Modeling the Panchromatic Spectral Energy Distributions of Galaxies

Abstract

The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical property of the system, including the star formation history, metal content, abundance pattern, dust mass, grain size distribution, star-dust geometry, and interstellar radiation field. The principal goal of stellar population synthesis (SPS) is to extract these variables from observed SEDs. In this review I provide an overview of the SPS technique and discuss what can be reliably measured from galaxy SEDs. Topics include stellar masses, star formation rates and histories, metallicities and abundance patterns, dust properties, and the stellar initial mass function.

66 pages, 14 figures, to appear in Annual Review of Astronomy and Astrophysics (ARAA), vol 51

References in corpus (72)

• Modules for Experiments in Stellar Astrophysics (MESA)
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
• The Dartmouth Stellar Evolution Database
• K-corrections and filter transformations in the ultraviolet, optical, and near infrared
• UV Star Formation Rates in the Local Universe
• A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
• Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample
• Detection of quiescent galaxies in a bicolor sequence from z=0-2
• 3D-HST: A wide-field grism spectroscopic survey with the Hubble Space Telescope
• A systematic variation of the stellar initial mass function in early-type galaxies
• Stellar Diameters and Temperatures II. Main Sequence K & M Stars
• The ACS Nearby Galaxy Survey Treasury
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• The SEGUE Stellar Parameter Pipeline. I. Description and Initial Validation Tests
• The effect of massive binaries on stellar populations and supernova progenitors
• The Stellar Initial Mass Function in Early-Type Galaxies From Absorption Line Spectroscopy. II. Results
• Evolution of asymptotic giant branch stars I. Updated synthetic TP-AGB models and their basic calibration
• Evidence for TP-AGB stars in high redshift galaxies, and their effect on deriving stellar population parameters
• What do we learn from IRAC observations of galaxies at 2 < z < 3.5?
• Population Synthesis in the Blue IV: Accurate Model Predictions for Lick Indices and UBV Colors in Single Stellar Populations
• The Initial-Final Mass Relation: Direct Constraints at the Low Mass End
• The Direct Detection of Lyman-Continuum Emission from Star-forming Galaxies at z~3
• The Characteristic Star Formation Histories of Galaxies at Redshifts z~2-7
• Sunrise: Polychromatic Dust Radiative Transfer in Arbitrary Geometries
• Medium-resolution Isaac Newton Telescope library of empirical spectra - II. The stellar atmospheric parameters
• Recovering galaxy star formation and metallicity histories from spectra using VESPA
• Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: IV The Controlling Parameters of the Starburst SED
• Stellar Evolutionary Effects on the Abundances of PAH and SN-Condensed Dust in Galaxies
• The Evolution of Stellar Mass and the Implied Star Formation History
• Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution, and implications for the IMF
• GOODS-Herschel:dust attenuation properties of UV selected high redshift galaxies
• Spectroscopic ages and metallicities of stellar populations: validation of full spectrum fitting
• Spectral models for solar-scaled and alpha-enhanced stellar populations
• Spitzer Mid-to-Far-Infrared Flux Densities of Distant Galaxies
• The ALHAMBRA Project: A large area multi medium-band optical and NIR photometric survey
• On the interpretation of age and chemical composition of composite stellar populations determined with line-strength indices
• A Large Stellar Evolution Database for Population Synthesis Studies. III. Inclusion of the full Asymptotic Giant Branch phase and Web tools for stellar population analyses
• Stellar Population and Kinematic Profiles in Spiral Bulges & Disks: Population Synthesis of Integrated Spectra
• Dissecting the Red Sequence--I. Star Formation Histories of Quiescent Galaxies: The Color-Magnitude vs. the Color-Sigma Relation
• SHARDS: an optical spectro-photometric survey of distant galaxies
• Stellar mass estimates in early-type galaxies: procedures, uncertainties and models dependence
• A Near-Infrared Spectroscopic Survey of K-selected Galaxies at z~2.3: Redshifts and Implications for Broadband Photometric Studies
• The stellar population histories of early-type galaxies. III. The Coma Cluster
• The Stellar Initial Mass Function in Early-Type Galaxies From Absorption Line Spectroscopy. I. Data and Empirical Trends
• A large stellar evolution database for population synthesis studies. IV. Integrated properties and spectra
• Near Infrared spectroscopy of post-starburst galaxies: a limited impact of TP-AGB stars on galaxy SEDs
• Systematic Uncertainties in Stellar Mass Estimation for Distinct Galaxy Populations
• Stellar Population Models and Individual Element Abundances I: Sensitivity of Stellar Evolution Models
• Galaxy-scale Star Formation on the Red Sequence: the Continued Growth of S0s and the Quiescence of Ellipticals
• Constraints on Physical Properties of z~6 Galaxies Using Cosmological Hydrodynamic Simulations
• UV dust attenuation in spiral galaxies: the role of age-dependent extinction and of the IMF
• The SWELLS survey - V. A Salpeter stellar initial mass function in the bulges of massive spiral galaxies
• Ultraviolet through Infrared Spectral Energy Distributions from 1000 SDSS Galaxies: Dust Attenuation
• Biases and Uncertainties in Physical Parameter Estimates of Lyman Break Galaxies from Broad-band Photometry
• The Mass-Loss Return from Evolved Stars to the Large Magellanic Cloud IV: Construction and Validation of a Grid of Models for Oxygen-Rich AGB Stars, Red Supergiants, and Extreme AGB Stars
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• Beyond UVJ: Color Selection of Galaxies in the JWST Era
• Dust properties and star formation of approximately a thousand local galaxies
• The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude
• Predicting star formation properties of galaxies using deep learning
• Kpc-scale Properties of Emission-line Galaxies
• The Diverse Morphology, Stellar Population, and Black Hole Scaling Relations of the Host Galaxies of Nearby Quasars
• Exploring the astrophysics of dark atoms
• Rebutting fake news on full spectral fitting
• No evidence for modifications of gravity from galaxy motions on cosmological scales
• Inverse stellar population age gradients of post-starburst galaxies at z=0.8 with LEGA-C
• Deep Synoptic Array science: A massive elliptical host among two galaxy-cluster fast radio bursts
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• Seeing sharper and deeper: JWST's first glimpse of the photometric and spectroscopic properties of galaxies in the epoch of reionisation
• A Bayesian Population Model for the Observed Dust Attenuation in Galaxies
• SDSS-IV MaNGA: Uncovering the Angular Momentum Content of Central and Satellite Early-type Galaxies
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• On the evolution of the central density of quiescent galaxies
• Galaxy And Mass Assembly (GAMA): The Consistency of GAMA and WISE Derived Mass-to-Light Ratios
• Linking Characteristics of the Polycyclic Aromatic Hydrocarbon Population with Galaxy Properties: A Quantitative Approach Using the NASA Ames PAH IR Spectroscopic Database
• Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate and α-enhancement
• Forward modeling of galaxy populations for cosmological redshift distribution inference
• ZFIRE: The Evolution of the Stellar Mass Tully-Fisher Relation to Redshift 2.0 < Z < 2.5 with MOSFIRE
• Value Added Catalog of physical properties of more than 1.3 million galaxies from the DESI Survey
• On the Red Giant Branch: Ambiguity in the Surface Boundary Condition Leads to ~100 K Uncertainty in Model Effective Temperatures
• Recovering stellar population parameters via different population models and stellar libraries
• Discovery of the optical afterglow and host galaxy of short GRB181123B at $z=1.754$: Implications for Delay Time Distributions
• Self-consistent Color-Mass-to-Light-Ratio relations for Low Surface Brightness Galaxies
• On the recovery of galaxy properties from SED fitting solutions
• Spatially Resolved Stellar Spectroscopy of the Ultra-diffuse Galaxy Dragonfly 44. III. Evidence for an Unexpected Star-Formation History
• Deep Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys
• Disentangling star formation and AGN activity in powerful infrared luminous radio galaxies at 1<z<4
• A Trio of Massive Black Holes Caught in the Act of Merging
• Archetype-Based Redshift Estimation for the Dark Energy Spectroscopic Instrument Survey
• Compact, bulge dominated structures of spectroscopically confirmed quiescent galaxies at z~3
• How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
• Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
• Surrogate modelling the Baryonic Universe I: The colour of star formation
• The Star-forming Main Sequence of the Host Galaxies of Low-redshift Quasars
• SDSS-IV MaNGA: Stellar M/L gradients and the M/L-colour relation in galaxies
• Young, Star-forming Galaxies and their local Counterparts: the Evolving Relationship of Mass-SFR-Metallicity since z ~ 2.1
• A Method to Distinguish Quiescent and Dusty Star-forming Galaxies with Machine Learning
• The Intrinsic Scatter of Galaxy Scaling Relations
• The Relation between Dynamical Mass-to-Light Ratio and Color for Massive Quiescent Galaxies out to z~2 and Comparison with Stellar Population Synthesis Models
• Dissecting Nearby Galaxies with piXedfit: I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• ZFIRE: Using H$\alpha$ equivalent widths to investigate the in situ initial mass function at z~2
• sMILES: A Library of Semi-Empirical MILES Stellar Spectra with Variable [$\alpha$/Fe] Abundances
• The Intrinsic Scatter of the Radial Acceleration Relation
• SDSS-IV MaNGA: Excavating the fossil record of stellar populations in spiral galaxies
• The average dust attenuation curve at z~1.3 based on HST grism surveys
• Probing Evolutionary Population Synthesis Models in the Near Infrared with Early Type Galaxies
• The SAMI galaxy survey: galaxy size can explain the offset between star-forming and passive galaxies in the mass-metallicity relationship
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• The distant, galaxy cluster environment of the short GRB 161104A at $z\sim 0.8$ and a comparison to the short GRB host population
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Biases and systematics in the observational derivation of galaxy properties: comparing different techniques on synthetic observations of simulated galaxies
• Unresolved versus resolved: testing the validity of young simple stellar population models with VLT/MUSE observations of NGC 3603
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• Reconstructing the observed ionizing photon production efficiency at z~2 using stellar population models
• Simultaneous Estimation of Photometric Redshifts and SED Parameters: Improved Techniques and a Realistic Error Budget
• Estimating dust attenuation from galactic spectra. I. methodology and tests
• Gemini NIFS survey of feeding and feedback processes in nearby Active Galaxies: VI -- Stellar Populations
• SDSS-II Supernova Survey: An Analysis of the Largest Sample of Type Ia Supernovae and Correlations with Host-Galaxy Spectral Properties
• Stellar Populations With Optical Spectra: Deep Learning vs. Popular Spectrum Fitting Codes
• Evaluating the impact of binary parameter uncertainty on stellar population properties
• Spatially Resolved Metal Loss from M31
• Empirical Constraints on the Nucleosynthesis of Nitrogen
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XIV. The main sequence relation in a rich environment down to M_star ~ 10^6 Mo
• Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82
• COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
• The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• The impact of the Star Formation Histories on the SFR-M${}_{\ast }$ relation at z$\ge$2
• Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshifts
• The Ionizing Spectra of Extremely Metal-Poor O Stars: Constraints from the Only HII Region in Leo P
• Impact of an AGN featureless continuum on estimation of stellar population properties
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• The First Metallicity Study of M83 using the integrated UV light of Star Clusters
• Exploring the chemical link between local ellipticals and their high-redshift progenitors
• Edge-on HI-bearing ultra diffuse galaxy candidates in the 40% ALFALFA catalog
• A Spectroscopic and Photometric Exploration of the C/M Ratio in the Disk of M31
• GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
• The cosmic evolution of the stellar mass$-$velocity dispersion relation of early-type galaxies
• The Variability of Star Formation Rate in Galaxies: II. Power Spectrum Distribution on the Main Sequence
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• Geometry effects on dust attenuation curves with different grain sources at high redshift
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• High-resolution, 3D radiative transfer modelling V. A detailed model of the M51 interacting pair
• MCSED: A flexible spectral energy distribution fitting code and its application to $z\sim 2$ emission-line galaxies
• Revisiting Attenuation Curves: the Case of NGC 3351
• Self-consistent population spectral synthesis with FADO - I. The importance of nebular emission in modelling star-forming galaxies
• Spatially resolved star formation and dust attenuation in Mrk848: Comparison of the integral field spectra and the UV-to-IR SED
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• Estimating dust attenuation from galactic spectra. II. Stellar and gas attenuation in star-forming and diffuse ionized gas regions in MaNGA
• Mapping the Diversity of Galaxy Spectra with Deep Unsupervised Machine Learning
• Circumstellar Dust, PAHs, and Stellar Populations in Early-Type Galaxies: Insights from GALEX and WISE
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• Dust masses of $z>5$ galaxies from SED fitting and ALMA upper limits
• ArtPop: A Stellar Population and Image Simulation Python Package
• The delay time distribution of supernovae from integral-field spectroscopy of nearby galaxies
• Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head Toward Quiescence at Cosmic Noon
• Ultraviolet Radiative Transfer Modeling of Nearby Galaxies with Extraplanar Dusts
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• Far-Ultraviolet Spectra of Main-Sequence O Stars at Extremely Low Metallicity
• J-PAS: Measuring emission lines with artificial neural networks
• DSPS: Differentiable Stellar Population Synthesis
• WEAVE-StePS. A stellar population survey using WEAVE at WHT
• BUDDI-MaNGA II: The Star-Formation Histories of Bulges and Discs of S0s
• Comparing Dark Energy Survey and HST-CLASH observations of the galaxy cluster RXC J2248.7-4431: implications for stellar mass versus dark matter
• Clues on the history of early-type galaxies from SDSS spectra and GALEX photometry
• On the impact of spectral template uncertainties in synthetic stellar populations
• Spatially resolved properties of galaxies from CANDELS+MUSE: Radial extinction profile and insights on quenching
• Identification and Characterization of a Large Sample of Distant Active Dwarf Galaxies in XMM-SERVS
• Young stellar population gradients in central cluster galaxies from NUV and optical spectroscopy
• Reproducing the UVJ Color Distribution of Star-forming Galaxies at 0.5 < z < 2.5 with a Geometric Model of Dust Attenuation
• Pixel Color Magnitude Diagrams for Semi-Resolved Stellar Populations: The Star Formation History of Regions within the Disk and Bulge of M31
• LLAMA: Stellar populations in the nuclei of ultra hard X-ray selected AGN and matched inactive galaxies
• Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsets
• Predicting the global far-infrared SED of galaxies via machine learning techniques
• The 50-100pc scale parent stellar populations of type II supernovae and limitations of single star evolution models
• High Resolution HST Imaging Survey of Local Star-Forming Galaxies I: Spatially-Resolved Obscured Star Formation with H$\alpha$ and Paschen-$\beta$ Recombination Lines
• Accretion properties of X-ray AGN: Evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution
• KMTNet Nearby Galaxy Survey II. Searching for Dwarf Galaxies in Deep and Wide-field Images of the NGC 1291 system
• Massive High-Redshift Quiescent Galaxies With JWST
• A SINFONI view of the nuclear activity and circumnuclear star formation in NGC 4303 - II: Spatially resolved stellar populations
• Mass-to-Light Ratios of Spatially Resolved Stellar Populations in M31
• On the accretion of a new group of galaxies onto Virgo: II. The effect of pre-processing on the stellar population content of dEs
• A tale of a rich cluster at z$\sim$0.8 as seen by the Star Formation Histories of its ETGs
• Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation
• Forensic reconstruction of galaxy colour evolution and population characterisation
• Dust attenuation, dust content and geometry of star-forming galaxies
• Sacrificing information for the greater good: how to select photometric bands for optimal accuracy
• TODDLERS: A new UV-mm emission library for star-forming regions. 1. Integration with SKIRT and public release
• Herschel and Hubble study of a lensed massive dusty starbursting galaxy at $z\sim 3$
• Synergies between low- and intermediate-redshift galaxy populations revealed with unsupervised machine learning
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• PopSED: Population-Level Inference for Galaxy Properties from Broadband Photometry with Neural Density Estimation
• Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-Time Distribution
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• An Extensive Photometric Catalog of CALIFA Galaxies
• SDSS-IV MaStar: Data-driven Parameter Derivation for the MaStar Stellar Library
• Deriving the star formation histories of galaxies from spectra with simulation-based inference
• Star Formation Histories Across the Interacting Galaxy NGC 6872, the Largest-Known Spiral
• The stellar metallicity distribution function of galaxies in the CALIFA survey
• CANDELS Meets GSWLC: Evolution of the Relationship Between Morphology and Star Formation Since z = 2
• Witnessing the star-formation quenching in $L_{\ast }$ ellipticals
• Exploring the AGN-Merger Connection in Arp 245 I: Nuclear Star Formation and Gas Outflow in NGC 2992
• Star Formation Histories from SEDs and CMDs Agree: Evidence for Synchronized Star Formation in Local Volume Dwarf Galaxies over the Past 3 Gyr
• The Stellar Kinematics of Void Dwarf Galaxies Using KCWI
• Andromeda Optical and Infrared Disk Survey I. New Insights in Wide-Field Near-IR Surface Photometry
• Fluctuation Spectroscopy: A New Probe of Old Stellar Populations
• The WAGGS project -- III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicity
• Solution to the conflict between the resolved and unresolved galaxy stellar mass estimation from the perspective of JWST
• On the Simultaneous Modelling of Dust and Stellar Populations for Interpretation of Galaxy Properties
• Steadily Increasing Star Formation Rates in Galaxies Observed at 3 <~ z <~ 5 in the CANDELS/GOODS-S Field
• The Gaia-ESO Survey: Old super-metal-rich visitors from the inner Galaxy
• Euclid: A complete Einstein ring in NGC 6505
• Variation of the Nebular Dust Attenuation Curve with the Properties of Local Star-forming Galaxies
• Stellar Population and Elemental Abundance Gradients of Early-type Galaxies
• Galaxy properties from J-PAS narrow-band photometry
• The X-shooter Lens Survey - II. Sample presentation and spatially resolved kinematics
• Constraining stellar population parameters from narrow band photometric surveys using convolutional neural networks
• The Panchromatic Hubble Andromeda Treasury XVII. Examining Obscured Star Formation with Synthetic Ultraviolet Flux Maps in M31
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• Time-slicing spiral galaxies with SDSS-IV MaNGA
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• On the maximum age resolution achievable through stellar population synthesis models
• The evolution of radial gradients of MaNGA quiescent elliptical galaxies: inside-out quenching or outer mass growth?
• Mr-Moose: An advanced SED-fitting tool for heterogeneous multi-wavelength datasets
• Satellite content and quenching of star formation in galaxy groups at z~1.8
• The SAMI Galaxy Survey: Gas Streaming and Dynamical M/L in Rotationally Supported Systems
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• A simple spectroscopic technique to identify rejuvenating 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
• Estimating stellar population and emission line properties in S-PLUS galaxies
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• Dust Extinction Law in Nearby Star-Resolved Galaxies. II. M33 Traced by Supergiants
• Panchromatic Photometry of Low-redshift, Massive Galaxies Selected from SDSS Stripe 82
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• The RR Lyrae Delay-Time Distribution: A Novel Perspective on Models of Old Stellar Populations
• Constraining the Milky Way's Ultraviolet to Infrared SED with Gaussian Process Regression
• Self-consistent population spectral synthesis with FADO: II. Star formation history of galaxies in spectral synthesis methods
• HETDEX [OIII] Emitters I: A spectroscopically selected low-redshift population of low-mass, low-metallicity galaxies
• Impact of stellar population synthesis choices on forward modelling-based redshift distribution estimates
• The Long and the Short of It: The Benefits and Leverage of Ultraviolet-Radio Galaxy Fitting
• New-generation dust emission templates for star-forming galaxies
• Low frequency radio continuum imaging and SED modeling of 11 LIRGs: radio-only and FUV to radio bands
• Flexible Models for Galaxy Star Formation Histories Both Shift and Scramble the Optical Color-M/L Relationship
• Physical properties of hyperluminous, dust-obscured quasars at $z\sim 3$: multiwavelength Spectral Energy Distribution analysis and cold gas content revealed by ALMA
• Unravelling the Dust Attenuation Scaling Relations and their Evolution
• The Imprint of Element Abundance Patterns on Quiescent Galaxy SEDs
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• Morphology-assisted galaxy mass-to-light predictions using deep learning
• The APOGEE Library of Infrared SSP Templates (A-LIST): High-Resolution Simple Stellar Population Spectral Models in the H-Band
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): The stellar populations and assembly of NGC 2903's bulge, bar, and outer disc
• Stellar Populations of Lyman-alpha Emitting Galaxies in the HETDEX Survey I: An Analysis of LAEs in the GOODS-N Field
• Modelling emission lines in star forming galaxies
• Neural Stellar Population Synthesis Emulator for the DESI PROVABGS
• Spatially Resolving the Star Formation Histories of Three Nearby Nuclear Star Clusters
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• The differences between mass- and light-derived structural parameters over time for MaNGA Elliptical galaxies
• pop-cosmos: Scaleable inference of galaxy properties and redshifts with a data-driven population model
• Getting ready for the LSST data -- estimating the physical properties of $z<2.5$ main sequence galaxies
• Lightning: An X-ray to Submillimeter Galaxy SED-Fitting Code With Physically-Motivated Stellar, Dust, and AGN Models
• Unravelling the Origin of the Counter-Rotating Core in IC 1459 with KMOS and MUSE
• Testing the tidal stripping scenario of ultra-compact dwarf galaxy formation by using internal properties
• Physical Properties of the Host Galaxies of Ca-rich Transients
• PROBES-I: A Compendium of Deep Rotation Curves and Matched multiband Photometry
• A common origin for the Fundamental Plane of quiescent and star-forming galaxies in the EAGLE simulations
• Relating galaxies across different redshift to study galaxy evolution
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• JWST/NIRCam Narrowband Survey of Pa$\beta$ Emitters in the Spiderweb Protocluster at z=2.16
• Chemical and photometric evolution models for disk, irregular and low mass galaxies
• Measuring Star-Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams I: Model Definition and Mock Tests
• Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
• Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z $\sim$2
• On the relationship between Type Ia supernova luminosity and host-galaxy properties
• Constraints on galactic outflows from the metallicity-stellar mass-SFR relation of EAGLE simulation and SDSS galaxies
• SDSS-IV MaNGA: The effect of stellar mass and halo mass on the assembly histories of satellite galaxies
• Universe opacity and EBL
• Physical and Morphological Properties of [O II] Emitting Galaxies in the HETDEX Pilot Survey
• Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z~3
• The PAU Survey: galaxy stellar population properties estimates with narrowband data
• A new galaxy spectral energy distribution model consistent with the evolution of dust
• Brackett-$\gamma$ as a Gold-standard Test of Star Formation Rates Derived from SED Fitting
• An excursion into the core of the cluster lens Abell 1689
• The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• Simulation-based inference of galaxy properties from JWST pixels
• Analysis of the spatially-resolved $V$-3.6$\mu$m colors and dust extinction in 257 nearby NGC and IC galaxies
• Applications of Stellar Population Synthesis in the Distant Universe
• Star Formation in Massive Galaxies at Redshift $z\sim 0.5$
• Resolved galactic superwinds reconstructed around their host galaxies at z>3
• Galaxy And Mass Assembly (GAMA): Stellar-to-Dynamical Mass Relation I. Constraining the Precision of Stellar Mass Estimates
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation
• Sunscreen: Photometric Signatures of Galaxies Partially Cloaked in Dyson Spheres
• On recent SFR calibrations and the constant SFR approximation
• Candidate List of Edge-on Galaxies with Substantial Extraplanar Dust
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Dependence of optical Active Galactic Nuclei identification on stellar population models
• Abundance matching tested on small scales with galaxy dynamics
• Observational signatures of the dust size evolution in isolated galaxy simulations
• Inferring redshift and galaxy properties via a multi-task neural net with probabilistic outputs: An application to simulated MOONS spectra
• Euclid preparation. LXVIII. Extracting physical parameters from galaxies with machine learning
• UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
• Galaxy populations of ProtoClusters in cosmological hydrodynamical simulations
• OMEGA - OSIRIS Mapping of Emission-line Galaxies in A901/2: IV. - Extinction of Star-Formation Estimators with Inclination
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Importance of modelling the nebular continuum in galaxy spectra
• Low-Frequency Turnover Star Forming Galaxies I: Radio Continuum Observations and Global Properties
• Leveraging Machine Learning for Accurate and Fast Stellar Mass Estimation of Galaxies
• Age-Divided Mean Stellar Populations from Full Spectrum Fitting as the Simplified Star Formation and Chemical Evolution History of a Galaxy: Methodology and Reliability
• How accurate are infrared luminosities from monochromatic photometric extrapolation?
• Galaxy Properties Derived with Spectral Energy Distribution Fitting in the Hawaii-Hubble Deep Field-North
• Measuring Dust Attenuation Curves of SINGS/KINGFISH Galaxies Using Swift/UVOT Photometry
• Iris: an Extensible Application for Building and Analyzing Spectral Energy Distributions
• The H$\alpha$ and [O III] $\lambda 5007$ Luminosity Functions of $1.2<z<1.9$ Emission-Line Galaxies from HST Grism Spectroscopy
• Dust Attenuation Curve for Local Subgalactic Star-forming Regions
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• Emission Line Predictions for Mock Galaxy Catalogues: a New Differentiable and Empirical Mapping from DESI
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• RadioSED I: Bayesian inference of radio SEDs from inhomogeneous surveys
• Star-dust geometry main determinant of dust attenuation in galaxies
• The recent star formation history of NGC 628 on resolved scales
• Stellar populations of galaxies in the LAMOST spectral survey
• The dark matter halo masses of elliptical galaxies as a function of observationally robust quantities
• Does Gravity Fall Down? Evidence for Gravitational Wave Deflection Along the Line of Sight to GW 170817
• Stellar populations of a sample of far-IR AGN and non-AGN green valley galaxies
• The impact of environment on the lives of disk galaxies as revealed by SDSS-IV MaNGA
• Understanding the Universal Dust Attenuation Scaling Relation of Star-Forming Galaxies
• Chemical characterisation of the X-shooter Spectral Library (XSL): [Mg/Fe] and [Ca/Fe] abundances
• Polynomial expansion of the star formation history in galaxies
• Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
• The Dependence of the Type Ia Supernova Host Bias on Observation or Fitting Technique
• Detecting episodes of star formation using Bayesian model selection
• Stellar metallicity from optical and UV spectral indices: Test case for WEAVE-StePS
• Flashlights: Prospects for constraining the Initial Mass Function around cosmic noon with caustic-crossing events
• What can distant galaxies teach us about massive stars?
• On the Thermally Pulsing Asymptotic Giant Branch Contribution to the Light of Nearby Disk Galaxies
• Panchromatic SED fitting codes and modelling techniques
• CoSHA: Code for Stellar properties Heuristic Assignment -- for the MaStar stellar library
• Galaxy Manifold: Characterizing and understanding galaxies with two parameters
• Bringing manifold learning and dimensionality reduction to SED fitters
• Morpho-Photometric Classification of KiDS DR5 Sources Based on Neural Networks: A Comprehensive Star-Quasar-Galaxy Catalog
• Lick-index entanglement and biased diagnostic of stellar populations in galaxies
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Assessing the dark matter content of two quasar host galaxies at z~6 through gas kinematics
• How the spectral energy distribution and galaxy morphology constrain each other, with application to morphological selection using galaxy colours
• Revisiting the Local Star-Forming Galaxies Observed in the HETDEX Pilot Survey
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• Extended Enriched Gas in a Multi-Galaxy Merger at Redshift 6.7
• Introducing a Real-time Interactive GUI Tool for Visualization of Galaxy Spectra
• The Intrinsic Flattening of Galaxy Disks
• The Spectroscopy and H-band Imaging of Virgo cluster galaxies (SHIVir) Survey: Data Catalogue and Kinematic Profiles
• A Shallow Slope for the Stellar Mass--Angular Momentum Relation of Star-Forming Galaxies at $1.5<z<2.5$
• COOL-LAMPS IV: A Sample of Bright Strongly-Lensed Galaxies at $3<z<4$
• Puzzling radial gradients of K-band absorption features in the giant elliptical galaxy M87
• Low-mass disc galaxies and the issue of stability: MOND vs dark matter
• Halo Properties from Observable Measures of Environment: I. Halo and Subhalo Masses
• The effects of star formation history in the SFR-M relation of HII galaxies
• Predicting far-infrared maps of galaxies via machine learning techniques
• Spectral Synthesis via Mean Field approach Independent Component Analysis
• Improved source classification and performance analysis using Gaia DR3
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Secondary Infall in the Seyfert's Sextet: A Plausible Way Out of the Short Crossing Time Paradox
• Systematics in the SED Fitting Parameter Estimation of Composite Galaxies
• Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
• NASIM: Revealing the low surface brightness Universe from legacy VISTA data
• Sengi: a small, fast, interactive viewer for spectral outputs from stellar population synthesis models
• A spectroscopic study of 14 structures behind Holm15A: Detecting a galaxy group candidate at z=0.58
• Hidden Figures of Globular Clusters: Integrated Stellar Populations Impacted by Hot Subdwarfs
• Physical Parameters of Stars in NGC 6397 Using ANN-Based Interpolation and Full Spectrum Fitting
• The COSMOS Wall at z$\sim$0.73: star-forming galaxies and their evolution in different environments
• Virial masses of late type galaxies from the SDSS DR16
• SEW: A full-spectrum linear fitting with stellar population synthesis method Based on "Equivalent Widths spectrum"
• Empirically-Driven Multiwavelength K-corrections At Low Redshift
• Exploring the spatially-resolved capabilities of the J-PAS survey with Py2DJPAS
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• Exploring the physical properties of Type II Quasar candidates at intermediate redshifts with CIGALE
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Ages and metallicities of stellar clusters using S-PLUS narrow-band integrated photometry: the Small Magellanic Cloud
• Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe
• SHAPE. I. A SOM-SED hybrid approach for efficient galaxy parameter estimation leveraging JWST
• Sub-Gyr variability around the SFMS and its contribution to the scatter
• The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering $\sim$ 5 virial radii around NGC 1399 with galaxy properties
• Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
• MIDIS: Unveiling the Star Formation History in massive galaxies at $1<z<4.5$ with spectro-photometric analysis
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• ULISSE: Determination of star-formation rate and stellar mass based on the one-shot galaxy imaging technique
• Infrared and Optical Emission-line Diagnostics
• Stars Born in the Wind: M82's Outflow and Halo Star Formation
• The multi-component fitting to the star formation histories in the TNG simulation
• Correcting the fiber-aperture bias affecting galaxy stellar populations in the Sloan Digital Sky Survey. Aperture corrections to absorption indices based on CALIFA integral field observations
• SMARTY: The mileS Moderate resolution neAr-infRared sTellar librarY
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• NutMaat: A Python package for stellar spectral classification on the MK system
• Ultraviolet-to-far-infra-red self-consistent analysis of the stellar populations of massive starburst galaxies at intermediate redshifts
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• Stellar population synthesis of galaxies with chemical evolution model
• Relation of internal attenuation, dust emission, and the size of spiral galaxies. Calibration at low-z and how to use it as a cosmological test at high-z
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• Beyond mirkwood: Enhancing SED Modeling with Conformal Predictions
• Interpreting Galaxy Properties with Improved Modelling
• Phenomenological constraints on QCD transport with quantified theory uncertainties
• Comparative Bayesian SED Fitting of PEARLSDG
• Initial Mass Function for Massive Galaxies at z$\sim$1
• Post-starburst galaxies in the centers of intermediate redshift clusters
• The X-shooter Spectral Library (XSL): Data Release 3
• Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
• Size-Mass Relation Shows Its Colours: Contrasting Physical Imprints of Galaxy Evolution in Rest-Frame UV and Optical
• Observational constraints on the origin of the elements. X. Combining NLTE and machine learning for chemical diagnostics of 4 million stars in the 4MIDABLE-HR survey
• Quiescent Host Galaxies of Extended Quasars Revealed by Spectrophotometric Decomposition
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• Testing the CCC+TL cosmology with cosmic-chronometer measurements of the Hubble parameter
• Fornax 3D project: assessing the diversity of IMF and stellar population maps within the Fornax Cluster
• Decomposing cool stellar populations with H-band spectral fluctuations: Long-period variable stars in NGC 5128 and carbon stars in NGC 5102
• A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
• Constraining the AGN tori at cosmic noon using high-resolution JWST imaging and simultaneous SED fitting
• UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
• The Panchromatic Hubble Andromeda Southern Treasury (PHAST). II. The Spatially Resolved Recent Star Formation History in M31
• Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim 1.74$ MaDCoWS2 galaxy cluster candidate
• The Treasury of Extremely Metal-Poor O Stars
• SDSS-IV MaStar: Determination of Stellar Parameters Using Bayesian Averaging
• GOTO identification and broadband modelling of the counterpart to the SVOM GRB 250818B
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Mentari: A pipeline to model the galaxy SED using semi analytic models
• The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER) II. The Spatially Resolved Recent Star Formation History of M33
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• Chemical evolution history of MaNGA galaxies
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Mocking IFU observations and metallicity diagnostics from cosmological simulations
• The BUFFALO HST Survey
• An empirical model of the extragalactic radio background
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Synergy between Roman and PRIMA imaging capabilities for large extragalactic surveys
• Quantifying Systematic Age Discrepancies in Very Young Star Clusters
• Probing cool giants in unresolved galaxies using fluctuation eigenspectra: a demonstration using high-resolution MUSE observations of NGC 5128
• The $10\mathrm{kpc}$ collar of early-type galaxies -- probing evolution by focusing on the inner stellar density profile