A dataset provided by the European Space Agency

Name OT1_hnetzer_1
Title Herschel study of black hole and galaxy evolution: The z<0.3 QUEST AGN sample.
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342255517&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342255517&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342255518&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342255518&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342255519&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342255519&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342255520&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342255520&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342256844&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342256844&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342258358&instrument_name=SPIRE&product_level=LEVEL0&compress=true
...
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342258358&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342258528&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342258528&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342258529&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342258529&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342259266&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342259266&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342259267&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342259267&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342259385&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342259385&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI 10.5270/esa-afijvwm
Author netzer, h.
Description We propose 15.6 hours of Herschel time to secure high quality data,over the entire 70-500 micron range, for a group of 27 local, luminous active galactic nuclei (the QUEST AGN sample). The sources represent well the optically selected PG-QSO sample with redshifts up to z=0.3, and have been investigated, in great detail, in almost all other wavelength bands. The new far infrared (FIR) data set will be ideal to study various fundamental questions related to the connection and co-evolution of AGN and their host galaxies. Our previous Spitzer-IRS work on the sample has already revealed a clear relationship between the total AGN luminosity and the star formation rate (SFR) in their hosts. However, the previously undetected FIR sources may be situated in red-and-dead hosts and the Herschel observations can find these objects and allow a direct comparison of their AGN properties, like black hole (BH) mass and accretion rate, with those of the sources with high SFR. The observations will also provide unique information about the "intrinsic infrared AGN spectrum" with consequences to dust properties and distribution in such objects. Our sample is a needed ingredient in any Herschel-based studies that combine FIR-selected (IRAS, Spitzer, Herschel) and optically selected samples with their different biases. Its later comparison with similar high redshift observations will provide invaluable information about the cosmological evolution of AGN and star forming galaxies.
Publication Intrinsic AGN SED & black hole growth in the Palomar-Green quasars . Lani Caterina et al. . Monthly Notices of the Royal Astronomical Society, Volume 471, Issue 1, p.59-79 . 471 . 10.1093\/mnras\/stx1374 . 2017MNRAS.471...59L ,
AGN are cooler than you think: the intrinsic far-IR emission from QSOs . Symeonidis M. et al. . Monthly Notices of the Royal Astronomical Society, Volume 459, Issue 1, p.257-276 . 459 . 10.1093\/mnras\/stw667 . 2016MNRAS.459..257S ,
On the Gas Content and Efficiency of AGN Feedback in Low-redshift Quasars . Shangguan Jinyi et al. . The Astrophysical Journal, Volume 854, Issue 2, article id. 158, 37 pp. (2018). . 854 . 10.3847\/1538-4357\/aaa9be . 2018ApJ...854..158S ,
The Infrared Emission and Opening Angle of the Torus in Quasars . Zhuang Ming-Yang et al. . The Astrophysical Journal, Volume 862, Issue 2, article id. 118, 15 pp. (2018). . 862 . 10.3847\/1538-4357\/aacc2d . 2018ApJ...862..118Z ,
The far-infrared emitting region in local galaxies and QSOs: Size and scaling relations . Lutz D. et al. . Astronomy & Astrophysics, Volume 591, id.A136, 23 pp. . 591 . 10.1051\/0004-6361\/201527706 . 2016A&A...591A.136L ,
Star formation in quasar hosts and the origin of radio emission in radio-quiet quasars . Zakamska Nadia L. et al. . Monthly Notices of the Royal Astronomical Society, Volume 455, Issue 4, p.4191-4211 . 455 . 10.1093\/mnras\/stv2571 . 2016MNRAS.455.4191Z ,
Herschel Survey of the Palomar-Green QSOs at Low Redshift . Petric Andreea O. e...
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage 2012-11-20T06:11:20Z/2013-01-10T13:14:08Z
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-07-10T13:09:32Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-07-10T13:09:32Z, OT1_hnetzer_1, SPG v14.2.0. https://doi.org/10.5270/esa-afijvwm