A dataset provided by the European Space Agency

Name GT1_lspinogl_2
Title Bright Seyfert Nuclei: FTS spectroscopy
URL

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DOI https://doi.org/10.5270/esa-ra39kjv
Author spinoglio, l.
Description This proposal is to measure the full 200-670um FTS spectra at high
resolution (virgul500 km/s) of 10 bright Seyfert nuclei. We are aiming to
detect the high-J CO lines, the [CI] and [NII] fine structure lines and
any other possible emission or absorption from H2O or other molecules.
The selected targets include four AGN1.s (two Seyfert 1.s and two
HBLR-Seyfert 2.s), three AGN2.s and three lower nuclear activity objects.
These objects have been chosen because they are the brightest at 60-100
um and their IR luminosity has been separated between AGN and Starburst
components through mid-IR spectroscopy. This program is fully
complementary to the Hercules OTKP, which is focused on SPIRE FTS
spectroscopy of the ULIRG/LIRG population, while the present proposal targets
optically bright nuclei, at a presumably later evolutionary stage.
We expect that the detection of the CO ladder in Seyfert nuclei will allow
us to measure the effects of the AGN on the circum-nuclear ISM of the galaxy
through detection of X-ray dominated regions. Moreover the molecular
spectroscopy could reveal the presence of the predicted molecular tori.
The 10 galaxies for which we request SPIRE FTS observations of their nuclei
in one single position can be observed in a total integration time of 14.7
hours. To complement the spectroscopic observations, photometric imaging with
SPIRE and PACS is also requested with a total time needed of 0.7 and 2.4
hours, respectively.
Publication L‧CO/LFIR Relations with CO Rotational Ladders of Galaxies Across the Herschel SPIRE Archive . Kamenetzky J. et al. . The Astrophysical Journal, Volume 829, Issue 2, article id. 93, 16 pp. (2016). . 829 . 10.3847\/0004-637X\/829\/2\/93 . 2016ApJ...829...93K ,
Herschel/SPIRE Submillimeter Spectra of Local Active Galaxies . Pereira-Santaella Miguel et al. . The Astrophysical Journal, Volume 768, Issue 1, article id. 55, 20 pp. (2013). . 768 . 10.1088\/0004-637X\/768\/1\/55 . 2013ApJ...768...55P ,
Local Swift-BAT active galactic nuclei prefer circumnuclear star formation . Lutz D. et al. . Astronomy & Astrophysics, Volume 609, id.A9, 7 pp. . 609 . 10.1051\/0004-6361\/201731423 . 2018A&A...609A...9L ,
Instrument SPIRE_SpireSpectrometer_, PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage 2010-08-03T15:23:23Z/2011-08-20T11:00:14Z
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 2012-02-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, spinoglio, l., 2012, GT1_lspinogl_2, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-ra39kjv