A dataset provided by the European Space Agency

Name 041299
Title EPIC Gain, contamination and CTI monitoring-Vela SNR
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990601
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991301
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991601

DOI 10.5270/esa-cttuza4
Author Dr Fred Jansen XMM-Newton MM
Description EPIC Routine Calibration: spectral capabilities and contamination monitoring PA=102 shall be used as default (was proposal 015976). obs1: exceptionally pointed at RA 08:49:30.0 Dec -45:35:00 (req. by K. Dennerl) (normally at RA 08:48:49.05 Dec -45:38:26.1) obs6: coord. changed to RA 08:48:49 Dec -45:38:27 (req. by K. Dennerl)
Publication Is Vela Jr. a young supernova remnant? . Katsuda, Satoru, Tsunemi, Hiroshi, . AdSpR . 43-895 . 2009 . 2009AdSpR..43..895K ,
The X-ray spectral signatures from the complex circumnuclear regions in the Compton thick AGN NGC 424 . Marinucci, A., Bianchi, S., et all. . A&A . 526-36 . 2011 . 2011A&A...526A..36M ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
Nonthermal emission properties of the northwestern rim of supernova remnant RX J0852.0-4622 . Kishishita, T., Hiraga, J., . A&A . 551-132 . 2013 . 2013A&A...551A.132K ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
A survey of stellar X-ray flares from the XMM-Newton serendipitous source catalogue: HIPPARCOS-Tycho cool stars . Pye...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-11-09T00:38:22Z/2017-10-31T09:44:04Z
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 2017-11-06T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-11-06T23:00:00Z, 041299, 17.56_20190403_1200. https://doi.org/10.5270/esa-cttuza4