The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC Mosaics
We present new Spitzer Infrared Array Camera (IRAC) 3.6 and 4.5 μ m 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...
Main Authors: | , , , , , , , , , , , , , , , , , , , , |
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Format: | Article |
Language: | English |
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IOP Publishing
2023-01-01
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Series: | The Astronomical Journal |
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Online Access: | https://doi.org/10.3847/1538-3881/acd773 |
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author | Marianna Annunziatella Anna Sajina Mauro Stefanon Danilo Marchesini Mark Lacy Ivo Labbé Lilianna Houston Rachel Bezanson Eiichi Egami Xiaohui Fan Duncan Farrah Jenny Greene Andy Goulding Yen-Ting Lin Xin Liu Thibaud Moutard Yoshiaki Ono Masami Ouchi Marcin Sawicki Jason Surace Katherine Whitaker |
author_facet | Marianna Annunziatella Anna Sajina Mauro Stefanon Danilo Marchesini Mark Lacy Ivo Labbé Lilianna Houston Rachel Bezanson Eiichi Egami Xiaohui Fan Duncan Farrah Jenny Greene Andy Goulding Yen-Ting Lin Xin Liu Thibaud Moutard Yoshiaki Ono Masami Ouchi Marcin Sawicki Jason Surace Katherine Whitaker |
author_sort | Marianna Annunziatella |
collection | DOAJ |
description | We present new Spitzer Infrared Array Camera (IRAC) 3.6 and 4.5 μ m 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 deg ^2 with a mean integration time of ≈1200s, providing a median 5 σ depth of 23.7(23.3) at 3.6(4.5) μ m 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. |
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issn | 1538-3881 |
language | English |
last_indexed | 2024-03-12T04:00:27Z |
publishDate | 2023-01-01 |
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series | The Astronomical Journal |
spelling | doaj.art-37776aafa62541799babe3a9f3f89fef2023-09-03T11:38:27ZengIOP PublishingThe Astronomical Journal1538-38812023-01-0116612510.3847/1538-3881/acd773The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC MosaicsMarianna Annunziatella0https://orcid.org/0000-0002-8053-8040Anna Sajina1https://orcid.org/0000-0002-1917-1200Mauro Stefanon2https://orcid.org/0000-0001-7768-5309Danilo Marchesini3https://orcid.org/0000-0001-9002-3502Mark Lacy4https://orcid.org/0000-0002-3032-1783Ivo Labbé5https://orcid.org/0000-0002-2057-5376Lilianna Houston6Rachel Bezanson7https://orcid.org/0000-0001-5063-8254Eiichi Egami8https://orcid.org/0000-0003-1344-9475Xiaohui Fan9https://orcid.org/0000-0003-3310-0131Duncan Farrah10https://orcid.org/0000-0003-1748-2010Jenny Greene11https://orcid.org/0000-0002-5612-3427Andy Goulding12https://orcid.org/0000-0003-4700-663XYen-Ting Lin13https://orcid.org/0000-0001-7146-4687Xin Liu14https://orcid.org/0000-0003-0049-5210Thibaud Moutard15https://orcid.org/0000-0002-3305-9901Yoshiaki Ono16https://orcid.org/0000-0001-9011-7605Masami Ouchi17https://orcid.org/0000-0002-1049-6658Marcin Sawicki18https://orcid.org/0000-0002-7712-7857Jason Surace19https://orcid.org/0000-0001-7291-0087Katherine Whitaker20https://orcid.org/0000-0001-7160-3632Centro de Astrobiología , (CAB, CSIC-INTA), Carretera de Ajalvir km 4, E-28850 Torrejón de Ardoz, Madrid, SpainTufts University , Medford, MA, USALeiden Observatory, Leiden University , PO Box 9513, NL-2300 RA, Leiden, The Netherlands; Departament d’Astronomia i Astrofísica, Universitat de València , C. Dr. Moliner 50, E-46100 Burjassot, València, SpainTufts University , Medford, MA, USANRAO, Charlottesville , VA, USACentre for Astrophysics and Supercomputing, Swinburne University of Technology , AustraliaTufts University , Medford, MA, USADepartment of Physics and Astronomy and PITT PACC, University of Pittsburgh , Pittsburgh, PA 15260, USASteward Observatory, University of Arizona , Tucson, AZ 85721, USASteward Observatory, University of Arizona , Tucson, AZ 85721, USAInstitute for Astronomy, University of Hawaii , 2680 Woodlawn Dr., Honolulu, HI, 96822, USA; Department of Physics and Astronomy, University of Hawaii at Mānoa , 2505 Correa Rd., Honolulu, HI, 96822, USADepartment of Astrophysical Sciences, Princeton University , Princeton, NJ 08544, USADepartment of Astrophysical Sciences, Princeton University , Princeton, NJ 08544, USAInstitute of Astronomy and Astrophysics , Academia Sinica, Taipei 10617, TaiwanDepartment of Astronomy, University of Illinois at Urbana-Champaign , Urbana, IL 61801, USA; National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign , Urbana, IL 61801, USAInstitute for Computational Astrophysics and Department of Astronomy and Physics, Saint Mary's University , 923 Robie Street, Halifax, Nova Scotia, B3H 3C3, Canada; Aix Marseille Universite , CNRS, CNES, LAM—Laboratoire d’Astrophysique de Marseille, 38 rue F. Joliot-Curie, F-13388 Marseille, FranceInstitute for Cosmic Ray Research, The University of Tokyo , Kashiwa-no-ha, Kashiwa 277-8582, JapanInstitute for Cosmic Ray Research, The University of Tokyo , Kashiwa-no-ha, Kashiwa 277-8582, JapanInstitute for Computational Astrophysics and Department of Astronomy and Physics, Saint Mary's University , 923 Robie Street, Halifax, Nova Scotia, B3H 3C3, CanadaInfrared Processing and Analysis Center , Pasadena, CA, USAUMass Amherst , Amherst, MA, USAWe present new Spitzer Infrared Array Camera (IRAC) 3.6 and 4.5 μ m 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 deg ^2 with a mean integration time of ≈1200s, providing a median 5 σ depth of 23.7(23.3) at 3.6(4.5) μ m 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.https://doi.org/10.3847/1538-3881/acd773Astronomy data analysisAstronomy data acquisition |
spellingShingle | Marianna Annunziatella Anna Sajina Mauro Stefanon Danilo Marchesini Mark Lacy Ivo Labbé Lilianna Houston Rachel Bezanson Eiichi Egami Xiaohui Fan Duncan Farrah Jenny Greene Andy Goulding Yen-Ting Lin Xin Liu Thibaud Moutard Yoshiaki Ono Masami Ouchi Marcin Sawicki Jason Surace Katherine Whitaker The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC Mosaics The Astronomical Journal Astronomy data analysis Astronomy data acquisition |
title | The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC Mosaics |
title_full | The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC Mosaics |
title_fullStr | The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC Mosaics |
title_full_unstemmed | The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC Mosaics |
title_short | The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC Mosaics |
title_sort | spitzer coverage of hsc deep with irac for z studies shiraz i irac mosaics |
topic | Astronomy data analysis Astronomy data acquisition |
url | https://doi.org/10.3847/1538-3881/acd773 |
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