A dataset provided by the European Space Agency

Name: X-ray follow-up observations of known transient INTEGRAL sources
Published: 2012-03-15T00:00:00Z

Proposal ID	040518
Title	X-ray follow-up observations of known transient INTEGRAL sources
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405180501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405181901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405182701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405183801
DOI	https://doi.org/10.5270/esa-msb2apq
Principal Investigator, PI	Dr Lara Sidoli
Abstract	We propose to trigger a maximum of 5 XMM follow-up observations on knowntransient sources discovered with INTEGRAL Observatory,if they undergo a newoutburst during AO5. We ask for 20 ks per observation,usign EPIC PN as primaryinstrument, in order to get a high-quality X-ray spectrum.XMM spectral andspatial capabilities are essential in unveiling their nature (still unknown forthe select targets), and in refining their sky positions, enablingmultiwavelength follow-up observations.
Publications	An alternative hypothesis for the outburst mechanism in supergiant fast X-ray transients: the case of IGR J11215-5952 \|Sidoli L. Romano P. et al. \| A&A \| 476-1307 \| 2007 \| 2007A&A...476.1307S \| http://ui.adsabs.harvard.edu/#abs/2007A&A...476.1307S The XMM-Newton view of supergiant fast X-ray transients: the case of IGR J16418-4532 \|Sidoli L. Mereghetti S. et al. \| MNRAS \| 420-554 \| 2012 \| 2012MNRAS.420..554S \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.420..554S XMM-Newton and INTEGRAL observations of the very faint X-ray transient IGR J17285-2922/XTE J1728-295 during the 2010 outburst \|Sidoli L. Paizis A. et al. \| MNRAS \| 415-2373 \| 2011 \| 2011MNRAS.415.2373S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.415.2373S General X-ray properties of hot massive stars \|Naze Yael \| BSRSL \| 80-109 \| 2011 \| 2011BSRSL..80..109N \| http://ui.adsabs.harvard.edu/#abs/2011BSRSL..80..109N Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin Dacheng Webb Natalie A. \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L Automatic Classification of Time-variable X-Ray Sources \|Lo Kitty K. Farrell Sean et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y An XMM-Newton view of FeKalpha in high-mass X-ray binaries \|Gimenez-Garcia A. Torrejon J. M. et al. \| A&A \| 576-108 \| 2015 \| 2015A&A...576A.108G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...576A.108G The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Modelling the effect of absorption from the interstellar medium on transient black hole X-ray binaries \|Eckersall A. J. Vaughan S. \| MNRAS \| 471-1468 \| 2017 \| 2017MNRAS.471.1468E \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1468E Supergiant fast X-ray transients versus classical supergiant high mass X-ray binaries: Does the difference lie in the companion wind? \|Pradhan P. Bozzo E. \| A&A \| 610-50 \| 2018 \| 2018A&A...610A..50P \| http://ui.adsabs.harvard.edu/#abs/2018A&A...610A..50P Supergiant Fast X-ray Transients uncovered by the EXTraS project: flares reveal the development of magnetospheric instability in accreting neutron stars \|Sidoli Lara Postnov Konstantin A. et al. \| MNRAS \| 487-420 \| 2019 \| 2019MNRAS.487..420S \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487..420S The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters \|Pastor-Marazuela I. Webb N. A. et al. \| A&A \| 640-124 \| 2020 \| 2020A&A...640A.124P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...640A.124P 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 Statistical Properties of X-Ray Flares from the Supergiant Fast X-Ray Transients \|Zhang Wen-Long Yi Shuang-Xi et al. \| RAA \| 22-65012 \| 2022 \| 2022RAA....22f5012Z \| http://ui.adsabs.harvard.edu/#abs/2022RAA....22f5012Z 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 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	2007-02-09T16:23:25Z/2011-02-24T00:32:26Z
Version	17.56_20190403_1200
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	2012-03-15T00:00:00Z
Last Update	2025-01-27
Keywords	"EPIC", "x ray", "select targets", "transient sources", "quality xray spectrum", "XMM", "integral observatory", "sky positions", "xmm spectral", "usign epic pn", "primary instrument", "transient integral sources"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Lara Sidoli, 2012, 'X-ray follow-up observations of known transient INTEGRAL sources', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-msb2apq