THE HERschel inventory of the agents of galaxy evolution in the magellanic clouds, a herschel open time key program
Author
dc.contributor.author
Meixner, M.
Author
dc.contributor.author
Panuzzo, P.
Author
dc.contributor.author
Roman Duval, Julia
Author
dc.contributor.author
Engelbracht, C.
Author
dc.contributor.author
Babler, B.
Author
dc.contributor.author
Seale, J. P.
Author
dc.contributor.author
Hony, S.
Author
dc.contributor.author
Montiel, E.
Author
dc.contributor.author
Sauvage, M.
Author
dc.contributor.author
Gordon, K.
Author
dc.contributor.author
Misselt, K.
Author
dc.contributor.author
Okumura, K.
Author
dc.contributor.author
Chanial, P.
Author
dc.contributor.author
Beck, T.
Author
dc.contributor.author
Bernard, J. P.
Author
dc.contributor.author
Bolatto, A.
Author
dc.contributor.author
Bot, C.
Author
dc.contributor.author
Boyer, M. L.
Author
dc.contributor.author
Carlson, L. R.
Author
dc.contributor.author
Clayton, G. C.
Author
dc.contributor.author
Chen, C.-H. R.
Author
dc.contributor.author
Cormier, D.
Author
dc.contributor.author
Fukui, Y.
Author
dc.contributor.author
Galametz, M.
Author
dc.contributor.author
Galliano, F.
Author
dc.contributor.author
Hora, J. L.
Author
dc.contributor.author
Hughes, A.
Author
dc.contributor.author
Indebetouw, R.
Author
dc.contributor.author
Israel, F.P.
Author
dc.contributor.author
Kawamura, A.
Author
dc.contributor.author
Kemper, F.
Author
dc.contributor.author
Kim, S.
Author
dc.contributor.author
Kwon, E.
Author
dc.contributor.author
Lebouteiller, V.
Author
dc.contributor.author
Li, A.
Author
dc.contributor.author
Long, K. S.
Author
dc.contributor.author
Madden, S. C.
Author
dc.contributor.author
Matsuura, M.
Author
dc.contributor.author
Muller, E.
Author
dc.contributor.author
Oliveira, J. M.
Author
dc.contributor.author
Onishi, T.
Author
dc.contributor.author
Otsuka, M.
Author
dc.contributor.author
Paradis, D.
Author
dc.contributor.author
Poglitsch, A.
Author
dc.contributor.author
Reach, W. T.
Author
dc.contributor.author
Robitaille, T. P.
Author
dc.contributor.author
Rubio López, Mónica
Author
dc.contributor.author
Sargent, B.
Author
dc.contributor.author
Sewiłlo, M.
Author
dc.contributor.author
Skibba, R.
Author
dc.contributor.author
Smith, L.
Author
dc.contributor.author
Srinivasan, S.
Author
dc.contributor.author
Tielens, A.
Author
dc.contributor.author
van Loon, J. Th.
Author
dc.contributor.author
Whitney, B.
Admission date
dc.date.accessioned
2015-06-16T19:33:59Z
Available date
dc.date.available
2015-06-16T19:33:59Z
Publication date
dc.date.issued
2013
Cita de ítem
dc.identifier.citation
The Astronomical Journal, 146:62 (35pp), 2013 September
en_US
Identifier
dc.identifier.other
doi:10.1088/0004-6256/146/3/62
Identifier
dc.identifier.uri
https://repositorio.uchile.cl/handle/2250/131150
General note
dc.description
Artículo de publicación ISI
en_US
Abstract
dc.description.abstract
We present an overview of the HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE) in the
Magellanic Clouds project, which is a Herschel Space Observatory open time key program. We mapped the Large
Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) at 100, 160, 250, 350, and 500μm with the Spectral
and Photometric Imaging Receiver (SPIRE) and Photodetector Array Camera and Spectrometer (PACS) instruments
on board Herschel using the SPIRE/PACS parallel mode. The overriding science goal of HERITAGE is to study
the life cycle of matter as traced by dust in the LMC and SMC. The far-infrared and submillimeter emission is an
effective tracer of the interstellar medium (ISM) dust, the most deeply embedded young stellar objects (YSOs), and
the dust ejected by the most massive stars. We describe in detail the data processing, particularly for the PACS data,
which required some custom steps because of the large angular extent of a single observational unit and overall
the large amount of data to be processed as an ensemble. We report total global fluxes for the LMC and SMC and
demonstrate their agreement with measurements by prior missions. The HERITAGE maps of the LMC and SMC
are dominated by the ISM dust emission and bear most resemblance to the tracers of ISM gas rather than the stellar
content of the galaxies. We describe the point source extraction processing and the criteria used to establish a catalog
for each waveband for the HERITAGE program. The 250μm band is the most sensitive and the source catalogs
for this band have ∼25,000 objects for the LMC and ∼5500 objects for the SMC. These data enable studies of
ISM dust properties, submillimeter excess dust emission, dust-to-gas ratio, Class 0 YSO candidates, dusty massive
evolved stars, supernova remnants (including SN1987A), H ii regions, and dust evolution in the LMC and SMC.
All images and catalogs are delivered to the Herschel Science Center as part of the community support aspects of the project. These HERITAGE images and catalogs provide an excellent basis for future research and follow up
with other facilities.