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CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip

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arxiv 1703.05768 v1 pith:PJ2NBKC5 submitted 2017-03-16 astro-ph.GA

CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip

Mauro Stefanon , Haojing Yan , Bahram Mobasher , Guillermo Barro , Jennifer L. Donley , Adriano Fontana , Shoubaneh Hemmati , Anton M. Koekemoer
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BoMee Lee Seong-Kook Lee Hooshang Nayyeri Michael Peth Janine Pforr Mara Salvato Tommy Wiklind Stijn Wuyts Matthew L. N. Ashby Marco Castellano Christopher J. Conselice Michael C. Cooper Asantha R. Cooray Timothy Dolch Henry Ferguson Audrey Galametz Mauro Giavalisco Yicheng Guo Steven P. Willner Mark E. Dickinson Sandra M. Faber Giovanni G. Fazio Jonathan P. Gardner Eric Gawiser Andrea Grazian Norman A. Grogin Dale Kocevski David C. Koo Kyoung-Soo Lee Ray A. Lucas Elizabeth J. McGrath Kirpal Nandra Jeffrey A. Newman Arjen van der Wel
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keywords candelscatalogcatalogsextendedf160wgrothstripcfht
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We present a 0.4-8$\mu$m multi-wavelength photometric catalog in the Extended Groth Strip (EGS) field. This catalog is built on the Hubble Space Telescope (HST) WFC3 and ACS data from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS), and it incorporates the existing HST data from the All-wavelength Extended Groth strip International Survey (AEGIS) and the 3D-HST program. The catalog is based on detections in the F160W band reaching a depth of F160W=26.62 AB (90% completeness, point-sources). It includes the photometry for 41457 objects over an area of $\approx 206$ arcmin$^2$ in the following bands: HST ACS F606W and F814W; HST WFC3 F125W, F140W and F160W; CFHT/Megacam $u^*$, $g'$, $r'$, $i'$ and $z'$; CFHT/WIRCAM $J$, $H$ and $K_\mathrm{S}$; Mayall/NEWFIRM $J1$, $J2$, $J3$, $H1$, $H2$, $K$; Spitzer IRAC $3.6\mu$m, $4.5\mu$m, $5.8\mu$m and $8.0\mu$m. We are also releasing value-added catalogs that provide robust photometric redshifts and stellar mass measurements. The catalogs are publicly available through the CANDELS repository.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies?

    astro-ph.GA 2026-06 unverdicted novelty 5.0

    Quiescent galaxies cluster more strongly than star-forming ones by 0.5-1 dex after halo-mass matching, with one-halo conformity up to z~2 that disappears at higher redshifts.

  2. Probing the faint end of simulated galaxy counts at z>3

    astro-ph.CO 2026-05 conditional novelty 5.0

    Hydrodynamical simulations underproduce faint compact galaxies at z>3 relative to CANDELS data, with the mismatch persisting after completeness corrections and pointing to deficiencies in star formation and feedback modeling.

  3. Probing the faint end of simulated galaxy counts at z>3

    astro-ph.CO 2026-05 unverdicted novelty 5.0

    TNG100 and EAGLE hydrodynamical simulations underproduce faint compact galaxies at z>3 relative to CANDELS observations even after forward modeling and completeness corrections, with the mismatch linked to both detect...

  4. Quantifying the inside-out formation of disk galaxies at $1.5 \le z \le 3.0$

    astro-ph.GA 2026-06 unverdicted novelty 4.0

    JWST observations show larger average rest-UV than rest-optical sizes in z=1.5-3 galaxies, supporting inside-out disk formation after dust correction.