CANDELS Multi-wavelength Catalogs: Source Detection and Photometry in the GOODS-South Field

Abstract

We present a UV-to-mid infrared multi-wavelength catalog in the CANDELS/GOODS-S field, combining the newly obtained CANDELS HST/WFC3 F105W, F125W, and F160W data with existing public data. The catalog is based on source detection in the WFC3 F160W band. The F160W mosaic includes the data from CANDELS deep and wide observations as well as previous ERS and HUDF09 programs. The mosaic reaches a 5$\sigma$ limiting depth (within an aperture of radius 0.17 arcsec) of 27.4, 28.2, and 29.7 AB for CANDELS wide, deep, and HUDF regions, respectively. The catalog contains 34930 sources with the representative 50% completeness reaching 25.9, 26.6, and 28.1 AB in the F160W band for the three regions. In addition to WFC3 bands, the catalog also includes data from UV (U-band from both CTIO/MOSAIC and VLT/VIMOS), optical (HST/ACS F435W, F606W, F775W, F814W, and F850LP), and infrared (HST/WFC3 F098M, VLT/ISAAC Ks, VLT/HAWK-I Ks, and Spitzer/IRAC 3.6, 4.5, 5.8, 8.0 $\mu$m) observations. The catalog is validated via stellar colors, comparison with other published catalogs, zeropoint offsets determined from the best-fit templates of the spectral energy distribution of spectroscopically observed objects, and the accuracy of photometric redshifts. The catalog is able to detect unreddened star-forming (passive) galaxies with stellar mass of 10^{10}M_\odot at a 50% completeness level to z$\sim$3.4 (2.8), 4.6 (3.2), and 7.0 (4.2) in the three regions. As an example of application, the catalog is used to select both star-forming and passive galaxies at z$\sim$2--4 via the Balmer break. It is also used to study the color--magnitude diagram of galaxies at 0<z<4.

The full resolution article is now published in ApJS (2013, 207, 24). 22 pages, 21 figures, and 5 tables. The catalogue is available on the CANDELS website: http://candels.ucolick.org/data_access/GOODS-S.html MAST: http://archive.stsci.edu/prepds/candels and Rainbow Database: https://arcoiris.ucolick.org/Rainbow_navigator_public and https://rainbowx.fis.ucm.es/Rainbow_navigator_public

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• Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts $z$$\simeq$2.3-4.1
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• Interloper bias in future large-scale structure surveys
• Close companions to two high-redshift quasars
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• The ASTRODEEP Frontier Fields Catalogues III. Multiwavelength photometry and rest frame properties of MACS-J0717 and MACS-J1149
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• I. Apples to apples $A^2$: realistic galaxy simulated catalogs and photometric redshift predictions for next-generation surveys
• CLEAR: High-Ionization [Ne V] $\lambda$3426 Emission-line Galaxies at $1.4<z<2.3$
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• Does black-hole growth depend fundamentally on host-galaxy compactness?
• Observations of the Initial Formation and Evolution of Spiral galaxies at $1<z<3$ in the CANDELS fields
• The structural properties of classical bulges and discs from z~2
• Star formation and quenching among the most massive galaxies at z~1.7
• Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at $1.5<z<6.4$
• SED-dependent Galactic Extinction Prescription for Euclid and Future Cosmological Surveys
• The interstellar medium and feedback in the progenitors of the compact passive galaxies at z~2
• A${}^3$COSMOS and A${}^3$GOODSS: Continuum Source Catalogues and Multi-band Number Counts
• The Origins of UV-optical Color Gradients in Star-forming Galaxies at z ~ 2: Predominant Dust Gradients But Negligible sSFR Gradients
• Fraction of Clumpy Star-Forming Galaxies at $0.5\le z\le 3$ in UVCANDELS: Dependence on Stellar Mass and Environment
• Changing physical conditions in star-forming galaxies between redshifts 0 < z < 4: [OIII]/Hb evolution
• Characterization and modeling of contamination for Lyman break galaxy samples at high redshift
• Simultaneous Estimation of Photometric Redshifts and SED Parameters: Improved Techniques and a Realistic Error Budget
• Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2$\lesssim$$z$$\lesssim$0.9
• Simulating the infrared sky with a Spritz
• Characterising the evolving $K$-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys
• The ionizing photon production efficiency of bright z$\sim$2-5 galaxies
• Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshifts
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies
• ALMA resolves extended star formation in high-z AGN host galaxies
• GA-NIFS: JWST/NIRSpec IFS view of the z~3.5 galaxy GS5001 and its close environment at the core of a large-scale overdensity
• The fundamental plane of black hole activity for low-luminosity radio active galactic nuclei across 1 < z < 4
• No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HST
• The stellar mass - size relation for cluster galaxies at z=1 with high angular resolution from the Gemini/GeMS multi-conjugate adaptive optics system
• The bulge-disk decomposition of AGN host galaxies
• The VANDELS survey: Discovery of massive overdensities of galaxies at z>2
• Revisiting the role of the Thermally-Pulsating Asymptotic Giant Branch phase in high-redshift galaxies
• Galaxy Structure, Stellar Populations, and Star Formation Quenching at 0.6 $\lesssim$ $z$ $\lesssim$ 1.2
• The impact of JWST broad-band filter choice on photometric redshift estimation
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• 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 galaxy mass-size relation in CARLA clusters and proto-clusters at 1.4 < z < 2.8: larger cluster galaxy sizes
• Probing the AGN Unification Model at redshift z $\sim$ 3 with MUSE observations of giant Ly$\alpha$ nebulae
• Galaxy populations in the most distant SPT-SZ clusters - I. Environmental quenching in massive clusters at $1.4\lesssim z\lesssim 1.7$
• Simulating MOS science on the ELT: Ly$\alpha$ forest tomography
• MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field
• On the Transition of the Galaxy Quenching Mode at 0.5<z<1 in CANDELS
• Comparison of Observed Galaxy Properties with Semianalytic Model Predictions using Machine Learning
• Studying the Physical Properties of Tidal Features I. Extracting Morphological Substructure in CANDELS Observations and VELA Simulations
• First Weak-lensing Results from "See Change": Quantifying Dark Matter in the Two Z>1.5 High-redshift Galaxy Clusters SPT-CL J2040-4451 and IDCS J1426+3508
• HALO7D I: The Line of Sight Velocities of Distant Main Sequence Stars in the Milky Way Halo
• Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift?
• Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head Toward Quiescence at Cosmic Noon
• Multiband galaxy morphologies for CLASH: a convolutional neural network transferred from CANDELS
• A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). V. Deep 450 Micron Imaging
• Galaxy Morphologies Revealed with Subaru HSC and Super-Resolution Techniques I: Major Merger Fractions of L_UV~3-15 L_UV* Dropout Galaxies at z~4-7
• H-ATLAS/GAMA: Quantifying the Morphological Evolution of the Galaxy Population Using Cosmic Calorimetry
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• The role of galaxy mass on AGN emission: a view from the VANDELS survey
• The Connection between Mergers and AGN Activity in Simulated and Observed Massive Galaxies
• MaNGA galaxy properties -- I. An extensive optical, mid-infrared photometric, and environmental catalogue
• II. Apples to apples $A^2$: cluster selection functions for next-generation surveys
• A comparative analysis of denoising algorithms for extragalactic imaging surveys
• Spatially resolved properties of galaxies from CANDELS+MUSE: Radial extinction profile and insights on quenching
• AGN accretion and black hole growth across compact and extended galaxy evolution phases
• On the Binary-Neutron-Star Post-Merger Magnetar Origin of XRT 210423
• The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging
• The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the ${\mathrm{L}}_{[\mathrm{CII}]}$-SFR relation
• Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
• The Stellar Age Dependence of X-ray Emission from Normal Star-Forming Galaxies in the GOODS Fields
• Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS survey
• A Correlation Between Lyα Spectral Line Profile and Rest-Frame UV Morphology
• The nature of giant clumps in high-z discs: a deep-learning comparison of simulations and observations
• Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. II. Are Highly Obscured AGNs the Missing Link in the Merger-Triggered AGN-Galaxy Coevolution Models?
• Probing the Star Formation Main Sequence down to $10^8$ M${}_{\odot }$ at $1.0<z<3.0$
• Photometric Redshift Estimation with Galaxy Morphology using Self-Organizing Maps
• The Lyman Continuum Escape Fraction of Star-forming Galaxies at $2.4\lesssim z\lesssim 3.0$ from UVCANDELS
• New Surface Brightness Fluctuations Spectroscopic Technique: NGC4449 and its Stellar Tidal Stream
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• When the Well Runs Dry: Modeling Environmental Quenching of High-mass Satellites in Massive Clusters at \boldmath$z\gtrsim 1$
• Revisiting the Properties of X-ray AGN in the SSA22 Protocluster: Normal SMBH and Host-Galaxy Growth for AGN in a $z=3.09$ Overdensity
• CANDELS Meets GSWLC: Evolution of the Relationship Between Morphology and Star Formation Since z = 2
• Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5
• Steadily Increasing Star Formation Rates in Galaxies Observed at 3 <~ z <~ 5 in the CANDELS/GOODS-S Field
• The UV luminosity function at 0.6 < z < 1 from UVCANDELS
• The Lyman Alpha Spectral Database (LASD)
• The LOFAR Two-metre Sky Survey Deep Fields -- Data Release 1: IV. Photometric redshifts and stellar masses
• On the Absence of High-Redshift AGNs: Little Growth in the Supermassive Black Hole Population at High Redshifts
• Deblending Galaxies with Generative Adversarial Networks
• Reconstructing the galaxy density field with photometric redshifts: II. Environment-dependent galaxy evolution since $z\simeq 3$
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• The VANDELS Survey: New constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5
• On the Impact of Inclination-Dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
• Local Analogs to High-Redshift Galaxies: I. Characterization of Dust Emission and Star Formation History
• Three Dimensional Optimal Spectral Extraction (TDOSE) from Integral Field Spectroscopy
• The Intergalactic medium transmission towards z>4 galaxies with VANDELS and the impact of dust attenuation
• No evidence for feedback: Unexceptional Low-ionization winds in Host galaxies of Low Luminosity Active Galactic Nuclei at Redshift z ~1
• The ATLAS 9.0 GHz Survey of the Extended Chandra Deep Field South: The Faint 9.0 GHz Radio Population
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies
• The SFR-radius connection: data and implications for wind strength and halo concentration
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• Deciphering the activity and quiescence of high-redshift cluster environments: ALMA observations of ClJ1449+0856 at z=2
• Emission line selected galaxies at $z=0.6-2$ in GOODS South: Stellar masses, SFRs, and large scale structure
• The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at $z\sim 5$
• The ALPINE-ALMA [CII] survey: double stellar population and AGN activity in a galaxy at $z\sim 5.5$
• Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
• Calibrating magnification bias for the $E_G$ statistic to test general relativity
• The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at $z\simeq 1$
• The Role of Bulge Formation in the Homogenization of Stellar Populations at $z\sim 2$ as revealed by Internal Color Dispersion in CANDELS
• Lightning: An X-ray to Submillimeter Galaxy SED-Fitting Code With Physically-Motivated Stellar, Dust, and AGN Models
• New JWST redshifts for the host galaxies of CDF-S XT1 and XT2: understanding their nature
• CDFS-6664: A candidate of Lyman-continuum Emission at z~3.8 detected by HDUV
• Have we seen all the galaxies that comprise the cosmic infrared background at 250\,$\mu$m $\le \lambda \le$ 500\,$\mu$m?
• The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-Forming Galaxy at z=1.3
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Massive molecular gas reservoir around the central AGN in the CARLA J1103+3449 cluster at z=1.44
• Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0
• Insights on star formation histories and physical properties of $1.2\le z\lesssim 4$ Herschel-detected galaxies
• 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
• Indications of M-dwarf Deficits in the Halo and Thick Disk of the Galaxy
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Chandra Observations of Excess Fe K$\alpha$ Line Emission in Galaxies with High Star Formation Rates: X-ray Reflection on Galaxy Scales?
• A new fitting concept for the robust determination of Sérsic model parameters
• A puzzling non-detection of [O III] and [C II] from a $z\approx 7.7$ galaxy observed with ALMA
• Accelerated structural evolution of galaxies in a starbursting cluster at z=2.51
• What is the nature of Little Red Dots and what is not, MIRI SMILES edition
• Star Formation Rate Function at $z\sim 4.5$: An Analysis from rest UV to Optical
• The Isophotal Structure of Star-forming Galaxies at $0.5<z<1.8$ in CANDELS: Implications for the Evolution of Galaxy Structure
• The Infrared Medium-deep Survey. IX. Discovery of Two New $z\sim 6$ Quasars and Space Density down to $M_{1450}\sim -23.5$ mag
• Unresolved z~8 point sources and their impact on the bright end of the galaxy luminosity function
• Candidate z ~ 2.5 Lyman Continuum Sources in the GOODS Fields
• The Importance of Dust Distribution in Ionizing-photon Escape: NIRCam and MIRI Imaging of a Lyman Continuum-emitting Galaxy at z ~ 3.8
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• HALO7D III: Chemical Abundances of Milky Way Halo Stars from Medium Resolution Spectra
• A mass threshold in the number density of passive galaxies at z$\sim$2
• Improved photometric redshifts with colour-constrained galaxy templates for future wide-area surveys
• The Dwarf Galaxy Population at $z\sim 0.7$: A Catalog of Emission Lines and Redshifts from Deep Keck Observations
• UV slope of z$\sim$3 bright ($L>L^{\ast }$) Lyman-break galaxies in the COSMOS field
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• Recent stellar mass assembly of low-mass star-forming galaxies at redshifts 0.3 < z < 0.9
• The Advanced X-ray Imaging Satellite
• Properties of galaxies at the faint end of the H$\alpha$ luminosity function at $z\sim 0.62$
• Denoising Diffusion Probabilistic Model for realistic and fast generated \textit{Euclid}-like data for weak lensing analysis
• Dark Energy Survey Year 3 Results: Deep Field Optical + Near-Infrared Images and Catalogue
• How the spectral energy distribution and galaxy morphology constrain each other, with application to morphological selection using galaxy colours
• Discovery of faint double-peak Halpha emission in the halo of low redshift galaxies
• The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
• The Gemini/HST galaxy cluster project: Redshift 0.2-1.0 cluster sample, X-ray data and optical photometry catalog
• Photometric properties of classical bulge and pseudo-bulge galaxies at $0.5\le z<1.0$
• Spectrophotometric redshifts for $\mathrm{z}\sim 1$ galaxies and predictions for number densities with WFIRST and Euclid
• Brighter and More Massive Galaxies in the Vicinity of Lyman-alpha Nebulae
• Does the lockstep growth between black holes and bulges create their mass relation?
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• Performance of Photometric Template Fitting for Ultra-High Redshift Galaxies
• Testing Models of Quasar Hosts With Strong Gravitational Lensing by Quasar Hosts
• The impact of bias row noise to photometric accuracy: case study based on a scientific CMOS detector
• Lower-Luminosity Obscured AGN Host Galaxies are Not Predominantly in Major-Merging Systems at Cosmic Noon
• ULTIMATE-deblending I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER survey
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• Measuring the gas reservoirs in $10^8<$ M${}_{\star }<10^{11}$ M${}_{\odot }$ galaxies at $1\le z\le 3$
• Bridging between the integrated and resolved main sequence of star formation
• The MUSE Hubble Ultra Deep Field Survey XIV. The evolution of the Lya emitter fraction from z=3 to z=6
• Compact [OIII] emission-line regions ("Green Seeds") in $\mathrm{H}\alpha$ emitters at Cosmic Noon from JWST Observations
• Spectral energy distribution similarity of the local galaxies and the 3.6um selected galaxies from the Spitzer Extended Deep Survey
• An empirical model of the extragalactic radio background
• KURVS: chemical properties from multiple strong line calibrations for star-forming galaxies at $z\sim 1.5$
• AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release