A dataset provided by the European Space Agency

Name GT2_mviero_1


DOI https://doi.org/10.5270/esa-j7eq1h3
Author viero, m.
Description We propose a unique addition to the HerMES family of maps, the HerMES Large Mode Survey (HeLMS), which will be observed as part of the remaining SPIRE GT time. The field covers 270 deg2 with two repeats over roughly 106 hours. It is chosen to overlap the SDSS Stripe 82 in a region where the Galactic cirrus with a mean flux density of 1.2 MJy sr1 is at its lowest. The ancillary coverage in this field is extensive, particularly in the optical, making it an attractive large field. The scientific advantages of having a field with the size and makeup of HeLMS are twofold: first, the large survey area, of which 55 deg2 overlaps Stripe 82, will allow us to resolve approximately 250, 000 sources, of which 250 500 will be gravitationally lensed. Second, the large, uniform and cross-linked area will allow for unprecedented measurement of large-scale modes (down to l 150). Such fidelity would be a unique asset in the submillimeter regime for the foreseeable future, and would enable cross-frequency correlation analysis with 80 deg2 of deep ACT maps, Planck over the full 270 deg2, as well as future observations with upcoming instruments like ALMA, ACTpol, and others.
Publication HerMES: a search for high-redshift dusty galaxies in the HerMES Large Mode Survey - catalogue, number counts and early results . Asboth V. et al. . Monthly Notices of the Royal Astronomical Society, Volume 462, Issue 2, p.1989-2000 . 462 . 10.1093\/mnras\/stw1769 . 2016MNRAS.462.1989A ,
The faint end of the 250 ?m luminosity function at z < 0.5 . Wang L. et al. . Astronomy & Astrophysics, Volume 592, id.L5, 6 pp. . 592 . 10.1051\/0004-6361\/201629076 . 2016A&A...592L...5W ,
The impact of clustering and angular resolution on far-infrared and millimeter continuum observations . B?thermin Matthieu et al. . Astronomy & Astrophysics, Volume 607, id.A89, 22 pp. . 607 . 10.1051\/0004-6361\/201730866 . 2017A&A...607A..89B ,
Co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background . Wang Lingyu et al. . Monthly Notices of the Royal Astronomical Society, Volume 449, Issue 4, p.4476-4493 . 449 . 10.1093\/mnras\/stv559 . 2015MNRAS.449.4476W ,
Far-infrared dust properties of highly dust-obscured active galactic nuclei from the AKARI and WISE all-sky surveys . Lam Anson et al. . Publications of the Astronomical Society of Japan, Volume 71, Issue 1, id.9 . 71 . 10.1093\/pasj\/psy081 . 2019PASJ...71....9L ,
Dust emissivity and absorption cross section in DustPedia late-type galaxies . Bianchi S. et al. . Astronomy and Astrophysics . null . null . 2019A&A...631A.102B ,
Extreme star formation events in quasar hosts over 0.5 < z < 4 . Pitchford L. K. ...
Instrument SPIRE_SpirePhoto_large
Temporal Coverage 2011-12-19T01:25:54Z/2012-12-17T22:21:33Z
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 2013-06-17T19:03:03Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-06-17T19:03:03Z, GT2_mviero_1, SPG v14.1.0. https://doi.org/10.5270/esa-j7eq1h3