A dataset provided by the European Space Agency

Name OT2_hspoon_1
Title Probing the multi-phase outflows in the 'Fire and Ice. galaxy IRAS F00183-7111 using far-IR PACS spectroscopy
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342245249&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342245250&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342245251&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342245458&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342245651&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342257636&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342258852&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI 10.5270/esa-m2u4v2a
Author spoon, h.
Description IRAS F00183-7111 is possibly the most luminous ULIRG discovered by IRAS. Nicknamed the .fire and ice galaxy. since its widely-cited first Spitzer-IRS observations were published in 2004, this galaxy has continued to amaze. Not only does it host the possibly most deeply obscured powerful AGN-quasar in the Local Universe (z<0.4), its extremely wide mid-IR neon line profiles and the extended red wing to the CO(J=1-0) line hint at massive outflows. These outflows may be powered by the radio jets, which appear to be young and which may be responsible for the optically-obscured, highly disturbed ionized neon gas line emission seen with Spitzer, the multiple spatial and kinematic [O III] 5007A components, and the off-nuclear soft X-ray bubble seen by XMM. So far this luminous z=0.328 merger has remained unobserved by Herschel. Here we propose to study its nuclear outflow at far-infrared wavelengths to reveal optically obscured high-velocity ionized gas outflow components, and to assess the extent and timescale of the neutral and molecular gas outflows, which may drive the evolution of IRAS F00183-7111 from a deeply buried merger remnant to a naked QSO. Our proposed observations may also benefit existing Herschel ULIRG outflow studies by providing measurements for a ULIRG that will extend the current L(AGN) range by a factor of two. This study will further also be r^ant for understanding the population of deeply obscured radio galaxies found at high redshifts.
Publication
Instrument PACS_PacsRangeSpec_point
Temporal Coverage 2012-05-02T12:47:53Z/2013-01-07T10:58:08Z
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 2013-07-07T08:31:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-07-07T08:31:00Z, OT2_hspoon_1, SPG v14.2.0. https://doi.org/10.5270/esa-m2u4v2a