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        Hi-GAL, the Herschel infrared Galactic Plane Survey : photometric maps and compact source catalogues. First data release for Inner Milky Way: +68°> l > -70°

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        Author
        Molinari, 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. di
        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. Del
        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.
        Attention
        2299/17446
        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|
        Publication date
        2016-07-04
        Published in
        Astronomy & Astrophysics
        Published version
        https://doi.org/10.1051/0004-6361/201526380
        License
        http://creativecommons.org/licenses/by/4.0/
        Other links
        http://hdl.handle.net/2299/17446
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