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dc.contributor.author
Jarrett, T. H.
dc.contributor.author
Masci, F.
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Tsai, C. W.
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Petty, S.
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Cluver, M. E.
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Assef, Roberto J.
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Benford, D.
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Blain, A.
dc.contributor.author
Bridge, C.
dc.contributor.author
Donoso, Emilio
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dc.contributor.author
Eisenhardt, P.
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Koribalski, Bärbel
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Lake, S.
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Neill, James D.
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Seibert, M.
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Sheth, K.
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Stanford, S.
dc.contributor.author
Wright, E.
dc.date.available
2019-02-01T18:04:32Z
dc.date.issued
2013-01
dc.identifier.citation
Jarrett, T. H.; Masci, F.; Tsai, C. W.; Petty, S.; Cluver, M. E.; et al.; Extending the nearby galaxy heritage with wise: First results from the wise enhanced resolution galaxy atlas; IOP Publishing; Astronomical Journal; 145; 1; 1-2013; 6-40
dc.identifier.issn
0004-6256
dc.identifier.uri
http://hdl.handle.net/11336/69196
dc.description.abstract
The Wide-field Infrared Survey Explorer (WISE) mapped the entire sky at mid-infrared wavelengths 3.4 μm, 4.6 μm, 12 μm, and 22 μm. The mission was primarily designed to extract point sources, leaving resolved and extended sources, for the most part, unexplored. Accordingly, we have begun a dedicated WISE Enhanced Resolution Galaxy Atlas (WERGA) project to fully characterize large, nearby galaxies and produce a legacy image atlas and source catalog. Here we demonstrate the first results of the WERGA project for a sample of 17 galaxies, chosen to be of large angular size, diverse morphology, and covering a range in color, stellar mass, and star formation. It includes many well-studied galaxies, such as M51, M81, M87, M83, M101, and IC342. Photometry and surface brightness decomposition is carried out after special super-resolution processing, achieving spatial resolutions similar to that of Spitzer Infrared Array Camera. The enhanced resolution method is summarized in the first paper of this two-part series. In this second work, we present WISE, Spitzer, and Galaxy Evolution Explorer (GALEX) photometric and characterization measurements for the sample galaxies, combining the measurements to study the global properties. We derive star formation rates using the polycyclic aromatic hydrocarbon sensitive 12 μm (W3) fluxes, warm-dust sensitive 22 μm (W4) fluxes, and young massive-star sensitive ultraviolet (UV) fluxes. Stellar masses are estimated using the 3.4 μm (W1) and 4.6 μm (W2) measurements that trace the dominant stellar mass content. We highlight and showcase the detailed results of M83, comparing the WISE/Spitzer results with the Australia Telescope Compact Array H I gas distribution and GALEX UV emission, tracing the evolution from gas to stars. In addition to the enhanced images, WISE's all-sky coverage provides a tremendous advantage over Spitzer for building a complete nearby galaxy catalog, tracing both stellar mass and star formation histories. We discuss the construction of a complete mid-infrared catalog of galaxies and its complementary role of studying the assembly and evolution of galaxies in the local universe.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
IOP Publishing
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dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Galaxies: Fundamental Parameters
dc.subject
Galaxies: Statistics
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Infrared: Galaxies – Surveys
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Techniques: Image Processing
dc.subject.classification
Astronomía
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dc.subject.classification
Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
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dc.title
Extending the nearby galaxy heritage with wise: First results from the wise enhanced resolution galaxy atlas
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2019-01-31T14:02:25Z
dc.journal.volume
145
dc.journal.number
1
dc.journal.pagination
6-40
dc.journal.pais
Reino Unido
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dc.journal.ciudad
Londres
dc.description.fil
Fil: Jarrett, T. H.. California Institute of Technology; Estados Unidos. University of Cape Town; Sudáfrica
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Fil: Masci, F.. California Institute of Technology; Estados Unidos
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Fil: Tsai, C. W.. California Institute of Technology; Estados Unidos
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Fil: Petty, S.. University of California at Los Angeles; Estados Unidos
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Fil: Cluver, M. E.. Australian Astronomical Observatory; Australia
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Fil: Assef, Roberto J.. University of California at Los Angeles; Estados Unidos
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Fil: Benford, D.. National Aeronautics and Space Administration; Estados Unidos
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Fil: Blain, A.. University of Leicester; Reino Unido
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Fil: Bridge, C.. University of California at Los Angeles; Estados Unidos
dc.description.fil
Fil: Donoso, Emilio. University of California at Los Angeles; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
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Fil: Eisenhardt, P.. University of California at Los Angeles; Estados Unidos
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Fil: Koribalski, Bärbel. CSIRO Astronomy & Space Science; Australia
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Fil: Lake, S.. University of California at Los Angeles; Estados Unidos
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Fil: Neill, James D.. University of California at Los Angeles; Estados Unidos
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Fil: Seibert, M.. Carnegie Institution for Science; Estados Unidos
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Fil: Sheth, K.. National Radio Astronomy Observatory; Estados Unidos
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Fil: Stanford, S.. University of California at Davis; Estados Unidos
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Fil: Wright, E.. University of California at Los Angeles; Estados Unidos
dc.journal.title
Astronomical Journal
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dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/0004-6256/145/1/6
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info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/0004-6256/145/1/6/meta
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1210.3628
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