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Spitzer Observations of the North Ecliptic Pole

Nayyeri, H. and Ghotbi, N. and Cooray, A. and Bock, J. and Clements, D. L. and Im, M. and Kim, M. G. and Korngut, P. and Lanz, A. and Lee, H. M. and Lee, D. H. and Malkan, M. and Matsuhara, H. and Matsumoto, T. and Matsuura, S. and Nam, U. W. and Pearson, C. and Serjeant, S. and Smidt, J. and Tsumura, K. and Wada, T. and Zemcov, M. (2018) Spitzer Observations of the North Ecliptic Pole. Astrophysical Journal Supplement Series, 234 (2). Art. No. 38. ISSN 1538-4365. https://resolver.caltech.edu/CaltechAUTHORS:20180212-073736632

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Abstract

We present a photometric catalog for Spitzer Space Telescope warm mission observations of the North Ecliptic Pole (NEP; centered at R.A. = 18^h00^m00^s, decl. = 66^d33^m38^s.552). The observations are conducted with IRAC in the 3.6 and 4.5 μm bands over an area of 7.04 deg^2, reaching 1σ depths of 1.29 μJy and 0.79 μJy in the 3.6 μm and 4.5 μm bands, respectively. The photometric catalog contains 380,858 sources with 3.6 and 4.5 μm band photometry over the full-depth NEP mosaic. Point-source completeness simulations show that the catalog is 80% complete down to 19.7 AB. The accompanying catalog can be used for constraining the physical properties of extragalactic objects, studying the AGN population, measuring the infrared colors of stellar objects, and studying the extragalactic infrared background light.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4365/aaa07eDOIArticle
http://iopscience.iop.org/article/10.3847/1538-4365/aaa07ePublisherArticle
https://arxiv.org/abs/1712.01290arXivDiscussion Paper
ORCID:
AuthorORCID
Nayyeri, H.0000-0001-8242-9983
Cooray, A.0000-0002-3892-0190
Bock, J.0000-0002-5710-5212
Clements, D. L.0000-0002-9548-5033
Im, M.0000-0002-8537-6714
Lee, H. M.0000-0003-4412-7161
Malkan, M.0000-0001-6919-1237
Matsuura, S.0000-0002-5698-9634
Pearson, C.0000-0001-6139-649X
Serjeant, S.0000-0002-0517-7943
Zemcov, M.0000-0001-8253-1451
Additional Information:© 2018 American Astronomical Society. Received 2017 September 3. Accepted 2017 November 19. Published 2018 February 8. We wish to thank the referee for reading the original manuscript and providing useful suggestions. Financial support for this work was provided by NSF through AST-1313319 for H.N. and A.C. The UCI group also acknowledges support from HST-GO-14083.002-A, HST-GO-13718.002-A, and NASA NNX16AF38G grants. M.I. acknowledge the support from the NRFK grant, No. 2017R1A3A3001362. This work was supported by NASA APRA research grants NNX07AI54G, NNG05WC18G, NNX07AG43G, NNX07AJ24G, and NNX10AE12G. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech.
Group:Infrared Processing and Analysis Center (IPAC), Astronomy Department
Funders:
Funding AgencyGrant Number
NSFAST-1313319
NASAHST-GO-14083.002-A
NASAHST-GO-13718.002-A
NASANNX16AF38G
National Research Foundation of Korea2017R1A3A3001362
NASANNX07AI54G
NASANNG05WC18G
NASANNX07AG43G
NASANNX07AJ24G
NASANNX10AE12G
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:infrared: galaxies; infrared: stars; surveys
Issue or Number:2
Record Number:CaltechAUTHORS:20180212-073736632
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180212-073736632
Official Citation:H. Nayyeri et al 2018 ApJS 234 38
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:84775
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:13 Feb 2018 17:50
Last Modified:09 Mar 2020 13:19

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