The XMM-Newton Serendipitous Source Catalogue
arXiv:astro-ph/0211567 · doi:10.1002/asna.200310023
Abstract
We describe the production, properties and scientific potential of the XMM-Newton catalogue of serendipitous X-ray sources. The first version of this catalogue is nearing completion and is planned to be released before the end of 2002.
Proceedings of the "X-ray surveys, in the light of the new observatories" workshop, Astronomische Nachrichten, in the press (4 pages, 3 eps figures, uses an.cls)
References in corpus (4)
- The Chandra Deep Survey of the Hubble Deep Field North Area. IV. An Ultradeep Image of the HDF-N
- The XMM-Newton Serendipitous Survey I. The role of XMM-Newton Survey Science Centre
- The XMM-Newton Serendipitous Survey. II. First results from the AXIS high galactic latitude medium sensitivity survey
- The impact of spheroid stars for Macho microlensing surveys of the Andromeda Galaxy
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- Background-Source Separation in astronomical images with Bayesian probability theory (I): the method
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- Searching for compact objects in SNRs G27.8+0.6 and G28.8+1.5
- X-ray variability of sigma Orionis young stars with ROSAT
- ESO Imaging Survey: Optical follow-up of 12 selected XMM-Newton fields
- Matched Filters for Source Detection in the Poissonian Noise Regime
- Star formation history of Canis Major OB1 - II. A bimodal X-ray population revealed by XMM-Newton
- A serendipitous survey for galaxy clusters by the XMM-Newton Survey Science Center
- Maximum-likelihood detection of sources among Poissonian noise
- The XMM-SSC survey of hard-spectrum XMM-Newton sources 1: optically bright sources