A dataset provided by the European Space Agency

Name 083179
Title ToO-DDT proposal for AO17
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0831790101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0831790201
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0831790601
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0831791001
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0831791701

DOI 10.5270/esa-om6sm8r
Author Dr NORBERT SCHARTEL (PS)
Description Obs#3 1ES 1927+65 for Kara Obs#4 ASASSN-18fv Obs#5 Mrk 1310 Obs#6 Mrk 335 Obs#7 GSN 069 Obs#8 RT Cru obs#9 Sco X-1 obs#10 ASASSN-19bt (1st obs) obs#11 ASASSN-19bt (2nd obs) obs#12 Swift J1858.6-0814 obs#13 G358.931-0.030
Publication Nine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus . Miniutti, G., Saxton, R. D., et all. . Natur . 573-381 . 2019 . 2019Natur.573..381M ,
Discovery and Early Evolution of ASASSN-19bt, the First TDE Detected by TESS . Holoien, Thomas W. -S., Vallely, Patrick J., et all. . ApJ . 883-111 . 2019 . 2019ApJ...883..111H ,
1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months . Trakhtenbrot, Benny, Arcavi, Iair, et all. . ApJ . 883-94 . 2019 . 2019ApJ...883...94T ,
The nuclear environment of the NLS1 Mrk 335: Obscuration of the X-ray line emission by a variable outflow . Parker, M. L., Longinotti, A. L., et all. . MNRAS . 490-683 . 2019 . 2019MNRAS.490..683P ,
X-ray spectroscopy of the u03b3-ray brightest nova V906 Car (ASASSN-18fv) . Sokolovsky, Kirill V., Mukai, Koji, et all. . MNRAS . 497-2569 . 2020 . 2020MNRAS.497.2569S ,
Direct evidence for shock-powered optical emission in a nova . Aydi, Elias, Sokolovsky, Kirill V., et all. . NatAs . 4-776 . 2020 . 2020NatAs...4..776A ,
The Destruction and Recreation of the X-Ray Corona in a Changing-look Active Galactic Nucleus . Ricci, C., Kara, E., et all. . ApJ . 898-1 . 2020 . 2020ApJ...898L...1R ,
Soft X-ray emission lines in the X-ray binary Swift J1858.6-0814 observed with XMM-Newton Reflection Grating Spectrometer: disc atmosphere or wind? . Buisson, D. J. K., Altamirano...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2018-11-22T10:07:06Z/2019-04-16T10:22:57Z
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 2019-10-22T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2019-10-22T22:00:00Z, 083179, 17.56_20190403_1200. https://doi.org/10.5270/esa-om6sm8r