A dataset provided by the European Space Agency

Name OT2_hdole_1
Title Herschel unveils the nature of high-z (2
URL

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DOI 10.5270/esa-fmr2ebp
Author dole, h.
Description The Planck mission has the unique capability of finding systematically and on the whole sky the rarest, most luminous high redshift submm sources. These can be lensed objects or proto-groups-clusters of galaxies containing many individual sources forming stars at very high rates. Our full sample of candidates contains about 1 source per 30 sq. deg., and already 3 candidates have been confirmed as interesting high-z sources: one was found to be a proto-group at z~3, based on a SPIRE OT1 pilot project; and 2 others are z~3-4.6 sources already found in the H-ATLAS and around A773. We now propose to use SPIRE to image a larger set of Planck sources to obtain a statistically significant sample of 70 high-z proto-groups and clusters. This will give new insights into the early evolution of galaxies in the highest density regions, improving our understanding of the relationship between the growth of structures and star-formation, and placing constraints on the level of non-Gaussianity within the LCDM model. This program exploits the exceptional synergy and complementarity between Planck and Herschel.
Publication DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands . Clark C. J. R. et al. . Astronomy & Astrophysics, Volume 609, id.A37, 30 pp. . 609 . 10.1051\/0004-6361\/201731419 . 2018A&A...609A..37C ,
Planck intermediate results. XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE . Planck Collaboration Aghanim et al. . Astronomy & Astrophysics, Volume 582, id.A30, 29 pp. . 582 . 10.1051\/0004-6361\/201424790 . 2015A&A...582A..30P ,
Dust emissivity and absorption cross section in DustPedia late-type galaxies . Bianchi S. et al. . Astronomy and Astrophysics . null . null . 2019A&A...631A.102B ,
DustPedia: the relationships between stars, gas, and dust for galaxies residing in different environments . Davies J. I. et al. . Astronomy and Astrophysics . null . null . 2019A&A...626A..63D ,
Old and young stellar populations in DustPedia galaxies and their role in dust heating . Nersesian A. et al. . Astronomy and Astrophysics . null . null . 2019A&A...624A..80N ,
Fraction of bolometric luminosity absorbed by dust in DustPedia galaxies . Bianchi S. et al. . Astronomy & Astrophysics, Volume 620, id.A112, 21 pp. . 620 . 10.1051\/0004-6361\/201833699 . 2018A&A...620A.112B ,
Dust emission profiles of DustPedia galaxies . Mosenkov A. V. et al. . Astronomy & Astrophysics, Volume 622, id.A132, 24 pp. . 622 . 10.1051\/0004-6361\/201833932 . 2019A&A...622A.132M ,
Instrument SPIRE_SpirePhoto_large
Temporal Coverage 2012-03-01T07:21:58Z/2013-01-21T03:12:58Z
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 2013-07-21T03:02:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-07-21T03:02:00Z, OT2_hdole_1, SPG v14.1.0. https://doi.org/10.5270/esa-fmr2ebp