A dataset provided by the European Space Agency

Name KPOT_seales01_2
Title The Herschel Thousand Degree Survey
URL

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DOI https://doi.org/10.5270/esa-mchmz73
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 virgul100,000 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 (virgul1000), 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, UKI...RT, SPT and the SKA-precusor telescopes, KAT, ASKAP and LOFAR, and so the survey will be of immense legacy value.
Publication A Herschel-ATLAS study of dusty spheroids: probing the minor-merger process in the local Universe . Kaviraj S. et al. . Monthly Notices of the Royal Astronomical Society, Volume 435, Issue 2, p.1463-1468 . 435 . 10.1093/mnras/stt1629 . 2013MNRAS.435.1463K ,
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 ,
The non-linear infrared-radio correlation of low-z galaxies: implications for redshift evolution, a new radio SFR recipe, and how to minimize selection bias . Molnár Dániel Cs et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2021MNRAS.504..118M ,
The unusual ISM in blue and dusty gas-rich galaxies (BADGRS) . Dunne L. et al. . Monthly Notices of the Royal Astronomical Society, Volume 479, Issue 1, p.1221-1239 . 479 . 10.1093/mnras/sty1465 . 2018MNRAS.479.1221D ,
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 ,
Candidate high-redshift protoclusters and lensed galaxies in the Planck list of high-z sources overlapping with Herschel-SPIRE imaging . Lammers Caleb et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2022MNRAS.514.5004L ,
DustPed...
Instrument SPIRE/PACS parallel_SpirePacsParallel_
Temporal Coverage 2010-01-24T23:12:16Z/2012-05-20T15:20:10Z
Version SPG v14.2.1
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 2012-11-20T13:47:19Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012, KPOT_seales01_2, SPG v14.2.1. https://doi.org/10.5270/esa-mchmz73