A dataset provided by the European Space Agency

Name 079571
Title Generic ToO-DDT Proposal for AO16
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795710101
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795712601

DOI 10.5270/esa-eim7kf4
Author Dr NORBERT SCHARTEL (PS)
Description 1) 1RXH J082623.6-505741 2) SDSS J1612+11 3) SDSS J1440+11 4) LSI +61 303 5) XMM J0244-455 6) IGR J17329-2731 7-10) MAXI J1535-571 11) SAX J1748.9-2021 12) Kelt-9 b 13-14) A-2017 U1 15) NGC 5907 ULX2
Publication A new ultraluminous X-ray source in the galaxy NGC 5907 . Pintore, F., Belfiore, A., et all. . MNRAS . 477-90 . 2018 . 2018MNRAS.477L..90P ,
IGR J17329-2731: The birth of a symbiotic X-ray binary . Bozzo, E., Bahramian, A., et all. . A&A . 613-22 . 2018 . 2018A&A...613A..22B ,
A faint outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021 in NGC 6440 . Pintore, F., Sanna, A., et all. . MNRAS . 479-4084 . 2018 . 2018MNRAS.479.4084P ,
A Population of Bona Fide Intermediate-mass Black Holes Identified as Low-luminosity Active Galactic Nuclei . Chilingarian, Igor V., Katkov, Ivan Yu., et all. . ApJ . 863-1 . 2018 . 2018ApJ...863....1C ,
A Spectral and Timing Study of MAXI J1535--571, Based on Swift-XRT, XMM-Newton, and NICER Observations Obtained in Fall 2017 . Stiele, H., Kong, A. K. H., . ApJ . 868-71 . 2018 . 2018ApJ...868...71S ,
A broad-band look of the accreting millisecond X-ray pulsar SAX J1748.9-2021 using AstroSat and XMM-Newton . Sharma, Rahul, Beri, Aru, et all. . MNRAS . 492-4361 . 2020 . 2020MNRAS.492.4361S ,
Diffuse X-ray emission around an ultraluminous X-ray pulsar . Belfiore, Andrea, Esposito, Paolo, et all. . NatAs . 4-147 . 2020 . 2020NatAs...4..147B ,
Evidence for periodic accretion-ejection in LS I +61u00b0303 . Massi, M., Chernyakova, M., et all. . MNRAS . 498-3592 . 2020 . ...,
Radio-X-ray correlations and variability in the X-ray binary LS I +61u00b0303 . Sharma, R., Massi, M., et all. . MNRAS . 500-4166 . 2021 . 2021MNRAS.500.4166S ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2017-06-13T21:26:52Z/2017-12-02T01:36:28Z
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 2018-06-12T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2018-06-12T22:00:00Z, 079571, 17.56_20190403_1200. https://doi.org/10.5270/esa-eim7kf4