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CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS Extended Groth Strip

Stefanon, Mauro; Yan, Haojing; Mobasher, Bahram; Barro, Guillermo; Donley, Jennifer L.; Fontana, Adriano; Hemmati, Shoubaneh; Koekemoer, Anton M.; Lee, BoMee; Lee, Seong-Kook; Nayyeri, Hooshang; Peth, Michael; Pforr, Janine; Salvato, Mara; Wiklind, Tommy; Wuyts, Stijn; Ashby, Matthew L. N.; Castellano, Marco; Conselice, Christopher J.; Cooper, Michael C.; Cooray, Asantha R.; Dolch, Timothy; Ferguson, Henry; Galametz, Audrey; Giavalisco, Mauro; Guo, Yicheng; Willner, Steven P.; Dickinson, Mark E.; Faber, Sandra M.; Fazio, Giovanni G.; Gardner, Jonathan P.; Gawiser, Eric; Grazian, Andrea; Grogin, Norman A.; Kocevski, Dale; Koo, David C.; Lee, Kyoung-Soo; Lucas, Ray A.; McGrath, Elizabeth J.; Nandra, Kirpal; Newman, Jeffrey A.; Wel, Arjen van der

Authors

Mauro Stefanon

Haojing Yan

Bahram Mobasher

Guillermo Barro

Jennifer L. Donley

Adriano Fontana

Shoubaneh Hemmati

Anton M. Koekemoer

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



Abstract

We present a 0.4-8μm 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 ~ 206 arcmin2 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 KS; Mayall/NEWFIRM J1, J2, J3, H1, H2, K; Spitzer IRAC 3.6μm, 4.5μm, 5.8μm and 8.0μm. 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.

Journal Article Type Article
Publication Date Apr 3, 2017
Journal Astrophysical Journal Supplement Series
Print ISSN 0067-0049
Electronic ISSN 1538-4365
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 229
Issue 2
Article Number 32
APA6 Citation Stefanon, M., Yan, H., Mobasher, B., Barro, G., Donley, J. L., Fontana, A., …Wel, A. V. D. (2017). CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS Extended Groth Strip. Astrophysical Journal Supplement, 229(2), https://doi.org/10.3847/1538-4365/aa66cb
DOI https://doi.org/10.3847/1538-4365/aa66cb
Keywords catalogs; galaxies: evolution; methods: data analysis; techniques: photometric
Publisher URL http://iopscience.iop.org/article/10.3847/1538-4365/aa66cb/meta
Copyright Statement Copyright information regarding this work can be found at the following address: http://eprints.nottingh.../end_user_agreement.pdf
Additional Information Journal title: The Astrophysical Journal Supplement Series; Article type: paper; Article title: CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip; Copyright information: © 2017. The American Astronomical Society. All rights reserved.; Date received: 2015-11-16; Date accepted: 2016-09-12; Online publication date: 2017-04-03

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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf





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