A dataset provided by the European Space Agency

Name GT2_pandre_5
Title Completion of the Gould Belt and HOBYS surveys
URL

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DOI https://doi.org/10.5270/esa-qpz07uc
Author andre, p.
Description As demonstrated by the Herschel first highlights, both the Gould Belt and the HOBYS survey have been extremely successful. While the quality of the corresponding Herschel data is generally excellent, we have identified a few coverage or saturation problems which we intend to fix using the additional observations proposed in the present application. These observations will increase the completeness and legacy value of both surveys. We also propose a small extension to the Gould Belt parallel-mode survey of the Taurus complex in order to cover an area which shows faint .striations. in CO observations. Combined with the existing Taurus data, the proposed extension will allow us to study, within the same cloud, the properties of the whole spectrum of filamentary structures from faint, non-star forming striations to dense star-forming filaments. Likewise, we propose to slightly extend our parallel-mode survey of the Cygnus X region, the most massive and most active star-forming complex targeted by the HOBYS key project, in order to improve the completeness of our census of high-mass protostars/prestellar cores in this important target cloud.
Publication A Multi-band Catalog of 10978 Star Clusters, Associations, and Candidates in the Milky Way . Bica Eduardo et al. . The Astronomical Journal, Volume 157, Issue 1, article id. 12, 14 pp. (2019). . 157 . 10.3847\/1538-3881\/aaef8d . 2019AJ....157...12B ,
The CALYPSO IRAM-PdBI survey of jets from Class 0 protostars. Exploring whether jets are ubiquitous in young stars . Podio L. et al. . Astronomy and Astrophysics . null . null . 2021A&A...648A..45P ,
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small, SPIRE\/PACS parallel_SpirePacsParallel_, SPIRE_SpirePhoto_large
Temporal Coverage 2012-01-05T21:22:41Z/2012-10-01T15:02:23Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/h®erschel/
Date Published 2013-04-01T14:30:09Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, andre, p., 2013, GT2_pandre_5, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-qpz07uc