BELLOCHE, A.; SCHULLER, F.; PARISE, B.; ANDRE, P.; HATCHELL, J.; JORGENSEN, J. K.; BONTEMPS, Sylvain; WEISS, A.; MENTEN, K. M.; MUDERS, D.

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Licence d’utilisation du document

BELLOCHE, A.
Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée [DAPNIA]

SCHULLER, F.
Max-Planck-Institut für Radioastronomie [MPIFR]

PARISE, B.
Centre d'étude spatiale des rayonnements [CESR]

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Autre document

Ce document a été publié dans

2011-01p. 79145

Résumé en anglais

Table 2 lists the sources extracted with GAUSSCLUMPS from the filtered 870 micron continuum emission map of Chamaeleon I obtained with the bolometer camera LABOCA at the APEX telescope. These sources are listed in the order in which they were found by GAUSSCLUMPS, i.e. roughly in order of decreasing peak flux density. The 870 micron dust continuum emission map of the Chamaeleon I molecular cloud is available in FITS format. The data were obtained with the bolometer camera LABOCA at the APEX telescope. They were calibrated, reduced, co-added, gridded, smoothed to an effective angular resolution of 21.2" (FWHM), and written in FITS format with the BoA software. The flux density unit is Jy/21.2"-beam. The coordinates are equatorial (J2000) and the offsets are in RADIO projection. (2 data files).< Réduire

Mots clés en anglais

Molecular clouds

Millimetric/submm sources

Origine

Importé de hal

Unités de recherche

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804