Inferring More from Less: Prospector as a Photometric Redshift Engine in the Era of JWST
arXiv:2302.08486 · doi:10.3847/2041-8213/acba99
Abstract
The advent of the James Webb Space Telescope (JWST) signals a new era in exploring galaxies in the high- universe. Current and upcoming JWST imaging will potentially detect galaxies out to , creating a new urgency in the quest to infer accurate photometric redshifts (photo-) for individual galaxies from their spectral energy distributions, as well as masses, ages and star formation rates. Here we illustrate the utility of informed priors encoding previous observations of galaxies across cosmic time in achieving these goals. We construct three joint priors encoding empirical constraints of redshifts, masses, and star formation histories in the galaxy population within the \prospector\ Bayesian inference framework. In contrast with uniform priors, our model breaks an age-mass-redshift degeneracy, and thus reduces the mean bias error in masses from 0.3 to 0.1 dex, and in ages from 0.6 to 0.2 dex in tests done on mock JWST observations. Notably, our model recovers redshifts at least as accurately as the state-of-the-art photo- code \eazy\ in deep JWST fields, but with two advantages: tailoring a model based on a particular survey renders mostly unnecessary given well-motivated priors; obtaining joint posteriors describing stellar, active galactic nuclei, gas, and dust contributions becomes possible. We can now confidently use the joint distribution to propagate full non-Gaussian redshift uncertainties into inferred properties of the galaxy population. This model, ``\prospector-'', is intended for fitting galaxy photometry where the redshift is unknown, and will be instrumental in ensuring the maximum science return from forthcoming photometric surveys with JWST. The code is made publicly available online as a part of \prospector.
arXiv commentAccepted for publication in ApJL. 13 pages, 6 figures, 2 tables. The code is made publicly available online as a part of Prospector; the version used in this work corresponds to the state of the Git repository at commit 820ad72
References in corpus (59)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- Astropy: A Community Python Package for Astronomy
- Stellar population synthesis at the resolution of 2003
- Galactic Stellar and Substellar Initial Mass Function
- The Dust Content and Opacity of Actively Star-Forming Galaxies
- MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences
- Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era
- MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones
- EAZY: A Fast, Public Photometric Redshift Code
- Stellar mass-to-light ratios and the Tully-Fisher relation
- A Simple Model for the Absorption of Starlight by Dust in Galaxies
- Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey
- The epochs of early-type galaxy formation as a function of environment
- New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
- UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
- UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10
- The ages and metallicities of galaxies in the local universe
- Bayesian photometric redshift estimation
- The propagation of uncertainties in stellar population synthesis modeling III: model calibration, comparison, and evaluation
- Measuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North
- Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms
- Stellar Population Inference with Prospector
- How to Measure Galaxy Star Formation Histories II: Nonparametric Models
- Deriving Physical Properties from Broadband Photometry with Prospector: Description of the Model and a Demonstration of its Accuracy Using 129 Galaxies in the Local Universe
- zCOSMOS - 10k-bright spectroscopic sample. The bimodality in the Galaxy Stellar Mass Function: exploring its evolution with redshift
- Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
- Nebular Continuum and Line Emission in Stellar Population Synthesis Models
- The Dearth of z~10 Galaxies in all HST Legacy Fields -- The Rapid Evolution of the Galaxy Population in the First 500 Myr
- A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging
- The GLASS James Webb Space Telescope Early Release Science Program. I. Survey Design and Release Plans
- How to measure galaxy star-formation histories I: Parametric models
- The Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA) and its first application: COSMOS
- A redshift-independent efficiency model: star formation and stellar masses in dark matter halos at z>4
- Recovering galaxy stellar population properties from broad-band spectral energy distribution fitting
- The Grism Lens-Amplified Survey from Space (GLASS). I. Survey overview and first data release
- On the Stellar Populations of Galaxies at z=9-11: The Growth of Metals and Stellar Mass at Early Times
- The evolution of star formation histories of quiescent galaxies
- How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting
- The JWST Extragalactic Mock Catalog: Modeling galaxy populations from the UV through the near-IR over thirteen billion years of cosmic history
- JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results
- Fast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8
- On the Last 10 Billion Years of Stellar Mass Growth in Star-Forming Galaxies
- A Critical Assessment of Stellar Mass Measurement Methods
- An Atlas of MUSE Observations towards Twelve Massive Lensing Clusters
- A New Census of the 0.2< z <3.0 Universe, Part II: The Star-Forming Sequence
- A New Census of the 0.2 < z < 3.0 Universe, Part I: The Stellar Mass Function
- Photometric Redshifts for Next-Generation Surveys
- Star formation histories of UV-luminous galaxies at : implications for stellar mass assembly at early cosmic times
- Dynamical Versus Stellar Masses in Compact Early-Type Galaxies: Further Evidence for Systematic Variation in the Stellar Initial Mass Function
- SPECULATOR: Emulating stellar population synthesis for fast and accurate galaxy spectra and photometry
- Optimized Photometric Redshifts for the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS)
- Forward modeling of galaxy populations for cosmological redshift distribution inference
- How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
- Hierarchical Bayesian inference of photometric redshifts with stellar population synthesis models
- Flexible Models for Galaxy Star Formation Histories Both Shift and Scramble the Optical Color-M/L Relationship
- Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
Cited by in corpus (31)
- A population of red candidate massive galaxies ~600 Myr after the Big Bang
- RUBIES: Evolved Stellar Populations with Extended Formation Histories at in Candidate Massive Galaxies Identified with JWST/NIRSpec
- JWST UNCOVER: Extremely red and compact object at triply imaged by Abell 2744
- UNCOVER: Illuminating the Early Universe -- JWST/NIRSpec Confirmation of Galaxies
- JWST reveals a population of ultra-red, flattened disk galaxies at 2<z<6 previously missed by HST
- RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow
- Quantifying the Effects of Known Unknowns on Inferred High-redshift Galaxy Properties: Burstiness, the IMF, and Nebular Physics
- The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning
- JWST FRESCO: a comprehensive census of H+[OIII] emitters at 6.8<z<9.0 in the GOODS fields
- The Extreme Low-mass End of the Mass-Metallicity Relation at
- SBI++: Flexible, Ultra-fast Likelihood-free Inference Customized for Astronomical Applications
- Early and Extensive Ultraviolet Through Near Infrared Observations of the Intermediate-Luminosity Type Iax Supernovae 2024pxl
- UNCOVERing the High-redshift AGN Population among Extreme UV Line Emitters
- Impact of stellar population synthesis choices on forward modelling-based redshift distribution estimates
- JADES Ultra-red Flattened Objects: Morphologies and Spatial Gradients in Color and Stellar Populations
- pop-cosmos: Scaleable inference of galaxy properties and redshifts with a data-driven population model
- DESI Complete Calibration of the Color-Redshift Relation (DC3R2): Results from early DESI data
- NOEMA reveals the true nature of luminous red JWST z>10 galaxy candidates
- Toward a stellar population catalog in the Kilo Degree Survey: the impact of stellar recipes on stellar masses and star formation rates
- Taking a Break at Cosmic Noon: Continuum-selected Low-mass Galaxies Require Long Burst Cycles
- Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with StarFormationHistories.jl
- pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
- Improved SED-Fitting Assumptions Result in Inside-Out Quenching at and Quenching at All Radii Simultaneously at
- Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
- CIGaRS I: Combined simulation-based inference from type Ia supernovae and host photometry
- Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
- GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference
- GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
- Everything Every Band All at Once I: A Global Morphology Catalog in Abell 2744 based on UNCOVER/MegaScience
- Emulating redshift mixing due to blending in weak gravitational lensing
- Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling