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Article: Highlights from the first year of Odin observations

TitleHighlights from the first year of Odin observations
Authors
KeywordsIsm: Molecules
Radio Lines: Ism
Space Vehicles: Instruments
Submillimeter
Techniques: Spectroscopic
Telescopes
Issue Date2003
PublisherE D P Sciences. The Journal's web site is located at http://www.aanda.org
Citation
Astronomy And Astrophysics, 2003, v. 402 n. 3, p. L39-L46 How to Cite?
AbstractKey Odin operational and instrumental features and highlights from our sub-millimetre and millimetre wave observations of H 2O, H 2 18O, NH 3, 15NH 3 and O 2 are presented, with some insights into accompanying Odin Letters in this A&A issue. We focus on new results where Odin's high angular resolution, high frequency resolution, large spectrometer bandwidths, high sensitivity or/and frequency tuning capability are crucial: H 2O mapping of the Orion KL, W3, DR 21, S 140 regions, and four comets; H 2O observations of Galactic Centre sources, of shock enhanced H 2O towards the SNR IC 443, and of the candidate infall source IRAS 16293-2422; H 2 18O detections in Orion KL and in comet Ikeya-Zhang; sub-mm detections of NH 3 in Orion KL (outflow, ambient cloud and bar) and ρ Oph, and very recently, of 15NH 3 in Orion KL. Simultaneous sensitive searches for the 119 GHz line of O 2 have resulted in very low abundance limits, which are difficult to accommodate in chemical models. We also demonstrate, by means of a quantitative comparison of Orion KL H 2O results, that the Odin and SWAS observational data sets are very consistently calibrated.
Persistent Identifierhttp://hdl.handle.net/10722/179666
ISSN
2014 Impact Factor: 4.378
2015 SCImago Journal Rankings: 2.446
References

 

DC FieldValueLanguage
dc.contributor.authorHjalmarson, Åen_US
dc.contributor.authorFrisk, Uen_US
dc.contributor.authorOlberg, Men_US
dc.contributor.authorBergman, Pen_US
dc.contributor.authorBernath, Pen_US
dc.contributor.authorBiver, Nen_US
dc.contributor.authorBlack, JHen_US
dc.contributor.authorBooth, RSen_US
dc.contributor.authorBuat, Ven_US
dc.contributor.authorCrovisier, Jen_US
dc.contributor.authorCurry, CLen_US
dc.contributor.authorDahlgren, Men_US
dc.contributor.authorEncrenaz, PJen_US
dc.contributor.authorFalgarone, Een_US
dc.contributor.authorFeldman, PAen_US
dc.contributor.authorFich, Men_US
dc.contributor.authorFlorén, HGen_US
dc.contributor.authorFredrixon, Men_US
dc.contributor.authorGerin, Men_US
dc.contributor.authorGregersen, EMen_US
dc.contributor.authorHagström, Men_US
dc.contributor.authorHarju, Jen_US
dc.contributor.authorHasegawa, Ten_US
dc.contributor.authorHorellou, Cen_US
dc.contributor.authorJohansson, LEBen_US
dc.contributor.authorKyrölä, Een_US
dc.contributor.authorKwok, Sen_US
dc.contributor.authorLarsson, Ben_US
dc.contributor.authorLecacheux, Aen_US
dc.contributor.authorLiljeström, Ten_US
dc.contributor.authorLindqvist, Men_US
dc.contributor.authorLiseau, Ren_US
dc.contributor.authorLlewellyn, EJen_US
dc.contributor.authorMattila, Ken_US
dc.contributor.authorMégie, Gen_US
dc.contributor.authorMitchell, GFen_US
dc.contributor.authorMurtagh, Den_US
dc.contributor.authorNyman, LÅen_US
dc.contributor.authorNordh, HLen_US
dc.contributor.authorOlofsson, AOHen_US
dc.contributor.authorOlofsson, Gen_US
dc.contributor.authorOlofsson, Hen_US
dc.contributor.authorPagani, Len_US
dc.contributor.authorPersson, Gen_US
dc.contributor.authorPlume, Ren_US
dc.contributor.authorRickman, Hen_US
dc.contributor.authorRistorcelli, Ien_US
dc.contributor.authorRydbeck, Gen_US
dc.contributor.authorSandqvist, Aaen_US
dc.contributor.authorVon Schéele, Fen_US
dc.contributor.authorSerra, Gen_US
dc.contributor.authorTorchinsky, Sen_US
dc.contributor.authorTothill, NFen_US
dc.contributor.authorVolk, Ken_US
dc.contributor.authorWiklind, Ten_US
dc.contributor.authorWilson, CDen_US
dc.contributor.authorWinnberg, Aen_US
dc.contributor.authorWitt, Gen_US
dc.date.accessioned2012-12-19T10:02:40Z-
dc.date.available2012-12-19T10:02:40Z-
dc.date.issued2003en_US
dc.identifier.citationAstronomy And Astrophysics, 2003, v. 402 n. 3, p. L39-L46en_US
dc.identifier.issn0004-6361en_US
dc.identifier.urihttp://hdl.handle.net/10722/179666-
dc.description.abstractKey Odin operational and instrumental features and highlights from our sub-millimetre and millimetre wave observations of H 2O, H 2 18O, NH 3, 15NH 3 and O 2 are presented, with some insights into accompanying Odin Letters in this A&A issue. We focus on new results where Odin's high angular resolution, high frequency resolution, large spectrometer bandwidths, high sensitivity or/and frequency tuning capability are crucial: H 2O mapping of the Orion KL, W3, DR 21, S 140 regions, and four comets; H 2O observations of Galactic Centre sources, of shock enhanced H 2O towards the SNR IC 443, and of the candidate infall source IRAS 16293-2422; H 2 18O detections in Orion KL and in comet Ikeya-Zhang; sub-mm detections of NH 3 in Orion KL (outflow, ambient cloud and bar) and ρ Oph, and very recently, of 15NH 3 in Orion KL. Simultaneous sensitive searches for the 119 GHz line of O 2 have resulted in very low abundance limits, which are difficult to accommodate in chemical models. We also demonstrate, by means of a quantitative comparison of Orion KL H 2O results, that the Odin and SWAS observational data sets are very consistently calibrated.en_US
dc.languageengen_US
dc.publisherE D P Sciences. The Journal's web site is located at http://www.aanda.orgen_US
dc.relation.ispartofAstronomy and Astrophysicsen_US
dc.subjectIsm: Moleculesen_US
dc.subjectRadio Lines: Ismen_US
dc.subjectSpace Vehicles: Instrumentsen_US
dc.subjectSubmillimeteren_US
dc.subjectTechniques: Spectroscopicen_US
dc.subjectTelescopesen_US
dc.titleHighlights from the first year of Odin observationsen_US
dc.typeArticleen_US
dc.identifier.emailKwok, S: deannote@hku.hken_US
dc.identifier.authorityKwok, S=rp00716en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.scopuseid_2-s2.0-0038363355en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0038363355&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume402en_US
dc.identifier.issue3en_US
dc.identifier.spageL39en_US
dc.identifier.epageL46en_US
dc.publisher.placeFranceen_US
dc.identifier.scopusauthoridHjalmarson, Å=15744175200en_US
dc.identifier.scopusauthoridFrisk, U=8966521600en_US
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dc.identifier.scopusauthoridBooth, RS=7202614585en_US
dc.identifier.scopusauthoridBuat, V=7003733332en_US
dc.identifier.scopusauthoridCrovisier, J=35448565400en_US
dc.identifier.scopusauthoridCurry, CL=7101672097en_US
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dc.identifier.scopusauthoridEncrenaz, PJ=6603978312en_US
dc.identifier.scopusauthoridFalgarone, E=7003349192en_US
dc.identifier.scopusauthoridFeldman, PA=7103377526en_US
dc.identifier.scopusauthoridFich, M=7003964696en_US
dc.identifier.scopusauthoridFlorén, HG=6602447564en_US
dc.identifier.scopusauthoridFredrixon, M=6507543564en_US
dc.identifier.scopusauthoridGerin, M=7005195915en_US
dc.identifier.scopusauthoridGregersen, EM=7005825957en_US
dc.identifier.scopusauthoridHagström, M=6603823220en_US
dc.identifier.scopusauthoridHarju, J=8908583000en_US
dc.identifier.scopusauthoridHasegawa, T=7404173711en_US
dc.identifier.scopusauthoridHorellou, C=6602105371en_US
dc.identifier.scopusauthoridJohansson, LEB=7401510283en_US
dc.identifier.scopusauthoridKyrölä, E=35375397400en_US
dc.identifier.scopusauthoridKwok, S=22980498300en_US
dc.identifier.scopusauthoridLarsson, B=7202678664en_US
dc.identifier.scopusauthoridLecacheux, A=7003423533en_US
dc.identifier.scopusauthoridLiljeström, T=6602325021en_US
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dc.identifier.scopusauthoridLiseau, R=6701345678en_US
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