A dataset provided by the European Space Agency

Name 041440
Title XMM long wavelength response (cross-calibration, RCO)
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0414400101

DOI 10.5270/esa-k0rybhv
Author Dr Arvind Parmar XMM-Newton MM
Description
Publication A detailed X-ray investigation of zeta Puppis. I. The dataset and some preliminary results . Naze, Y., Flores, C. A., . A&A . 538-22 . 2012 . 2012A&A...538A..22N ,
X-rays, clumping and wind structures . Oskinova, Lidia, Hamann, Wolf-Rainer, et all. . BSRSL . 80-54 . 2011 . 2011BSRSL..80...54O ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
Hot stars observed by XMM-Newton. I. The catalog and the properties of OB stars . Naze, Y., . A&A . 506-1055 . 2009 . 2009A&A...506.1055N ,
A Detailed X-Ray Investigation of zeta Puppis. II. The Variability on Short and Long Timescales . Naze, Yael, Oskinova, Lidia M., . ApJ . 763-143 . 2013 . 2013ApJ...763..143N ,
Constraints on the Ubiquity of Coronal X-Ray Cycles . Hoffman, John, Gunther, Hans M., . ApJ . 759-145 . 2012 . 2012ApJ...759..145H ,
A detailed X-ray investigation of zeta Puppis. III. Spectral analysis of the whole RGS spectrum . Herve, A., Rauw, G., . A&A . 551-83 . 2013 . 2013A&A...551A..83H ,
Constraints on Porosity and Mass Loss in O-star Winds from the Modeling of X-Ray Emission Line Profile Shapes . Leutenegger, Maurice A...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-04-09T14:05:18Z/2007-04-10T07:50:28Z
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 2007-04-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-04-10T00:00:00Z, 041440, 17.56_20190403_1200. https://doi.org/10.5270/esa-k0rybhv