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
    Last Update 2026-03-02
    Keywords Herschel Space Observatory data, ESA Herschel mission dataset, far-infrared astronomy observations, submillimeter astronomy data, infrared space telescope observations, PACS photometer data, PACS spectrometer data, SPIRE photometer data, SPIRE Fourier transform spectrometer data, HIFI heterodyne spectroscopy data, far-infrared spectroscopy dataset, submillimeter spectral line observations, cold universe observations dataset, star formation infrared data, molecular cloud far-infrared observations, interstellar medium spectroscopy data, protoplanetary disk infrared observations, galaxy evolution far-infrared data, dust emission submillimeter observations, cosmic infrared background measurements, extragalactic infrared survey data, calibrated level 2 data products, FITS files astronomy, spectral cubes far-infrared, flux-calibrated maps, continuum photometry data, spectral energy distribution measurements, ESA Herschel Science Archive data
    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