A dataset provided by the European Space Agency

Name OT2_baltieri_5
Title Star formation in proto-clusters
URL

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DOI 10.5270/esa-ncafgao
Author altieri, b.
Description Massive clusters of galaxies have been found to date from as early as 3-4 billion years after the Big Bang. Cosmological simulations using the current cold dark matter model predict that these systems should descend from .proto-clusters. - early overdensities of massive galaxies that merge hierarchically to form a cluster. These protocluster regions themselves are built up hierarchically and so are expected to contain extremely massive galaxies, progenitors of the quiescent behemoths observed in cores of the present day massive galaxy clusters. Observational evidence for this picture, however, is sparse because high-redshift proto-clusters are rare and difficult to observe. Here we propose to probe with Herschel SPIRE the very beginning of the cluster and massive galaxies formation process by observing 5 proto-clusters at 3
Publication
Instrument SPIRE_SpirePhoto_large
Temporal Coverage 2012-02-29T23:47:23Z/2012-10-01T10:02:08Z
Version SPG v14.1.0
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-04-01T09:53:19Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-04-01T09:53:19Z, OT2_baltieri_5, SPG v14.1.0. https://doi.org/10.5270/esa-ncafgao