A dataset provided by the European Space Agency

Name 056158
Title Generic non-GRB ToO proposal


DOI 10.5270/esa-6dxeze0
Description 1) XTE 1739-302 2) DDT: REJ1034+396 3) DDT: U Sco, eclipse mapping
Publication Swift X-Ray Observations of Classical Novae. II. The Super Soft Source Sample . Schwarz, Greg J., Ness, Jan-Uwe, et all. . ApJS . 197-31 . 2011 . 2011ApJS..197...31S ,
From X-Ray Dips to Eclipse: Witnessing Disk Reformation in the Recurrent Nova U Sco . Ness, J.-U., Schaefer, B. E., et all. . ApJ . 745-43 . 2012 . 2012ApJ...745...43N ,
Evolution of the spectral curvature in the ultraluminous X-ray source Holmberg II X-1 . Kajava, J. J. E., Poutanen, J., et all. . MNRAS . 422-990 . 2012 . 2012MNRAS.422..990K ,
Searching for the trigger of the active galactic nucleus quasi-periodic oscillation: 8 years of RE J1034+396 . Middleton, Matthew, Uttley, Phil, . MNRAS . 417-250 . 2011 . 2011MNRAS.417..250M ,
The supergiant fast X-ray transients XTE J1739-302 and IGR J08408-4503 in quiescence with XMM-Newton . Bozzo, E., Stella, L., et all. . A&A . 519-6 . 2010 . 2010A&A...519A...6B ,
X-ray reverberation close to the black hole in RE J1034+396 . Zoghbi, A., Fabian, A. C., . MNRAS . 418-2642 . 2011 . 2011MNRAS.418.2642Z ,
X-ray variability of 104 active galactic nuclei. XMM-Newton power-spectrum density profiles . Gonzalez-Martin, O., Vaughan, S., . A&A . 544-80 . 2012 . 2012A&A...544A..80G ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-03-11T14:53:28Z/2010-03-27T00:18:20Z
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 2010-10-22T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-10-22T00:00:00Z, 056158, 17.56_20190403_1200. https://doi.org/10.5270/esa-6dxeze0