pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
arXiv:2506.12122 · doi:10.3847/1538-4357/ae0936
Abstract
We present an extension of the pop-cosmos model for the evolving galaxy population up to redshift . The model is trained on distributions of observed colors and magnitudes, from 26-band photometry of galaxies in the COSMOS2020 catalog with Spitzer IRAC . The generative model includes a flexible distribution over 16 stellar population synthesis (SPS) parameters, and a depth-dependent photometric uncertainty model, both represented using score-based diffusion models. We use the trained model to predict scaling relationships for the galaxy population, such as the stellar mass function, star-forming main sequence, and gas-phase and stellar metallicity vs. mass relations, demonstrating reasonable-to-excellent agreement with previously published results. We explore the connection between mid-infrared emission from active galactic nuclei (AGN) and star-formation rate, finding high AGN activity for galaxies above the star-forming main sequence at . Using the trained population model as a prior distribution, we perform inference of the redshifts and SPS parameters for 429,669 COSMOS2020 galaxies, including 39,588 with publicly available spectroscopic redshifts. The resulting redshift estimates exhibit minimal bias (), scatter (), and outlier fraction () for the full spectroscopic compilation. These results establish that pop-cosmos can achieve the accuracy and realism needed to forward-model modern wide--deep surveys for Stage IV cosmology. We publicly release pop-cosmos software, mock galaxy catalogs, and COSMOS2020 redshift and SPS parameter posteriors.
47 pages, 34 figures. Accepted for publication in ApJ. Mock galaxy catalogs available at https://doi.org/10.5281/zenodo.15757717 . MCMC chains available at https://doi.org/10.5281/zenodo.15850536 . Software available at https://github.com/Cosmo-Pop
References in corpus (94)
- Array Programming with NumPy
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- Modules for Experiments in Stellar Astrophysics (MESA)
- Cosmic Star Formation History
- Binary interaction dominates the evolution of massive stars
- Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
- The Cosmic Evolution Survey (COSMOS) -- Overview
- 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
- EAZY: A Fast, Public Photometric Redshift Code
- A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
- A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
- The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
- COSMOS Photometric Redshifts with 30-bands for 2-deg2
- Simba: Cosmological Simulations with Black Hole Growth and Feedback
- An Observational Determination of the Bolometric Quasar Luminosity Function
- zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
- 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
- Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
- Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
- UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
- Active Galactic Nuclei: what's in a name?
- Strong Nebular Line Ratios in the Spectra of z~2-3 Star-forming Galaxies: First Results from KBSS-MOSFIRE
- AGN Dusty Tori: I. Handling of Clumpy Media
- The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
- GALEX-SDSS-WISE Legacy Catalog (GSWLC): Star Formation Rates, Stellar Masses and Dust Attenuations of 700,000 Low-redshift Galaxies
- The Mass-Metallicity and the Fundamental Metallicity Relation revisited on a fully Te-based abundance scale for galaxies
- The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
- The Universal Relation of Galactic Chemical Evolution: The Origin of the Mass-Metallicity Relation
- The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees
- The galaxy stellar mass function at 3.5<z<7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields
- The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end
- The Intrinsic Alignment of Galaxies and its Impact on Weak Gravitational Lensing in an Era of Precision Cosmology
- Nebular Emission Line Ratios in z~2-3 Star-Forming Galaxies with KBSS-MOSFIRE: Exploring the Impact of Ionization, Excitation, and Nitrogen-to-Oxygen Ratio
- Constraining the properties of AGN host galaxies with Spectral Energy Distribution modeling
- Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions
- The WISE AGN Catalog
- Star Formation at From the Spitzer Large Area Survey with Hyper-Suprime-Cam (SPLASH)
- Galaxy Interactions Trigger Rapid Black Hole Growth: an unprecedented view from the Hyper Suprime-Cam Survey
- A definitive merger-AGN connection at z~0 with CFIS: mergers have an excess of AGN and AGN hosts are more frequently disturbed
- Half of the Most Luminous Quasars May Be Obscured: Investigating the Nature of WISE-Selected Hot, Dust-Obscured Galaxies
- Charting the evolution of the ages and metallicities of massive galaxies since z=0.7
- The Cosmic Evolution of Metallicity from the SDSS Fossil Record
- Large Structures and Galaxy Evolution in COSMOS at z < 1.1
- Photometric Redshift with Bayesian Priors on Physical Properties of Galaxies
- CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field
- Ages of Type Ia Supernovae Over Cosmic Time
- Widespread and Hidden Active Galactic Nuclei in Star-Forming Galaxies at Redshift > 0.3
- The VANDELS survey: the stellar metallicities of star-forming galaxies at 2.5 < z < 5.0
- Stellar Absorption Line Analysis of Local Star-Forming Galaxies: The Relation Between Stellar Mass, Metallicity, Dust Attenuation and Star Formation Rate
- Incidence of WISE-Selected Obscured AGNs in Major Mergers and Interactions from the SDSS
- Photometric Redshifts for Next-Generation Surveys
- The MOSDEF survey: AGN multi-wavelength identification, selection biases and host galaxy properties
- A Monte Carlo simulation of the intergalactic absorption and the detectability of the Lyman continuum from distant galaxies
- Reconciling the observed star-forming sequence with the observed stellar mass function
- Coevolution of metallicity and star formation in galaxies to z=3.7: I. A fundamental plane
- The Dependence of Theoretical Synthetic Spectra on -enhancement in Young, Binary Stellar Populations
- COLDz: A High Space Density of Massive Dusty Starburst Galaxies ~1 Billion Years after the Big Bang
- GMASS Ultradeep Spectroscopy of Galaxies at redshift z~2. I. The stellar metallicity
- Modelling type 1 quasar colours in the era of Rubin and Euclid
- Multi-wavelength properties of Type 1 and Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey
- A proto-cluster at z=2.45
- Inferring More from Less: Prospector as a Photometric Redshift Engine in the Era of JWST
- Infrared Selection of Obscured Active Galactic Nuclei in the COSMOS Field
- A spectroscopic study of blue supergiant stars in the Sculptor galaxy NGC 55: chemical evolution and distance
- BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
- The correlations between optical/UV broad lines and X-ray emission for a large sample of quasars
- Interpreting high [O III]/Hbeta ratios with maturing starbursts
- The VANDELS survey: the relation between UV continuum slope and stellar metallicity in star-forming galaxies at z~3
- Exploring AGN and Star Formation Activity of Massive Galaxies at Cosmic Noon
- COSMOS2020: Discovery of a protocluster of massive quiescent galaxies at
- Circumstellar Dust Around AGB Stars and Implications for Infrared Emission from Galaxies
- SDSS-IV eBOSS Spectroscopy of X-ray and WISE AGN in Stripe 82X: Overview of the Demographics of X-ray and Mid-Infrared Selected Active Galactic Nuclei
- The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields
- A galaxy-driven model of type Ia supernova luminosity variations
- Matching the Evolution of the Stellar Mass Function Using Log-normal Star Formation Histories
- Diversity of Galaxy Dust Attenuation Curves Drives the Scatter in the IRX-beta Relation
- Further evidence that galaxy age drives observed type Ia supernova luminosity differences
- A new look at local ultraluminous infrared galaxies: the atlas and radiative transfer models of their complex physics
- Data-driven, interpretable photometric redshifts trained on heterogeneous and unrepresentative data
- How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
- A Large Population of Luminous Active Galactic Nuclei Lacking X-ray Detections: Evidence for Heavy Obscuration?
- High-ionization emission line ratios from quasar broad line regions: metallicity or density?
- Impact of an AGN featureless continuum on estimation of stellar population properties
- Bayesian hierarchical modelling of the -SFR relation from 1<z<6 in ASTRODEEP
- How not to obtain the redshift distribution from probabilistic redshift estimates: Under what conditions is it not inappropriate to estimate the redshift distribution N(z) by stacking photo-z PDFs?
- Starduster: A multi-wavelength SED model based on radiative transfer simulations and deep learning
- The Intergalactic medium transmission towards z>4 galaxies with VANDELS and the impact of dust attenuation
- Impact of stellar population synthesis choices on forward modelling-based redshift distribution estimates
- Where Do Obscured AGN Fit in A Galaxy's Timeline?
- AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
- Cosmological feedback from a halo assembly perspective
- Population and spectral synthesis: it doesn't work without binaries
- Exploring the physical properties of Type II Quasar candidates at intermediate redshifts with CIGALE