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The Herschel Virgo Cluster survey, XV : Planck submillimetre sources in the Virgo Cluster

Maarten Baes (UGent) , D Herranz, S Bianchi, L Ciesla, M Clemens, G De Zotti, Flor Allaert (UGent) , R Auld, GJ Bendo, M Boquien, et al.
(2014) ASTRONOMY & ASTROPHYSICS. 562.
Author
Organization
Abstract
We cross-correlate the Planck Catalogue of Compact Sources (PCCS) with the fully sampled 84 deg(2) Herschel Virgo Cluster Survey (HeViCS) fields. We search for and identify the 857 and 545 GHz PCCS sources in the HeViCS fields by studying their FIR/submm and optical counterparts. We find 84 and 48 compact Planck sources in the HeViCS fields at 857 and 545 GHz, respectively. Almost all sources correspond to individual bright Virgo Cluster galaxies. The vast majority of the Planck detected galaxies are late-type spirals, with the Sc class dominating the numbers, while early-type galaxies are virtually absent from the sample, especially at 545 GHz. We compare the HeViCS SPIRE flux densities for the detected galaxies with the four different PCCS flux density estimators and find an excellent correlation with the aperture photometry flux densities, even at the highest flux density levels. We find only seven PCCS sources in the HeViCS fields without a nearby galaxy as obvious counterpart, and conclude that all of these are dominated by Galactic cirrus features or are spurious detections. No Planck sources in the HeViCS fields seem to be associated to high-redshift proto-clusters of dusty galaxies or strongly lensed submm sources. Finally, our study is the first empirical confirmation of the simulation-based estimated completeness of the PCCS, and provides a strong support of the internal PCCS validation procedure.
Keywords
submillimeter: galaxies, galaxies: ISM, EARLY-TYPE GALAXIES, SPECTRAL ENERGY-DISTRIBUTION, STRONGLY LENSED GALAXIES, COMPACT SOURCE CATALOG, GAS MASS-RATIO, NEARBY GALAXIES, INFRARED-EMISSION, DWARF GALAXIES, LUMINOSITY FUNCTION, INTERSTELLAR DUST

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Citation

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MLA
Baes, Maarten, et al. “The Herschel Virgo Cluster Survey, XV : Planck Submillimetre Sources in the Virgo Cluster.” ASTRONOMY & ASTROPHYSICS, vol. 562, 2014, doi:10.1051/0004-6361/201322384.
APA
Baes, M., Herranz, D., Bianchi, S., Ciesla, L., Clemens, M., De Zotti, G., … Vlahakis, C. (2014). The Herschel Virgo Cluster survey, XV : Planck submillimetre sources in the Virgo Cluster. ASTRONOMY & ASTROPHYSICS, 562. https://doi.org/10.1051/0004-6361/201322384
Chicago author-date
Baes, Maarten, D Herranz, S Bianchi, L Ciesla, M Clemens, G De Zotti, Flor Allaert, et al. 2014. “The Herschel Virgo Cluster Survey, XV : Planck Submillimetre Sources in the Virgo Cluster.” ASTRONOMY & ASTROPHYSICS 562. https://doi.org/10.1051/0004-6361/201322384.
Chicago author-date (all authors)
Baes, Maarten, D Herranz, S Bianchi, L Ciesla, M Clemens, G De Zotti, Flor Allaert, R Auld, GJ Bendo, M Boquien, A Boselli, DL Clements, L Cortese, JI Davies, Ilse De Looze, SD Alighieri, Jacopo Fritz, Gianfranco Gentile, J González-Nuevo, Thomas Hughes, MWL Smith, Joris Verstappen, Sébastien Viaene, and C Vlahakis. 2014. “The Herschel Virgo Cluster Survey, XV : Planck Submillimetre Sources in the Virgo Cluster.” ASTRONOMY & ASTROPHYSICS 562. doi:10.1051/0004-6361/201322384.
Vancouver
1.
Baes M, Herranz D, Bianchi S, Ciesla L, Clemens M, De Zotti G, et al. The Herschel Virgo Cluster survey, XV : Planck submillimetre sources in the Virgo Cluster. ASTRONOMY & ASTROPHYSICS. 2014;562.
IEEE
[1]
M. Baes et al., “The Herschel Virgo Cluster survey, XV : Planck submillimetre sources in the Virgo Cluster,” ASTRONOMY & ASTROPHYSICS, vol. 562, 2014.
@article{4385081,
  abstract     = {{We cross-correlate the Planck Catalogue of Compact Sources (PCCS) with the fully sampled 84 deg(2) Herschel Virgo Cluster Survey (HeViCS) fields. We search for and identify the 857 and 545 GHz PCCS sources in the HeViCS fields by studying their FIR/submm and optical counterparts. We find 84 and 48 compact Planck sources in the HeViCS fields at 857 and 545 GHz, respectively. Almost all sources correspond to individual bright Virgo Cluster galaxies. The vast majority of the Planck detected galaxies are late-type spirals, with the Sc class dominating the numbers, while early-type galaxies are virtually absent from the sample, especially at 545 GHz. We compare the HeViCS SPIRE flux densities for the detected galaxies with the four different PCCS flux density estimators and find an excellent correlation with the aperture photometry flux densities, even at the highest flux density levels. We find only seven PCCS sources in the HeViCS fields without a nearby galaxy as obvious counterpart, and conclude that all of these are dominated by Galactic cirrus features or are spurious detections. No Planck sources in the HeViCS fields seem to be associated to high-redshift proto-clusters of dusty galaxies or strongly lensed submm sources. Finally, our study is the first empirical confirmation of the simulation-based estimated completeness of the PCCS, and provides a strong support of the internal PCCS validation procedure.}},
  articleno    = {{A106}},
  author       = {{Baes, Maarten and Herranz, D and Bianchi, S and Ciesla, L and Clemens, M and De Zotti, G and Allaert, Flor and Auld, R and Bendo, GJ and Boquien, M and Boselli, A and Clements, DL and Cortese, L and Davies, JI and De Looze, Ilse and Alighieri, SD and Fritz, Jacopo and Gentile, Gianfranco and González-Nuevo, J and Hughes, Thomas and Smith, MWL and Verstappen, Joris and Viaene, Sébastien and Vlahakis, C}},
  issn         = {{0004-6361}},
  journal      = {{ASTRONOMY & ASTROPHYSICS}},
  keywords     = {{submillimeter: galaxies,galaxies: ISM,EARLY-TYPE GALAXIES,SPECTRAL ENERGY-DISTRIBUTION,STRONGLY LENSED GALAXIES,COMPACT SOURCE CATALOG,GAS MASS-RATIO,NEARBY GALAXIES,INFRARED-EMISSION,DWARF GALAXIES,LUMINOSITY FUNCTION,INTERSTELLAR DUST}},
  language     = {{eng}},
  pages        = {{16}},
  title        = {{The Herschel Virgo Cluster survey, XV : Planck submillimetre sources in the Virgo Cluster}},
  url          = {{http://dx.doi.org/10.1051/0004-6361/201322384}},
  volume       = {{562}},
  year         = {{2014}},
}
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