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Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies

Dale, D. A. and Cook, D. O. and Roussel, H. and Turner, J. A. and Armus, L. and Bolatto, A. D. and Boquien, M. and Brown, M. J. I. and Calzetti, D. and De Looze, I. and Galametz, M. and Gordon, K. D. and Groves, B. A. and Jarrett, T. H. and Helou, G. and Herrera-Camus, R. and Hinz, J. L. and Hunt, L. K. and Kennicutt, R. C. and Murphy, E. J. and Rest, A. and Sandstrom, K. M. and Smith, J.-D. T. and Tabatabaei, F. S. and Wilson, C. D. (2017) Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies. Astrophysical Journal, 837 (1). Art. No. 90. ISSN 1538-4357. https://resolver.caltech.edu/CaltechAUTHORS:20170601-134218692

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Abstract

We present an update to the ultraviolet-to-radio database of global broadband photometry for the 79 nearby galaxies that comprise the union of the KINGFISH (Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel) and SINGS (Spitzer Infrared Nearby Galaxies Survey) samples. The 34-band data set presented here includes contributions from observational work carried out with a variety of facilities including GALEX, SDSS, Pan-STARRS1, NOAO, 2MASS, Wide-Field Infrared Survey Explorer, Spitzer, Herschel, Planck, JCMT, and the VLA. Improvements of note include recalibrations of previously published SINGS BVR _CI_C and KINGFISH far-infrared/submillimeter photometry. Similar to previous results in the literature, an excess of submillimeter emission above model predictions is seen primarily for low-metallicity dwarf or irregular galaxies. This 33-band photometric data set for the combined KINGFISH+SINGS sample serves as an important multiwavelength reference for the variety of galaxies observed at low redshift. A thorough analysis of the observed spectral energy distributions is carried out in a companion paper.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4357/aa6032DOIArticle
http://iopscience.iop.org/article/10.3847/1538-4357/aa6032/metaPublisherArticle
https://arxiv.org/abs/1702.05205arXivDiscussion Paper
ORCID:
AuthorORCID
Dale, D. A.0000-0002-5782-9093
Cook, D. O.0000-0002-6877-7655
Turner, J. A.0000-0003-2261-5746
Armus, L.0000-0003-3498-2973
Bolatto, A. D.0000-0002-5480-5686
Boquien, M.0000-0003-0946-6176
Brown, M. J. I.0000-0002-1207-9137
Calzetti, D.0000-0002-5189-8004
Galametz, M.0000-0002-0283-8689
Groves, B. A.0000-0002-9768-0246
Jarrett, T. H.0000-0002-4939-734X
Helou, G.0000-0003-3367-3415
Herrera-Camus, R.0000-0002-2775-0595
Hunt, L. K.0000-0001-9162-2371
Kennicutt, R. C.0000-0001-5448-1821
Murphy, E. J.0000-0001-7089-7325
Sandstrom, K. M.0000-0002-4378-8534
Smith, J.-D. T.0000-0003-1545-5078
Wilson, C. D.0000-0001-5817-0991
Additional Information:© 2017 American Astronomical Society. Received 2016 December 5. Accepted 2017 February 10. Published 2017 March 7. We thank the referee for excellent suggestions that improved this work. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. This work is based on observations made with the Spitzer Space Telescope and utilizes the NASA/IPAC Infrared Science Archive, both operated by JPL/Caltech under a contract with NASA. We gratefully acknowledge NASA's support for construction, operation, and science analysis for the GALEX mission, developed in cooperation with the Centre National d'Etudes Spatiales of France and the Korean Ministry of Science and Technology. Funding for the Sloan Digital Sky Survey and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the NSF, the U.S. Department of Energy, NASA, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the JPL/Caltech, funded by NASA. The Pan-STARRS1 Surveys have been made possible through contributions of the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the NSF, the University of Maryland, and Eotvos Lorand University and the Los Alamos National Laboratory.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
Alfred P. Sloan FoundationUNSPECIFIED
NSFUNSPECIFIED
Department of Energy (DOE)UNSPECIFIED
Japanese MonbukagakushoUNSPECIFIED
Max Planck SocietyUNSPECIFIED
Higher Education Funding Council for EnglandUNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:galaxies: photometry; galaxies: ISM; infrared: ISM; ISM: general
Issue or Number:1
Record Number:CaltechAUTHORS:20170601-134218692
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170601-134218692
Official Citation:D. A. Dale et al 2017 ApJ 837 90
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:77893
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:01 Jun 2017 21:05
Last Modified:09 Mar 2020 13:19

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