A dataset provided by the European Space Agency

Name 012510
Title EPIC GAIN, CTE AND CONTAMINATION MONITORING-N132D
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0125100101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0125100201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0125100301

DOI 10.5270/esa-sk46pc0
Author Dr Fred Jansen XMM-Newton PS
Description CAL- During periods of low visibility, the primary target 1es0102 will be supplemented by observations of the bright LMC supernova remnant N132D. Due to source brightmess, small windows are used in EPIC -2.5ks overhead. Only UVW2 and UV grism usable in OM. Overhead 1ks per filter. A tempalate for a repeated observation without PA constraint is provided
Publication The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Quasi-stellar Object Selection Algorithm Using Time Variability and Machine Learning: Selection of 1620 Quasi-stellar Object Candidates from MACHO Large Magellanic Cloud Database . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 735-68 . 2011 . 2011ApJ...735...68K ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
A Refined QSO Selection Method Using Diagnostics Tests: 663 QSO Candidates in the Large Magellanic Cloud . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 747-107 . 2012 . 2012ApJ...747..107K ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
High-resolution X-ray spectroscopy and imaging of supernova remnant N132D . Behar, E., Rasmussen, A. P., et all. . A&A . 365-242 . 2001 . 2001A&A...365L.242B ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog . Georgakakis, A. E., Chavushyan, V., et all. ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-05-22T08:58:48Z/2000-05-23T20:08:23Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2002-02-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-02-20T00:00:00Z, 012510, 17.56_20190403_1200. https://doi.org/10.5270/esa-sk46pc0