The far-infrared/radio correlation as probed by Herschel
dc.contributor.author | Ivison, R. | |
dc.contributor.author | Magnelli, B. | |
dc.contributor.author | Ibar, E. | |
dc.contributor.author | Andreani, P. | |
dc.contributor.author | Elbaz, D. | |
dc.contributor.author | Altieri, B. | |
dc.contributor.author | Amblard, A. | |
dc.contributor.author | Arumugam, V. | |
dc.contributor.author | Auld, R. | |
dc.contributor.author | Aussel, H. | |
dc.contributor.author | Babbedge, T. | |
dc.contributor.author | Berta, S. | |
dc.contributor.author | Blain, A. | |
dc.contributor.author | Bock, J. | |
dc.contributor.author | Bongiovanni, A. | |
dc.contributor.author | Boselli, A. | |
dc.contributor.author | Buat, V. | |
dc.contributor.author | Burgarella, D. | |
dc.contributor.author | Castro-Rodríguez, N. | |
dc.contributor.author | Cava, A. | |
dc.contributor.author | Cepa, J. | |
dc.contributor.author | Chanial, P. | |
dc.contributor.author | Cimatti, A. | |
dc.contributor.author | Cirasuolo, M. | |
dc.contributor.author | Clements, D. | |
dc.contributor.author | Conley, A. | |
dc.contributor.author | Conversi, L. | |
dc.contributor.author | Cooray, A. | |
dc.contributor.author | Daddi, E. | |
dc.contributor.author | Dominguez, H. | |
dc.contributor.author | Dowell, C. | |
dc.contributor.author | Dwek, E. | |
dc.contributor.author | Eales, S. | |
dc.contributor.author | Farrah, D. | |
dc.contributor.author | FörsterSchreiber, N. | |
dc.contributor.author | Fox, M. | |
dc.contributor.author | Franceschini, A. | |
dc.contributor.author | Gear, W. | |
dc.contributor.author | Genzel, R. | |
dc.contributor.author | Glenn, J. | |
dc.contributor.author | Griffin, M. | |
dc.contributor.author | Gruppioni, C. | |
dc.contributor.author | Halpern, M. | |
dc.contributor.author | Hatziminaoglou, E. | |
dc.contributor.author | Isaak, K. | |
dc.contributor.author | Lagache, G. | |
dc.contributor.author | Levenson, L. | |
dc.contributor.author | Lu, N. | |
dc.contributor.author | Lutz, D. | |
dc.contributor.author | Madden, S. | |
dc.contributor.author | Maffei, B. | |
dc.contributor.author | Magdis, G. | |
dc.contributor.author | Mainetti, G. | |
dc.contributor.author | Maiolino, R. | |
dc.contributor.author | Marchetti, L. | |
dc.contributor.author | Morrison, G. | |
dc.contributor.author | Mortier, A. | |
dc.contributor.author | Nguyen, H. | |
dc.contributor.author | Nordon, R. | |
dc.contributor.author | O'Halloran, B. | |
dc.contributor.author | Oliver, S. | |
dc.contributor.author | Omont, A. | |
dc.contributor.author | Owen, F. | |
dc.contributor.author | Page, M. | |
dc.contributor.author | Panuzzo, P. | |
dc.contributor.author | Papageorgiou, A. | |
dc.contributor.author | Pearson, C. | |
dc.contributor.author | Pérez-Fournon, I. | |
dc.contributor.author | García, A. | |
dc.contributor.author | Poglitsch, A. | |
dc.contributor.author | Pohlen, M. | |
dc.contributor.author | Popesso, P. | |
dc.contributor.author | Pozzi, F. | |
dc.contributor.author | Rawlings, J. | |
dc.contributor.author | Raymond, G. | |
dc.contributor.author | Rigopoulou, D. | |
dc.contributor.author | Riguccini, L. | |
dc.contributor.author | Rizzo, D. | |
dc.contributor.author | Rodighiero, G. | |
dc.contributor.author | Roseboom, I. | |
dc.contributor.author | Rowan-Robinson, M. | |
dc.contributor.author | Saintonge, A. | |
dc.contributor.author | SanchezPorta, M. | |
dc.contributor.author | Santini, P. | |
dc.contributor.author | Schulz, B. | |
dc.contributor.author | Scott, D. | |
dc.contributor.author | Seymour, Nick | |
dc.contributor.author | Shao, L. | |
dc.date.accessioned | 2017-01-30T13:34:13Z | |
dc.date.available | 2017-01-30T13:34:13Z | |
dc.date.created | 2016-09-12T08:37:03Z | |
dc.date.issued | 2010 | |
dc.identifier.citation | Ivison, R. and Magnelli, B. and Ibar, E. and Andreani, P. and Elbaz, D. and Altieri, B. and Amblard, A. et al. 2010. The far-infrared/radio correlation as probed by Herschel. Astronomy and Astrophysics. 518 (4). | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/32949 | |
dc.identifier.doi | 10.1051/0004-6361/201014552 | |
dc.description.abstract |
We set out to determine the ratio, qIR, of rest-frame 8-1000-µm flux, SIR, to monochromatic radio flux, S 1.4 GHz, for galaxies selected at far-infrared (IR) and radio wavelengths, to search for signs that the ratio evolves with redshift, luminosity or dust temperature, Td, and to identify any far-IR-bright outliers - useful laboratories for exploring why the far-IR/radio correlation (FIRRC) is generally so tight when the prevailing theory suggests variations are almost inevitable. We use flux-limited 250-µm and 1.4-GHz samples, obtained using Herschel and the Very Large Array (VLA) in GOODS-North (-N). We determine bolometric IR output using ten bands spanning ?obs = 24-1250 µm, exploiting data from PACS and SPIRE (PEP; HerMES), as well as Spitzer, SCUBA, AzTEC and MAMBO. We also explore the properties of an L IR-matched sample, designed to reveal evolution of qIR with redshift, spanning log LIR = 11-12 L? and z = 0-2, by stacking into the radio and far-IR images. For 1.4-GHz-selected galaxies in GOODS-N, we see tentative evidence of a break in the flux ratio, q IR, at L1.4 GHz ~ 1022.7 W Hz-1, where active galactic nuclei (AGN) are starting to dominate the radio power density, and of weaker correlations with redshift and Td. From our 250-µm-selected sample we identify a small number of far-IR-bright outliers, and see trends of qIR with L1.4 GHz, LIR, Td and redshift, noting that some of these are inter-related. For our LIR-matched sample, there is no evidence that qIR changes significantly as we move back into the epoch of galaxy formation: we find qIR (1+z)?, where ? = -0.04±0.03 at z = 0-2; however, discounting the least reliable data at z < 0.5 we find ? = -0.26±0.07, modest evolution which may be related to the radio background seen by ARCADE 2, perhaps driven by <10-µJy radio activity amongst ordinary star-forming galaxies at z>1. © ESO 2010. | |
dc.publisher | EDP Sciences | |
dc.title | The far-infrared/radio correlation as probed by Herschel | |
dc.type | Journal Article | |
dcterms.source.volume | 518 | |
dcterms.source.number | 4 | |
dcterms.source.issn | 0004-6361 | |
dcterms.source.title | Astronomy and Astrophysics | |
curtin.department | Department of Physics and Astronomy | |
curtin.accessStatus | Open access via publisher |
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