The XXL Survey: VI. the 1000 brightest X-ray point sources

S. Fotopoulou, F. Pacaud, S. Paltani, P. Ranalli, M. E. Ramos-Ceja, L. Faccioli, M. Plionis, C. Adami, A. Bongiorno, M. Brusa, L. Chiappetti, S. Desai, A. Elyiv, C. Lidman, O. Melnyk, M. Pierre, E. Piconcelli, C. Vignali, S. Alis, F. ArdilaS. Arnouts, I. Baldry, M. Bremer, D. Eckert, L. Guennou, C. Horellou, A. Iovino, E. Koulouridis, J. Liske, S. Maurogordato, Felipe Menanteau, J. J. Mohr, M. Owers, B. Poggianti, E. Pompei, T. Sadibekova, A. Stanford, R. Tuffs, J. Willis

Research output: Contribution to journalReview article

Abstract

Context. X-ray extragalactic surveys are ideal laboratories for the study of the evolution and clustering of active galactic nuclei (AGN). Usually, a combination of deep and wide surveys is necessary to create a complete picture of the population. Deep X-ray surveys provide the faint population at high redshift, while wide surveys provide the rare bright sources. Nevertheless, very wide area surveys often lack the ancillary information available for modern deep surveys. The XXL survey spans two fields of a combined 50 deg2 observed for more than 6Ms with XMM-Newton, occupying the parameter space that lies between deep surveys and very wide area surveys; at the same time it benefits from a wealth of ancillary data. Aims. This paper marks the first release of the XXL point source catalogue including four optical photometry bands and redshift estimates. Our sample is selected in the 2 - 10 keV energy band with the goal of providing a sizable sample useful for AGN studies. The limiting flux is F2 - 10 keV = 4.8 × 10-14 erg s-1 cm-2. Methods. We use both public and proprietary data sets to identify the counterparts of the X-ray point-like sources by means of a likelihood ratio test. We improve upon the photometric redshift determination for AGN by applying a Random Forest classification trained to identify for each object the optimal photometric redshift category (passive, star forming, starburst, AGN, quasi-stellar objects (QSO)). Additionally, we assign a probability to each source that indicates whether it might be a star or an outlier. We apply Bayesian analysis to model the X-ray spectra assuming a power-law model with the presence of an absorbing medium. Results. We find that the average unabsorbed photon index is <Γ> = 1.85 ± 0.40 while the average hydrogen column density is log <NH> = 21.07 ± 1.2 cm-2. We find no trend of Γ or NH with redshift and a fraction of 26% absorbed sources (log NH> 22) consistent with the literature on bright sources (log Lx> 44). The counterpart identification rate reaches 96.7% for sources in the northern field, 97.7% for the southern field, and 97.2% in total. The photometric redshift accuracy is 0.095 for the full XMM-XXL with 28% catastrophic outliers estimated on a sample of 339 sources. Conclusions. We show that the XXL-1000-AGN sample number counts extended the number counts of the COSMOS survey to higher fluxes and are fully consistent with the Euclidean expectation. We constrain the intrinsic luminosity function of AGN in the 2 - 10 keV energy band where the unabsorbed X-ray flux is estimated from the X-ray spectral fit up to z = 3. Finally, we demonstrate the presence of a supercluster size structure at redshift 0.14, identified by means of percolation analysis of the XXL-1000-AGN sample. The XXL survey, reaching a medium flux limit and covering a wide area, is a stepping stone between current deep fields and planned wide area surveys.

Original languageEnglish (US)
Article numberA5
JournalAstronomy and Astrophysics
Volume592
DOIs
StatePublished - Jan 1 2016

Fingerprint

point sources
point source
active galactic nuclei
x rays
XMM-Newton telescope
outlier
energy bands
stars
likelihood ratio
Bayesian analysis
size structure
erg
newton
catalogs
photometry
energy
power law
coverings
luminosity
hydrogen

Keywords

  • Catalogs
  • Galaxies: active
  • Surveys
  • X-rays: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Fotopoulou, S., Pacaud, F., Paltani, S., Ranalli, P., Ramos-Ceja, M. E., Faccioli, L., ... Willis, J. (2016). The XXL Survey: VI. the 1000 brightest X-ray point sources. Astronomy and Astrophysics, 592, [A5]. https://doi.org/10.1051/0004-6361/201527402

The XXL Survey : VI. the 1000 brightest X-ray point sources. / Fotopoulou, S.; Pacaud, F.; Paltani, S.; Ranalli, P.; Ramos-Ceja, M. E.; Faccioli, L.; Plionis, M.; Adami, C.; Bongiorno, A.; Brusa, M.; Chiappetti, L.; Desai, S.; Elyiv, A.; Lidman, C.; Melnyk, O.; Pierre, M.; Piconcelli, E.; Vignali, C.; Alis, S.; Ardila, F.; Arnouts, S.; Baldry, I.; Bremer, M.; Eckert, D.; Guennou, L.; Horellou, C.; Iovino, A.; Koulouridis, E.; Liske, J.; Maurogordato, S.; Menanteau, Felipe; Mohr, J. J.; Owers, M.; Poggianti, B.; Pompei, E.; Sadibekova, T.; Stanford, A.; Tuffs, R.; Willis, J.

In: Astronomy and Astrophysics, Vol. 592, A5, 01.01.2016.

Research output: Contribution to journalReview article

Fotopoulou, S, Pacaud, F, Paltani, S, Ranalli, P, Ramos-Ceja, ME, Faccioli, L, Plionis, M, Adami, C, Bongiorno, A, Brusa, M, Chiappetti, L, Desai, S, Elyiv, A, Lidman, C, Melnyk, O, Pierre, M, Piconcelli, E, Vignali, C, Alis, S, Ardila, F, Arnouts, S, Baldry, I, Bremer, M, Eckert, D, Guennou, L, Horellou, C, Iovino, A, Koulouridis, E, Liske, J, Maurogordato, S, Menanteau, F, Mohr, JJ, Owers, M, Poggianti, B, Pompei, E, Sadibekova, T, Stanford, A, Tuffs, R & Willis, J 2016, 'The XXL Survey: VI. the 1000 brightest X-ray point sources', Astronomy and Astrophysics, vol. 592, A5. https://doi.org/10.1051/0004-6361/201527402
Fotopoulou S, Pacaud F, Paltani S, Ranalli P, Ramos-Ceja ME, Faccioli L et al. The XXL Survey: VI. the 1000 brightest X-ray point sources. Astronomy and Astrophysics. 2016 Jan 1;592. A5. https://doi.org/10.1051/0004-6361/201527402
Fotopoulou, S. ; Pacaud, F. ; Paltani, S. ; Ranalli, P. ; Ramos-Ceja, M. E. ; Faccioli, L. ; Plionis, M. ; Adami, C. ; Bongiorno, A. ; Brusa, M. ; Chiappetti, L. ; Desai, S. ; Elyiv, A. ; Lidman, C. ; Melnyk, O. ; Pierre, M. ; Piconcelli, E. ; Vignali, C. ; Alis, S. ; Ardila, F. ; Arnouts, S. ; Baldry, I. ; Bremer, M. ; Eckert, D. ; Guennou, L. ; Horellou, C. ; Iovino, A. ; Koulouridis, E. ; Liske, J. ; Maurogordato, S. ; Menanteau, Felipe ; Mohr, J. J. ; Owers, M. ; Poggianti, B. ; Pompei, E. ; Sadibekova, T. ; Stanford, A. ; Tuffs, R. ; Willis, J. / The XXL Survey : VI. the 1000 brightest X-ray point sources. In: Astronomy and Astrophysics. 2016 ; Vol. 592.
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abstract = "Context. X-ray extragalactic surveys are ideal laboratories for the study of the evolution and clustering of active galactic nuclei (AGN). Usually, a combination of deep and wide surveys is necessary to create a complete picture of the population. Deep X-ray surveys provide the faint population at high redshift, while wide surveys provide the rare bright sources. Nevertheless, very wide area surveys often lack the ancillary information available for modern deep surveys. The XXL survey spans two fields of a combined 50 deg2 observed for more than 6Ms with XMM-Newton, occupying the parameter space that lies between deep surveys and very wide area surveys; at the same time it benefits from a wealth of ancillary data. Aims. This paper marks the first release of the XXL point source catalogue including four optical photometry bands and redshift estimates. Our sample is selected in the 2 - 10 keV energy band with the goal of providing a sizable sample useful for AGN studies. The limiting flux is F2 - 10 keV = 4.8 × 10-14 erg s-1 cm-2. Methods. We use both public and proprietary data sets to identify the counterparts of the X-ray point-like sources by means of a likelihood ratio test. We improve upon the photometric redshift determination for AGN by applying a Random Forest classification trained to identify for each object the optimal photometric redshift category (passive, star forming, starburst, AGN, quasi-stellar objects (QSO)). Additionally, we assign a probability to each source that indicates whether it might be a star or an outlier. We apply Bayesian analysis to model the X-ray spectra assuming a power-law model with the presence of an absorbing medium. Results. We find that the average unabsorbed photon index is <Γ> = 1.85 ± 0.40 while the average hydrogen column density is log <NH> = 21.07 ± 1.2 cm-2. We find no trend of Γ or NH with redshift and a fraction of 26{\%} absorbed sources (log NH> 22) consistent with the literature on bright sources (log Lx> 44). The counterpart identification rate reaches 96.7{\%} for sources in the northern field, 97.7{\%} for the southern field, and 97.2{\%} in total. The photometric redshift accuracy is 0.095 for the full XMM-XXL with 28{\%} catastrophic outliers estimated on a sample of 339 sources. Conclusions. We show that the XXL-1000-AGN sample number counts extended the number counts of the COSMOS survey to higher fluxes and are fully consistent with the Euclidean expectation. We constrain the intrinsic luminosity function of AGN in the 2 - 10 keV energy band where the unabsorbed X-ray flux is estimated from the X-ray spectral fit up to z = 3. Finally, we demonstrate the presence of a supercluster size structure at redshift 0.14, identified by means of percolation analysis of the XXL-1000-AGN sample. The XXL survey, reaching a medium flux limit and covering a wide area, is a stepping stone between current deep fields and planned wide area surveys.",
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author = "S. Fotopoulou and F. Pacaud and S. Paltani and P. Ranalli and Ramos-Ceja, {M. E.} and L. Faccioli and M. Plionis and C. Adami and A. Bongiorno and M. Brusa and L. Chiappetti and S. Desai and A. Elyiv and C. Lidman and O. Melnyk and M. Pierre and E. Piconcelli and C. Vignali and S. Alis and F. Ardila and S. Arnouts and I. Baldry and M. Bremer and D. Eckert and L. Guennou and C. Horellou and A. Iovino and E. Koulouridis and J. Liske and S. Maurogordato and Felipe Menanteau and Mohr, {J. J.} and M. Owers and B. Poggianti and E. Pompei and T. Sadibekova and A. Stanford and R. Tuffs and J. Willis",
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T1 - The XXL Survey

T2 - VI. the 1000 brightest X-ray point sources

AU - Fotopoulou, S.

AU - Pacaud, F.

AU - Paltani, S.

AU - Ranalli, P.

AU - Ramos-Ceja, M. E.

AU - Faccioli, L.

AU - Plionis, M.

AU - Adami, C.

AU - Bongiorno, A.

AU - Brusa, M.

AU - Chiappetti, L.

AU - Desai, S.

AU - Elyiv, A.

AU - Lidman, C.

AU - Melnyk, O.

AU - Pierre, M.

AU - Piconcelli, E.

AU - Vignali, C.

AU - Alis, S.

AU - Ardila, F.

AU - Arnouts, S.

AU - Baldry, I.

AU - Bremer, M.

AU - Eckert, D.

AU - Guennou, L.

AU - Horellou, C.

AU - Iovino, A.

AU - Koulouridis, E.

AU - Liske, J.

AU - Maurogordato, S.

AU - Menanteau, Felipe

AU - Mohr, J. J.

AU - Owers, M.

AU - Poggianti, B.

AU - Pompei, E.

AU - Sadibekova, T.

AU - Stanford, A.

AU - Tuffs, R.

AU - Willis, J.

PY - 2016/1/1

Y1 - 2016/1/1

N2 - Context. X-ray extragalactic surveys are ideal laboratories for the study of the evolution and clustering of active galactic nuclei (AGN). Usually, a combination of deep and wide surveys is necessary to create a complete picture of the population. Deep X-ray surveys provide the faint population at high redshift, while wide surveys provide the rare bright sources. Nevertheless, very wide area surveys often lack the ancillary information available for modern deep surveys. The XXL survey spans two fields of a combined 50 deg2 observed for more than 6Ms with XMM-Newton, occupying the parameter space that lies between deep surveys and very wide area surveys; at the same time it benefits from a wealth of ancillary data. Aims. This paper marks the first release of the XXL point source catalogue including four optical photometry bands and redshift estimates. Our sample is selected in the 2 - 10 keV energy band with the goal of providing a sizable sample useful for AGN studies. The limiting flux is F2 - 10 keV = 4.8 × 10-14 erg s-1 cm-2. Methods. We use both public and proprietary data sets to identify the counterparts of the X-ray point-like sources by means of a likelihood ratio test. We improve upon the photometric redshift determination for AGN by applying a Random Forest classification trained to identify for each object the optimal photometric redshift category (passive, star forming, starburst, AGN, quasi-stellar objects (QSO)). Additionally, we assign a probability to each source that indicates whether it might be a star or an outlier. We apply Bayesian analysis to model the X-ray spectra assuming a power-law model with the presence of an absorbing medium. Results. We find that the average unabsorbed photon index is <Γ> = 1.85 ± 0.40 while the average hydrogen column density is log <NH> = 21.07 ± 1.2 cm-2. We find no trend of Γ or NH with redshift and a fraction of 26% absorbed sources (log NH> 22) consistent with the literature on bright sources (log Lx> 44). The counterpart identification rate reaches 96.7% for sources in the northern field, 97.7% for the southern field, and 97.2% in total. The photometric redshift accuracy is 0.095 for the full XMM-XXL with 28% catastrophic outliers estimated on a sample of 339 sources. Conclusions. We show that the XXL-1000-AGN sample number counts extended the number counts of the COSMOS survey to higher fluxes and are fully consistent with the Euclidean expectation. We constrain the intrinsic luminosity function of AGN in the 2 - 10 keV energy band where the unabsorbed X-ray flux is estimated from the X-ray spectral fit up to z = 3. Finally, we demonstrate the presence of a supercluster size structure at redshift 0.14, identified by means of percolation analysis of the XXL-1000-AGN sample. The XXL survey, reaching a medium flux limit and covering a wide area, is a stepping stone between current deep fields and planned wide area surveys.

AB - Context. X-ray extragalactic surveys are ideal laboratories for the study of the evolution and clustering of active galactic nuclei (AGN). Usually, a combination of deep and wide surveys is necessary to create a complete picture of the population. Deep X-ray surveys provide the faint population at high redshift, while wide surveys provide the rare bright sources. Nevertheless, very wide area surveys often lack the ancillary information available for modern deep surveys. The XXL survey spans two fields of a combined 50 deg2 observed for more than 6Ms with XMM-Newton, occupying the parameter space that lies between deep surveys and very wide area surveys; at the same time it benefits from a wealth of ancillary data. Aims. This paper marks the first release of the XXL point source catalogue including four optical photometry bands and redshift estimates. Our sample is selected in the 2 - 10 keV energy band with the goal of providing a sizable sample useful for AGN studies. The limiting flux is F2 - 10 keV = 4.8 × 10-14 erg s-1 cm-2. Methods. We use both public and proprietary data sets to identify the counterparts of the X-ray point-like sources by means of a likelihood ratio test. We improve upon the photometric redshift determination for AGN by applying a Random Forest classification trained to identify for each object the optimal photometric redshift category (passive, star forming, starburst, AGN, quasi-stellar objects (QSO)). Additionally, we assign a probability to each source that indicates whether it might be a star or an outlier. We apply Bayesian analysis to model the X-ray spectra assuming a power-law model with the presence of an absorbing medium. Results. We find that the average unabsorbed photon index is <Γ> = 1.85 ± 0.40 while the average hydrogen column density is log <NH> = 21.07 ± 1.2 cm-2. We find no trend of Γ or NH with redshift and a fraction of 26% absorbed sources (log NH> 22) consistent with the literature on bright sources (log Lx> 44). The counterpart identification rate reaches 96.7% for sources in the northern field, 97.7% for the southern field, and 97.2% in total. The photometric redshift accuracy is 0.095 for the full XMM-XXL with 28% catastrophic outliers estimated on a sample of 339 sources. Conclusions. We show that the XXL-1000-AGN sample number counts extended the number counts of the COSMOS survey to higher fluxes and are fully consistent with the Euclidean expectation. We constrain the intrinsic luminosity function of AGN in the 2 - 10 keV energy band where the unabsorbed X-ray flux is estimated from the X-ray spectral fit up to z = 3. Finally, we demonstrate the presence of a supercluster size structure at redshift 0.14, identified by means of percolation analysis of the XXL-1000-AGN sample. The XXL survey, reaching a medium flux limit and covering a wide area, is a stepping stone between current deep fields and planned wide area surveys.

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KW - Galaxies: active

KW - Surveys

KW - X-rays: general

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