A dataset provided by the European Space Agency

Name SDP_rkennicu_3
Title Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (KINGFISH)
URL

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DOI 10.5270/esa-8384jk8
Author kennicutt, r.
Description We propose the KINGFISH project (Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel) of nearby (D<30 Mpc) galaxies mostly drawn from the SINGS sample, which span a large range of star forming (SF) environments found in the nearby Universe. KINGFISH will provide for the first time (1) imaging across the peak of the dust SED at a spatial resolution that matches individual SF complexes, and (2) spectroscopic maps of key diagnostic lines to constrain the cooling and heating processes of the warm neutral medium and the obscured ionized ISM. The PACS and SPIRE imaging from 75 to 500 microns will produce the first comprehensive census of dust in different galactic environments on a spatially resolved basis. KINGFISH.s spectral line mapping will sample the full range of SF environments in regions that have already been targeted by SINGS IRS mapping. Leveraging the synergy between imaging and spectroscopy, KINGFISH will provide robust measures of the bolometric luminosity and star formation rates, the mass and spatial distribution of cold dust and the r^ance of different heating mechanisms in the energy balance of the dust in distinctly different environments. Measurements of [CII]158 micron, [OI]63 micron, [OIII]88 micron, and [NII]122, 205 micron, will finally provide the diagnostics needed to understand two crucial, but so far ill-understood, components of the star formation and feedback matter cycle: the warm neutral medium and the obscured ionized medium. The analysis and modeling of KINGFISH.s imaging and spectroscopy will draw on the unique expertise from the Spitzer SINGS survey at shorter wavelengths. The resulting dataset will be of immense astrophysical power and enormous long-term legacy value, bringing us a crucial step closer to understanding star formation and energy feedback on scales of galaxies. It will also provide an invaluable foundation for interpreting observations of more distant galaxies with Herschel, ALMA, and other facilities.
Publication The Radio Spectral Energy Distribution and Star-formation Rate Calibration in Galaxies . Tabatabaei F. S. et al. . The Astrophysical Journal, Volume 836, Issue 2, article id. 185, 24 pp. (2017). . 836 . 10.3847\/1538-4357\/836\/2\/185 . 2017ApJ...836..185T ,
The local luminosity function of star-forming galaxies derived from the Planck Early Release Compact Source Catalogue . Negrello M. et al. . Monthly Notices of the Royal Astronomical Society, Volume 429, Issue 2, p.1309-1323 . 429 . 10.1093\/mnras\/sts417 . 2013MNRAS.429.1309N ,
KINGFISH—Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel: Survey Description and Image Atlas . Kennicutt R. C. et al. . Publications of the Astronomical Society of the Pacific, Volume 123, Issue 910, pp. 1347 (2011). . 123 . 10.1086\/663818 . 2011PASP..123.1347K ,
DustPedia: the relationships between stars, gas, and dust for galaxies residing in different environments . Davies J. I. et al. . Astronomy and Astrophysics . null . null . 2019A&A...626A..63D ,
Old and young stellar populations in DustPedia galaxies and their role in dust heating . Nersesian A. et al. . Astronomy and Astrophysics . null . null . 2019A&A...624A..80N ,
Updated 34-band Photometry for the Sings-KINGFISH Samples of Nearby Galaxies . Dale D. A. et al. . The Astrophysical Journal, Volume 837, Issue 1, article id. 90, 20 pp. (2017). . 837 . 10.3847\/1538-4357\/aa6032 . 2017ApJ...837...90D ,
The Star Formation in Radio Survey: GBT 33 GHz Observations of Nearby Galaxy Nuclei and Extranuclear Star-forming Regions . Murphy E. J. et al. . The Astrop...
Instrument PACS_PacsPhoto_largeScan, PACS_PacsLineSpec_large, SPIRE_SpirePhoto_large
Temporal Coverage 2009-11-18T00:40:51Z/2010-01-22T09:02:18Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2010-03-03T08:55:39Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-03-03T08:55:39Z, SDP_rkennicu_3, SPG v14.2.0. https://doi.org/10.5270/esa-8384jk8