A dataset provided by the European Space Agency

Name OT1_dweedman_1
Title Comparing [CII] 158 micron Luminosities to Spectral Properties of Luminous Starburst Galaxies and AGN
URL

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DOI 10.5270/esa-tijwujr
Author weedman, d.
Description Herschel PACS spectroscopy of the [CII] emission line at 158 microns is proposed for a carefully selected sample of 123 sources that already have complete low and high resolution mid-infrared spectra between 5 microns and 35 microns from the Spitzer Infrared Spectrograph, and which also have spectral energy distributions (SEDs) from IRAS and Akari photometry. [CII] 158 um is the strongest far-infrared emission line and therefore crucial to compare with other features in luminous, dusty galaxies. Sources have 0.004 < z < 0.34 and 43.0 < log L(IR) < 46.8 (erg per sec) and cover the full range of starburst galaxy and AGN classifications. Obtaining these [CII] line fluxes with PACS will allow: 1. determining how precisely [CII] luminosity measures star formation rate by comparing to PAH features and emission lines that arise in starburst galaxies; 2. determining how [CII] luminosity and equivalent width changes with starburst-AGN fraction, by comparing with strength and equivalent width of PAH and [NeII] emission arising from starbursts, and with strength of high ionization lines [NeV] and [OIV] and silicate absorption or emission arising from AGN; 3. determining how [CII] luminosity and equivalent width changes with dust temperature and bolometric luminosity, as derived from spectral energy distributions, and whether this depends on the starburst-AGN fraction. These determinations will allow interpretation of high redshift sources for which the only available diagnostics are the luminosity and equivalent width of the [CII] line and the far-infrared rest-frame SED. The total observing program requires 20.2 hours of Herschel observing time.
Publication Strong C+ Emission in Galaxies at z ~ 1-2: Evidence for Cold Flow Accretion Powered Star Formation in the Early Universe . Brisbin Drew et al. . The Astrophysical Journal, Volume 799, Issue 1, article id. 13, 18 pp. (2015). . 799 . 10.1088\/0004-637X\/799\/1\/13 . 2015ApJ...799...13B ,
A Herschel-PACS Far-infrared Line Emission Survey of Local Luminous Infrared Galaxies . Díaz-Santos T. et al. . The Astrophysical Journal, Volume 846, Issue 1, article id. 32, 22 pp. (2017). . 846 . 10.3847\/1538-4357\/aa81d7 . 2017ApJ...846...32D ,
[C II] 158 μm Luminosities and Star Formation Rate in Dusty Starbursts and Active Galactic Nuclei . Sargsyan L. et al. . The Astrophysical Journal, Volume 755, Issue 2, article id. 171, 13 pp. (2012). . 755 . 10.1088\/0004-637X\/755\/2\/171 . 2012ApJ...755..171S ,
Extended [C II] Emission in Local Luminous Infrared Galaxies . Díaz-Santos T. et al. . The Astrophysical Journal Letters, Volume 788, Issue 1, article id. L17, 5 pp. (2014). . 788 . 10.1088\/2041-8205\/788\/1\/L17 . 2014ApJ...788L..17D ,
The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types . De Looze Ilse et al. . Astronomy & Astrophysics, Volume 568, id.A62, 34 pp. . 568 . 10.1051\/0004-6361\/201322489 . 2014A&A...568A..62D ,
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Instrument PACS_PacsLineSpec_point
Temporal Coverage 2011-05-01T20:06:36Z/2012-03-25T15:21:52Z
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 2012-09-25T15:08:39Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-09-25T15:08:39Z, OT1_dweedman_1, SPG v14.2.0. https://doi.org/10.5270/esa-tijwujr