CaltechAUTHORS
  A Caltech Library Service

The Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshift

Brisbin, D. and Blain, A. and Bock, J. and Cooray, A. and Dowell, C. D. and Levenson, L. and Lu, N. and Nguyen, H. T. and Schulz, B. and Shupe, D. L. and Xu, C. K. and Zemcov, M. (2010) The Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshift. Monthly Notices of the Royal Astronomical Society, 409 (1). pp. 66-74. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20101213-112741295

[img]
Preview
PDF - Published Version
See Usage Policy.

2208Kb

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20101213-112741295

Abstract

The Spectral and Photometric Imaging Receiver on-board Herschel has been carrying out deep extragalactic surveys, one of the aims of which is to establish spectral energy distributions of individual galaxies spanning the infrared/submillimetre (IR/SMM) wavelength region. We report observations of the IR/SMM emission from the Lockman North field and Great Observatories Origins Deep Survey Field-North. Because galaxy images in the wavelength range covered by Herschel generally represent a blend with contributions from neighbouring galaxies, we present sets of galaxies in each field, especially free of blending at 250, 350 and 500 μm. We identify the cumulative emission of these galaxies and the fraction of the FIR cosmic background radiation they contribute. Our surveys reveal a number of highly luminous galaxies at redshift z ≲ 3 and a novel relationship between IR and visible emission that shows a dependence on luminosity and redshift.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1111/j.1365-2966.2010.17643.xDOIUNSPECIFIED
Additional Information:© 2010 The Authors. Journal compilation © 2010 RAS. Accepted 2010 September 3. Received 2010 September 2; in original form 2010 June 11. Article first published online: 25 Oct. 2010. Herschel is an ESA space observatory with science instruments provided by the European-led Principal Investigator consortia and with important participation from the NASA. This work is based in part on observations made with Herschel, a European Space Agency Cornerstone Mission with significant participation by the NASA. Support for this work was provided by the NASA through an award issued by JPL/Caltech. The SPIRE has been developed by a consortium of institutes led by Cardiff University (UK) and including Univ. Lethbridge (Canada); NAOC(China); CEA, OAMP(France); IFSI, Univ. Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, Univ. Sussex (UK); and Caltech/JPL, IPAC, Univ. Colorado (USA). This development has been supported by national funding agencies: CSA (Canada); NAOC (China); CEA, CNES, CNRS (France); ASI (Italy); MCINN (Spain); SNSB (Sweden); STFC (UK); and NASA (USA). We thank the referee of this paper, Stephen J. Messenger, for his incisive comments and helpful recommendations.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NASAUNSPECIFIED
Canadian Space Agency (CSA) UNSPECIFIED
National Astronomical Observatories, Chinese Academy of Sciences (NAOC) UNSPECIFIED
Commissariat à l’Energie Atomique (CEA) (France)UNSPECIFIED
Centre National d'Études Spatiales (CNES) (France)UNSPECIFIED
Centre National de la Recherche Scientifique (CNRS) (France)UNSPECIFIED
Agenzia Spaziale Italiana (ASI) UNSPECIFIED
Ministerio de Ciencia e Innovación (MCINN) (Spain)UNSPECIFIED
Swedish National Space Board (SNSB)UNSPECIFIED
Science and Technology Facilities Council (STFC)UNSPECIFIED
Subject Keywords:galaxies: high-redshift; galaxies: starburst; galaxies: star formation; infrared: galaxies
Record Number:CaltechAUTHORS:20101213-112741295
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20101213-112741295
Official Citation:Brisbin, D., Harwit, M., Altieri, B., Amblard, A., Arumugam, V., Aussel, H., Babbedge, T., Blain, A., Bock, J., Boselli, A., Buat, V., Castro-Rodríguez, N., Cava, A., Chanial, P., Clements, D. L., Conley, A., Conversi, L., Cooray, A., Dowell, C. D., Dwek, E., Eales, S., Elbaz, D., Fox, M., Franceschini, A., Gear, W., Glenn, J., Griffin, M., Halpern, M., Hatziminaoglou, E., Ibar, E., Isaak, K., Ivison, R. J., Lagache, G., Levenson, L., Lonsdale, C. J., Lu, N., Madden, S., Maffei, B., Mainetti, G., Marchetti, L., Morrison, G. E., Nguyen, H. T., O’Halloran, B., Oliver, S. J., Omont, A., Owen, F. N., Pannella, M., Panuzzo, P., Papageorgiou, A., Pearson, C. P., Pérez-Fournon, I., Pohlen, M., Rizzo, D., Roseboom, I. G., Rowan-Robinson, M., Portal, M. S., Schulz, B., Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Strazzullo, V., Symeonidis, M., Trichas, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Vigroux, L., Wang, L., Ward, R., Wright, G., Xu, C. K. and Zemcov, M. (2010), The Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshift. Monthly Notices of the Royal Astronomical Society, 409: 66–74. doi: 10.1111/j.1365-2966.2010.17643.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:21321
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:17 Dec 2010 16:09
Last Modified:23 Dec 2013 23:09

Repository Staff Only: item control page