A dataset provided by the European Space Agency

Name 012613
Title AB Dor: RGS wavelenght scale routine calibration


DOI 10.5270/esa-pwsfgqi
Author Dr Fred Jansen XMM-Newton PS
Publication Three years in the coronal life of AB Dor. I. Plasma emission measure distributions and abundances at different activity levels . Sanz-Forcada, J., Maggio, A., . A&A . 408-1087 . 2003 . 2003A&A...408.1087S ,
gamma Cassiopeiae: an X-ray Be star with personality . Lopes de Oliveira, R., Smith, M. A., . A&A . 512-22 . 2010 . 2010A&A...512A..22L ,
The XMM-Newton view of stellar coronae: X-ray spectroscopy of the corona of AB Doradus . Gudel, M., Audard, M., et all. . A&A . 365-336 . 2001 . 2001A&A...365L.336G ,
X-ray activity cycle on the active ultra-fast rotator AB Doradus A?. Implication of correlated coronal and photometric variability . Lalitha, S., Schmitt, J. H. M. M., . A&A . 559-119 . 2013 . 2013A&A...559A.119L ,
Simulated X-ray cycles in rapidly rotating solar-like stars . McIvor, T., Jardine, M., et all. . MNRAS . 367-592 . 2006 . 2006MNRAS.367..592M ,
The population of X-ray supernova remnants in the Large Magellanic Cloud . Maggi, P., Haberl, F., et all. . A&A . 585-162 . 2016 . 2016A&A...585A.162M ,
The Rotation of the Hot Gas around the Milky Way . Hodges-Kluck, Edmund J., Miller, Matthew J., . ApJ . 822-21 . 2016 . 2016ApJ...822...21H ,
Why solar astronomers should be interested in stars . Pallavicini, R., . AdSpR . 32-885 . 2003 . 2003AdSpR..32..885P ,
Identification of hig...
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2000-06-07T05:29:46Z/2000-06-07T21:53:16Z
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 2001-10-30T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2001-10-30T00:00:00Z, 012613, 17.56_20190403_1200. https://doi.org/10.5270/esa-pwsfgqi