A dataset provided by the European Space Agency

Name: Generic ToO/DDT Proposal for AO16
Published: 2018-06-12T22:00:00Z

Proposal ID	079571
Title	Generic ToO/DDT Proposal for AO16
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795710101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795711301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795711401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795711501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795711701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795711801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795711901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795712001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795712101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795712201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795712301 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795712401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795712601
DOI	https://doi.org/10.5270/esa-eim7kf4
Principal Investigator, PI	Dr NORBERT SCHARTEL (PS)
Abstract	1) 1RXH J082623.6-505741 2) SDSS J1612+113) SDSS J1440+11 4) LSI +61 3035) XMM J0244-455 6) IGR J17329-27317-10) MAXI J1535-571 11) SAX J1748.9-2021 12) Kelt-9 b 13-14) A/2017 U115) NGC 5907 ULX2
Publications	A new ultraluminous X-ray source in the galaxy NGC 5907 \|Pintore F. Belfiore A. et al. \| MNRAS \| 477-90 \| 2018 \| 2018MNRAS.477L..90P \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477L..90P IGR J17329-2731: The birth of a symbiotic X-ray binary \|Bozzo E. Bahramian A. et al. \| A&A \| 613-22 \| 2018 \| 2018A&A...613A..22B \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 479-4084 \| 2018 \| 2018MNRAS.479.4084P \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 863-1 \| 2018 \| 2018ApJ...863....1C \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 492-4361 \| 2020 \| 2020MNRAS.492.4361S \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.492.4361S Diffuse X-ray emission around an ultraluminous X-ray pulsar \|Belfiore Andrea Esposito Paolo et al. \| NatAs \| 4-147 \| 2020 \| 2020NatAs...4..147B \| http://ui.adsabs.harvard.edu/#abs/2020NatAs...4..147B Evidence for periodic accretion-ejection in LS I +61u00b0303 \|Massi M. Chernyakova M. et al. \| MNRAS \| 498-3592 \| 2020 \| 2020MNRAS.498.3592M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.498.3592M Radio/X-ray correlations and variability in the X-ray binary LS I +61u00b0303 \|Sharma R. Massi M. et al. \| MNRAS \| 500-4166 \| 2021 \| 2021MNRAS.500.4166S \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.4166S Fast infrared variability from the black hole candidate MAXI J1535-571 and tight constraints on the modelling \|Vincentelli F. M. Casella P. et al. \| MNRAS \| 503-614 \| 2021 \| 2021MNRAS.503..614V \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503..614V Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Science with the AstroSat Soft X-ray telescope: An overview \|Bhattacharyya Sudip Singh Kulinder Pal et al. \| JApA \| 42-17 \| 2021 \| 2021JApA...42...17B \| http://ui.adsabs.harvard.edu/#abs/2021JApA...42...17B Modelling multiwavelength emission of Ultra-luminous X-ray Sources accreting above the Eddington limit \|Ambrosi E. Zampieri L. et al. \| MNRAS \| 509-4694 \| 2022 \| 2022MNRAS.509.4694A \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.4694A 1RXH J082623.6-505741: A New Long-period Cataclysmic Variable with an Evolved Donor and a Low Mass-transfer Rate \|Sokolovsky Kirill V. Strader Jay et al. \| ApJ \| 934-142 \| 2022 \| 2022ApJ...934..142S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...934..142S 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 Properties of Milky Way globular clusters associated with X-ray sources \|Botev Svetoslav Nedialkov Petko \| BlgAJ \| 40-59 \| 2024 \| 2024BlgAJ..40...59B \| http://ui.adsabs.harvard.edu/#abs/2024BlgAJ..40...59B Energy dependence of quasi-periodic oscillations in accreting X-ray pulsars \|Manikantan Hemanth Paul Biswajit et al. \| MNRAS \| 531-530 \| 2024 \| 2024MNRAS.531..530M \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.531..530M 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 Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2017-06-13T21:26:52Z/2017-12-02T01:36:28Z
Version	19.17_20220121_1250
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	2018-06-12T22:00:00Z
Last Update	2025-01-27
Keywords	"maxi j1535 571", "igr j17329 2731", "sdss j1612", "SDSS", "sax j1748", "1rxh j082623", "2017 u1", "J1748.9", "sdss j1440", "XMM", "NGC 5907", "xmm j0244 455", "ngc 5907 ulx2"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr NORBERT SCHARTEL (PS), 2018, 'Generic ToO/DDT Proposal for AO16', 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-eim7kf4