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

Abstract

The stellar masses, mean ages, metallicities, and star formation histories of galaxies are now commonly estimated via stellar population synthesis (SPS) techniques. SPS relies on stellar evolution calculations from the main sequence to stellar death, stellar spectral libraries, phenomenological dust models, and stellar initial mass functions (IMFs). The present work is the first in a series that explores the impact of uncertainties in key phases of stellar evolution and the IMF on the derived physical properties of galaxies and the expected luminosity evolution for a passively evolving set of stars. A Monte-Carlo Markov-Chain approach is taken to fit near-UV through near-IR photometry of a representative sample of low- and high-redshift galaxies with this new SPS model. Significant results include the following: 1) including uncertainties in stellar evolution, stellar masses at z~0 carry errors of ~0.3 dex at 95% CL with little dependence on luminosity or color, while at z~2, the masses of bright red galaxies are uncertain at the ~0.6 dex level; 2) either current stellar evolution models, current observational stellar libraries, or both, do not adequately characterize the metallicity-dependence of the thermally-pulsating asymptotic giant branch phase; 3) conservative estimates on the uncertainty of the slope of the IMF in the solar neighborhood imply that luminosity evolution per unit redshift is uncertain at the ~0.4 mag level in the K-band, which is a substantial source of uncertainty for interpreting the evolution of galaxy populations across time; 4) The more plausible assumption of a distribution of stellar metallicities, rather than a fixed value as is usually assumed, can have significant effects on the interpretation of colors blueward of the V-band. (ABRIDGED)

21 pages, 17 figures, ApJ in press

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• Self-consistent Color-Mass-to-Light-Ratio relations for Low Surface Brightness Galaxies
• CO Emission, Molecular Gas, and Metallicity in Main-Sequence Star-Forming Galaxies at $z\sim 2.3$
• A Catalog of Host Galaxies for WISE-Selected AGN: Connecting Host Properties with Nuclear Activity and Identifying Contaminants
• Discovery of the optical afterglow and host galaxy of short GRB181123B at $z=1.754$: Implications for Delay Time Distributions
• The Minimum Halo Mass for Star Formation at z = 6 - 8
• A Case for a Binary Black Hole System Revealed via Quasi-Periodic Outflows
• Zapped then Napped? A rapidly quenched remnant leaker candidate with a steep spectroscopic ${\beta }_{UV}$ slope at z=8.5
• Deep Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
• MaNGA DynPop -- III. Stellar dynamics versus stellar population relations in 6000 early-type and spiral galaxies: Fundamental Plane, mass-to-light ratios, total density slopes, and dark matter fractions
• Detection of a White Dwarf companion to a Blue Straggler Star in the outskirts of globular cluster NGC 5466 with the Ultraviolet Imaging Telescope (UVIT)
• The evolution of barred galaxies in the EAGLE simulations
• The Next Generation Virgo cluster Survey (NGVS). XXV. Fiducial panchromatic colors of Virgo core globular clusters and their comparison to model predictions
• How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
• Monochromatic globular clusters as a critical test of formation models for the dark matter deficient galaxies NGC1052-DF2 and NGC1052-DF4
• COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys
• Testing the Prediction of Fuzzy Dark Matter Theory in the Milky Way Center
• Initial Mass Function Variability (or not) Among \\ Low-Velocity Dispersion, Compact Stellar Systems
• The first 62 AGN observed with SDSS-IV MaNGA -- III: stellar and gas kinematics
• A fast radio burst localized at detection to an edge-on galaxy using very-long-baseline interferometry
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XIII. The role of ram-pressure stripping in transforming the diffuse and ultra-diffuse galaxies in the Virgo cluster
• Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
• Stellar mass functions and implications for a variable IMF
• A Dramatic Decrease in Carbon Star Formation in M31
• The MOSDEF Survey: First Measurement of Nebular Oxygen Abundance at $z>4$
• The bulge masses of TDE host galaxies and their scaling with black hole mass
• The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
• A recently quenched isolated dwarf galaxy outside of the Local Group environment
• The MaNGA FIREFLY Value-Added-Catalogue: resolved stellar populations of 10,010 nearby galaxies
• Correlation between the gas-phase metallicity and ionization parameter in extragalactic HII regions
• Dissecting Nearby Galaxies with piXedfit: I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting
• From Carbon to Cobalt: Chemical compositions and ages of $z\sim 0.7$ quiescent galaxies
• Stromlo Stellar Tracks: non-solar scaled abundances for massive stars
• Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at $1.5<z<6.4$
• 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
• HST/WFC3 grism observations of $z\sim 1$ clusters: Evidence for rapid outside-in environmental quenching from spatially resolved H$\alpha$ maps
• Minutes-duration Optical Flares with Supernova Luminosities
• The Compact Structures of Massive $z\sim 0.7$ Post-Starburst Galaxies in the SQuIGG$\vec{L}$E Sample
• The Zwicky Transient Facility phase I sample of hydrogen-rich superluminous supernovae without strong narrow emission lines
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• The Stellar Mass of M31 as inferred by the Andromeda Optical & Infrared Disk Survey
• Demonstrating Diversity in Star Formation Histories with the CSI Survey
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• COSMOS2020: UV selected galaxies at $z\ge 7.5$
• Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2$\lesssim$$z$$\lesssim$0.9
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• An exquisitely deep view of quenching galaxies through the gravitational lens: Stellar population, morphology, and ionized gas
• The Stripe 82 Massive Galaxy Project III: A Lack of Growth Among Massive Galaxies
• A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
• Deriving ages and horizontal branch properties of integrated stellar populations
• Evaluating the impact of binary parameter uncertainty on stellar population properties
• A First Look at Spatially Resolved Star Formation at $4.8<z<6.5$ with JWST FRESCO NIRCam Slitless Spectroscopy
• 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
• Hierarchical Bayesian inference of photometric redshifts with stellar population synthesis models
• CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between $0.5\lesssim z\lesssim 1.7$ using H$\alpha$ Emission Line Maps
• IR SED and Dust Masses of Sub-solar Metallicity Galaxies at z~2.3
• MOSEL: Strong [OIII]5007 Å Emitting Galaxies at (3<z<4) from the ZFOURGE Survey
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• SuperBoRG: Search for The Brightest of Reionizing Galaxies and Quasars in HST Parallel Imaging Data
• A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• Texas Spectroscopic Search for Ly$\alpha$ Emission at the End of Reionization II. The Deepest Near-Infrared Spectroscopic Observation at $z\gtrsim 7$
• Physical Properties of Massive Compact Starburst Galaxies with Extreme Outflows
• Constraining the Tail-End of Reionization Using Lyman-$\alpha$ Transmission Spikes
• The Link Between Light and Mass in Late-type Spiral Galaxy Disks
• The dawn of disks: unveiling the turbulent ionised gas kinematics of the galaxy population at $z\sim 4-6$ with JWST/NIRCam grism spectroscopy
• Determining the Halo Mass Scale where Galaxies Lose Their Gas
• Implications of a Temperature Dependent IMF II: An Updated View of the Star-Forming Main Sequence
• Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5
• A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at $z=4.5$ revealed by JWST
• Constraining the dark matter content of NGC 1291 using hydrodynamic gas response simulations
• CLEAR: Survey Overview, Data Analysis and Products
• What Are Those Tiny Things? A First Study of Compact Star Clusters in the SMACS0723 Field with JWST
• AGN Feedback in Quiescent Galaxies at Cosmic Noon Traced by Ionized Gas Emission
• A search for the afterglows, kilonovae, and host galaxies of two short GRBs: GRB 211106A and GRB 211227A
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• The Ages and Metallicities of the Globular Clusters in the Sparkler
• MCSED: A flexible spectral energy distribution fitting code and its application to $z\sim 2$ emission-line galaxies
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• The Horizontal Branch population of NGC 1851 as revealed by the Ultra-violet Imaging Telescope (UVIT)
• The evolution of the UV luminosity function of globular clusters in the E-MOSAICS simulations
• An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in $1.3\le z\le 2.6$ Star-Forming Galaxies from MOSDEF
• Clumpy Star Formation and AGN Activity in Dwarf-Dwarf Galaxy Merger Mrk 709
• Stochastic Modelling of Star Formation Histories III. Constraints from Physically-Motivated Gaussian Processes
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• Ultra-Diffuse Galaxies as Extreme Star-forming Environments I: Mapping Star Formation in HI-Rich UDGs
• Host Galaxy Mass Combined with Local Stellar Age Improve Type Ia Supernovae Distances
• A spatially resolved analysis of star-formation burstiness by comparing UV and H$\alpha$ in galaxies at z$\sim$1 with UVCANDELS
• JWST's PEARLS: TN J1338-1942 -- I. Extreme jet triggered star-formation in a $z=4.11$ luminous radio galaxy
• The NEWFIRM HETDEX Survey: Photometric Catalog and a Conservative Sample of Massive Quiescent Galaxies at z=3-5 over 17.5 deg^2 in the SHELA Field
• A Multiwavelength view of IC 860: What Is in Action inside Quenching 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
• Mass Metallicity Relationship of SDSS Star Forming Galaxies: Population Synthesis Analysis and Effects of Star Burst Length, Extinction Law, Initial Mass Function and Star Formation Rate
• A luminous dust-obscured Tidal Disruption Event candidate in a star forming galaxy at 42 Mpc
• REQUIEM-2D: A diversity of formation pathways in a sample of spatially-resolved massive quiescent galaxies at z~2
• ArtPop: A Stellar Population and Image Simulation Python Package
• SN2020qlb: A hydrogen-poor superluminous supernova with well-characterized light curve undulations
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• The galaxy morphology-density relation in the EAGLE simulation
• DSPS: Differentiable Stellar Population Synthesis
• The inner mass distribution of late-type spiral galaxies from SAURON stellar kinematic maps
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Mapping Accreted Stars in Early-Type Galaxies Across the Mass-Size Plane
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• The In-situ Origins of Dwarf Stellar Outskirts in FIRE-2
• HR-pyPopStar: high wavelength-resolution stellar populations evolutionary synthesis model
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Kinematics, Structure, and Mass Outflow Rates of Extreme Starburst Galactic Outflows
• Far-Ultraviolet Spectra of Main-Sequence O Stars at Extremely Low Metallicity
• Ubiquitous [OII] Emission in Quiescent Galaxies at z ~ 0.85
• Streamlined Lensed Quasar Identification in Multiband Images via Ensemble Networks
• The radio detection and accretion properties of the peculiar nuclear transient AT 2019avd
• The KMOS Cluster Survey (KCS) III: fundamental plane of cluster galaxies at $z\simeq 1.80$ in JKCS 041
• Multiple Peaks and a Long Precursor in the Type IIn Supernova 2021qqp: An Energetic Explosion in a Complex Circumstellar Environment
• The Next Generation Virgo cluster Survey (NGVS). XXVI. The issues of photometric age and metallicity estimates for globular clusters
• Star formation and molecular gas properties of post-starburst galaxies
• Anatomy of an ionized bubble: NIRCam grism spectroscopy of the $z=6.6$ double-peaked Lyman-$\alpha$ emitter COLA1 and its environment
• Reproducing the UVJ Color Distribution of Star-forming Galaxies at 0.5 < z < 2.5 with a Geometric Model of Dust Attenuation
• Metallicity calibrations based on auroral lines from PHANGS-MUSE data
• High Resolution HST Imaging Survey of Local Star-Forming Galaxies I: Spatially-Resolved Obscured Star Formation with H$\alpha$ and Paschen-$\beta$ Recombination Lines
• Some observational tests of a minimal galaxy formation model
• Euclid preparation. XXI. Intermediate-redshift contaminants in the search for $z>6$ galaxies within the Euclid Deep Survey
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• The HETDEX Survey: The Ly$\alpha$ Escape Fraction from 3D-HST Emission Line Galaxies at $z\sim 2$
• The cosmic spectral energy distribution in the EAGLE simulation
• DUVET: Spatially Resolved Observations of Star Formation Regulation via Galactic Outflows in a Starbursting Disk Galaxy
• Removing biases in resolved stellar mass-maps of galaxy disks through successive Bayesian marginalization
• Globular clusters in the far-ultraviolet: evidence for He-enriched second populations in extra-galactic globular clusters?
• Ultra-Diffuse Galaxies as Extreme Star-forming Environments II: Star Formation and Pressure Balance in HI-Rich UDGs
• Dissecting Nearby Galaxies with piXedfit: II. Spatially Resolved Scaling Relations Among Stars, Dust, and Gas
• A candidate relativistic tidal disruption event at 340 Mpc
• A merging pair of massive quiescent galaxies at $z=3.44$ in the Cosmic Vine
• Hitting the slopes: A spectroscopic view of UV continuum slopes of galaxies reveals a reddening at z > 9.5
• Separating the blue cloud and the red sequence using Otsu's method for image segmentation
• The COSMOS-Web ring: in-depth characterization of an Einstein ring lensing system at z~2
• First Light And Reionisation Epoch Simulations (FLARES) XIII: The Lyman-continuum emission of high-redshift galaxies
• SDSS-IV MaStar: Data-driven Parameter Derivation for the MaStar Stellar Library
• PopSED: Population-Level Inference for Galaxy Properties from Broadband Photometry with Neural Density Estimation
• Photometric studies on the host galaxies of gamma-ray bursts using 3.6m Devasthal Optical Telescope
• Evidence of a Bottom-heavy Initial Mass Function in Massive Early-type Galaxies from Near-infrared Metal Lines
• Deriving the star formation histories of galaxies from spectra with simulation-based inference
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• Intracluster light in the core of z~2 galaxy proto-clusters
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• SN 2021adxl: A luminous nearby interacting supernova in an extremely low metallicity environment
• HectoMAP: The Complete Redshift Survey (Data Release 2)
• Star Formation Histories from SEDs and CMDs Agree: Evidence for Synchronized Star Formation in Local Volume Dwarf Galaxies over the Past 3 Gyr
• Euclid: A complete Einstein ring in NGC 6505
• ODIN: Improved Narrowband Ly$\alpha$ Emitter Selection Techniques for $z$ = 2.4, 3.1, and 4.5
• The WAGGS project -- III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicity
• The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing
• The mass-metallicity and fundamental metallicity relations in non-AGN and AGN-host galaxies
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• Fluctuation Spectroscopy: A New Probe of Old Stellar Populations
• Recovering age-metallicity distributions from integrated spectra: validation with MUSE data of a nearby nuclear star cluster
• Steadily Increasing Star Formation Rates in Galaxies Observed at 3 <~ z <~ 5 in the CANDELS/GOODS-S Field
• Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies
• Dead or Alive? How Bursty Star Formation and Patchy Dust Can Cause Temporary Quiescence in High Redshift Galaxies
• The Stellar Kinematics of Void Dwarf Galaxies Using KCWI
• Multi-Phase ISM in the z = 5.7 Hyperluminous Starburst SPT0346-52
• Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogs
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• The impact of r-process heating on the dynamics of neutron star merger accretion disc winds and their electromagnetic radiation
• Rubin Observatory LSST Stars Milky Way and Local Volume Star Clusters Roadmap
• High-velocity outflows persist up to 1 Gyr after a starburst in recently-quenched galaxies at z > 1
• Testing galaxy formation models with galaxy stellar mass functions
• Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters: I. Ages of Quiescent Member Galaxies at 0.3 < z < 1.4
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• The LOFAR Two-metre Sky Survey Deep Fields -- Data Release 1: IV. Photometric redshifts and stellar masses
• Modelling the galaxy-halo connection with semi-recurrent neural networks
• Globular cluster metallicity distributions in the E-MOSAICS simulations
• A large population of strongly lensed faint submillimetre galaxies in future dark energy surveys inferred from JWST imaging
• Galaxy interactions in filaments and sheets: effects of the large-scale structures versus the local density
• Implications of a Temperature Dependent IMF III: Mass Growth and Quiescence
• Metallicity and Age of the Stellar Stream Around the Disk Galaxy NGC 5907
• First Light And Reionisation Epoch Simulations (FLARES) XI: [OIII] emitting galaxies at $5<z<10$
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• The Panchromatic Hubble Andromeda Treasury XVII. Examining Obscured Star Formation with Synthetic Ultraviolet Flux Maps in M31
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• The Panchromatic Hubble Andromeda Treasury. VI. The reliability of far-ultraviolet flux as a star formation tracer on sub-kpc scales
• Semi-analytic spectral fitting: simultaneously modelling the mass accumulation and chemical evolution in MaNGA spiral galaxies
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• Large Scale Overdensity of Lyman Break Galaxies Around the z=6.3 Ultraluminous Quasar J0100+2802
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• On the Reionization-Era Globular Cluster in Low-Mass Galaxy Eridanus II
• On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
• Panning for gold, but finding helium: discovery of the ultra-stripped supernova SN2019wxt from gravitational-wave follow-up observations
• MaNGA 8313-1901: gas accretion observed in a blue compact dwarf galaxy?
• The Ursa Major cluster redefined as a `supergroup'
• Starduster: A multi-wavelength SED model based on radiative transfer simulations and deep learning
• The nascent milliquasar VT J154843.06+220812.6: tidal disruption event or extreme accretion-state change?
• The Evolution of AGN Activity in Brightest Cluster Galaxies
• Improved mass constraints for two nearby strong-lensing elliptical galaxies from Hubble Space Telescope Imaging
• A simple spectroscopic technique to identify rejuvenating galaxies
• An Orientation Bias in Observations of Submillimetre Galaxies
• The Imprint of Element Abundance Patterns on Quiescent Galaxy SEDs
• Flexible Models for Galaxy Star Formation Histories Both Shift and Scramble the Optical Color-M/L Relationship
• The First Galaxy Cluster Discovered by the VISTA Variables in the Vía Láctea Survey
• HETDEX [OIII] Emitters I: A spectroscopically selected low-redshift population of low-mass, low-metallicity galaxies
• Galaxies of the $z\sim 2$ Universe. I. Grism-Selected Rest-Frame Optical Emission Line Galaxies
• On the Origin of the Scatter in the Red Sequence: An Analysis of Four CLASH Clusters
• Strong spectral features from asymptotic giant branch stars in distant quiescent galaxies
• The incidence of AGN in galaxies with different stellar population ages
• Impact of stellar population synthesis choices on forward modelling-based redshift distribution estimates
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• JADES reveals a large population of low mass black holes at high redshift
• On the Precision of Full-spectrum Fitting of Simple Stellar Populations. I. Well-sampled Populations
• Galaxy And Mass Assembly (GAMA): Defining Passive Galaxy Samples and Searching for the UV Upturn
• JADES Ultra-red Flattened Objects: Morphologies and Spatial Gradients in Color and Stellar Populations
• On the nature of Small Galaxy Systems
• The Nature and Evolution of Early Massive Quenched Galaxies in the Simba-C Simulation
• pop-cosmos: Scaleable inference of galaxy properties and redshifts with a data-driven population model
• Improving Photometric Redshift Estimates with Training Sample Augmentation
• The SLACS strong lens sample, debiased
• Neural Stellar Population Synthesis Emulator for the DESI PROVABGS
• An Unexplained Origin for the Unusual Globular Cluster System in the Ultra-diffuse Galaxy FCC 224
• Explaining ultra-massive quiescent galaxies at $3<z<5$ in the context of their environments
• Stellar Populations of Lyman-alpha Emitting Galaxies in the HETDEX Survey I: An Analysis of LAEs in the GOODS-N Field
• Multi-wavelength observations of the Luminous Fast Blue Optical Transient AT2023fhn
• Modelling emission lines in star forming galaxies
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• Spatially Resolving the Star Formation Histories of Three Nearby Nuclear Star Clusters
• Size and Spectroscopic Evolution of HectoMAP Quiescent Galaxies
• Variation in the stellar initial mass function from the chromospheric activity of M dwarfs in early-type galaxies
• Beacons In the Dark: Using Novae and Supernovae to Detect Dwarf Galaxies in the Local Universe
• Molecular gas and dust in the highly magnified z = 2.8 galaxy behind the Bullet Cluster
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• pySTARBURST99: The Next Generation of STARBURST99
• Stellar population synthesis models with a physically varying IMF
• Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim 9-17$
• Dust Buried Compact Sources in the Dwarf Galaxy NGC 4449
• Can we use Weak Lensing to Measure Total Mass Profiles of Galaxies on 20 kiloparsec Scales?
• The large-scale structure of globular clusters in the NGC 1052 group
• Ionising Feedback Effects on Star Formation in Globular Clusters with Multiple Stellar Populations
• Cold gas mass measurements for the era of large optical spectroscopic surveys
• The age gradients of galaxies in EAGLE: outside-in quenching as the origin of young bulges in cluster galaxies
• Physical Properties of the Host Galaxies of Ca-rich Transients
• Testing the tidal stripping scenario of ultra-compact dwarf galaxy formation by using internal properties
• Lightning: An X-ray to Submillimeter Galaxy SED-Fitting Code With Physically-Motivated Stellar, Dust, and AGN Models
• The MOSDEF Survey: Calibrating the relationship between H$\alpha$ star-formation rate and radio continuum luminosity at $1.4<z<2.6$
• DESI Survey Validation Spectra Reveal an Increasing Fraction of Recently Quenched Galaxies at $z\sim 1$
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Environmental Effects on the UV Upturn in Local Clusters of Galaxies
• Validation of optimised population synthesis through mock spectra and Galactic globular clusters
• A galactic outflow traced by its extended Mg II emission out to a $\sim 30$ kpc radius in the Hubble Ultra Deep Field with MUSE
• The Outer Stellar Populations and Environments of Unusually HI-rich Galaxies
• On the relationship between Type Ia supernova luminosity and host-galaxy properties
• Exploring the Gas-Phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
• Emission Line Galaxies in the SHARDS Frontier Fields I: Candidate Selection and the Discovery of Bursty Hα Emitters
• Asymmetry Revisited: The Effect of Dust Attenuation and Galaxy Inclination
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• On the origin of red spirals: Does assembly bias play a role?
• No Need for Extreme Stellar Masses at z~7: A Test-case Study of COS-87259
• Subaru FOCAS IFU observations of two z=0.12 strong-lensing elliptical galaxies from SDSS MaNGA
• SDSS-IV MaNGA: The effect of stellar mass and halo mass on the assembly histories of satellite galaxies
• The BoRG-$JWST$ Survey: Abundance and Mass-to-light Ratio of Luminous $z=7-9$ Galaxies from Independent Sight Lines with NIRSpec
• The PAU Survey: galaxy stellar population properties estimates with narrowband data
• Brackett-$\gamma$ as a Gold-standard Test of Star Formation Rates Derived from SED Fitting
• Applications of Stellar Population Synthesis in the Distant Universe
• Size, shade or shape? The contribution of galaxies of different types to the star-formation history of the Universe from SDSS-IV MaNGA
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Resolved galactic superwinds reconstructed around their host galaxies at z>3
• Double Trouble: Two spectroscopically confirmed low-mass quiescent galaxies at z>5 in overdensities
• On the precision of full-spectrum fitting of simple stellar populations. II. The dependence on star cluster mass in the wavelength range 0.3-5.0 $\mu$m
• The JWST Emission Line Survey (JELS): Extending rest-optical narrow-band emission line selection into the Epoch of Reionization
• The Dark Matter Halos of HI Selected Galaxies
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Revisiting stellar properties of star-forming galaxies with stellar and nebular spectral modelling
• Super-massive black hole wake or bulgeless edge-on galaxy?
• SPT-CL J2215-3537: A Massive Starburst at the Center of the Most Distant Relaxed Galaxy Cluster
• Galaxy And Mass Assembly (GAMA): Stellar-to-Dynamical Mass Relation I. Constraining the Precision of Stellar Mass Estimates
• A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy
• Simulation-based inference of galaxy properties from JWST pixels
• SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation
• A Fresh Look at AGN Spectral Energy Distribution Fitting with the XMM-SERVS AGN Sample
• The Massive and Distant Clusters of WISE Survey. VIII. Radio Activity in Massive Galaxy Clusters
• Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
• Galaxy clusters and their outskirts: the "red sequence", star formation rate, stellar mass
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• The correlations between galaxy properties in different environments of the cosmic web
• Do minor interactions trigger star formation in galaxy pairs?
• Unveiling the Universe with Emerging Cosmological Probes
• On the Precision of Full-spectrum Fitting of Stellar Populations. III. Identifying Age Spreads
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• SN 2020zbf: A fast-rising hydrogen-poor superluminous supernova with strong carbon lines
• SMART: spectral energy distributions Markov chain analysis with radiative transfer models
• The leakage of Lyman-continuum photons from a major merger at $z\sim 1$
• The Space Density of Intermediate Redshift, Extremely Compact, Massive Starburst Galaxies
• PEARLS: Low Stellar Density Galaxies in the El Gordo Cluster Observed with JWST
• Improved Measurements of Galaxy Star Formation Stochasticity from the Intrinsic Scatter of Burst Indicators
• What is the nature of Little Red Dots and what is not, MIRI SMILES edition
• Evidence for a steeper SMBH-Bulge mass relationship extended to low masses using TDE host galaxies
• Thermal Regulation and the Star-Forming Main Sequence
• The dependence of cluster galaxy properties on the central entropy of their host cluster
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Evidence for Non-smooth Quenching in Massive Galaxies at $z\sim 1$
• On the Precision of Full-Spectrum Fitting of Simple Stellar Populations. IV. A Systematic Comparison with Results from Colour-Magnitude Diagrams
• Globular Cluster Ultraluminous X-ray Sources in the Furthest Early-Type Galaxies
• Microlensing at Cosmological Distances: Event Rate Predictions in the Warhol Arc of MACS 0416
• The Importance of Dust Distribution in Ionizing-photon Escape: NIRCam and MIRI Imaging of a Lyman Continuum-emitting Galaxy at z ~ 3.8
• Spatially Resolved Circumgalactic Medium around a Star-Forming Galaxy Driving a Galactic Outflow at $z\approx 0.8$
• GA-NIFS: Dissecting the multiple sub-structures and probing their complex interactions in the \Lyalpha emitter galaxy CR7 at z = 6.6 with JWST/NIRSpec
• Unveiling the Cosmic Gems Arc at $z\sim 10$ with JWST NIRCam
• ALMA 1.1mm Observations of a Conservative Sample of High Redshift Massive Quiescent Galaxies in SHELA
• Measuring Dust Attenuation Curves of SINGS/KINGFISH Galaxies Using Swift/UVOT Photometry
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• Observational Signatures of Carbon-Oxygen White Dwarf Merger Remnants
• Is the X-ray bright z = 5.5 quasar SRGE J170245.3+130104 a blazar?
• Near-infrared characterization of ultra-diffuse galaxies in Abell 2744 by JWST/NIRISS imaging
• The H$\alpha$ and [O III] $\lambda 5007$ Luminosity Functions of $1.2<z<1.9$ Emission-Line Galaxies from HST Grism Spectroscopy
• Unveiling the formation of NGC 2915 with MUSE: A counter-rotating stellar disk embedded in a disordered gaseous environment
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• Stellar, Gas, and Dust Emission of Star Forming Galaxies out to z~2
• Observing EAGLE galaxies with JWST: predictions for Milky Way progenitors and their building blocks
• Red Dragon: A Redshift-Evolving Gaussian Mixture Model for Galaxies
• Polynomial expansion of the star formation history in galaxies
• Taking a Break at Cosmic Noon: Continuum-selected Low-mass Galaxies Require Long Burst Cycles
• Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc
• The JWST/AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-Unity Dust Covering Fractions
• Extremely Low Molecular Gas Content in the Vicinity of a Red Nugget Galaxy at $z=1.91$
• Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
• Study of UV bright stellar populations in the globular cluster NGC 1261 using AstroSat
• Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with StarFormationHistories.jl
• Detecting episodes of star formation using Bayesian model selection
• Where has all the $r$-process gone? Timescales for GRB-Kilonovae to Enrich their Host Galaxies
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Fading Light, Fierce Winds: JWST Snapshot of a Sub-Eddington Quasar at Cosmic Dawn
• Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
• A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view
• SN 2019hcc: A Type II Supernova Displaying Early O II Lines
• Evolution of the Ultraviolet Upturn at $0.3<z<1$: exploring helium rich stellar populations
• Ionized gas in quiescent galaxies: Temperature measurement and constraint on the ionization source
• A Closer Look at an Unusual Ultra-Diffuse Galaxy
• Using Galaxy Formation Simulations to optimise LIGO Follow-Up Observations
• Tracing the green valley with entropic thresholding
• JWST Discovery of a High-Redshift Tidal Disruption Event Candidate in COSMOS-Web
• The Dependence of the Type Ia Supernova Host Bias on Observation or Fitting Technique
• Searching for Spectroscopic Signatures of Ongoing Quenching in SDSS Galaxies
• The Earliest Stage of Galactic Star Formation
• A massive quiescent galaxy confirmed in a protocluster at z=3.09
• Simple Stellar Population Modeling of Low S/N Galaxy Spectra and Quasar Host Galaxy Applications
• Digging deeper into NGC\,6868 I: stellar population
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• On the Thermally Pulsing Asymptotic Giant Branch Contribution to the Light of Nearby Disk Galaxies
• Galaxy Rest-Frame UV Colors at z ~ 2-4 with HST UVCANDELS
• GAMA 526784: the progenitor of a globular cluster-rich ultra-diffuse galaxy? I. Star clusters, stellar body and ionised gas properties
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Dwarf-Dwarf interactions and their influence on star formation : Insights from post-merger galaxies
• Insights into environmental quenching at $z\sim 1$: an enhancement of faint, low-mass passive galaxies in clusters
• Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• The Ultraviolet Upturn in field Luminous Red Galaxies at $0.3<z<0.7$
• Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• JWST's PEARLS: A z=6 quasar in a train-wreck galaxy merger system
• Rapid, out of equilibrium metal enrichment indicated by a flat mass-metallicity relation at z~6 from NIRCam grism spectroscopy
• Extreme Neutral Outflow in a non-AGN Quiescent Galaxy at z~1.3
• The Local Ultraviolet to Infrared Treasury I. Survey Overview of the Broadband Imaging
• Black hole mass of a quiescent galaxy hosting a Type 1 AGN at z=2.09: Implications for black hole - galaxy co-evolution and AGN quenching at high redshift
• CoSHA: Code for Stellar properties Heuristic Assignment -- for the MaStar stellar library
• Multiphase gas in elliptical galaxies: the role of Type Ia supernovae
• Pixel-level modelling of group-scale strong lens CASSOWARY 19
• JWSTs PEARLS: NIRCam imaging and NIRISS spectroscopy of a $z=3.6$ star-forming galaxy lensed into a near-Einstein Ring by a $z=1.258$ massive elliptical galaxy
• SDSS J1059+4251, a highly magnified z ~ 2.8 star-forming galaxy: ESI observations of the rest-frame UV spectrum
• Stellar Initial Mass Function (IMF) Probed with Supernova Rates and Neutrino Background: Cosmic Average IMF Slope is $\simeq 2-3$ Similar to the Salpeter IMF
• HST Grism Observations of a z~1.8 Cluster Candidate from the Clusters Occupied by Bent Radio AGN (COBRA) Survey
• A Shallow Slope for the Stellar Mass--Angular Momentum Relation of Star-Forming Galaxies at $1.5<z<2.5$
• The DEHVILS in the Details: Type Ia Supernova Hubble Residual Comparisons and Mass Step Analysis in the Near-Infrared
• Counting stars from the integrated spectra of galaxies
• TP-AGB stars and stellar population properties of a post-starburst galaxy at $z\sim 2$ through optical and NIR spectroscopy with JWST
• The Type Ia Supernova and Asymptotic Giant Branch Stellar Ejecta-regulated Interstellar Medium of Massive Galaxies
• Star clusters as simple stellar populations
• Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference
• The Impact of Bars, Spirals and Bulge-Size on Gas-Phase Metallicity Gradients in MaNGA Galaxies
• Narrow absorption lines from intervening material in supernovae. II. Galaxy properties
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• COOL-LAMPS IV: A Sample of Bright Strongly-Lensed Galaxies at $3<z<4$
• Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
• Probing neutral outflows in z ~ 2 galaxies using JWST observations of Ca II H and K absorption lines
• The Stellar Population of Metal-Poor Galaxies at z $\approx$ 0.8 and the Evolution of the Mass-Metallicity Relation
• UVIT-HST-Gaia-VISTA study of KRON 3 in the Small Magellanic Cloud: A cluster with an extended red clump in UV
• Even redder than we knew: color and $A_{\mathrm{V}}$ evolution up to $z=2.5$ from JWST/NIRCam photometry
• JADES Dark Horse: demonstrating high-multiplex observations with JWST/NIRSpec dense-shutter spectroscopy in the JADES Origins Field
• Introducing a Real-time Interactive GUI Tool for Visualization of Galaxy Spectra
• A study of the central stellar populations of galaxies in SDSS-IV MaNGA: identification of a sub-sample with unusually young and massive stars
• Densities and mass assembly histories of the Milky Way satellites are not a challenge to $\Lambda$CDM
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• Study of UV bright sources in globular cluster NGC 4590 using Ultraviolet Imaging Telescope (UVIT) observations
• The present-day globular cluster kinematics of lenticular galaxies from the E-MOSAICS simulations and their relation to the galaxy assembly histories
• Low-density star cluster formation: discovery of a young faint fuzzy on the outskirts of the low-mass spiral galaxy NGC 247
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• The slope and scatter of the star forming main sequence at z~5 : reconciling observations with simulations
• A long-duration gamma-ray burst of dynamical origin from the nucleus of an ancient galaxy
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Rapid onset of a Comptonisation zone in the repeating tidal disruption event XMMSL2 J140446.9-251135
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Interpreting deep learning-based stellar mass estimation via causal analysis and mutual information decomposition
• Star-forming Galaxies in Intermediate Redshift Clusters: Stellar vs. Dynamical Masses of Luminous Compact Blue Galaxies
• SEW: A full-spectrum linear fitting with stellar population synthesis method Based on "Equivalent Widths spectrum"
• You Are What You Eat: The Circumgalactic Medium Around BreakBRD Galaxies has Low Mass and Angular Momentum
• Simulating continuum-based redshift measurement in the \textit{Roman's} High Latitude Spectroscopy Survey
• COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS
• Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
• Kinematic Lensing Inference II: Cluster Lensing with $\mathcal{O}$(1) Galaxies
• New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1
• Far Ultra-Violet Insights Into NGC 1399's Globular Cluster Population
• Unveiling the Dark Side of UV/Optical Bright Galaxies: Optically Thick Dust Absorption
• The Kaleidoscope Survey: Strong Gravitational Lensing in Galaxy Clusters with Radial Arcs
• Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• Candidate strongly lensed type Ia supernovae in the Zwicky Transient Facility archive
• Galaxy-scale lens search in the PEARLS NEP TDF and CEERS JWST fields
• Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• The effects of star formation history in the SFR-M relation of HII galaxies
• Velocity dispersion functions of pressure-supported galaxies in EAGLE simulations with varying active galactic nucleus feedback
• Double white dwarf binary population in MOCCA star clusters -- Comparisons with observations of close and wide binaries
• A physically-motivated template set for high-z galaxy SED fitting
• Reconstructing the Assembly of Massive Galaxies. III: Quiescent Galaxies Loose Angular Momentum as They Evolve in a Mass-dependent Fashion
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• The Parallel Ionizing Emissivity Survey (PIE). I. Survey design and selection of candidate Lyman Continuum leakers at 3.1<z<3.5
• A stellar dynamical mass measurement of an inactive black hole at redshift 2
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• The AURORA Survey: Tracing Galactic Outflows at $z\gtrsim 2.5$ with JWST/NIRSpec NUV Absorption Lines
• 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
• Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe
• A first look at a complete view of spatially resolved star formation at 1<z<1.8 with JWST NGDEEP+FRESCO slitless spectroscopy
• Deblending the MIGHTEE-COSMOS survey with XID+: The resolved radio source counts to $S_{1.4}\approx 5\mu$Jy
• MICONIC: JWST/MIRI-MRS reveals heavily reprocessed PAH emission in the circum-nuclear disc of Centaurus A
• Discovery of a Barred-Spiral Galaxy at $z_{spec}$ = 3.16 II. The Star Formation History
• Nowhere Left to Hide: Uncovering All of the Massive Young Embedded Star Clusters in the Antennae with JWST
• Extragalactic globular cluster near-infrared spectroscopy: I. Integrated near-infrared spectra of Centaurus A/NGC 5128
• SMARTY: The mileS Moderate resolution neAr-infRared sTellar librarY
• Supermassive black holes in a mass-limited galaxy sample
• HST WFC3/Grism Observations of the Candidate Ultra-High-Redshift Radio Galaxy GLEAM J0917-0012
• Two years of optical and NIR observations of the superluminous supernova UID 30901 discovered by the UltraVISTA SN survey
• SNITCH: Seeking a simple, informative star formation history inference tool
• MEGASTAR (III). Stellar parameters and data products for DR1 late-type stars
• Can we constrain galaxy geometry parameters using spatially integrated SED fitting?
• Now you see it, now you don't: Star formation truncation precedes the loss of molecular gas by ~100 Myr in massive post-starburst galaxies at z~0.6
• The Delegate Survey: KOALA/AAOmega-IFU spectroscopy of three nearby dwarf galaxies
• Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
• Comparative Bayesian SED Fitting of PEARLSDG
• Study of dynamical status of the globular cluster NGC 1851 using Ultraviolet Imaging Telescope
• Semiresolved Stellar Populations as Distance Indicators
• The satellite population around luminous red galaxies in the 25 square degree DESI Legacy Imaging Surveys Early Data Release
• Size-Mass Relation Shows Its Colours: Contrasting Physical Imprints of Galaxy Evolution in Rest-Frame UV and Optical
• Late-time evolution of the interacting stripped-envelope supernova 2017dio
• Nonlinear Color-Metallicity Relations of Globular Clusters. XI. Nonlinearity Effect Revealed by NGC 5128 (Centaurus A) and NGC 4594 (Sombrero) Galaxies
• Testing the CCC+TL cosmology with cosmic-chronometer measurements of the Hubble parameter
• Lightstack: A Python Package for Creating Photometric Data Cubes
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• Galaxy Zoo: Clump Scout: Surveying the Local Universe for Giant Star-forming Clumps
• A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
• No Stream Left Unscathed: The imprint of a host galaxy
• The Panchromatic Hubble Andromeda Southern Treasury (PHAST). II. The Spatially Resolved Recent Star Formation History in M31
• The Progenitor Systems of Classical Novae in M31
• AT2024lhc and AT2024kmq in the landscape of featureless tidal disruption events
• Understanding the Nature of an Unusual Post-Starburst Quasar with Exceptionally Strong Ne V Emission
• GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• GOTO identification and broadband modelling of the counterpart to the SVOM GRB 250818B
• Multiwavelength Characterization of a Dynamically Relaxed Cool Core Galaxy Cluster at $z=1.5$
• NGC 147 Corroborates the Break in the Stellar Mass-Stellar Metallicity Relation for Galaxies
• SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars
• The Photometric Analysis of the Environment Around Two Dusty Star-Forming Galaxies at $z\sim 2$
• HR-pyPopStar II: high spectral resolution evolutionary synthesis models low metallicity expansion and the properties of the stellar populations of dwarf galaxies
• Fornax 3D project: assessing the diversity of IMF and stellar population maps within the Fornax Cluster
• A Pearl in the Shell: an ultra-compact dwarf within the tidal debris surrounding spiral galaxy NGC 7531
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• A Radio-selected Population of Dark, Long Gamma-ray Bursts: Comparison to the Long Gamma-ray Burst Population and Implications for Host Dust Distributions
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• Emulating redshift mixing due to blending in weak gravitational lensing
• Structural evolution of quiescent galaxies at intermediate redshifts at UV and red rest-frame wavelengths
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• A New Analytic Galactic Luminosity Profile Function
• The stellar remnants of high redshift nuclear starburst discs: a potential origin for nuclear star clusters?
• Oxyster: A Circumgalactic Low-ionization Oxygen Nebula next to a Starburst Galaxy at $z\sim 1$
• Toward a Zero-Parameter Model for Galaxy Rotation Curve Data
• Circular Mystery: Exploring Diffuse Emission Surrounding a Radio Galaxy with uGMRT and VLA Multiwavelength Observations
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Quiescent Galaxy Size, Velocity Dispersion, and Dynamical Mass Evolution
• The Population Synthesis Toolkit (PST) Python library
• Optimal strategies for measuring gas-phase metallicities in intermediate-redshift non-AGN and AGN-host galaxies using future instrumentation
• SDSS-IV MaStar: Theoretical Atmospheric Parameters for the MaNGA Stellar Library
• Probing AGN duty cycle and cluster-driven morphology in a giant episodic radio galaxy
• SQuIGGLE: Studying Quenching in Intermediate-z Galaxies -- Gas, AnguLar Momentum, and Evolution