The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC Mosaics
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Annunziatella, M.Sajina, A.
Stefanon, M.
Marchesini, D.
Lacy, M.
Labbé, I.
Houston, L.
Bezanson, R.
Egami, E.
Fan, X.
Farrah, D.
Greene, J.
Goulding, A.
Lin, Y.-T.
Liu, X.
Moutard, T.
Ono, Y.
Ouchi, M.
Sawicki, M.
Surace, J.
Whitaker, K.
Affiliation
Steward Observatory, University of ArizonaIssue Date
2023-06-23
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American Astronomical SocietyCitation
Marianna Annunziatella et al 2023 AJ 166 25Journal
Astronomical JournalRights
© 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We present new Spitzer Infrared Array Camera (IRAC) 3.6 and 4.5 μm mosaics of three fields, E-COSMOS, DEEP2-F3, and ELAIS-N1. Our mosaics include both new IRAC observations as well as reprocessed archival data in these fields. These fields are part of the HSC-Deep grizy survey and have a wealth of additional ancillary data. The addition of these new IRAC mosaics is critical in allowing for improved photometric redshifts and stellar population parameters at cosmic noon and earlier epochs. The total area mapped by this work is ∼17 deg2 with a mean integration time of ≈1200s, providing a median 5σ depth of 23.7(23.3) at 3.6(4.5) μm in AB. We perform SExtractor photometry both on the combined mosaics as well as the single-epoch mosaics taken ≈6 months apart. The resultant IRAC number counts show good agreement with previous studies. In combination with the wealth of existing and upcoming spectrophotometric data in these fields, our IRAC mosaics will enable a wide range of galactic evolution and AGN studies. With that goal in mind, we make the combined IRAC mosaics and coverage maps of these three fields publicly available. © 2023. The Author(s). Published by the American Astronomical Society.Note
Open access journalISSN
0004-6256Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.3847/1538-3881/acd773
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Except where otherwise noted, this item's license is described as © 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.

