Herschel-ATLAS: The far-infrared-radio correlation at z <0.5

Matt Jarvis; D Smith; D Bonfield; M Hardcastle; J Falder; J Stevens; R Ivison; R Auld; M Baes; Ivan Baldry; Steven Bamford; N Bourne; S Buttiglione; A Cava; Asantha Cooray; A Dariush; G De Zotti; James Dunlop; L Dunne; S Dye; S Eales; J Fritz; D Hill; R Hopwood; D Hughes; E Ibar; David Jones; L Kelvin; Andy Lawrence; L Leeuw; J Loveday; S Maddox; M Michalowski; M Negrello; Peder Norberg; M Pohlen; Matthew Prescott; E Rigby; A Robotham; G Rodighiero; Douglas Scott; Robert Sharp; P Temi; M 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 Jarvis, D Smith, D Bonfield, M Hardcastle, J Falder, J Stevens, R Ivison, R Auld, M Baes, Ivan Baldry, Steven Bamford, N Bourne, S Buttiglione, A Cava, Asantha Cooray, A Dariush, G De Zotti, James Dunlop, L Dunne, S DyeS Eales, J Fritz, D Hill, R Hopwood, D Hughes, E Ibar, David Jones, L Kelvin, Andy Lawrence, L Leeuw, J Loveday, S Maddox, M Michalowski, M Negrello, Peder Norberg, M Pohlen, Matthew Prescott, E Rigby, A Robotham, G Rodighiero, Douglas Scott, Robert Sharp, P Temi, M Thompson, P van der Werf, E van Kampen, C Vlahakis, G White

Research output: Contribution to journal › Article › Research › peer-review

88 Citations (Scopus)

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 >5I? 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, qIR, over this range is qIR= 2.40 A? 0.12 (and a mean of qIR= 2.52 A? 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 Universe.

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 - 2010
Externally published	Yes

Access to Document

10.1111/j.1365-2966.2010.17772.x

Cite this

Jarvis, M., Smith, D., Bonfield, D., Hardcastle, M., Falder, J., Stevens, J., Ivison, R., Auld, R., Baes, M., Baldry, I., Bamford, S., Bourne, N., Buttiglione, S., Cava, A., Cooray, A., Dariush, A., De Zotti, G., Dunlop, J., 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{ff18e03749244caebd552faf77861118,

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 5I? 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, qIR, over this range is qIR= 2.40 A? 0.12 (and a mean of qIR= 2.52 A? 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 Universe.",

author = "Matt Jarvis and D Smith and D Bonfield and M Hardcastle and J Falder and J Stevens and R Ivison and R Auld and M Baes and Ivan Baldry and Steven Bamford and N Bourne and S Buttiglione and A Cava and Asantha Cooray and A Dariush and {De Zotti}, G and James Dunlop and L Dunne and S Dye and S Eales and J Fritz and D Hill and R Hopwood and D Hughes and E Ibar and David Jones and L Kelvin and Andy Lawrence and L Leeuw and J Loveday and S Maddox and M Michalowski and M Negrello and Peder Norberg and M Pohlen and Matthew Prescott and E Rigby and A Robotham and G Rodighiero and Douglas Scott and Robert Sharp and P Temi and M Thompson and {van der Werf}, P and {van Kampen}, E and C Vlahakis and G White",

year = "2010",

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, M, Smith, D, Bonfield, D, Hardcastle, M, Falder, J, Stevens, J, Ivison, R, Auld, R, Baes, M, Baldry, I, Bamford, S, Bourne, N, Buttiglione, S, Cava, A, Cooray, A, Dariush, A, De Zotti, G, Dunlop, J, Dunne, L, Dye, S, Eales, S, Fritz, J, Hill, D, Hopwood, R, Hughes, D, Ibar, E, Jones, D, Kelvin, L, Lawrence, A, Leeuw, L, Loveday, J, Maddox, S, Michalowski, M, Negrello, M, Norberg, P, Pohlen, M, Prescott, M, Rigby, E, Robotham, A, Rodighiero, G, Scott, D, Sharp, R, Temi, P, Thompson, M, 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

AU - Smith, D

AU - Bonfield, D

AU - Hardcastle, M

AU - Falder, J

AU - Stevens, J

AU - Ivison, R

AU - Auld, R

AU - Baes, M

AU - Baldry, Ivan

AU - Bamford, Steven

AU - Bourne, N

AU - Buttiglione, S

AU - Cava, A

AU - Cooray, Asantha

AU - Dariush, A

AU - De Zotti, G

AU - Dunlop, James

AU - Dunne, L

AU - Dye, S

AU - Eales, S

AU - Fritz, J

AU - Hill, D

AU - Hopwood, R

AU - Hughes, D

AU - Ibar, E

AU - Jones, David

AU - Kelvin, L

AU - Lawrence, Andy

AU - Leeuw, L

AU - Loveday, J

AU - Maddox, S

AU - Michalowski, M

AU - Negrello, M

AU - Norberg, Peder

AU - Pohlen, M

AU - Prescott, Matthew

AU - Rigby, E

AU - Robotham, A

AU - Rodighiero, G

AU - Scott, Douglas

AU - Sharp, Robert

AU - Temi, P

AU - Thompson, M

AU - van der Werf, P

AU - van Kampen, E

AU - Vlahakis, C

AU - White, G

PY - 2010

Y1 - 2010

N2 - We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared-radio correlation over the redshift range 0 5I? 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, qIR, over this range is qIR= 2.40 A? 0.12 (and a mean of qIR= 2.52 A? 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 Universe.

AB - We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared-radio correlation over the redshift range 0 5I? 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, qIR, over this range is qIR= 2.40 A? 0.12 (and a mean of qIR= 2.52 A? 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 Universe.

UR - http://onlinelibrary.wiley.com.ezproxy.lib.monash.edu.au/doi/10.1111/j.1365-2966.2010.17772.x/pdf

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

Abstract

Access to Document

Other files and links

Cite this