A dataset provided by the European Space Agency

Name DDT_dbockele_3
Title Origin of water outgassing from asteroid CERES
URL

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http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342270856&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI 10.5270/esa-gbhf3zm
Author bockelee-morvan, d.
Description Herschel observations of the large asteroid Ceres led to a major discovery, namely the first detection of an exosphere made of water vapour around an asteroid. The first detection occurred on 11 October, 2012, and was confirmed from HIFI observations conducted on 24th October and 6 March 2013 (guaranteed time program MACH 11, PI L. O.Rourke, and follow up from a DDT, PI M. Kueppers).
Publication Herschel celestial calibration sources. Four large main-belt asteroids as prime flux calibrators for the far-IR-sub-mm range . Müller Thomas et al. . Experimental Astronomy, Volume 37, Issue 2, pp.253-330 . 37 . 10.1007\/s10686-013-9357-y . 2014ExA....37..253M ,
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2013-04-23T17:41:19Z/2013-04-24T05:16:34Z
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/herschel/
Date Published 2013-10-24T05:11:48Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-10-24T05:11:48Z, DDT_dbockele_3, SPG v14.2.0. https://doi.org/10.5270/esa-gbhf3zm