A dataset provided by the European Space Agency

Name GT1_lspinogl_4
Title Bright Seyfert nuclei: PACS spectroscopy
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342197796&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342197797&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342197798&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342197909&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342197910&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342197911&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342197912&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342197913&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342197914&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342208880&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342212222&instrument_name=PACS&product_level=LEVEL0&compress=true
...
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342212223&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342212224&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342216210&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342216211&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342216212&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342218185&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342218186&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342218187&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342218488&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342218489&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342218490&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342221357&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-aogiafo
Author spinoglio, l.
Description This proposal is to obtain PACS spectroscopy of 10 bright Seyfert nuclei
to observe the 6 ionic fine-structure lines, four high-J CO lines and three
OH doublets. The selected targets include four AGN1.s (two Seyfert 1.s
and two HBLR-Seyfert 2.s), three AGN2.s and three lower activity objects.
These objects have been chosen because they are the brightest at
60-100 micron, their luminosity has been separated between AGN and
Starburst components through mid-IR spectroscopy.
The immediate goals are to obtain a large set of FIR tracers to be able to
classify and model the various levels of non-thermal and starburst
activity in local Seyferts, using both atomic (Herschel and Spitzer) and
molecular (Herschel and H2 from Spitzer) transitions. The mid-to far-IR
classification of activity in galaxies will be essential in the close future to
interpret the spectroscopic surveys at long wavelength that will be
performed by Herschel, ALMA and SPICA.
The range spectroscopy with PACS has been optimized to allow detection
of 4 CO lines, 3 OH doublets and 6 fine structure lines in a total time of
14.0 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 ,
The Search for Molecular Outflows in Local Volume AGNs with Herschel-PACS . Stone M. et al. . The Astrophysical Journal, Volume 826, Issue 2, article id. 111, 24 pp. (2016). . 826 . 10.3847\/0004-637X\/826\/2\/111 . 2016ApJ...826..111S ,
Neon and [C II] 158 μm Emission Line Profiles in Dusty Starbursts and Active Galactic Nuclei . Samsonyan Anahit et al. . The Astrophysical Journal Supplement Series, Volume 226, Issue 1, article id. 11, 18 pp. (2016). . 226 . 10.3847\/0067-0049\/226\/1\/11 . 2016ApJS..226...11S ,
Instrument PACS_PacsRangeSpec_point
Temporal Coverage 2010-06-05T12:39:13Z/2011-05-18T14:27:22Z
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 2011-12-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, spinoglio, l., 2011, GT1_lspinogl_4, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-aogiafo