CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field
arXiv:1612.07364 · doi:10.3847/1538-4365/228/1/7
Abstract
We present a multi-wavelength photometric catalog in the COSMOS field as part of the observations by the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS). The catalog is based on Hubble Space Telescope Wide Field Camera 3 (HST/WFC3) and Advanced Camera for Surveys (ACS) observations of the COSMOS field (centered at RA: , Dec:). The final catalog has 38671 sources with photometric data in forty two bands from UV to the infrared (). This includes broad-band photometry from the HST, CFHT, Subaru, VISTA and Spitzer Space Telescope in the visible, near infrared and infrared bands along with intermediate and narrow-band photometry from Subaru and medium band data from Mayall NEWFIRM. Source detection was conducted in the WFC3 F160W band (at ) and photometry is generated using the Template FITting algorithm. We further present a catalog of the physical properties of sources as identified in the HST F160W band and measured from the multi-band photometry by fitting the observed spectral energy distributions of sources against templates.
28 Pages, 22 Figures and 10 Tables. Accepted for Publication in the ApJS
References in corpus (45)
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- The Cosmic Evolution Survey (COSMOS) -- Overview
- EAZY: A Fast, Public Photometric Redshift Code
- UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
- COSMOS Photometric Redshifts with 30-bands for 2-deg2
- An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
- zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
- 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
- The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
- The Chandra COSMOS Survey, I: Overview and Point Source Catalog
- The Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies
- Evidence for TP-AGB stars in high redshift galaxies, and their effect on deriving stellar population parameters
- The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
- What do we learn from IRAC observations of galaxies at 2 < z < 3.5?
- The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
- The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6
- Faint AGNs at z>4 in the CANDELS GOODS-S field: looking for contributors to the reionization of the Universe
- The VLA-COSMOS Survey: II. Source Catalog of the Large Project
- The mass evolution of the first galaxies: stellar mass functions and star formation rates at in the CANDELS GOODS-South field
- Stellar masses from the CANDELS survey: the GOODS-South and UDS fields
- High resolution mid-infrared spectroscopy of ultraluminous infrared galaxies
- A Spectroscopic Redshift Measurement for a Luminous Lyman Break Galaxy at z=7.730 using Keck/MOSFIRE
- MegaPipe: the MegaCam image stacking pipeline at the Canadian Astronomical Data Centre
- Optical spectroscopy and X-ray detections of a sample of quasars and AGN selected in the mid-infrared from two Spitzer wide-area surveys
- Large Structures and Galaxy Evolution in COSMOS at z < 1.1
- GALAPAGOS: From Pixels to Parameters
- The XMM-Newton wide-field survey in the COSMOS field II: X-ray data and the logN-logS
- New redshift z ~ 9 galaxies in the Hubble Frontier Fields: Implications for early evolution of the UV luminosity density
- Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history
- Photometric Redshifts of Galaxies in COSMOS
- ZFOURGE/CANDELS: On the Evolution of M* Galaxy Progenitors from z=3 to 0.5
- The Detection of a Red Sequence of Massive Field Galaxies at z~2.3 and its Evolution to z~0
- A Comparative Study of Density Field Estimation for Galaxies: New Insights into the Evolution of Galaxies with Environment in COSMOS out to z~3
- A Population of Massive and Evolved Galaxies at z$\ga$5
- Cosmic Web and Star Formation Activity in Galaxies at z~1
- Evolution of the H+[OIII] and [OII] luminosity functions and the [OII] star-formation history of the Universe up to ~ 5 from HiZELS
- The Spitzer mid-infrared AGN survey. II-the demographics and cosmic evolution of the AGN population
- Investigating H, UV, and IR star-formation rate diagnostics for a large sample of z ~ 2 galaxies
- The environmental impacts on the star formation main sequence: an H-alpha study of the newly discovered rich cluster at z=1.52
- ConvPhot: A Profile-Matching Algorithm for Precision Photometry
- A Study of Massive and Evolved Galaxies at High Redshift
- The Local [CII] 158 um Emission Line Luminosity Function
- Kpc-scale Properties of Emission-line Galaxies
- The interstellar medium and feedback in the progenitors of the compact passive galaxies at z~2
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- Dust temperature and mid-to-total infrared color distributions for star-forming galaxies at 0<z<4
- Observational constraints on the merger history of galaxies since : Probabilistic galaxy pair counts in the CANDELS fields
- Non-parametric Star Formation History Reconstruction with Gaussian Processes I: Counting Major Episodes of Star Formation
- Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0
- Relations Between the Sizes of Galaxies and their Dark Matter Halos at Redshifts
- Evident black hole-bulge coevolution in the distant universe
- Large Scale Structures in the CANDELS Fields: The Role of the Environment in Star Formation Activity
- The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5
- Stellar Masses of Giant Clumps in CANDELS and Simulated Galaxies Using Machine Learning
- Mock Lightcones and Theory Friendly Catalogs for the CANDELS Survey
- The mass-metallicity relation at z~1-2 and its dependence on star formation rate
- Investigating the Effect of Galaxy Interactions on Star Formation at 0.5<z<3.0
- CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies
- The MOSDEF Survey: Environmental dependence of the gas-phase metallicity of galaxies at
- Selection of massive evolved galaxies at in the CANDELS fields
- The Stellar Mass Function in CANDELS and Frontier Fields: the build-up of low mass passive galaxies since z~3
- Stellar population and structural properties of dwarf galaxies and young stellar systems in the M81 group
- Observations of the Initial Formation and Evolution of Spiral galaxies at in the CANDELS fields
- The KMOS Galaxy Evolution Survey (KGES): the angular momentum of star-forming galaxies over the last ~10 Gyr
- Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.20.9
- The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at
- The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the -SFR relation
- Spatially resolved properties of galaxies from CANDELS+MUSE: Radial extinction profile and insights on quenching
- K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at -
- Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies
- Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
- UV-Bright Star-Forming Clumps and Their Host Galaxies in UVCANDELS at 0.5 z 1
- The AGN fraction in high-redshift protocluster candidates selected by Planck and Herschel
- Unresolved z~8 point sources and their impact on the bright end of the galaxy luminosity function
- Identifying Lyα emitter candidates with Random Forest: learning from galaxies in CANDELS survey
- UV and NIR size of the low-mass field galaxies: the UV compact galaxies
- The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers