VizieR Online Data Catalog: XMM-Newton brightest serendipitous sources (Marelli+, 2016)
Abstract
Our deep XMM-Newton observation of PSR J2055+2539, lasting 136.2 ks, was performed on 2013 May 1 (ObsID 0724090101). The PN camera (Struder et al. 2001AJ....121.1413P) of the EPIC instrument was operating in Large Window mode, with a time resolution of 47.7 ms on a 27'x13' field of view (FOV). The high time resolution, combined with the large FOV, allows for both the timing analysis of the J2055 pulsar and the spatial analysis of the nebular structures. The Metal Oxide Semiconductor (MOS) detectors (Turner et al. 2001A&A...365L..27T) were set in full-frame mode (2.6 s time resolution on a 15' radius FOV). The thin optical filter was used for both PN and MOSs. We also analyzed XMM-Newton observations 0605470401 and 0605470901, taken on 2009 October 26 and on 2010 April 21, and lasting 24.5 and 17.9 ks, respectively.
(1 data file).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- February 2018
- DOI:
- 10.26093/cds/vizier.18190040
- Bibcode:
- 2018yCat..18190040M
- Keywords:
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- Pulsars;
- X-ray sources;
- Nebulae