English

The XMM-LSS catalogue: X-ray sources and associated optical data. Version I

Astrophysics 2015-12-15 v1

Abstract

Following the presentation of the XMM-LSS X-ray source detection package by Pacaud et al., we provide the source lists for the first 5.5 surveyed square degrees. The catalogues pertain to the [0.5-2] and [2-10] keV bands and contain in total 3385 point-like or extended sources above a detection likelihood of 15 in either band. The agreement with deep logN-logS is excellent. The main parameters considered are position, countrate, source extent with associated likelihood values. A set of additional quantities such as astrometric corrections and fluxes are further calculated while errors on the position and countrate are deduced from simulations. We describe the construction of the band-merged catalogue allowing rapid sub-sample selection and easy cross-correlation with external multi-wavelength catalogues. A small optical CFHTLS multi-band subset of objects is associated wich each source along with an X-ray/optical overlay. We make the full X-ray images available in FITS format. The data are available at CDS and, in a more extended form, at the Milan XMM-LSS database.

Keywords

Cite

@article{arxiv.0708.3299,
  title  = {The XMM-LSS catalogue: X-ray sources and associated optical data. Version I},
  author = {M. Pierre and L. Chiappetti and F. Pacaud and A. Gueguen and C. Libbrecht and B. Altieri and H. Aussel and P. Gandhi and O. Garcet and E. Gosset and L. Paioro and T. J. Ponman and A. M. Read and A. Refregier and J. -L. Starck and J. Surdej and I. Valtchanov and C. Adami and D. Alloin and A. Alshino and S. Andreon and M. Birkinshaw and M. Bremer and A. Detal and P. -A. Duc and G. Galaz and L. Jones and J. -P. Le Fèvre and O. Le Fèvre and D. Maccagni and A. Mazure and H. Quintana and H. J. A. Röttgering and P. -G. Sprimont and C. Tasse and G. Trinchieri and J. P. Willis},
  journal= {arXiv preprint arXiv:0708.3299},
  year   = {2015}
}

Comments

13 pages, 7 figures and 11 tables (fig. 1 and 6 are enclosed in reduced resolution), MNRAS Latex, accepted by MNRAS

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