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  The XMM-Newton serendipitous survey IX. The fourth XMM-Newton serendipitous source catalogue

Webb, N. A., Coriat, M., Traulsen, I., Ballet, J., Motch, C., Carrera, F. J., et al. (2020). The XMM-Newton serendipitous survey IX. The fourth XMM-Newton serendipitous source catalogue. Astronomy and Astrophysics, 641: A136. doi:10.1051/0004-6361/201937353.

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The XMM-Newton serendipitous survey IX. The fourth XMM-Newton serendipitous source catalogue.pdf (beliebiger Volltext), 617KB
 
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Webb, N. A., Autor
Coriat, M., Autor
Traulsen, I., Autor
Ballet, J., Autor
Motch, C., Autor
Carrera, F. J., Autor
Koliopanos, F., Autor
Authier, J., Autor
de la Calle, I., Autor
Ceballos, M. T., Autor
Colomo, E., Autor
Chuard, D., Autor
Freyberg, M.1, Autor           
Garcia, T., Autor
Kolehmainen, M., Autor
Lamer, G., Autor
Lin, D., Autor
Maggi, P., Autor
Michel, L., Autor
Page, C. G., Autor
Page, M. J., AutorPerea-Calderon, J. V., AutorPineau, F.-X., AutorRodriguez, P., AutorRosen, S. R., AutorLleo, M. Santos, AutorSaxton, R. D., AutorSchwope, A., AutorTomás, L., AutorWatson, M. G., AutorZakardjian, A., Autor mehr..
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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 Zusammenfassung: Context. Sky surveys produce enormous quantities of data on extensive regions of the sky. The easiest way to access this information is through catalogues of standardised data products. XMM-Newton has been surveying the sky in the X-ray, ultra-violet, and optical bands for 20 years.
Aims. The XMM-Newton Survey Science Centre has been producing standardised data products and catalogues to facilitate access to the serendipitous X-ray sky.
Methods. Using improved calibration and enhanced software, we re-reduced all of the 14 041 XMM-Newton X-ray observations, of which 11 204 observations contained data with at least one detection and with these we created a new, high quality version of the XMM-Newton serendipitous source catalogue, 4XMM-DR9.
Results. 4XMM-DR9 contains 810 795 detections down to a detection significance of 3σ, of which 550 124 are unique sources, which cover 1152 degrees2 (2.85%) of the sky. Filtering 4XMM-DR9 to retain only the cleanest sources with at least a 5σ detection significance leaves 433 612 detections. Of these detections, 99.6% have no pileup. Furthermore, 336 columns of information on each detection are provided, along with images. The quality of the source detection is shown to have improved significantly with respect to previous versions of the catalogues. Spectra and lightcurves are also made available for more than 288 000 of the brightest sources (36% of all detections).

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Sprache(n): eng - English
 Datum: 2020-09-23
 Publikationsstatus: Online veröffentlicht
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 Ort, Verlag, Ausgabe: -
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 Art der Begutachtung: -
 Identifikatoren: DOI: 10.1051/0004-6361/201937353
Anderer: LOCALID: 3270346
 Art des Abschluß: -

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Titel: Astronomy and Astrophysics
  Andere : Astron. Astrophys.
Genre der Quelle: Zeitschrift
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Ort, Verlag, Ausgabe: France : EDP Sciences S A
Seiten: - Band / Heft: 641 Artikelnummer: A136 Start- / Endseite: - Identifikator: ISSN: 1432-0746
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1