A dataset provided by the European Space Agency

Name: ToO proposal for AO18
Published: 2020-07-28T22:00:00Z

Proposal ID	085398
Title	ToO proposal for AO18
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853980101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853980201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853980301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853980401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853980601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853980701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853980801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853980901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853981001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853981101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853981201 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853981301
DOI	https://doi.org/10.5270/esa-opkbde9
Principal Investigator, PI	Dr NORBERT SCHARTEL (PS)
Abstract	#1 V378 Vul (Y. Sugawara)#2 AT2018fyk (D. Pasham)#3 XTE J1739-285 (A. Sanna)#5 NGC7793-P13 (R. Soria)#6 KS 1947+300 (N. La Palombara)#7 PKS 2004-447 (R. Ojha)#8 MAXI J0637-430 (M. Armas-Padilla)#9 SXP 1062 (S. Tsygankov)#10 SDSS J203047.34+041330.9 (R. Saxton)
Publications	The unusual behavior of the young X-ray pulsar SXP 1062 during the 2019 outburst \|Tsygankov Sergey S. Doroshenko Victor et al. \| A&A \| 637-33 \| 2020 \| 2020A&A...637A..33T \| http://ui.adsabs.harvard.edu/#abs/2020A&A...637A..33T A new candidate pulsating ULX in NGC 7793 \|Quintin E. Webb N. A. et al. \| MNRAS \| 503-5485 \| 2021 \| 2021MNRAS.503.5485Q \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5485Q The first GeV flare of the radio-loud narrow-line Seyfert 1 galaxy PKS 2004-447 \|Gokus A. Paliya V. S. et al. \| A&A \| 649-77 \| 2021 \| 2021A&A...649A..77G \| http://ui.adsabs.harvard.edu/#abs/2021A&A...649A..77G Rapid Accretion State Transitions following the Tidal Disruption Event AT2018fyk \|Wevers T. Pasham D. R. et al. \| ApJ \| 912-151 \| 2021 \| 2021ApJ...912..151W \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912..151W Long-term pulse period evolution of the ultra-luminous X-ray pulsar NGC 7793 P13 \|Fu00fcrst F. Walton D. J. et al. \| A&A \| 651-75 \| 2021 \| 2021A&A...651A..75F \| http://ui.adsabs.harvard.edu/#abs/2021A&A...651A..75F Quest for the Upcoming Periastron Passage of an Episodic Dust Maker and Particle-accelerating Colliding-wind Binary: WR 125 \|Arora Bharti Pandey J. C. et al. \| AJ \| 162-257 \| 2021 \| 2021AJ....162..257A \| http://ui.adsabs.harvard.edu/#abs/2021AJ....162..257A Investigation of the Timing and Spectral Properties of an Ultraluminous X-Ray Pulsar NGC 7793 P13 \|Lin Lupin Chun-Che Hu Chin-Ping et al. \| ApJ \| 924-65 \| 2022 \| 2022ApJ...924...65L \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...924...65L XMM-Newton detection of soft time lags in the TDE candidate AT 2018fyk \|Zhang Wenda \| MNRAS \| 511-19 \| 2022 \| 2022MNRAS.511L...9Z \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.511L...9Z XMM-Newton detection of soft time lags in the TDE candidate AT 2018fyk \|Zhang Wenda \| MNRAS \| 511-19 \| 2022 \| 2022MNRAS.511L..19Z \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.511L..19Z X-ray emission from the microquasar S26 observed by XMM-Newton \|Rizzo F. N. Sotomayor Checa P. \| BAAA \| 63-283 \| 2022 \| 2022BAAA...63..283R \| http://ui.adsabs.harvard.edu/#abs/2022BAAA...63..283R The peculiar spectral evolution of the new X-ray transient MAXI J0637-430 \|Ma R. C. Soria R. et al. \| MNRAS \| 514-5238 \| 2022 \| 2022MNRAS.514.5238M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514.5238M Research on the Magnetic Field of NGC 7793 P13 and Other Confirmed Pulsating Ultraluminous X-Ray Sources \|Meng Fan-Liang Pan Yuan-Yue \| RAA \| 22-115018 \| 2022 \| 2022RAA....22k5018M \| http://ui.adsabs.harvard.edu/#abs/2022RAA....22k5018M From X-rays to physical parameters: a comprehensive analysis of thermal tidal disruption event X-ray spectra \|Mummery Andrew Wevers Thomas et al. \| MNRAS \| 519-5828 \| 2023 \| 2023MNRAS.519.5828M \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519.5828M The current state of disk wind observations in BHLMXBs through X-ray absorption lines in the iron band \|Parra M. Petrucci P. -O. et al. \| A&A \| 681-49 \| 2024 \| 2024A&A...681A..49P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...681A..49P The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P A Systematic Analysis of the X-Ray Emission in Optically Selected Tidal Disruption Events: Observational Evidence for the Unification of the Optically and X-Ray-selected Populations \|Guolo Muryel Gezari Suvi et al. \| ApJ \| 966-160 \| 2024 \| 2024ApJ...966..160G \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...966..160G From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-10-02T12:09:36Z/2019-12-02T14:40:20Z
Version	PPS_NOT_AVAILABLE
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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	2020-07-28T22:00:00Z
Last Update	2025-01-27
Keywords	"2004 447", "la palombara", "SDSS", "maxi j0637 430", "armas padilla", "ngc7793 p13", "xte j1739 285", "sxp 1062", "v378 vul", "sdss j203047", "NGC7793"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr NORBERT SCHARTEL (PS), 2020, 'ToO proposal for AO18', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-opkbde9