A dataset provided by the European Space Agency

Name SDP_seales01_4
Title The Herschel Reference Survey


DOI https://doi.org/10.5270/esa-3crzmcm
Author European Space Agency
Description Despite IRAS, ISO and Spitzer, there is still much we do know about
dust in galaxies, partly because of sensitivity limitations and partly
because previous telescopes were insensitive to dust colder than about
15 K. Our knowledge is especially poor for ellipticals which have barely
been detected by previous telescopes. As part of the SPIRE GT programme,
we propose to obtain images at 250, 350 and 520 microns of a sample of
323 galaxies selected to be useful both for studying the dust in individual
galaxies and for drawing statistical conclusions about the role of dust in
galaxies in general. The Herschel Reference Survey will be the first survey
sensitive to all the dust in galaxies and which will detect dust in galaxies of all
Hubble types. Apart from its legacy value, we intend to use the survey for
the following projects: 1) We will make a comprehensive study of dust
along the Hubble sequence, investigating how the dust mass varies with
Hubble type. mass of stars, current star formation rate, past star formation
rate, and the masses of molecular and atomic gas. 2) We will investigate
within individual galaxies the connections between the star formation
rate and the different phases of the ISM, from the nucleus to the HI outside
the optical disk. 3) We will investigate how the mass and distribution of
dust depend on a galaxy.s environment. 4) We will investigate whether
there is an intergalactic dust cycle by looking for dusty halos, dusty
superwinds and tidally-stripped dust around galaxies. 5) We will
investigate the origin of dust in ellipticals, and the evolution
of the galaxies themselves, by looking for dust disks and dust shells
and by looking for correlations between the mass and distribution
of the dust and the other properties of the galaxy. 6) We will measure
the local luminosity and dust-mass functions, which will... be necessary to
interpret the results of the deep surveys, another part of the
proposed GT programme. The total time required for the survey is
112.6 hours.
Publication Far-infrared and dust properties of present-day galaxies in the EAGLE simulations . Camps Peter et al. . Monthly Notices of the Royal Astronomical Society, Volume 462, Issue 1, p.1057-1075 . 462 . 10.1093\/mnras\/stw1735 . 2016MNRAS.462.1057C ,
Investigating the growing population of massive quiescent galaxies at cosmic noon . Sherman Sydney et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2020MNRAS.499.4239S ,
Using dust, gas and stellar mass-selected samples to probe dust sources and sinks in low-metallicity galaxies . De Vis P. et al. . Monthly Notices of the Royal Astronomical Society, Volume 471, Issue 2, p.1743-1765 . 471 . 10.1093\/mnras\/stx981 . 2017MNRAS.471.1743D ,
Submillimetre photometry of 323 nearby galaxies from the Herschel Reference Survey . Ciesla L. et al. . Astronomy & Astrophysics, Volume 543, id.A161, 95 pp. . 543 . 10.1051\/0004-6361\/201219216 . 2012A&A...543A.161C ,
Far-reaching dust distribution in galaxy discs . Smith Matthew W. L. et al. . Monthly Notices of the Royal Astronomical Society, Volume 462, Issue 1, p.331-344 . 462 . 10.1093\/mnras\/stw1611 . 2016MNRAS.462..331S ,
Scaling relations and baryonic cycling in local star-forming galaxies. I. The sample . Ginolfi M. et al. . Astronomy and Astrophysics . null . null . 2020A&A...638A...4G ,
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 ,
The high-redshift SFR-M* relation is sensitive to the employed ...
Instrument SPIRE_SpirePhoto_large
Temporal Coverage 2009-10-06T21:23:14Z/2009-11-30T03:30:13Z
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 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/h®erschel/
Date Published 2010-11-30T01:49:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010, The Herschel Reference Survey, SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-3crzmcm