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 European Space Agency
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 larg...e fields
in the sky and will be the targets of future surveys with VISTA,
VST, UKIRT, 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 ,
D...
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, The Herschel Thousand Degree Survey, SPG v14.2.1, European Space Agency, https://doi.org/10.5270/esa-mchmz73