Herschel-ATLAS: the far-infrared-radio correlation at z 0.5

Matt J. Jarvis; D. J. B. Smith; D. G. Bonfield; M. J. Hardcastle; J. T. Falder; J. A. Stevens; R. J. Ivison; R. Auld; M. Baes; I. K. Baldry; S. P. Bamford; N. Bourne; S. Buttiglione; A. Cava; A. Cooray; A. Dariush; G. de Zotti; J. S. Dunlop; L. Dunne; S. Dye; S. Eales; J. Fritz; D. T. Hill; R. Hopwood; D. H. Hughes; E. Ibar; D. H. Jones; L. Kelvin; A. Lawrence; L. Leeuw; S. J. Maddox; M. J. Michalowski; M. Negrello; P. Norberg; M. Pohlen; M. Prescott; E. E. Rigby; A. Robotham; G. Rodighiero; D. Scott; R. Sharp; P. Temi; M. A. Thompson; P. van der Werf; E. van Kampen; C. Vlahakis; G. White

doi:10.1111/j.1365-2966.2010.17772.x

Herschel-ATLAS: the far-infrared-radio correlation at z 0.5

Matt J. Jarvis, D. J. B. Smith, D. G. Bonfield, M. J. Hardcastle, J. T. Falder, J. A. Stevens, R. J. Ivison, R. Auld, M. Baes, I. K. Baldry, S. P. Bamford, N. Bourne, S. Buttiglione, A. Cava, A. Cooray, A. Dariush, G. de Zotti, J. S. Dunlop, L. Dunne, S. DyeS. Eales, J. Fritz, D. T. Hill, R. Hopwood, D. H. Hughes, E. Ibar, D. H. Jones, L. Kelvin, A. Lawrence, L. Leeuw, S. J. Maddox, M. J. Michalowski, M. Negrello, P. Norberg, M. Pohlen, M. Prescott, E. E. Rigby, A. Robotham, G. Rodighiero, D. Scott, R. Sharp, P. Temi, M. A. Thompson, P. van der Werf, E. van Kampen, C. Vlahakis, G. White

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Abstract / Description of output

We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared-radio correlation over the redshift range 0 < z < 0.5. Using the total far-infrared luminosity of all > 5 sigma sources in the Herschel-ATLAS Science Demonstration Field and cross-matching these data with radio data from the Faint Images of the Radio Sky at Twenty-Centimetres (FIRST) survey and the NRAO Very Large Array (VLA) Northern Sky Survey (NVSS), we obtain 104 radio counterparts to the Herschel sources. With these data we find no evidence for evolution in the far-infrared-radio correlation over the redshift range 0 < z < 0.5, where the median value for the ratio between far-infrared and radio luminosity, q(IR), over this range is q(IR) = 2.40 +/- 0.12 (and a mean of q(IR) = 2.52 +/- 0.03 accounting for the lower limits), consistent with both the local value determined from IRAS and values derived from surveys targeting the high-redshift

Original language	English
Pages (from-to)	92-101
Number of pages	10
Journal	Monthly Notices of the Royal Astronomical Society
Volume	409
Issue number	1
DOIs	https://doi.org/10.1111/j.1365-2966.2010.17772.x
Publication status	Published - Nov 2010

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Jarvis, M. J., Smith, D. J. B., Bonfield, D. G., Hardcastle, M. J., Falder, J. T., Stevens, J. A., Ivison, R. J., Auld, R., Baes, M., Baldry, I. K., Bamford, S. P., Bourne, N., Buttiglione, S., Cava, A., Cooray, A., Dariush, A., de Zotti, G., Dunlop, J. S., Dunne, L., ... White, G. (2010). Herschel-ATLAS: the far-infrared-radio correlation at z 0.5. Monthly Notices of the Royal Astronomical Society, 409(1), 92-101. https://doi.org/10.1111/j.1365-2966.2010.17772.x

@article{86c86ea6186c44b9be1d18f20c159c4c,

title = "Herschel-ATLAS: the far-infrared-radio correlation at z 0.5",

abstract = "We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared-radio correlation over the redshift range 0 < z < 0.5. Using the total far-infrared luminosity of all > 5 sigma sources in the Herschel-ATLAS Science Demonstration Field and cross-matching these data with radio data from the Faint Images of the Radio Sky at Twenty-Centimetres (FIRST) survey and the NRAO Very Large Array (VLA) Northern Sky Survey (NVSS), we obtain 104 radio counterparts to the Herschel sources. With these data we find no evidence for evolution in the far-infrared-radio correlation over the redshift range 0 < z < 0.5, where the median value for the ratio between far-infrared and radio luminosity, q(IR), over this range is q(IR) = 2.40 +/- 0.12 (and a mean of q(IR) = 2.52 +/- 0.03 accounting for the lower limits), consistent with both the local value determined from IRAS and values derived from surveys targeting the high-redshift",

author = "Jarvis, {Matt J.} and Smith, {D. J. B.} and Bonfield, {D. G.} and Hardcastle, {M. J.} and Falder, {J. T.} and Stevens, {J. A.} and Ivison, {R. J.} and R. Auld and M. Baes and Baldry, {I. K.} and Bamford, {S. P.} and N. Bourne and S. Buttiglione and A. Cava and A. Cooray and A. Dariush and {de Zotti}, G. and Dunlop, {J. S.} and L. Dunne and S. Dye and S. Eales and J. Fritz and Hill, {D. T.} and R. Hopwood and Hughes, {D. H.} and E. Ibar and Jones, {D. H.} and L. Kelvin and A. Lawrence and L. Leeuw and Maddox, {S. J.} and Michalowski, {M. J.} and M. Negrello and P. Norberg and M. Pohlen and M. Prescott and Rigby, {E. E.} and A. Robotham and G. Rodighiero and D. Scott and R. Sharp and P. Temi and Thompson, {M. A.} and {van der Werf}, P. and {van Kampen}, E. and C. Vlahakis and G. White",

year = "2010",

month = nov,

doi = "10.1111/j.1365-2966.2010.17772.x",

language = "English",

volume = "409",

pages = "92--101",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

}

Jarvis, MJ, Smith, DJB, Bonfield, DG, Hardcastle, MJ, Falder, JT, Stevens, JA, Ivison, RJ, Auld, R, Baes, M, Baldry, IK, Bamford, SP, Bourne, N, Buttiglione, S, Cava, A, Cooray, A, Dariush, A, de Zotti, G, Dunlop, JS, Dunne, L, Dye, S, Eales, S, Fritz, J, Hill, DT, Hopwood, R, Hughes, DH, Ibar, E, Jones, DH, Kelvin, L, Lawrence, A, Leeuw, L, Maddox, SJ, Michalowski, MJ, Negrello, M, Norberg, P, Pohlen, M, Prescott, M, Rigby, EE, Robotham, A, Rodighiero, G, Scott, D, Sharp, R, Temi, P, Thompson, MA, van der Werf, P, van Kampen, E, Vlahakis, C & White, G 2010, 'Herschel-ATLAS: the far-infrared-radio correlation at z 0.5', Monthly Notices of the Royal Astronomical Society, vol. 409, no. 1, pp. 92-101. https://doi.org/10.1111/j.1365-2966.2010.17772.x

TY - JOUR

T1 - Herschel-ATLAS: the far-infrared-radio correlation at z 0.5

AU - Jarvis, Matt J.

AU - Smith, D. J. B.

AU - Bonfield, D. G.

AU - Hardcastle, M. J.

AU - Falder, J. T.

AU - Stevens, J. A.

AU - Ivison, R. J.

AU - Auld, R.

AU - Baes, M.

AU - Baldry, I. K.

AU - Bamford, S. P.

AU - Bourne, N.

AU - Buttiglione, S.

AU - Cava, A.

AU - Cooray, A.

AU - Dariush, A.

AU - de Zotti, G.

AU - Dunlop, J. S.

AU - Dunne, L.

AU - Dye, S.

AU - Eales, S.

AU - Fritz, J.

AU - Hill, D. T.

AU - Hopwood, R.

AU - Hughes, D. H.

AU - Ibar, E.

AU - Jones, D. H.

AU - Kelvin, L.

AU - Lawrence, A.

AU - Leeuw, L.

AU - Maddox, S. J.

AU - Michalowski, M. J.

AU - Negrello, M.

AU - Norberg, P.

AU - Pohlen, M.

AU - Prescott, M.

AU - Rigby, E. E.

AU - Robotham, A.

AU - Rodighiero, G.

AU - Scott, D.

AU - Sharp, R.

AU - Temi, P.

AU - Thompson, M. A.

AU - van der Werf, P.

AU - van Kampen, E.

AU - Vlahakis, C.

AU - White, G.

PY - 2010/11

Y1 - 2010/11

N2 - We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared-radio correlation over the redshift range 0 < z < 0.5. Using the total far-infrared luminosity of all > 5 sigma sources in the Herschel-ATLAS Science Demonstration Field and cross-matching these data with radio data from the Faint Images of the Radio Sky at Twenty-Centimetres (FIRST) survey and the NRAO Very Large Array (VLA) Northern Sky Survey (NVSS), we obtain 104 radio counterparts to the Herschel sources. With these data we find no evidence for evolution in the far-infrared-radio correlation over the redshift range 0 < z < 0.5, where the median value for the ratio between far-infrared and radio luminosity, q(IR), over this range is q(IR) = 2.40 +/- 0.12 (and a mean of q(IR) = 2.52 +/- 0.03 accounting for the lower limits), consistent with both the local value determined from IRAS and values derived from surveys targeting the high-redshift

AB - We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared-radio correlation over the redshift range 0 < z < 0.5. Using the total far-infrared luminosity of all > 5 sigma sources in the Herschel-ATLAS Science Demonstration Field and cross-matching these data with radio data from the Faint Images of the Radio Sky at Twenty-Centimetres (FIRST) survey and the NRAO Very Large Array (VLA) Northern Sky Survey (NVSS), we obtain 104 radio counterparts to the Herschel sources. With these data we find no evidence for evolution in the far-infrared-radio correlation over the redshift range 0 < z < 0.5, where the median value for the ratio between far-infrared and radio luminosity, q(IR), over this range is q(IR) = 2.40 +/- 0.12 (and a mean of q(IR) = 2.52 +/- 0.03 accounting for the lower limits), consistent with both the local value determined from IRAS and values derived from surveys targeting the high-redshift

U2 - 10.1111/j.1365-2966.2010.17772.x

DO - 10.1111/j.1365-2966.2010.17772.x

M3 - Article

SN - 0035-8711

VL - 409

SP - 92

EP - 101

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

Herschel-ATLAS: the far-infrared-radio correlation at z 0.5

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