A dataset provided by the European Space Agency

Name SDP_seales01_6
Title The Herschel Thousand Degree Survey

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187170&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187171&instrument_name=SPIRE\/PACS parallel&product_level=LEVEL0&compress=true

DOI 10.5270/esa-eeyfzcm
Author eales, s.
Description We still know little about dust in the nearby universe, because IRAS was only sensitive to the 10% of dust warm enough to radiate in the far-IR, and submm surveys have not covered enough area to sample a representative volume of the local universe. We propose to use Herschel to survery 1000 square degrees in five bands. The survey will detect ~100,000 galaxies at z <0.3, and we will use the results in six key projects: (1) By using the the SDSS and 2dFGRS redshifts that will exist for half the galaxies, we will carry out an unprecedented study of dust and dust-obscured star formation in the nearby universe, determining for example how these depend on Hubble type, metallicity and environment. We will also measure the submm luminosity function, a key benchmark for galaxy evolution models, and test .down-sizing.models by investigating the cosmic evolution that is known to have occurred over the last 3 billion years. (2) We will detemine the relative contributions of the SZ effect and dusty galaxies in Planck sources, which will make it possible to measure the number-density and bulk flows of clusters in the high-z universe - two fundamental tests of the cosmological paradigm. (3) Using the largest ever sample of gravitational lenses (~1000), we will investigate the evolution of the mass profiles of galaxies, another key test of cosmological models. (4) We will investigate the relationship between the formation of the black holes and stars in quasars by observing the 20,000 SDSS quasars in our fields. (5) By measuring the structure of the submm sky up to a scale of 1000 Mpc, we will estimate the masses of the dark-matter halos containing the far-IR-submm sources. (6) We will carry out the first census of dust and protostars at high galactic latitudes. Our fields are the best-studied large fields in the sky and will be the targets of future surveys with VISTA, VST, UKIRT, SPT and the SKA-precu...
Publication VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35 . Villanueva V. et al. . Monthly Notices of the Royal Astronomical Society, Volume 470, Issue 4, p.3775-3805 . 470 . 10.1093\/mnras\/stx1338 . 2017MNRAS.470.3775V ,
Herschel-ATLAS: the link between accretion luminosity and star formation in quasar host galaxies . Bonfield D. G. et al. . Monthly Notices of the Royal Astronomical Society, Volume 416, Issue 1, pp. 13-21. . 416 . 10.1111\/j.1365-2966.2011.18826.x . 2011MNRAS.416...13B ,
Herschel-ATLAS: The angular correlation function of submillimetre galaxies at high and low redshift . Maddox S. J. et al. . Astronomy and Astrophysics, Volume 518, id.L11, 5 pp. . 518 . 10.1051\/0004-6361\/201014663 . 2010A&A...518L..11M ,
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 ,
A unified multiwavelength model of galaxy formation . Lacey Cedric G. et al. . Monthly Notices of the Royal Astronomical Society, Volume 462, Issue 4, p.3854-3911 . 462 . 10.1093\/mnras\/stw1888 . 2016MNRAS.462.3854L ,
DustPedia: A Definitive Study of Cosmic Dust in the Local Universe . Davies J. I. et al. . Publications of the Astronomical Society of the Pacific, Volume 129, Issue 974, pp. 044102 (2017). . 129 . 10.1088\/1538-3873\/129\/974\/044102 . 2017PASP..129d4102D ,
Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours...
Instrument SPIRE\/PACS parallel_SpirePacsParallel_
Temporal Coverage 2009-11-22T00:30:39Z/2009-11-22T16:28:19Z
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/herschel/
Date Published 2010-11-22T08:27:48Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-11-22T08:27:48Z, SDP_seales01_6, SPG v14.2.0. https://doi.org/10.5270/esa-eeyfzcm