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AEGIS-X: Deep Chandra Imaging of the Central Groth Strip

Nandra, K. and Laird, E. S. and Aird, J. A. and Salvato, M. and Georgakakis, A. and Barro, G. and Pérez-González, P. G. and Barmby, P. and Chary, R.-R. and Coil, A. and Cooper, M. C. and Davis, M. and Dickinson, M. and Faber, S. M. and Fazio, G. G. and Guhathakurta, P. and Gwyn, S. and Hsu, L.-T. and Huang, J.-S. and Ivison, R. J. and Koo, D. C. and Newman, J. A. and Rangel, C. and Yamada, T. and Willmer, C. (2015) AEGIS-X: Deep Chandra Imaging of the Central Groth Strip. Astrophysical Journal Supplement Series, 220 (1). Art. No. 10. ISSN 0067-0049. https://resolver.caltech.edu/CaltechAUTHORS:20151201-155604532

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Abstract

We present the results of deep Chandra imaging of the central region of the Extended Groth Strip, the AEGIS-X Deep (AEGIS-XD) survey. When combined with previous Chandra observations of a wider area of the strip, AEGIS-X Wide (AEGIS-XW), these provide data to a nominal exposure depth of 800 ks in the three central ACIS-I fields, a region of approximately 0.29 deg2. This is currently the third deepest X-ray survey in existence; a factor ~2-3 shallower than the Chandra Deep Fields (CDFs), but over an area ~3 times greater than each CDF. We present a catalog of 937 point sources detected in the deep Chandra observations, along with identifications of our X-ray sources from deep ground-based, Spitzer, GALEX, and Hubble Space Telescope imaging. Using a likelihood ratio analysis, we associate multiband counterparts for 929/937 of our X-ray sources, with an estimated 95% reliability, making the identification completeness approximately 94% in a statistical sense. Reliable spectroscopic redshifts for 353 of our X-ray sources are available predominantly from Keck (DEEP2/3) and MMT Hectospec, so the current spectroscopic completeness is ~38%. For the remainder of the X-ray sources, we compute photometric redshifts based on multiband photometry in up to 35 bands from the UV to mid-IR. Particular attention is given to the fact that the vast majority the X-ray sources are active galactic nuclei and require hybrid templates. Our photometric redshifts have mean accuracy of σ = 0.04 and an outlier fraction of approximately 5%, reaching σ = 0.03 with less than 4% outliers in the area covered by CANDELS. The X-ray, multiwavelength photometry, and redshift catalogs are made publicly available.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0067-0049/220/1/10DOIArticle
http://iopscience.iop.org/article/10.1088/0067-0049/220/1/10/metaPublisherArticle
http://arxiv.org/abs/1503.09078arXivDiscussion Paper
ORCID:
AuthorORCID
Nandra, K.0000-0002-7150-9192
Aird, J. A.0000-0003-1908-8463
Salvato, M.0000-0001-7116-9303
Barro, G.0000-0001-6813-875X
Pérez-González, P. G.0000-0003-4528-5639
Barmby, P.0000-0003-2767-0090
Chary, R.-R.0000-0001-7583-0621
Cooper, M. C.0000-0003-1371-6019
Dickinson, M.0000-0001-5414-5131
Faber, S. M.0000-0003-4996-214X
Fazio, G. G.0000-0002-0670-0708
Guhathakurta, P.0000-0001-8867-4234
Ivison, R. J.0000-0001-5118-1313
Koo, D. C.0000-0003-3385-6799
Newman, J. A.0000-0001-8684-2222
Additional Information:© 2015 American Astronomical Society. Received 2014 April 8; accepted 2015 March 29; published 2015 September 9. We thank those who built and operate the Chandra X-ray observatory so successfully. We acknowledge financial support from Chandra grant G08-9129 A, NSF grant AST-0808133, US National Science Foundation via grant AST-0806732. P. G. P.-P. acknowledges support from the Spanish Programa Nacional de Astronomía y Astrofísica under grant AYA2012-37727. This work made use of the Rainbow Cosmological Surveys Database, which is operated by the Universidad Complutense de Madrid (UCM) partnered with the University of California Observatories at Santa Cruz (UCO/Lick,UCSC). Facilities: CXO(ACIS) - Chandra X-ray Observatory satellite, CFHT - Canada-France-Hawaii Telescope, GALEX - Galaxy Evolution Explorer satellite, Hale - Palomar Observatory's 5.1m Hale Telescope, HST - Hubble Space Telescope satellite, Keck: I - , Keck: II - , Mayall - Kitt Peak National Observatory's 4 meter Mayall Telescope, MMT - MMT at Fred Lawrence Whipple Observatory, Sloan - Sloan Digital Sky Survey Telescope, Subaru - Subaru Telescope, Spitzer(IRAC) - Spitzer Space Telescope satellite.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASAG08-9129 A
NSFAST-0808133
NSFAST-0806732
Nacional de Astronomía y AstrofísicaAYA2012-37727
Subject Keywords:galaxies: active – galaxies: nuclei – surveys
Issue or Number:1
Record Number:CaltechAUTHORS:20151201-155604532
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20151201-155604532
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:62522
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:02 Dec 2015 17:04
Last Modified:09 Mar 2020 13:19

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