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dc.contributor.authorMolinari, S.
dc.contributor.authorSchisano, E.
dc.contributor.authorElia, D.
dc.contributor.authorPestalozzi, M.
dc.contributor.authorTraficante, A.
dc.contributor.authorPezzuto, S.
dc.contributor.authorSwinyard, B. M.
dc.contributor.authorNoriega-Crespo, A.
dc.contributor.authorBally, J.
dc.contributor.authorMoore, T. J. T.
dc.contributor.authorPlume, R.
dc.contributor.authorZavagno, A.
dc.contributor.authorGiorgio, A. M. di
dc.contributor.authorLiu, S. J.
dc.contributor.authorPilbratt, G. L.
dc.contributor.authorMottram, J. C.
dc.contributor.authorRusseil, D.
dc.contributor.authorPiazzo, L.
dc.contributor.authorVeneziani, M.
dc.contributor.authorBenedettini, M.
dc.contributor.authorCalzoletti, L.
dc.contributor.authorFaustini, F.
dc.contributor.authorNatoli, P.
dc.contributor.authorPiacentini, F.
dc.contributor.authorMerello, M.
dc.contributor.authorPalmese, A.
dc.contributor.authorGrande, R. Del
dc.contributor.authorPolychroni, D.
dc.contributor.authorRygl, K. L. J.
dc.contributor.authorPolenta, G.
dc.contributor.authorBarlow, M. J.
dc.contributor.authorBernard, J. -P.
dc.contributor.authorMartin, P. G.
dc.contributor.authorTesti, L.
dc.contributor.authorAli, B.
dc.contributor.authorAndrè, P.
dc.contributor.authorBeltrán, M. T.
dc.contributor.authorBillot, N.
dc.contributor.authorBrunt, C.
dc.contributor.authorCarey, S.
dc.contributor.authorCesaroni, R.
dc.contributor.authorCompiègne, M.
dc.contributor.authorEden, D.
dc.contributor.authorFukui, Y.
dc.contributor.authorGarcia-Lario, P.
dc.contributor.authorHoare, M. G.
dc.contributor.authorHuang, M.
dc.contributor.authorJoncas, G.
dc.contributor.authorLim, T. L.
dc.contributor.authorLord, S. D.
dc.contributor.authorMartinavarro-Armengol, S.
dc.contributor.authorMotte, F.
dc.contributor.authorPaladini, R.
dc.contributor.authorParadis, D.
dc.contributor.authorPeretto, N.
dc.contributor.authorRobitaille, T.
dc.contributor.authorSchilke, P.
dc.contributor.authorSchneider, N.
dc.contributor.authorSchulz, B.
dc.contributor.authorSibthorpe, B.
dc.contributor.authorStrafella, F.
dc.contributor.authorThompson, M. A.
dc.contributor.authorUmana, G.
dc.contributor.authorWard-Thompson, D.
dc.contributor.authorWyrowski, F.
dc.date.accessioned2016-12-19T11:41:32Z
dc.date.available2016-12-19T11:41:32Z
dc.date.issued2016-07-04
dc.identifier.citationMolinari , S , Schisano , E , Elia , D , Pestalozzi , M , Traficante , A , Pezzuto , S , Swinyard , B M , Noriega-Crespo , A , Bally , J , Moore , T J T , Plume , R , Zavagno , A , Giorgio , A M D , Liu , S J , Pilbratt , G L , Mottram , J C , Russeil , D , Piazzo , L , Veneziani , M , Benedettini , M , Calzoletti , L , Faustini , F , Natoli , P , Piacentini , F , Merello , M , Palmese , A , Grande , R D , Polychroni , D , Rygl , K L J , Polenta , G , Barlow , M J , Bernard , J -P , Martin , P G , Testi , L , Ali , B , Andrè , P , Beltrán , M T , Billot , N , Brunt , C , Carey , S , Cesaroni , R , Compiègne , M , Eden , D , Fukui , Y , Garcia-Lario , P , Hoare , M G , Huang , M , Joncas , G , Lim , T L , Lord , S D , Martinavarro-Armengol , S , Motte , F , Paladini , R , Paradis , D , Peretto , N , Robitaille , T , Schilke , P , Schneider , N , Schulz , B , Sibthorpe , B , Strafella , F , Thompson , M A , Umana , G , Ward-Thompson , D & Wyrowski , F 2016 , ' Hi-GAL, the Herschel infrared Galactic Plane Survey : photometric maps and compact source catalogues. First data release for Inner Milky Way: +68° > l > -70° ' , Astronomy & Astrophysics , vol. 591 , A149 . https://doi.org/10.1051/0004-6361/201526380
dc.identifier.issn0004-6361
dc.identifier.otherArXiv: http://arxiv.org/abs/1604.05911v1
dc.identifier.otherORCID: /0000-0001-5392-909X/work/30970772
dc.identifier.urihttp://hdl.handle.net/2299/17446
dc.descriptionReproduced with permission from Astronomy & Astrophysics, © ESO
dc.description.abstract(Abridged) We present the first public release of high-quality data products (DR1) from Hi-GAL, the {\em Herschel} infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite of continuum Galactic Plane surveys from the near-IR to the radio, and covers five wavebands at 70, 160, 250, 350 and 500 micron, encompassing the peak of the spectral energy distribution of cold dust for 8 l > -70{\deg} in a |b|en
dc.format.extent33
dc.format.extent7916234
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.subjectastro-ph.GA
dc.titleHi-GAL, the Herschel infrared Galactic Plane Survey : photometric maps and compact source catalogues. First data release for Inner Milky Way: +68°> l > -70°en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1051/0004-6361/201526380
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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