Lensed Dusty, Star-Forming Galaxies
• Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2
• Galaxy And Mass Assembly (GAMA): impact of the group environment on galaxy star formation
• The Molecular Gas Reservoirs of $z\sim 2$ Galaxies: A comparison of CO(1-0) and dust-based molecular gas masses
• Enhanced Warm H2 Emission in the Compact Group Mid-Infrared "Green Valley"
• SINFONI spectra of heavily obscured AGNs in COSMOS: evidence of outflows in a MIR/O target at z$\sim 2.5$
• Virgo Filaments I: Processing of gas in cosmological filaments around the Virgo cluster
• The role of atomic hydrogen in regulating the scatter of the mass-metallicity relation
• Large scale structure around a z=2.1 cluster
• Mid-Infrared Spectral Measures of Star-Formation and AGN Activity in Normal Galaxies
• Resolving the AGN and host emission in the mid-infrared using a model-independent spectral decomposition
• Pégase.3: A code for modeling the UV-to-IR/submm spectral and chemical evolution of galaxies with dust
• The MUSE Hubble Ultra Deep Field Survey: IV. Global properties of C III] emitters
• The Structure and Stellar Content of the Outer Disks of Galaxies: A New View from the Pan-STARRS1 Medium Deep Survey
• Ultraviolet Extinction at High Galactic Latitudes
• On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Proto-Clusters at z~2.0-2.5
• Understanding the Scatter in the Spatially-resolved Star Formation Main Sequence of Local Massive Spiral Galaxies
• Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relations
• Measuring Galaxy Star Formation Rates From Integrated Photometry: Insights from Color-Magnitude Diagrams of Resolved Stars
• The temperature dependence of the far-infrared-radio correlation in the Herschel-ATLAS
• Introducing piXedfit -- a Spectral Energy Distribution Fitting Code Designed for Resolved Sources
• A panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals
• A fast ionised wind in a Star Forming-Quasar system at z~1.5 resolved through Adaptive Optics assisted near-infrared data
• The Impact of Star Formation Histories on Stellar Mass Estimation: Implications from the Local Group Dwarf Galaxies
• Quantifying non-star formation associated 8um dust emission in NGC 628
• Herschel reveals the obscured star formation in HiZELS Hα emitters at z=1.47
• Ultra-strong MgII Absorbers as a Signature of Cool Intragroup Gas
• The bolometric and UV attenuation in normal spiral galaxies of the Herschel Reference Survey
• An Empirical Determination of the Dust Mass Absorption Coefficient, ${\kappa }_d$, Using the Herschel Reference Survey
• The growth of the central region by acquisition of counter-rotating gas in star-forming galaxies
• Exploring AGN and Star Formation Activity of Massive Galaxies at Cosmic Noon
• Investigating the Effect of Galaxy Interactions on AGN Enhancement at $0.5<z<3.0$
• The First Maps of ${\kappa }_d$ -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia
• EGG: hatching a mock Universe from empirical prescriptions
• A new estimate of the cosmic star formation density from a radio-selected sample, and the contribution of $H$-dark galaxies at $z\ge 3$
• Characterization of Two 2mm-detected Optically-Obscured Dusty Star-Forming Galaxies
• Measurements of the dust properties in z~1-3 SMGs with ALMA
• Cosmic evolution of low-excitation radio galaxies in the LOFAR Two-meter Sky Survey Deep Fields
• Isothermal dust models of Herschel-ATLAS galaxies
• Star Formation Suppression in Compact Group Galaxies: A New Path to Quenching?
• The evolution of rest-frame UV properties, Lya EWs and the SFR-Stellar mass relation at z~2-6 for SC4K LAEs
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• The second closest gamma-ray burst: sub-luminous GRB 111005A with no supernova in a super-solar metallicity environment
• GRB 080517: A local, low luminosity GRB in a dusty galaxy at z=0.09
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• VALES: III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies
• A${}^3$COSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time
• A Dust spectral energy distribution model with hierarchical Bayesian inference. I. Formalism & benchmarking
• Deriving star formation histories from photometry using energy balance spectral energy distribution modelling
• CO excitation, molecular gas density and interstellar radiation field in local and high-redshift galaxies
• Star Formation Suppression Due to Jet Feedback in Radio Galaxies with Shocked Warm Molecular Gas
• The Relationship between Stellar Mass, Gas Metallicity, and Star Formation Rate for Halpha-selected Galaxies at z~0.8 from the NewHalpha Survey
• GAMA/H-ATLAS: The Dust Opacity - Stellar Mass Surface Density Relation for Spiral Galaxies
• The SAMI Galaxy Survey: stellar population and structural trends across the Fundamental Plane
• The New Galaxy Evolution Paradigm Revealed by the Herschel Surveys
• CHILES VI: HI and H$\alpha$ Observations for z < 0.1 Galaxies; Probing HI Spin Alignment with Filaments in the Cosmic Web
• The SCUBA-2 Cosmology Legacy Survey: The EGS deep field - II. Morphological transformation and multi-wavelength properties of faint submillimetre galaxies
• Being WISE I: Validating Stellar Population Models and M/L ratios at 3.4 and 4.6 microns
• ALMA Twenty-six arcmin${}^2$ Survey of GOODS-S at One-millimeter (ASAGAO): X-ray AGN Properties of Millimeter-Selected Galaxies
• A Multi-wavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio Population
• Spatially-resolved dust properties of the GRB 980425 host galaxy
• The Strength of the 2175Å Feature in the Attenuation Curves of Galaxies at 0.1<z<3
• JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: I. Survey overview and first results
• To use or not to use synthetic stellar spectra in population synthesis models?
• Characterizing Dust Attenuation in Local Star Forming Galaxies: Inclination Effects and the 2175Å Feature
• Comprehensive Gas Characterization of a $z=2.5$ Protocluster: A Cluster Core Caught in the Beginning of Virialization?
• The Causes of the Red Sequence, the Blue Cloud, the Green Valley and the Green Mountain
• Radiative equilibrium estimates of dust temperature and mass in high-redshift galaxies
• Empirical predictions for (sub-)millimeter line and continuum deep fields
• NGC1266 as a Local Candidate for Rapid Cessation of Star Formation
• G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR
• MIGHTEE: Are giant radio galaxies more common than we thought?
• Infrared Spectral Energy Distribution and Variability of Active Galactic Nuclei: Clues to the Structure of Circumnuclear Material
• Herschel-ATLAS and ALMA: HATLAS J142935.3-002836, a lensed major merger at redshift 1.027
• A mid-IR study of Hickson Compact Groups II. Multi-wavelength analysis of the complete GALEX-Spitzer Sample
• Star formation histories, extinction, and dust properties of strongly lensed z~1.5-3 star-forming galaxies from the Herschel Lensing Survey
• Stellar content of extremely red quiescent galaxies at z>2
• X-ray flux in the SED modelling: An application of X-CIGALE in the XMM-XXL field
• Jet-ISM Interaction in the Radio Galaxy 3C293: Jet-driven Shocks Heat ISM to Power X-ray and Molecular H2 emission
• Modelling the cosmic spectral energy distribution and extragalactic background light over all time
• The miniJPAS survey: Identification and characterization of galaxy populations with the J-PAS photometric system
• The infrared-radio correlation of spheroid- and disc-dominated star-forming galaxies to z $\sim$ 1.5 in the COSMOS field
• Molecular Gas, Dust and Star Formation in Galaxies: II. Dust properties and scalings in \sim\ 1600 nearby galaxies
• The Evolving Interstellar Medium of Star-Forming Galaxies, as traced by $\text{Stardust}$
• The diverse evolutionary pathways of post-starburst galaxies
• GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching
• The SAMI Galaxy Survey: Satellite galaxies undergo little structural change during their quenching phase
• GAMA/H-ATLAS: The Local Dust Mass Function and Cosmic Density as a Function of Galaxy Type - A Benchmark for Models of Galaxy Evolution
• Star-Formation Bimodality in Early-Type Galaxies
• Early Science with the Large Millimeter Telescope: COOL BUDHIES I - a pilot study of molecular and atomic gas at z~0.2
• Optical vs. infrared studies of dusty galaxies and AGN: (I) Nebular emission lines
• Radio continuum size evolution of star-forming galaxies over 0.35 < z < 2.25
• Horizon-AGN virtual observatory -- 2: Template-free estimates of galaxy properties from colours
• Predicting the stellar and non-equilibrium dust emission spectra of high-resolution simulated galaxies with DART-Ray
• Machine-learning classification of astronomical sources: estimating F1-score in the absence of ground truth
• Two sub-millimetre bright protoclusters bounding the epoch of peak star-formation activity
• VALES: I. The molecular gas content in star-forming dusty H-ATLAS galaxies up to z=0.35
• The SAMI Galaxy Survey: Gas velocity dispersions in low-$z$ star-forming galaxies and the drivers of turbulence
• A mid-IR study of Hickson Compact Groups I : Probing the Effects of Environment in Galaxy Interactions
• Herschel Observations of Major Merger Pairs at z=0: Dust Mass and Star Formation
• Nebular emission from young stellar populations including binary stars
• Untangling the Nature of Spatial Variations of Cold Dust Properties in Star Forming Galaxies
• ALMA Lensing Cluster Survey: an ALMA galaxy signposting a MUSE galaxy group at z=4.3 behind 'El Gordo'
• Superluminous Spiral Galaxies
• The Far-Infrared Radio Correlation at low radio frequency with LOFAR/H-ATLAS
• Identifying active galactic nuclei via brightness temperature with sub-arcsecond International LOFAR Telescope observations
• The many faces of LINER-like galaxies: a WISE view
• Panchromatic SED modelling of spatially-resolved galaxies
• Co-evolution of black hole accretion and star formation in galaxies up to z=3.5
• The Spectral Energy Distributions of Active Galactic Nuclei
• Diversity of Galaxy Dust Attenuation Curves Drives the Scatter in the IRX-beta Relation
• The Spectral Energy Distributions of Active Galactic Nuclei
• Infrared signature of active massive black holes in nearby dwarf galaxies
• Resolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales
• A Comparison of the Stellar, CO and Dust-Continuum Emission from Three, Star-Forming HUDF Galaxies at $z\sim 2$
• Decoding spectral energy distributions of dust-obscured starburst-AGN
• Dust continuum, CO, and [C I] 1-0 lines: self-consistent H2 mass estimates and the possibility of globally CO-dark galaxies at $z=0.35$
• Investigating the Effect of Galaxy Interactions on Star Formation at 0.5<z<3.0
• Resolving the age bimodality of galaxy stellar populations on kpc scales
• The star-formation law at GMC scales in M33, the Triangulum Galaxy
• GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
• High-Resolution Radiative Transfer Modelling of M33
• Calibration of hybrid resolved star formation rate recipes based on PHANGS-MUSE H$\alpha$ and H$\beta$ maps
• JWST's PEARLS: A JWST/NIRCam view of ALMA sources
• ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-Forming Galaxies across $z\simeq 0.5-6$
• An ALMA view of star formation efficiency suppression in early-type galaxies after gas-rich minor mergers
• Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS
• The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly-alpha emitters at z>3
• A new look at local ultraluminous infrared galaxies: the atlas and radiative transfer models of their complex physics
• The dust mass function from z~0 to z~2
• Star-formation histories of local luminous infrared galaxies
• A near-infrared excess in the continuum of high-redshift galaxies: a tracer of star formation and circumstellar disks?
• Star-forming early- and quiescent late-type galaxies in the local Universe
• The Fundamental Plane in the LEGA-C Survey: unraveling the $M/L$ variations of massive star-forming and quiescent galaxies at $z\sim 0.8$
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• A panchromatic spatially-resolved analysis of nearby galaxies -- I. Sub-kpc scale Main Sequence in grand-design spirals
• Herschel-ATLAS: Correlations between Dust and Gas in Local Submm-Selected Galaxies
• AGN Selection Methods Have Profound Impacts on the Distributions of Host Galaxy Properties
• Infrared Contributions of X-Ray Selected Active Galactic Nuclei in Dusty Star-Forming Galaxies
• The ALMA Frontier Fields Survey - II. Multiwavelength Photometric analysis of 1.1mm continuum sources in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Dust properties and star formation of approximately a thousand local galaxies
• Beyond UVJ: Color Selection of Galaxies in the JWST Era
• GAMA/H-ATLAS: The ultraviolet spectral slope and obscuration in galaxies
• High-resolution, 3D radiative transfer modelling III. The DustPedia barred galaxies
• The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at $7<z<8$
• Multi-wavelength characterisation of z~2 clustered, dusty star forming galaxies discovered by Planck
• Close-up view of a luminous star-forming galaxy at z=2.95
• The Number Densities and Stellar Populations of Massive Galaxies at 3 < z < 6: A Diverse, Rapidly Forming Population in the Early Universe
• Predicting star formation properties of galaxies using deep learning
• Spatially resolved dust properties and quasar-galaxy decomposition of a HyLIRG at z = 4.4
• The fate of the interstellar medium in early-type galaxies. I. First direct measurement of the timescale of dust removal
• SDSS IV MaNGA: Dependence of Global and Spatially-resolved SFR-M* Relations on Galaxy Properties
• SDSS-IV MaNGA: spatially resolved dust attenuation in spiral galaxies
• ALMA constraints on star-forming gas in a prototypical z=1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps
• The resolved scaling relations in DustPedia: Zooming in on the local Universe
• ALMA + VLT observations of a Damped Lyman-α absorbing galaxy: Massive, wide CO emission, gas-rich but with very low SFR
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• Herschel observations of Hickson compact groups of galaxies: Unveiling the properties of cold dust
• High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project
• The Evolution of the Interstellar Medium in Post-Starburst Galaxies
• Simulated Galaxy Interactions as Probes of Merger Spectral Energy Distributions
• A High-Resolution Investigation of the Multi-Phase ISM in a Galaxy during the First Two Billion Years
• A Bayesian Population Model for the Observed Dust Attenuation in Galaxies
• Shaping the dust mass - star-formation rate relation
• ALMA Deep Field in SSA22: A near-infrared-dark submillimeter galaxy at z=4.0
• The kiloparsec-scale gas kinematics in two star-forming galaxies at $z\sim 1.47$ seen with ALMA and VLT-SINFONI
• The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends
• ALMA reveals a stable rotating gas disk in a paradoxical low-mass, ultra-dusty galaxy at z = 4.274
• The complex physics of dusty star-forming galaxies at high redshifts as revealed by Herschel and Spitzer
• Galaxy And Mass Assembly (GAMA): The Consistency of GAMA and WISE Derived Mass-to-Light Ratios
• Value Added Catalog of physical properties of more than 1.3 million galaxies from the DESI Survey
• The MUSE Extremely Deep Field: a first panoramic view of an Mg II emitting intragroup medium
• On the recovery of galaxy properties from SED fitting solutions
• Star Formation and Molecular Gas Diagnostics with Mid- and Far-Infrared Emission
• Obscured Active Galactic Nuclei triggered in compact star-forming galaxies
• Galaxy And Mass Assembly (GAMA): Blue spheroids within 87 Mpc
• Self-consistent Color-Mass-to-Light-Ratio relations for Low Surface Brightness Galaxies
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio correlation for High-redshift Dusty Star-forming Galaxies
• GAMA+KiDS: Alignment of galaxies in galaxy groups and its dependence on galaxy scale
• ProFuse: Physical Multi-Band Structural Decomposition of Galaxies and the Mass-Size-Age Plane
• AGN impact on the molecular gas in galactic centers as probed by CO lines
• Identifying the Location in the Host Galaxy of the Short GRB 111117A with the Chandra Sub-arcsecond Position
• Spatially resolving the dust properties and submillimetre excess in M 33
• ALMA Lensing Cluster Survey: a strongly lensed multiply imaged dusty system at $z\ge$6
• Bright, Relatively Isolated Star Clusters in PHANGS-HST Galaxies: Aperture Corrections, Quantitative Morphologies, and Comparison with Synthetic Stellar Population Models
• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• Planck's dusty GEMS. V. Molecular wind and clump stability in a strongly lensed star-forming galaxy at z=2.2
• The NIRSpec Wide GTO Survey
• The ALMA Frontier Fields Survey III: 1.1 mm Emission Line Identifications in Abell 2744, MACSJ0416.1-2403, MACSJ1149.5+2223, Abell 370, and Abell S1063
• Disentangling star formation and AGN activity in powerful infrared luminous radio galaxies at 1<z<4
• VIS3COS: II. Nature and nurture in galaxy structure and morphology
• COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys
• Gradients of Stellar Population Properties and Evolution Clues in a Nearby Galaxy M 101
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• Radio spectra and sizes of ALMA-identified submillimetre galaxies: evidence of age-related spectral curvature and cosmic ray diffusion?
• Galaxy And Mass Assembly (GAMA): Timescales for galaxies crossing the green valley
• Exploring the early dust-obscured phase of galaxy formation with blind mid-/far-IR spectroscopic surveys
• The KMOS Galaxy Evolution Survey (KGES): the angular momentum of star-forming galaxies over the last ~10 Gyr
• Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
• Welcome to the Twilight Zone: The Mid-Infrared Properties of Poststarburst Galaxies
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• De-blending Deep Herschel Surveys: A Multi-wavelength Approach
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• Star formation and quenching among the most massive galaxies at z~1.7
• Planck far-infrared detection of Hyper Suprime-Cam protoclusters at $\mathbf{z}\sim 4$: hidden AGN and star formation activity
• The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
• JINGLE V: Dust properties of nearby galaxies derived from hierarchical Bayesian SED fitting
• Dissecting Nearby Galaxies with piXedfit: I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting
• Probing multiphase gas in local massive elliptical galaxies via multiwavelength observations
• The Delay Times of Type Ia Supernova
• A Catalog of the Most Optically Luminous Galaxies at z<0.3: Super Spirals, Super Lenticulars, Super Post-Mergers, and Giant Ellipticals
• The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of highly star-forming galaxies
• A dynamical view on stellar metallicity gradient diversity across the Hubble sequence with CALIFA
• The Star Formation Reference Survey III: A Multi-wavelength View of Star Formation in Nearby Galaxies
• Cosmic evolution of radio-AGN feedback: confronting models with data
• ALMA observations of a metal-rich damped Lyα absorber at z = 2.5832: evidence for strong galactic winds in a galaxy group
• A${}^3$COSMOS and A${}^3$GOODSS: Continuum Source Catalogues and Multi-band Number Counts
• From Carbon to Cobalt: Chemical compositions and ages of $z\sim 0.7$ quiescent galaxies
• Properties of host galaxies of submillimeter sources as revealed by JWST Early Release Observations in SMACS J0723.3-7327
• The UV 2175Å Attenuation Bump and its Correlation with PAH Emission at z~2
• Biases and systematics in the observational derivation of galaxy properties: comparing different techniques on synthetic observations of simulated galaxies
• VIS3COS: III. environmental effects on the star formation histories of galaxies at z~0.8 seen in [OII], H$\delta$, and Dn4000
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• The bright end of the infrared luminosity functions and the abundance of hyperluminous infrared galaxies
• VIS3COS: I. survey overview and the role of environment and stellar mass on star formation
• The Kormendy Relation of Galaxies in the Frontier Fields Clusters: Abell S1063 and MACS J1149.5+2223
• Discovery of an extremely-luminous dust-obscured galaxy observed with SDSS, WISE, JCMT, and SMA
• Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• The first Hubble diagram and cosmological constraints using superluminous supernova
• Asymmetric mass models of disk galaxies - I. Messier 99
• High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
• The role of molecular gas in galaxy transition in compact groups
• The clustering of submillimeter galaxies detected with ALMA
• Jet-Shocked H2 and CO in the Anomalous Arms of Molecular Hydrogen Emission Galaxy NGC 4258
• Why do many early-type galaxies lack emission lines? I. Fossil clues
• Probing cold gas in a massive, compact star-forming galaxy at z=6
• Simulating the infrared sky with a Spritz
• The Role of Star-Formation and AGN in Dust Heating of z=0.3-2.8 Galaxies - II. Informing IR AGN fraction estimates through simulations
• NoSOCS in SDSS. V. Red Disc and Blue Bulge Galaxies Across Different Environments
• Stellar and Dust Properties of a Complete Sample of Massive Dusty Galaxies at $1\le z\le 4$ from MAGPHYS Modeling of UltraVISTA DR3 and Herschel Photometry
• New insights on the recoiling/binary black hole candidate J0927+2943 via molecular gas observations
• Impact of an AGN featureless continuum on estimation of stellar population properties
• The ISM Properties and Gas Kinematics of a Redshift 3 Massive Dusty Star-forming Galaxy
• IR SED and Dust Masses of Sub-solar Metallicity Galaxies at z~2.3
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• The molecular gas properties in local Seyfert 2 galaxies
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• Spectral Energy Distributions of Companion Galaxies to z$\sim$6 Quasars
• The impact of the Star Formation Histories on the SFR-M${}_{\ast }$ relation at z$\ge$2
• The dustier early-type galaxies deviate from late-type galaxies' scaling relations
• Signatures of long-lived spiral patterns
• S2COSMOS: Evolution of Gas Mass with Redshift Using Dust Emission
• The VISIR@VLT Mid-IR view of 47Tuc: A further step in solving the puzzle of RGB mass loss
• Properties and redshift evolution of star-forming galaxies with high [OIII]/[OII] ratios with MUSE at 0.28<z<0.85
• Massive Star Cluster Formation and Destruction in Luminous Infrared Galaxies in GOALS II: An ACS/WFC3 Survey of Nearby LIRGs
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Multi-frequency studies of galaxies and groups: I. Environmental effect on galaxy stellar mass and morphology
• In pursuit of giants: II. Evolution of dusty quiescent galaxies over the last six billion years from the hCOSMOS survey
• Revisiting Attenuation Curves: the Case of NGC 3351
• Galaxy And Mass Assembly (GAMA): Properties and evolution of red spiral galaxies
• The LOFAR Two-metre Sky Survey Deep fields: A new analysis of low-frequency radio luminosity as a star-formation tracer in the Lockman Hole region
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• MCSED: A flexible spectral energy distribution fitting code and its application to $z\sim 2$ emission-line galaxies
• FR-type radio sources at 3 GHz VLA-COSMOS: Relation to physical properties and large-scale environment
• Spectral Energy Distributions for 258 Local Volume Galaxies
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• Being WISE II: Reducing the Influence of Star Formation History on the Mass-to-Light Ratio of Quiescent Galaxies
• The AGN contribution to the UV-FIR luminosities of interacting galaxies and its role in identifying the Main Sequence
• Extended and Filamentary Lyman Alpha Emission from the Formation of a Protogalactic Halo at z=2.63
• Star formation in galaxies hosting AGN: A flat trend of star-formation rate with X-ray luminosity of galaxies hosting AGN in the SCUBA-2 Cosmology Legacy Survey
• A controlled study of cold dust content in galaxies from $z=0-2$
• The Dynamics and Distribution of Angular Momentum in HiZELS Star-Forming Galaxies at z = 0.8 - 3.3
• What shapes the far-infrared spectral energy distributions of galaxies?
• Spitzer Imaging of Herschel-ATLAS Gravitationally Lensed Submillimeter Sources
• ALMA reveals the molecular gas properties of 5 star-forming galaxies across the main sequence at 3 < z < 3.5
• A Multiwavelength view of IC 860: What Is in Action inside Quenching Galaxies
• Dust masses of $z>5$ galaxies from SED fitting and ALMA upper limits
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$): Detection of a dusty star-forming galaxy within the enormous Lyman $\alpha$ nebula at $z=2.3$ sheds light on its origin
• Identification of AKARI infrared sources by Deep HSC Optical Survey: Construction of New Band-Merged Catalogue in the NEP-Wide field
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• The spectral energy distribution of the hyperluminous, hot dust-obscured galaxy W2246$-$0526
• H-ATLAS/GAMA: The nature and characteristics of optically red galaxies detected at submillimetre wavelengths
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies IV. Physical properties derived from spectral energy distributions
• A photo-z cautionary tale: Redshift confirmation of COSBO-7 at z=2.625
• An H$\alpha$ Imaging Survey of the Low-surface-brightness Galaxies Selected from the Fall Sky Region of the 40$\%$ ALFALFA \ion{H}{1} Survey
• OH Megamasers in HI Surveys: Forecasts and a Machine Learning Approach to Separating Disks from Mergers
• Neutral carbon and highly excited CO in a massive star-forming main sequence galaxy at z=2.2
• Galaxy And Mass Assembly: the evolution of the cosmic spectral energy distribution from z = 1 to z = 0
• Genuine Retrieval of the AGN Host Stellar Population (GRAHSP)
• H-ATLAS/GAMA: Quantifying the Morphological Evolution of the Galaxy Population Using Cosmic Calorimetry
• The $z<1.2$ optical luminosity function from a sample of $\sim 410000$ galaxies in bootes
• From Peculiar Morphologies to Hubble-type Spirals: The relation between galaxy dynamics and morphology in star-forming galaxies at z~1.5
• The Star Formation Reference Survey-V: the effect of extinction, stellar mass, metallicity, and nuclear activity on star-formation rates based on H$\alpha$ emission
• The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
• Probing star formation and ISM properties using galaxy disk inclination I: Evolution in disk opacity since $z\sim 0.7$
• The X-ray and radio activity of typical and luminous Lya emitters from z~2 to z~6: evidence for a diverse, evolving population
• ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies (SMGs) Selected by Herschel: Discovery of Spatially Extended SMGs and Implications
• Investigating a population of infrared-bright gamma-ray burst host galaxies
• Evidence of a Flat Outer Rotation Curve in a Starbursting Disk Galaxy at $z=1.6$
• Multiwavelength Study of an X-ray Tidal Disruption Event Candidate in NGC 5092
• The Spatial Extent and Distribution of Star Formation in 3D-HST Mergers at z~1.5
• Star Formation in Intermediate Redshift 0.2 < z < 0.7 Brightest Cluster Galaxies
• The SAMI Galaxy Survey: Kinematics of Dusty Early-Type Galaxies
• A kpc-scale resolved study of unobscured and obscured star-formation activity in normal galaxies at z = 1.5 and 2.2 from ALMA and HiZELS
• Bayesian hierarchical modelling of the ${\mathrm{M}}_{\star }$-SFR relation from 1<z<6 in ASTRODEEP
• The submillimetre view of massive clusters at z~0.8-1.6
• Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets
• The dust SED of dwarf galaxies I. The case of NGC 4214
• Dust, gas, and metal content in star-forming galaxies at $z\sim 3.3$ revealed with ALMA and Near-IR spectroscopy
• Dust and Ionized Gas Association in E/S0 Galaxies with Dust Lanes: Clues to their Origin
• Observed versus modelled u,g,r,i,z-band photometry of local galaxies - Evaluation of model performance
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• The high-ionization IR fine-structure lines as bolometric indicators of the AGN power: study of the complete 12 micron AGN sample
• Simulations Find Our Accounting of Dust-Obscured Star Formation May Be Incomplete
• Galaxy And Mass Assembly (GAMA): The environmental dependence of the galaxy main sequence
• Discovery of a Dusty, Chemically Mature Companion to a z$\sim$4 Starburst Galaxy in JWST ERS Data
• SOFIA/HAWC+ View of an Extremely Luminous Infrared Galaxy, WISE1013+6112
• Galaxy And Mass Assembly (GAMA): The unimodal nature of the dwarf galaxy population
• Radio spectral properties of star-forming galaxies between 150-5000MHz in the ELAIS-N1 field
• Do galaxies die? Different views from simulations and observations in the Local Universe
• The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV & [OII]λ3727 luminosities
• Millisecond Pulsars Modify the Radio-SFR Correlation in Quiescent Galaxies
• The IBISCO survey: I. Multiphase discs and winds in the Seyfert galaxy Markarian 509
• The cosmic spectral energy distribution in the EAGLE simulation
• Accretion-Inhibited Star Formation in the Warm Molecular Disk of the Green-valley Elliptical Galaxy NGC 3226
• Rest-Frame Near-Infrared Radial Light Profiles up to z=3 from JWST/NIRCam: Wavelength Dependence of the Sérsic Index
• A Herschel-ATLAS study of dusty spheroids: probing the minor-merger process in the local Universe
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since $z=1.2$
• A multi-wavelength study of a massive, active galaxy at $z\sim 2$: coupling the kinematics of the ionized and molecular gas
• Single Colour Diagnostics of the Mass-to-light Ratio: Predictions from Galaxy Formation Models
• Predicting the global far-infrared SED of galaxies via machine learning techniques
• SMBH accretion properties of radio-selected AGN out to z~4
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• Probing the Timescale of the 1.4 GHz Radio emissions as a Star formation tracer
• Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsets
• The impact of the dynamical state of galaxy groups on the stellar populations of central galaxies
• Herschel and Hubble study of a lensed massive dusty starbursting galaxy at $z\sim 3$
• Observational Aspects of Galactic Accretion at Redshift 3.3
• H-ATLAS/GAMA and HeViCS - Dusty Early-Type Galaxies in Different Environments
• An $\mathrm{H}\alpha$ Imaging Survey of the Low Surface Brightness Galaxies Selected from the Spring Sky Region of the 40% ALFALFA HI Survey
• Dust attenuation, dust content and geometry of star-forming galaxies
• An ultra-deep multi-band VLA survey of the faint radio sky (COSMOS-XS): New constraints on the cosmic star formation history
• Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation
• Illuminating the Dark Side of Cosmic Star Formation III: Building the largest homogeneous sample of Radio-Selected Dusty Star-Forming Galaxies in COSMOS with PhoEBO
• Gravitational orbits in the expanding universe revisited
• X-ray Emission from the Taffy (VV254) Galaxies and Bridge
• Sacrificing information for the greater good: how to select photometric bands for optimal accuracy
• A closer look at the deep radio sky: Multi-component radio sources at 3-GHz VLA-COSMOS
• Measuring the average molecular gas content of star-forming galaxies at $z=3-4$
• Forensic reconstruction of galaxy colour evolution and population characterisation
• Removing biases in resolved stellar mass-maps of galaxy disks through successive Bayesian marginalization
• Stellar populations and physical properties of starbursts in the Antennae galaxy from self-consistent modelling of MUSE spectra
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• The most distant HI galaxies discovered by the 500 m dish FAST
• Synergies between low- and intermediate-redshift galaxy populations revealed with unsupervised machine learning
• Star Formation Rates and Stellar Masses of H-alpha Selected Star-Forming Galaxies at z=0.84: A Quantification of the Downsizing
• BEDE: Bayesian Estimates of Dust Evolution For Nearby Galaxies
• Spitzer catalog of Herschel-selected ultrared dusty, star-forming galaxies
• Physical Properties of Local Star-Forming Analogues to z~5 Lyman Break Galaxies
• Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5
• Reproducible $k$-means clustering in galaxy feature data from the GAMA survey
• Herschel Spectroscopy of the Taffy Galaxies (UGC 12914/12915 = VV 254): Enhanced [C II] emission in the collisionally-formed bridge
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• The XXL Survey: XXXI. Classification and host galaxy properties of 2.1 GHz ATCA XXL-S radio sources
• {\em Herschel}-ATLAS/GAMA: The Environmental Density of Far-Infrared Bright Galaxies at $z\le 0.5$
• On the Simultaneous Modelling of Dust and Stellar Populations for Interpretation of Galaxy Properties
• The Ultraviolet and Infrared Star Formation Rates of Compact Group Galaxies: An Expanded Sample
• VALES VII: Molecular and ionized gas properties in pressure balanced interstellar medium of starburst galaxies at z ~ 0.15
• Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
• A radiative transfer model for the spiral galaxy M33
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman break Galaxies
• Resolved optical-infrared SEDs of galaxies: universal relations and their break-down on local scales
• A single galaxy population? statistical evidence that the Star-Forming Main Sequence might be the tip of the iceberg
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at $z\approx 0.2$-$0.6$
• COLDz: Deep 34 GHz Continuum Observations and Free-free Emission in High-redshift Star-forming Galaxies
• An extremely low gas-to-dust ratio in the dust-lane lenticular galaxy NGC 5485
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• Galaxy properties from J-PAS narrow-band photometry
• Star-formation rates of cluster galaxies: nature vs nurture
• Resolved and Integrated Stellar Masses in the SDSS-IV/MaNGA Survey, Paper I: PCA spectral fitting & stellar mass-to-light ratio estimates
• SSGSS: The Spitzer-SDSS-GALEX Spectroscopic Survey
• Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio-galaxies?
• The evolution of the UV luminosity and stellar mass functions of Lyman-alpha emitters from z~2 to z~6
• Ongoing Massive Star Formation in NGC 604
• Mr-Moose: An advanced SED-fitting tool for heterogeneous multi-wavelength datasets
• The resolved chemical abundance properties within the interstellar medium of star-forming galaxies at $\text{z}\approx 1.5$
• On the Absence of High-Redshift AGNs: Little Growth in the Supermassive Black Hole Population at High Redshifts
• The Survey of Lines in M31 (SLIM): The Drivers of the [CII]/TIR Variation
• Starduster: A multi-wavelength SED model based on radiative transfer simulations and deep learning
• Multiple AGN in the crowded field of the compact group SDSSJ0959+1259
• The role of stochastic and smooth processes in regulating galaxy quenching
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• NGC4370: a case study for testing our ability to infer dust distribution and mass in nearby galaxies
• On the Impact of Inclination-Dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
• Galaxy and Mass Assembly (GAMA): Probing the merger histories of massive galaxies via stellar populations
• MAGPHYS: a publicly available tool to interpret observed galaxy SEDs
• Panchromatic Photometry of Low-redshift, Massive Galaxies Selected from SDSS Stripe 82
• The Stellar Masses of ~40,000 UV Selected Galaxies from the WiggleZ Survey at 0.3<z<1.0: Analogues of Lyman Break Galaxies?
• The `Cosmic Seagull': a highly magnified disk-like galaxy at z~2.8 behind the Bullet Cluster
• The ALMA-CRISTAL survey: Dust temperature and physical conditions of the interstellar medium in a typical galaxy at z=5.66
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• COSMOS-Web: A history of galaxy migrations over the stellar mass-star formation rate plane
• Discovery of a giant and luminous Lya+CIV+HeII nebula at z=3.326 with extreme emission line ratios
• Estimating stellar population and emission line properties in S-PLUS galaxies
• The Physical Drivers of the Luminosity-Weighted Dust Temperatures in High-Redshift Galaxies
• GOODS-$Herschel$: identification of the individual galaxies responsible for the 80-290$\mu$m cosmic infrared background
• Modelling the spectral energy distribution of galaxies: introducing the artificial neural network
• COLDz: Probing Cosmic Star Formation With Radio Free-free Emission
• Star-Forming, Rotating Spheroidal Galaxies in the GAMA and SAMI Surveys
• A More Efficient Search for H2O Megamaser Galaxies : The Power of the X-ray and Mid-infrared Photometry
• The impact of stellar bars on star-formation quenching: Insights from a spatially resolved analysis in the local Universe
• Molecular Gas Kinematics and Star Formation Properties of the Strongly-Lensed Quasar Host Galaxy RXS J1131-1231
• Unveiling Sizes of Compact AGN Hosts with ALMA
• ALMA 26 arcmin${}^2$ survey of GOODS-S at one-millimeter (ASAGAO): millimeter properties of stellar mass selected galaxies
• NOEMA confirmation of an optically dark ALMA-AzTEC submillimetre galaxy at $z=5.24$. A late-stage starburst prior to quenching
• UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?
• The Herschel Virgo Cluster Survey. XIX. Physical properties of low luminosity FIR sources at $z<$ 0.5
• Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing
• Three Dusty Star Forming Galaxies at $z\sim 1.5$: Mergers and Disks on the Main Sequence
• New-generation dust emission templates for star-forming galaxies
• Morphology-assisted galaxy mass-to-light predictions using deep learning
• Galaxy And Mass Assembly: Group and field galaxy morphologies in the star-formation rate - stellar mass plane
• Dust grain size evolution in local galaxies: a comparison between observations and simulations
• Physical properties of hyperluminous, dust-obscured quasars at $z\sim 3$: multiwavelength Spectral Energy Distribution analysis and cold gas content revealed by ALMA
• Local Analogs to High-Redshift Galaxies: I. Characterization of Dust Emission and Star Formation History
• On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
• Detection of [O III] at z~3: A Galaxy above the Main Sequence, Rapidly Assembling its Stellar Mass
• The physical properties of Spitzer/IRS galaxies derived from their UV to 22 $\mu$m spectral energy distribution
• After the interaction: an efficiently star-forming molecular disk in NGC5195
• Galaxy classification: A machine learning analysis of GAMA catalogue data
• Flexible Models for Galaxy Star Formation Histories Both Shift and Scramble the Optical Color-M/L Relationship
• Infrared view of the multiphase ISM in NGC 253 I. Observations and fundamental parameters of the ionised gas
• The Long and the Short of It: The Benefits and Leverage of Ultraviolet-Radio Galaxy Fitting
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) II: Structural Properties and Near-Infrared Morphologies of Faint Submillimeter Galaxies
• Alma Reveals A Gas-rich, Maximum-starburst In The Hyperluminous, Dust-obscured Quasar W0533-3401 AT $z\sim 2.9$
• The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas
• Over-density of SMGs in fields containing z~0.3 galaxies: magnification bias and the implications for studies of galaxy evolution
• The ALMA Spectroscopic Survey in the HUDF: Constraining the Molecular Content at $\log (M_{\ast }/M_{\odot })\sim 9.5$ with CO stacking of MUSE detected $z\sim 1.5$ Galaxies
• The eROSITA Final Equatorial-Depth Survey (eFEDS): An X-ray bright, extremely luminous infrared galaxy at z = 1.87
• The slippery slope of dust attenuation curves: Correlation of dust attenuation laws with star-to-dust compactness up to z = 4
• The molecular gas in the central region of NGC 7213
• A deep radio view of the evolution of the cosmic star-formation rate density from a stellar-mass selected sample in VLA-COSMOS
• Improving machine learning-derived photometric redshifts and physical property estimates using unlabelled observations
• The ALPINE-ALMA [CII] survey: double stellar population and AGN activity in a galaxy at $z\sim 5.5$
• Revealing the Nature of a Lyman-$\alpha$ Halo in a Strongly Lensed Interacting System at $z=2.92$
• Measuring the Obscuring Column of a Disk Megamaser AGN in a Nearby Merger
• Systematic errors on optical-SED stellar mass estimates for galaxies across cosmic time and their impact on cosmology
• Star-formation rates of two GRB host galaxies at z~2 and a [CII] deficit observed with ALMA
• Where Do Obscured AGN Fit in A Galaxy's Timeline?
• Galaxy And Mass Assembly (GAMA): Self-Organizing Map Application on Nearby Galaxies
• Tracing the co-evolution path of super massive black holes and spheroids with AKARI-selected ultra-luminous IR galaxies at intermediate redshifts
• The ALMA Frontier Fields survey V: ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Galaxy And Mass Assembly: Galaxy Zoo spiral arms and star formation rates
• Spitzer Imaging of Strongly-Lensed Herschel-Selected Dusty Star Forming Galaxies
• Star forming and gas rich brightest cluster galaxies at $z\sim 0.4$ in the Kilo-Degree Survey
• Unraveling Joint Evolution of Bars, Star Formation, and Active Galactic Nuclei of Disk Galaxies
• Galaxy And Mass Assembly (GAMA): Defining Passive Galaxy Samples and Searching for the UV Upturn
• LoCuSS: exploring the connection between local environment, star formation and dust mass in Abell 1758
• Characteristics of mid-infrared PAH emission from star-forming galaxies selected at 250 μm in the North Ecliptic Pole (NEP) field
• MOSEL survey: JWST reveals major mergers/strong interactions drive the extreme emission lines in the early universe
• Age and metal gradients in massive quiescent galaxies at $0.6\lesssim z\lesssim 1.0$: implications for quenching and assembly histories
• Ages and metallicities of quiescent galaxies: confronting broadband ($UVJ$) colours with stellar absorption lines
• VALES: IV. Exploring the transition of star formation efficiencies between normal and starburst galaxies using APEX/SEPIA Band-5 and ALMA at low redshift
• Tightly coupled morpho-kinematic evolution for massive star-forming and quiescent galaxies across 7 Gyr of cosmic time
• ACCESS IV: The quenching of star formation in a cluster population of dusty S0s
• Dust Properties of Local Dust-Obscured Galaxies with the Submillimeter Array
• Bar rejuvenation in S0 galaxies?
• AGN in Dusty Starbursts at Z=2: Feedback Still To Kick In
• Star formation activity beyond the outer Arm I: WISE-selected candidate star-forming regions
• A VLT/FORS2 Narrowband Imaging Search for MgII Emission Around z ~ 0.7 Galaxies
• SAMI-HI: The HI view of the H$\alpha$ Tully-Fisher relation and data release
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Molecular gas budget and characterization of intermediate-mass star-forming galaxies at $z\approx 2-3$
• Cold gas mass measurements for the era of large optical spectroscopic surveys
• The shock-induced star formation sequence resulting from a constant spiral pattern speed
• SEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1$-$1148 at $z\sim 0.5$
• Cosmic dance in the Shapley Concentration Core - I. A study of the radio emission of the BCGs and tailed radio galaxies
• Lightning: An X-ray to Submillimeter Galaxy SED-Fitting Code With Physically-Motivated Stellar, Dust, and AGN Models
• Physical Properties of the Host Galaxies of Ca-rich Transients
• Universe opacity and EBL
• Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z $\sim$2
• The star-forming main sequence and the contribution of dust-obscured star formation since $z\sim 4$ from the FUV+IR luminosity functions
• Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at $z\sim 7$
• The Loneliest Galaxies in the Universe: A GAMA and GalaxyZoo Study on Void Galaxy Morphology
• Relativistic supernova 2009bb exploded close to an atomic gas cloud
• GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting
• Radiative and mechanical energies in galaxies I. Contributions of molecular shocks and PDRs in 3C 326 N
• Multi-wavelength lens reconstruction of a $\text{Planck}$ $\&$ $\text{Herschel}$-detected star-bursting galaxy
• Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0
• Analytic models of dust temperature in high-redshift galaxies
• Evolution of grain size distribution with enhanced abundance of small carbonaceous grains in galactic environments
• Identifying radio active galactic nuclei among radio-emitting galaxies
• An accurate new method of calculating absolute magnitudes and K-corrections applied to the Sloan filter set
• Redshift Evolution of the H2/HI Mass Ratio In Galaxies
• COLDz: Karl G. Jansky Very Large Array discovery of a gas-rich galaxy in COSMOS
• Infrared Spectral Energy Distribution of Galaxies in the AKARI All Sky Survey: Correlations with Galaxy Properties, and Their Physical Origin
• Modeling IR Spectral Energy Distributions: A Pilot Study of Starburst Parameters and Silicate Absorption Curves for Some GOALS Galaxies
• Disentangling the AGN and Star-Formation Contributions to the Radio-X-ray Emission of Radio-Loud Quasars at 1<z<2
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
• COSMOS2020: Investigating the AGN-obscured accretion phase at $z\sim 1$ via [NeV] selection
• High dense gas fraction in a gas-rich star-forming galaxy at z = 1.2
• The Opacity of Spiral Galaxy Disks IX; Dust and Gas Surface Densities
• Dying of the Light: An X-ray Fading Cold Quasar at z ~ 0.405
• Radio-Infrared Correlation for Local Dusty Galaxies and Dusty AGNs from the AKARI All Sky Survey
• Accretion History of AGN: Estimating the Host Galaxy Properties in X-ray Luminous AGN from z=0-3
• $\text{Herschel}$ Photometric Observations of $\mathrm{L}\mathrm{ITTLE}$ $\mathrm{T}\mathrm{HINGS}$ Dwarf Galaxies
• CO Excitation and Line Energy Distributions in Gas-selected Galaxies
• The spectral energy distribution of galaxies at z > 2.5: Implications from the Herschel/SPIRE color-color diagram
• Do bulges stop stars forming?
• Galaxy And Mass Assembly (GAMA): Stellar-to-Dynamical Mass Relation I. Constraining the Precision of Stellar Mass Estimates
• A Method to improve line flux and redshift measurements with narrowband filters
• Applications of Stellar Population Synthesis in the Distant Universe
• Probing star formation and ISM properties using galaxy disk inclination III: Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
• Physical properties of strong 1 < z < 3 Balmer and Paschen lines emitters observed with JWST
• KMTNet Nearby Galaxy Survey III. Deficient H$\alpha$ flux in the Extended Disks of Spiral Galaxies
• Probing the interstellar medium of NGC1569 with Herschel
• The variation of the gas content of galaxy groups and pairs compared to isolated galaxies
• Re-assessing the stellar population scaling relations of the galaxies in the Local Universe
• Observational signatures of the dust size evolution in isolated galaxy simulations
• [CII] and CO Emission Along the Bar and Counter-Arms of NGC 7479
• SMART: spectral energy distributions Markov chain analysis with radiative transfer models
• Stellar Populations of Early-type Galaxies with Mid-Infrared Excess Emission
• Merging Galaxies in Isolated Environments II. Evolution of Star Formation and Accretion Activity during the Merging Process
• Radio-only and Radio-to-far-ultraviolet Spectral Energy Distribution Modeling of 14 ULIRGs: Insights into the Global Properties of Infrared Bright Galaxies
• VALES V: A kinematic analysis of the molecular gas content in $H$-ATLAS galaxies at $z\sim 0.03-0.35$ using ALMA
• UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample
• Radio Variability and Broad-Band Spectra of Infrared Galaxies with and without OH Megamaser Emission
• Cosmic evolution of grain size distribution in galaxies using the ${\nu }^2$GC semi-analytic model
• Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
• SkyMapper colours of Seyfert galaxies and Changing-Look AGN
• SEEDisCS II. Molecular gas in galaxy clusters and their large scale structure: low gas fraction galaxies, the case of CL1301.7$-$1139
• A multi-band AGN-SFG classifier for extragalactic radio surveys using machine learning
• How accurate are infrared luminosities from monochromatic photometric extrapolation?
• Exploring Damped Lyman-$\alpha$ System Host Galaxies using Gamma-ray Bursts
• The Physical Characteristics of Interstellar Medium in NGC 3665 with Herschel Observations
• Stellar, Gas, and Dust Emission of Star Forming Galaxies out to z~2
• Environmental effects in Herschel observations of the ionized carbon content of star forming dwarf galaxies in the Virgo cluster
• Galaxy Properties Derived with Spectral Energy Distribution Fitting in the Hawaii-Hubble Deep Field-North
• Dark Matter Fraction in Disk-Like Galaxies Over the Past 10 Gyr
• Star forming brightest cluster galaxies at $z\sim 0.4$ in KiDS. Further studies of cold gas and stellar properties
• The multi-phase ISM in the nearby composite AGN-SB galaxy NGC 4945: large (parsecs) scale mechanical heating
• The infrared-radio relation in the local universe
• Restarting radio activity and dust emission in radio-loud broad absorption line quasars
• UV-FIR SED modeling of AGN in IR-luminous galaxies up to z~2.5: Understanding the effects of torus models
• Mapping the working of environmental effects in A963
• Observations of Far-Ultraviolet Diffuse Emission from the Small Magellanic Cloud
• Are superthin galaxies low surface brightness galaxies seen edge-on? The star formation probe
• Measuring Dust Attenuation Curves of SINGS/KINGFISH Galaxies Using Swift/UVOT Photometry
• A simple numerical experiment on the dust temperature bias for Lyman break galaxies at $z\gtrsim 5$
• RadioSED I: Bayesian inference of radio SEDs from inhomogeneous surveys
• Major mergers with small galaxies - the discovery of a Magellanic-type galaxy at z=0.12
• SAMI-HI: the connection between global asymmetry in the ionised and neutral atomic hydrogen gas in galaxies
• Galaxy Evolution in the Cluster Abell 85: New Insights from the Dwarf Population
• Galaxy and Mass Assembly (GAMA): Low-redshift Quasars and Inactive Galaxies Have Similar Neighbors
• A Bayesian chemical evolution model of the DustPedia Galaxy M74
• Virgo Filaments V: Disrupting the Baryon Cycle in the NGC 5364 Galaxy Group
• Suppression of Star Formation in the Hosts of Low-Excitation Radio Galaxies
• Disk Mass-to-Light ratio distribution from stellar population synthesis: Application to rotation curve decomposition of NGC 5278 (KPG 390A)
• Massive molecular gas reservoir in a luminous sub-millimeter galaxy during cosmic noon
• Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Milky Way-Like Gas Excitation in an Ultrabright Submillimeter Galaxy at $z=1.6$
• Outer and inner mass distributions of the irregular galaxies UGC 4284 and UGC 11861: Constraining the baryonic content through stellar population synthesis studies
• Detecting episodes of star formation using Bayesian model selection
• The Spitzer-IRAC/MIPS Extragalactic Survey (SIMES): II enhanced nuclear accretion rate in galaxy groups at z$\sim$0.2
• H$\alpha$-based Star Formation Rates in and around z $\sim$ 0.5 EDisCS clusters
• A subarcsecond near-infrared view of massive galaxies at z > 1 with Gemini Multiconjugate Adaptive Optics
• Dynamics of the galactic component of Abell S1063 and MACS J1206.2$-$0847
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• A MeerKAT view on galaxy clusters: a radio-optical study of Abell 1300 and MACS J1931.8--2634
• HI properties and star formation history of a fly-by pair of blue compact dwarf galaxies
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• A new distant Giant Radio Galaxy in the Boötes field serendipitously detected by Chandra
• The Einstein ring GAL-CLUS-022058s: a Lensed Ultrabright Submillimeter Galaxy at z=1.4796
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Compact groups of galaxies in GAMA -- Probing the densest minor systems at intermediate redshifts
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• The unusual ISM in Blue and Dusty Gas Rich Galaxies (BADGRS)
• Panchromatic SED fitting codes and modelling techniques
• VALES VIII: Weak ionized gas outflows in star-forming galaxies at $z\sim 0.15$ traced with VLT/MUSE
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• On the Thermally Pulsing Asymptotic Giant Branch Contribution to the Light of Nearby Disk Galaxies
• Star formation and black hole accretion activity in rich local clusters of galaxies
• Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
• Merging galaxies in isolated environments I. Multiband photometry, classification, stellar masses, and star formation rates
• The far-infrared emission of the radio-loud quasar 3C318
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Hot-Dust (690K) Luminosity Density and its Evolution in the last 7.5Gyr
• Far-IR dust properties of highly dust obscured AGNs from the AKARI and WISE all-sky surveys
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• The black hole masses of extremely luminous radio-WISE selected galaxies
• The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA
• SDSS J122958.84+000138.0: A Compact, Optically red galaxy
• Cool Interstellar Medium as an Evolutionary Tracer in ALMA-Observed Local Dusty Early-Type Galaxies
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• IC 630: Piercing the Veil of the Nuclear Gas
• A Submillimeter Continuum Survey of Local Dust-Obscured Galaxies
• Identifying and Characterizing the Most Heavily Dust-Obscured Galaxies at $1\le z\le 4$
• The dust-star interplay in late-type galaxies at z < 0.5: forecasts for the JWST
• LEGA-C stellar populations scaling relations. I: Chemo-archaeological downsizing trends at z~0.7
• Euclid preparation. Estimating galaxy physical properties using CatBoost chained regressors with attention
• Predicting far-infrared maps of galaxies via machine learning techniques
• Unsupervised Domain Adaptation for Constraining Star Formation Histories
• Star formation activity in a young galaxy cluster at z=0.866
• A unique distant submillimeter galaxy with an X-ray-obscured radio-luminous active galactic nucleus
• General circular velocity relation of a test particle in a 3D gravitational potential: application to the rotation curves analysis and total mass determination of UGC 8490 and UGC 9753
• A comparative study of galaxy evolution with four different active galactic nucleus torus models and two different host geometries
• A Catalog of Stellar and Dust Properties for 500,000 Stars in the Southwest Bar of the Small Magellanic Cloud
• Molecular gas content and high excitation of a massive main-sequence galaxy at z = 3
• The molecular-gas properties in the gravitationally lensed merger HATLAS J142935.3-002836
• Euclid view of dusty star forming galaxies at z>~1.5 detected in wide area submillimetre surveys
• Dust contribution to the panchromatic galaxy emission
• SOFIA/HAWC+ detection of a gravitationally lensed starburst galaxy at $z$ = 1.03
• Infrared galaxies detected by the Atacama Cosmology Telescope
• Systematics in the SED Fitting Parameter Estimation of Composite Galaxies
• Overdense fireworks in GOODS-N: Unveiling a record number of massive dusty star forming galaxies at z$\sim$5.2 with the N2CLS
• Impact of galactic and intergalactic dust on the stellar EBL
• Reconstructing the mid-infrared spectra of galaxies using ultraviolet to submillimeter photometry and Deep Generative Networks
• The LEGA-C and SAMI Galaxy Surveys: Quiescent Stellar Populations and the Mass-Size Plane across 6 Gyr
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Galaxy And Mass Assembly: A new approach to quantifying dust in galaxies
• Beetroots: spatially-regularized Bayesian inference of physical parameter maps -- Application to Orion
• Dashing through the cluster: An X-ray to radio view of UGC 10420 undergoing ram-pressure stripping
• Investigating the role of turbulence in the interstellar medium in $z\sim 3$ dusty star-forming galaxies using kpc-resolution ALMA dust and gas maps
• Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
• A simple model to interpret the ultraviolet, optical and infrared SEDs of galaxies
• Galaxy And Mass Assembly (GAMA): The Dependence of Star Formation on Surface Brightness in Low Redshift Galaxies
• SHAPE. I. A SOM-SED hybrid approach for efficient galaxy parameter estimation leveraging JWST
• On the ages of the stellar populations of galaxies at $z=0.1$-7
• Ultraviolet-to-far-infra-red self-consistent analysis of the stellar populations of massive starburst galaxies at intermediate redshifts
• Dust removal timescale in galaxies across cosmic time
• AstroSat observations of interacting galaxies NGC 7469 and IC 5283
• The GAMA Panchromatic Survey
• Missing Lensed Images and the Galaxy Disk Mass in CXOCY J220132.8-320144
• The SEDs of Interacting Galaxies
• Interpreting Galaxy Properties with Improved Modelling
• Dust in dwarf galaxies: The case of NGC 4214
• WISE J044232.92+322734.9: A star-forming galaxy at redshift 1.1 seen through a Galactic dust clump?
• Challenges in Stellar Population Studies
• UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
• Oxyster: A Circumgalactic Low-ionization Oxygen Nebula next to a Starburst Galaxy at $z\sim 1$
• The Nature of Hyperluminous Infrared Galaxies
• Galaxy evolution on resolved scales: ageing and quenching in CALIFA
• A complete census of AGN and their hosts from optical surveys?
• Hunting Star-Forming Galaxies in the Gamma-Ray Domain
• Identifying AGN host galaxies by Machine Learning with HSC+WISE
• Unravelling the origin of extended radio emission in narrow-line Seyfert 1 galaxies with the JVLA
• Extensive Lensing Survey of Optical and Near-Infrared Dark Objects (El Sonido): HST H-Faint Galaxies behind 101 Lensing Clusters
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Spectral energy distribution similarity of the local galaxies and the 3.6um selected galaxies from the Spitzer Extended Deep Survey
• A comparison of dust content and properties in GAMA/G10-COSMOS/3D-HST and SIMBA cosmological simulations
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Atomic hydrogen reservoirs in quiescent galaxies at z = 0.4
• H${}_2$ content of galaxies inside and around intermediate redshift clusters
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars
• Theoretical clues about dust accumulation and galaxy obscuration at high and low redshift
• The Redshifts from 122 Bands: Comparative Redshift Forecast for Low-Resolution Spectra from SPHEREx and 7-Dimensional Sky Survey (7DS)
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
• Spatial disconnection between stellar and dust emissions: the test of the Antennae Galaxies (Arp 244)
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• Topological models to infer multiphase interstellar medium properties
• Far-infrared observations of dust in Ly$\alpha$ emitters at z=2-6
• AstroSat-UVIT observations of a possibly interacting pair of galaxies in HCG 77
• KURVS: chemical properties from multiple strong line calibrations for star-forming galaxies at $z\sim 1.5$
• Low star-formation activity and low gas content of quiescent galaxies at $z=$ 3.5-4.0 constrained with ALMA
• Cold Quasar Investigation: Comparing Star Formation Rates to Black Hole Growth
• JWST MIRI color classification of mid-infrared selected galaxies: MIRI color classification toward cosmic noon
• A multiwavelength study of an early galaxy group merger in COSMOS revealed by two tailed radio galaxies at z = 0.35
• What is the amount of baryonic dark matter in galaxies?
• Synergy between Roman and PRIMA imaging capabilities for large extragalactic surveys
• The gMOSS: the galaxy survey and galaxy populations of the large homogeneous field