A dataset provided by the European Space Agency

Name GT2_lspinogl_6
Title PACS spectroscopy of bright Seyfert galaxies in the [OIV]26um line.
URL

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DOI https://doi.org/10.5270/esa-rhdw3j6
Author spinoglio, l.
Description This proposal is aimed at obtaining PACS spectroscopic data
of 10 bright (5 type-1 and 5 type-2) Seyfert nuclei for six
atomic fine-structure lines ([OIII]52um, [OI]63um, [OIII]88um,
[NII]122um, [OI]145um and [CII]157um) and two molecular
lines (CO J=18-17 and OH 119um). It will complete the
coverage of the same ionic lines of another 11 Seyfert
galaxies, already observed or reserved, by targeting the
[OIII]52um line only. All targets were selected based on
their optical classification and on the strength of their
[OIV]25.9um fine-structure-line emission, proportional
to their AGN bolometric luminosity. The proposed targets
are among the brightest accretion-powered sources in the
local Universe. The two [OIII] lines, together with the [OIV]
line measured by Spitzer, will be used for the determination
of their narrow-line-region gas density. The FIR spectroscopic
tracers, combined with the MIR ones obtained with Spitzer,
will enable us to classify and model the various levels of
non-thermal and starburst activity in local bright Seyferts.
The mid-to far-IR line ratio diagnostic diagrams that we
will construct will be essential for the future interpretation
of spectroscopic surveys at long wavelengths with ALMA and
SPICA. The high spectral resolution of PACS will allow us to
further study the dynamics of the nuclear gas, in combination
with lines spectrally resolved by Spitzer IRS. The range
spectroscopy with PACS has been optimized to allow the
detection of 6 fine structure lines, 1 CO line, 1 OH doublet
in a total time of 18.0 hours.
Publication Far-infrared Line Spectra of Active Galaxies from the Herschel/PACS Spectrometer: The Complete Database . Fernández-Ontiveros Juan Antonio et al. . The Astrophysical Journal Supplement Series, Volume 226, Issue 2, article id. 19, 26 pp. (2016). . 226 . 10.3847\/0067-0049\/226\/2\/19 . 2016ApJS..226...19F ,
Far-infrared Line Spectra of Seyfert Galaxies from the Herschel-PACS Spectrometer . Spinoglio Luigi et al. . The Astrophysical Journal, Volume 799, Issue 1, article id. 21, 20 pp. (2015). . 799 . 10.1088\/0004-637X\/799\/1\/21 . 2015ApJ...799...21S ,
Instrument PACS_PacsRangeSpec_point, PACS_PacsLineSpec_point
Temporal Coverage 2011-12-19T20:59:20Z/2012-10-21T15:39:36Z
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/h®erschel/
Date Published 2013-04-21T14:27:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, spinoglio, l., 2013, GT2_lspinogl_6, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-rhdw3j6