The XMM-Newton wide-field survey in the COSMOS field: Statistical properties of clusters of galaxies

A. Finoguenov; L. Guzzo; G. Hasinger; N. Z. Scoville; H. Aussel; H. Böhringer; M. Brusa; P. Capak; N. Cappelluti; A. Comastri; S. Giodini; R. E. Griffiths; C. Impey; A. M. Koekemoer; J. P. Kneib; A. Leauthaud; O. Le Fèvre; S. Lilly; V. Mainieri; R. Massey; H. J. Mccracken; B. Mobasher; T. Murayama; J. A. Peacock; I. Sakelliou; E. Schinnerer; J. D. Silverman; V. Smolčić; Y. Taniguchi; L. Tasca; J. E. Taylor; J. R. Trump; G. Zamorani

doi:10.1086/516577

The XMM-Newton wide-field survey in the COSMOS field: Statistical properties of clusters of galaxies

A. Finoguenov, L. Guzzo, G. Hasinger, N. Z. Scoville, H. Aussel, H. Böhringer, M. Brusa, P. Capak, N. Cappelluti, A. Comastri, S. Giodini, R. E. Griffiths, C. Impey, A. M. Koekemoer, J. P. Kneib, A. Leauthaud, O. Le Fèvre, S. Lilly, V. Mainieri, R. MasseyH. J. Mccracken, B. Mobasher, T. Murayama, J. A. Peacock, I. Sakelliou, E. Schinnerer, J. D. Silverman, V. Smolčić, Y. Taniguchi, L. Tasca, J. E. Taylor, J. R. Trump, G. Zamorani

Astronomy

Research output: Contribution to journal › Review article › peer-review

225 Scopus citations

Abstract

We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the Cosmic Evolution Survey (COSMOS) field. We reach a depth for a total cluster flux in the 0.5-2 keVband of 3 × 10 ^-15 ergs cm ^-2 s ^-1, having one of the widest XMM-Newton contiguous raster surveys, covering an area of 2.1 deg ². Cluster candidates are identified through a wavelet detection of extended X-ray emission. Verification of the cluster candidates is done based on a galaxy concentration analysis in redshift slices of thickness 0.1 -0.2 in redshift, using the multiband photometric catalog of the COSMOS field and restricting the search to z < 1.3 and i _AB < 25. We identify 72 clusters and derive their properties based on the X-ray cluster scaling relations. A statistical description of the survey in terms of the cumulative log (N > S)-log S distribution compares well with previous results, although yielding a somewhat higher number of clusters at similar fluxes. The X-ray luminosity function of COSMOS clusters matches well the results of nearby surveys, providing a comparably tight constraint on the faint-end slope of α = 1.93 ±0.04. For the probed luminosity range of (8 × 10 ⁴²)-(2 × 10 ⁴⁴) ergs s ^-1, our survey is in agreement with and adds significantly to the existing data on the cluster luminosity function at high redshifts and implies no substantial evolution at these luminosities to z = 1.3.

Original language	English (US)
Pages (from-to)	182-195
Number of pages	14
Journal	Astrophysical Journal, Supplement Series
Volume	172
Issue number	1
DOIs	https://doi.org/10.1086/516577
State	Published - 2007

Keywords

Cosmology: observations
Dark matter
Large-scale structure of universe
Surveys

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/516577

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Finoguenov, A., Guzzo, L., Hasinger, G., Scoville, N. Z., Aussel, H., Böhringer, H., Brusa, M., Capak, P., Cappelluti, N., Comastri, A., Giodini, S., Griffiths, R. E., Impey, C., Koekemoer, A. M., Kneib, J. P., Leauthaud, A., Le Fèvre, O., Lilly, S., Mainieri, V., ... Zamorani, G. (2007). The XMM-Newton wide-field survey in the COSMOS field: Statistical properties of clusters of galaxies. Astrophysical Journal, Supplement Series, 172(1), 182-195. https://doi.org/10.1086/516577

The XMM-Newton wide-field survey in the COSMOS field : Statistical properties of clusters of galaxies. / Finoguenov, A.; Guzzo, L.; Hasinger, G.; Scoville, N. Z.; Aussel, H.; Böhringer, H.; Brusa, M.; Capak, P.; Cappelluti, N.; Comastri, A.; Giodini, S.; Griffiths, R. E.; Impey, C.; Koekemoer, A. M.; Kneib, J. P.; Leauthaud, A.; Le Fèvre, O.; Lilly, S.; Mainieri, V.; Massey, R.; Mccracken, H. J.; Mobasher, B.; Murayama, T.; Peacock, J. A.; Sakelliou, I.; Schinnerer, E.; Silverman, J. D.; Smolčić, V.; Taniguchi, Y.; Tasca, L.; Taylor, J. E.; Trump, J. R.; Zamorani, G.

In: Astrophysical Journal, Supplement Series, Vol. 172, No. 1, 2007, p. 182-195.

Research output: Contribution to journal › Review article › peer-review

Finoguenov, A, Guzzo, L, Hasinger, G, Scoville, NZ, Aussel, H, Böhringer, H, Brusa, M, Capak, P, Cappelluti, N, Comastri, A, Giodini, S, Griffiths, RE, Impey, C, Koekemoer, AM, Kneib, JP, Leauthaud, A, Le Fèvre, O, Lilly, S, Mainieri, V, Massey, R, Mccracken, HJ, Mobasher, B, Murayama, T, Peacock, JA, Sakelliou, I, Schinnerer, E, Silverman, JD, Smolčić, V, Taniguchi, Y, Tasca, L, Taylor, JE, Trump, JR & Zamorani, G 2007, 'The XMM-Newton wide-field survey in the COSMOS field: Statistical properties of clusters of galaxies', Astrophysical Journal, Supplement Series, vol. 172, no. 1, pp. 182-195. https://doi.org/10.1086/516577

Finoguenov, A. ; Guzzo, L. ; Hasinger, G. ; Scoville, N. Z. ; Aussel, H. ; Böhringer, H. ; Brusa, M. ; Capak, P. ; Cappelluti, N. ; Comastri, A. ; Giodini, S. ; Griffiths, R. E. ; Impey, C. ; Koekemoer, A. M. ; Kneib, J. P. ; Leauthaud, A. ; Le Fèvre, O. ; Lilly, S. ; Mainieri, V. ; Massey, R. ; Mccracken, H. J. ; Mobasher, B. ; Murayama, T. ; Peacock, J. A. ; Sakelliou, I. ; Schinnerer, E. ; Silverman, J. D. ; Smolčić, V. ; Taniguchi, Y. ; Tasca, L. ; Taylor, J. E. ; Trump, J. R. ; Zamorani, G. / The XMM-Newton wide-field survey in the COSMOS field : Statistical properties of clusters of galaxies. In: Astrophysical Journal, Supplement Series. 2007 ; Vol. 172, No. 1. pp. 182-195.

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title = "The XMM-Newton wide-field survey in the COSMOS field: Statistical properties of clusters of galaxies",

abstract = "We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the Cosmic Evolution Survey (COSMOS) field. We reach a depth for a total cluster flux in the 0.5-2 keVband of 3 × 10 -15 ergs cm -2 s -1, having one of the widest XMM-Newton contiguous raster surveys, covering an area of 2.1 deg 2. Cluster candidates are identified through a wavelet detection of extended X-ray emission. Verification of the cluster candidates is done based on a galaxy concentration analysis in redshift slices of thickness 0.1 -0.2 in redshift, using the multiband photometric catalog of the COSMOS field and restricting the search to z < 1.3 and i AB < 25. We identify 72 clusters and derive their properties based on the X-ray cluster scaling relations. A statistical description of the survey in terms of the cumulative log (N > S)-log S distribution compares well with previous results, although yielding a somewhat higher number of clusters at similar fluxes. The X-ray luminosity function of COSMOS clusters matches well the results of nearby surveys, providing a comparably tight constraint on the faint-end slope of α = 1.93 ±0.04. For the probed luminosity range of (8 × 10 42)-(2 × 10 44) ergs s -1, our survey is in agreement with and adds significantly to the existing data on the cluster luminosity function at high redshifts and implies no substantial evolution at these luminosities to z = 1.3.",

keywords = "Cosmology: observations, Dark matter, Large-scale structure of universe, Surveys",

author = "A. Finoguenov and L. Guzzo and G. Hasinger and Scoville, {N. Z.} and H. Aussel and H. B{\"o}hringer and M. Brusa and P. Capak and N. Cappelluti and A. Comastri and S. Giodini and Griffiths, {R. E.} and C. Impey and Koekemoer, {A. M.} and Kneib, {J. P.} and A. Leauthaud and {Le F{\`e}vre}, O. and S. Lilly and V. Mainieri and R. Massey and Mccracken, {H. J.} and B. Mobasher and T. Murayama and Peacock, {J. A.} and I. Sakelliou and E. Schinnerer and Silverman, {J. D.} and V. Smol{\v c}i{\'c} and Y. Taniguchi and L. Tasca and Taylor, {J. E.} and Trump, {J. R.} and G. Zamorani",

year = "2007",

doi = "10.1086/516577",

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T1 - The XMM-Newton wide-field survey in the COSMOS field

T2 - Statistical properties of clusters of galaxies

AU - Finoguenov, A.

AU - Guzzo, L.

AU - Hasinger, G.

AU - Scoville, N. Z.

AU - Aussel, H.

AU - Böhringer, H.

AU - Brusa, M.

AU - Capak, P.

AU - Cappelluti, N.

AU - Comastri, A.

AU - Giodini, S.

AU - Griffiths, R. E.

AU - Impey, C.

AU - Koekemoer, A. M.

AU - Kneib, J. P.

AU - Leauthaud, A.

AU - Le Fèvre, O.

AU - Lilly, S.

AU - Mainieri, V.

AU - Massey, R.

AU - Mccracken, H. J.

AU - Mobasher, B.

AU - Murayama, T.

AU - Peacock, J. A.

AU - Sakelliou, I.

AU - Schinnerer, E.

AU - Silverman, J. D.

AU - Smolčić, V.

AU - Taniguchi, Y.

AU - Tasca, L.

AU - Taylor, J. E.

AU - Trump, J. R.

AU - Zamorani, G.

PY - 2007

Y1 - 2007

N2 - We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the Cosmic Evolution Survey (COSMOS) field. We reach a depth for a total cluster flux in the 0.5-2 keVband of 3 × 10 -15 ergs cm -2 s -1, having one of the widest XMM-Newton contiguous raster surveys, covering an area of 2.1 deg 2. Cluster candidates are identified through a wavelet detection of extended X-ray emission. Verification of the cluster candidates is done based on a galaxy concentration analysis in redshift slices of thickness 0.1 -0.2 in redshift, using the multiband photometric catalog of the COSMOS field and restricting the search to z < 1.3 and i AB < 25. We identify 72 clusters and derive their properties based on the X-ray cluster scaling relations. A statistical description of the survey in terms of the cumulative log (N > S)-log S distribution compares well with previous results, although yielding a somewhat higher number of clusters at similar fluxes. The X-ray luminosity function of COSMOS clusters matches well the results of nearby surveys, providing a comparably tight constraint on the faint-end slope of α = 1.93 ±0.04. For the probed luminosity range of (8 × 10 42)-(2 × 10 44) ergs s -1, our survey is in agreement with and adds significantly to the existing data on the cluster luminosity function at high redshifts and implies no substantial evolution at these luminosities to z = 1.3.

AB - We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the Cosmic Evolution Survey (COSMOS) field. We reach a depth for a total cluster flux in the 0.5-2 keVband of 3 × 10 -15 ergs cm -2 s -1, having one of the widest XMM-Newton contiguous raster surveys, covering an area of 2.1 deg 2. Cluster candidates are identified through a wavelet detection of extended X-ray emission. Verification of the cluster candidates is done based on a galaxy concentration analysis in redshift slices of thickness 0.1 -0.2 in redshift, using the multiband photometric catalog of the COSMOS field and restricting the search to z < 1.3 and i AB < 25. We identify 72 clusters and derive their properties based on the X-ray cluster scaling relations. A statistical description of the survey in terms of the cumulative log (N > S)-log S distribution compares well with previous results, although yielding a somewhat higher number of clusters at similar fluxes. The X-ray luminosity function of COSMOS clusters matches well the results of nearby surveys, providing a comparably tight constraint on the faint-end slope of α = 1.93 ±0.04. For the probed luminosity range of (8 × 10 42)-(2 × 10 44) ergs s -1, our survey is in agreement with and adds significantly to the existing data on the cluster luminosity function at high redshifts and implies no substantial evolution at these luminosities to z = 1.3.

KW - Cosmology: observations

KW - Dark matter

KW - Large-scale structure of universe

KW - Surveys

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The XMM-Newton wide-field survey in the COSMOS field: Statistical properties of clusters of galaxies

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