A dataset provided by the European Space Agency

Name SDP_seales01_4
Title The Herschel Reference Survey
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342185539&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342186862&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187173&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187185&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187263&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187322&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187323&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187324&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187325&instrument_name=SPIRE&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-3crzmcm
Author eales, s.
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 barelybeen 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 individualgalaxies and for drawing statistical conclusions about the role of dust in galaxies in general. The Herschel Reference Survey will be the first surveysensitive 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 forthe following projects: 1) We will make a comprehensive study of dust along the Hubble sequence, investigating how the dust mass varies withHubble type. mass of stars, current star formation rate, past star formationrate, 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 outsidethe 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 distributionof the dust and the other properties of the galaxy. 6) We will measurethe local luminosity and dust-mass functions, which will be necessary to interpret the results of the deep surveys, another part of theproposed 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 | http://adsabs.harvard.edu/abs/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 | http://adsabs.harvard.edu/abs/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 | http://adsabs.harvard.edu/abs/2012A%26A...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 | http://adsabs.harvard.edu/abs/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 star formation rate and stellar mass indicators: towards addressing the tension between observations and simulations | Katsianis A. et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2020MNRAS.492.5592K |
  • 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 |
  • The bolometric and UV attenuation in normal spiral galaxies of the Herschel Reference Survey | Viaene S. et al. | Astronomy & Astrophysics Volume 586 id.A13 13 pp. | 586 | 10.1051\\/0004-6361\\/201527586 | 2016A&A...586A..13V | http://adsabs.harvard.edu/abs/2016A%26A...586A..13V
  • Lurking systematics in predicting galaxy cold gas masses using dust luminosities and star formation rates | Janowiecki Steven et al. | Monthly Notices of the Royal Astronomical Society Volume 476 Issue 1 p.1390-1404 | 476 | 10.1093\\/mnras\\/sty242 | 2018MNRAS.476.1390J | http://adsabs.harvard.edu/abs/2018MNRAS.476.1390J
  • The Galaxy End Sequence | Eales Stephen et al. | Monthly Notices of the Royal Astronomical Society Volume 465 Issue 3 p.3125-3133 | 465 | 10.1093\\/mnras\\/stw2875 | 2017MNRAS.465.3125E | http://adsabs.harvard.edu/abs/2017MNRAS.465.3125E
  • Dust spectral energy distributions of nearby galaxies: an insight from the Herschel Reference Survey | Ciesla L. et al. | Astronomy & Astrophysics Volume 565 id.A128 33 pp. | 565 | 10.1051\\/0004-6361\\/201323248 | 2014A&A...565A.128C | http://adsabs.harvard.edu/abs/2014A%26A...565A.128C
  • Global Star Formation Rates and Dust Emission over the Galaxy Interaction Sequence | Lanz Lauranne et al. | The Astrophysical Journal Volume 768 Issue 1 article id. 90 33 pp. (2013). | 768 | 10.1088\\/0004-637X\\/768\\/1\\/90 | 2013ApJ...768...90L | http://adsabs.harvard.edu/abs/2013ApJ...768...90L
  • 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 | http://adsabs.harvard.edu/abs/2017PASP..129d4102D
  • The ISM scaling relations in DustPedia late-type galaxies: A benchmark study for the Local Universe | Casasola V. et al. | Astronomy and Astrophysics | null | null | 2020A&A...633A.100C |
  • DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands | Clark C. J. R. et al. | Astronomy & Astrophysics Volume 609 id.A37 30 pp. | 609 | 10.1051\\/0004-6361\\/201731419 | 2018A&A...609A..37C | http://adsabs.harvard.edu/abs/2018A%26A...609A..37C
  • Panchromatic spectral energy distributions of simulated galaxies: results at redshift z = 0 | Goz David et al. | Monthly Notices of the Royal Astronomical Society Volume 469 Issue 4 p.3775-3791 | 469 | 10.1093\\/mnras\\/stx869 | 2017MNRAS.469.3775G | http://adsabs.harvard.edu/abs/2017MNRAS.469.3775G
  • The selective effect of environment on the atomic and molecular gas-to-dust ratio of nearby galaxies in the Herschel Reference Survey | Cortese L. et al. | Monthly Notices of the Royal Astronomical Society Volume 459 Issue 4 p.3574-3584 | 459 | 10.1093\\/mnras\\/stw801 | 2016MNRAS.459.3574C | http://adsabs.harvard.edu/abs/2016MNRAS.459.3574C
  • FIR colours and SEDs of nearby galaxies observed with Herschel | Boselli A. et al. | Astronomy and Astrophysics Volume 518 id.L61 5 pp. | 518 | 10.1051\\/0004-6361\\/201014534 | 2010A&A...518L..61B | http://adsabs.harvard.edu/abs/2010A%26A...518L..61B
  • The distribution of interstellar dust in CALIFA edge-on galaxies via oligochromatic radiative transfer fitting | De Geyter Gert et al. | Monthly Notices of the Royal Astronomical Society Volume 441 Issue 1 p.869-885 | 441 | 10.1093\\/mnras\\/stu612 | 2014MNRAS.441..869D | http://adsabs.harvard.edu/abs/2014MNRAS.441..869D
  • Do bulges stop stars forming? | Eales Stephen et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2020MNRAS.491...69E |
  • A nearby galaxy perspective on dust evolution. Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples | Galliano Frederic et al. | Astronomy and Astrophysics | null | null | 2021A&A...649A..18G |
  • Variations of the ISM Compactness Across the Main Sequence of Star Forming Galaxies: Observations and Simulations | Martinez-Galarza J. R. et al. | The Astrophysical Journal Volume 817 Issue 1 article id. 76 18 pp. (2016). | 817 | 10.3847\\/0004-637X\\/817\\/1\\/76 | 2016ApJ...817...76M | http://adsabs.harvard.edu/abs/2016ApJ...817...76M
  • The bivariate luminosity and mass functions of the local HRS galaxy sample. The stellar, dust, and gas mass functions | Andreani P. et al. | Astronomy & Astrophysics Volume 617 id.A33 12 pp. | 617 | 10.1051\\/0004-6361\\/201832873 | 2018A&A...617A..33A | http://adsabs.harvard.edu/abs/2018A%26A...617A..33A
  • Simulated Galaxy Interactions as Probes of Merger Spectral Energy Distributions | Lanz Lauranne et al. | The Astrophysical Journal Volume 785 Issue 1 article id. 39 20 pp. (2014). | 785 | 10.1088\\/0004-637X\\/785\\/1\\/39 | 2014ApJ...785...39L | http://adsabs.harvard.edu/abs/2014ApJ...785...39L
  • Dust emissivity and absorption cross section in DustPedia late-type galaxies | Bianchi S. et al. | Astronomy and Astrophysics | null | null | 2019A&A...631A.102B |
  • Predicting the global far-infrared SED of galaxies via machine learning techniques | Dobbels W. et al. | Astronomy and Astrophysics | null | null | 2020A&A...634A..57D |
  • Far-infrared colours of nearby late-type galaxies in the Herschel Reference Survey | Boselli A. et al. | Astronomy & Astrophysics Volume 540 id.A54 22 pp. | 540 | 10.1051\\/0004-6361\\/201118602 | 2012A&A...540A..54B | http://adsabs.harvard.edu/abs/2012A%26A...540A..54B
  • The molecular mass function of the local Universe | Andreani P. et al. | Astronomy and Astrophysics | null | null | 2020A&A...643L..11A |
  • Dust grain size evolution in local galaxies: a comparison between observations and simulations | Relano M. et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2022MNRAS.515.5306R |
  • Fraction of bolometric luminosity absorbed by dust in DustPedia galaxies | Bianchi S. et al. | Astronomy & Astrophysics Volume 620 id.A112 21 pp. | 620 | 10.1051\\/0004-6361\\/201833699 | 2018A&A...620A.112B | http://adsabs.harvard.edu/abs/2018A%26A...620A.112B
  • UV to submillimetre luminosity functions of TNG50 galaxies | Trcka Ana et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2022MNRAS.516.3728T |
  • Dust and star formation properties of a complete sample of local galaxies drawn from the Planck Early Release Compact Source Catalogue | Clemens M. S. et al. | Monthly Notices of the Royal Astronomical Society Volume 433 Issue 1 p.695-711 | 433 | 10.1093\\/mnras\\/stt760 | 2013MNRAS.433..695C | http://adsabs.harvard.edu/abs/2013MNRAS.433..695C
  • AKARI and IRAS: From beam corrections to SEDs | Clements David L. et al. | Publications of the Astronomical Society of Japan Volume 71 Issue 1 id.7 | 71 | 10.1093\\/pasj\\/psy099 | 2019PASJ...71....7C | http://adsabs.harvard.edu/abs/2019PASJ...71....7C
  • The bivariate K-band-submillimetre luminosity functions of the local HRS galaxy sample | Andreani P. et al. | Astronomy & Astrophysics Volume 566 id.A70 8 pp. | 566 | 10.1051\\/0004-6361\\/201322747 | 2014A&A...566A..70A | http://adsabs.harvard.edu/abs/2014A%26A...566A..70A
  • Dust emission profiles of DustPedia galaxies | Mosenkov A. V. et al. | Astronomy & Astrophysics Volume 622 id.A132 24 pp. | 622 | 10.1051\\/0004-6361\\/201833932 | 2019A&A...622A.132M | http://adsabs.harvard.edu/abs/2019A%26A...622A.132M
  • The new galaxy evolution paradigm revealed by the Herschel surveys | Eales Stephen et al. | Monthly Notices of the Royal Astronomical Society Volume 473 Issue 3 p.3507-3524 | 473 | 10.1093\\/mnras\\/stx2548 | 2018MNRAS.473.3507E | http://adsabs.harvard.edu/abs/2018MNRAS.473.3507E
  • Probing the spectral shape of dust emission with the DustPedia galaxy sample | Nersesian Angelos et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2021MNRAS.506.3986N |
  • JINGLE - IV. Dust, H I gas, and metal scaling laws in the local Universe | De Looze I. et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2020MNRAS.496.3668D |
  • The dust scaling relations of the Herschel Reference Survey | Cortese L. et al. | Astronomy & Astrophysics Volume 540 id.A52 17 pp. | 540 | 10.1051\\/0004-6361\\/201118499 | 2012A&A...540A..52C | http://adsabs.harvard.edu/abs/2012A%26A...540A..52C
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
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, eales et al., 2010, 'The Herschel Reference Survey', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-3crzmcm