A dataset provided by the European Space Agency

Name DDT_ebergin_9
Title DDT request to observe the Herschel/HIFI ULine in the Orion Bar and W49
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342244038&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342244039&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342244402&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342244403&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342244404&instrument_name=HIFI&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-yrili9k
Author bergin, e.
Description One of the key science goals of the HIFI instrument on Herschel has beenthe ability to quickly perform unbiased spectral line surveys. Thehoped-for outcome, besides the analysis of known molecules throughmultiple lines, has been the detection of previously unknown species. Andindeed, a number of unidentified lines have been found, both inemission and in absorption. The most spectacular, but also mostpuzzling of these is the 617 GHz absorption line feature first foundtoward Sgr~B2 and now seen in absorption towards other galactic sources.It is the only U-line found that does not trace the core or envelope ofSgr~B2, but rather the gas in the line-of-sight clouds in the spiral arms and Galactic center, between us and Sgr~B2. At present there is no knowncarrier for this feature.We request DDT observing time to improve a potential detection of this linein emission towards one galactic source and another source withnarrow absorption lines. If the detection is confirmed the narrowlines of these sources will enable a search for hyperfine structure whichcan be used to narrow the search for molecular carriers.
Publication
    Instrument HIFI_HifiPoint_dbs
    Temporal Coverage 2012-04-10T04:12:47Z/2012-04-14T15:54:32Z
    Version SPG v14.1.0
    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 2012-10-14T15:52:34Z
    Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
    Publisher And Registrant European Space Agency
    Credit Guidelines European Space Agency, bergin et al., 2012, 'DDT request to observe the Herschel/HIFI ULine in the Orion Bar and W49', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-yrili9k