A dataset provided by the European Space Agency

Name: A NEW CLASS OF HIGHLY ABSORBED PERSISTENT HMXB
Published: 2007-05-31T00:00:00Z

Proposal ID	030617
Title	A NEW CLASS OF HIGHLY ABSORBED PERSISTENT HMXB
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306170201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306170401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306170901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306171201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306172001
DOI	https://doi.org/10.5270/esa-hxfknyc
Principal Investigator, PI	Dr Roland Walter
Abstract	To date more than 40 new bright hard X-ray Galactic plane sources have beendiscovered with INTEGRAL, and 10 of them have follow-up observations withXMM-Newton or Chandra. In most cases, the X-ray data exhibit slow pulsations,and the absorbing column density appear much larger than expected in the Galaxyor in front of the companion star. Many of those sources are persistent and seemto belong to a new class of HMXB, with a slow pulsar orbiting in a densecircumstellar material or within the companion stellar envelope itself. The goalof this proposal is twofold. We propose (1) to observe several additionalpersistent new INTEGRAL sources and (2) to study more in depth a few alreadystudied sources.
Publications	The broad-band XMM-Newton and INTEGRAL spectra of bright type 1 Seyfert galaxies \|Panessa, F., Bassani, L., et al. \| A&A \| 483-151 \| 2008 \| 2008A&A...483..151P \| http://ui.adsabs.harvard.edu/#abs/2008A&A...483..151P INTEGRAL and XMM-Newton observations of AX J1845.0-0433 \|Zurita Heras, J. A., Walter, R., \| A&A \| 494-1013 \| 2009 \| 2009A&A...494.1013Z \| http://ui.adsabs.harvard.edu/#abs/2009A&A...494.1013Z The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The INTEGRAL complete sample of type 1 AGN \|Molina, M., Bassani, L., et al. \| MNRAS \| 399-1293 \| 2009 \| 2009MNRAS.399.1293M \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.399.1293M IGR J17254-3257, a new bursting neutron star \|Chenevez, J., Falanga, M., et al. \| A&A \| 469-27 \| 2007 \| 2007A&A...469L..27C \| http://ui.adsabs.harvard.edu/#abs/2007A&A...469L..27C Discovery of an Energetic 38.5 ms Pulsar Powering the Gamma-ray Source IGR J18490-0000/HESS J1849-000 \|Gotthelf, E. V., Halpern, J. P., et al. \| ApJ \| 729-16 \| 2011 \| 2011ApJ...729L..16G \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...729L..16G The Galactic plane at faint X-ray fluxes - I. Properties and characteristics of the X-ray source population \|Warwick, R. S., Perez-Ramirez, D., \| MNRAS \| 413-595 \| 2011 \| 2011MNRAS.413..595W \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.413..595W Fe Kalpha line profile in AGNs: average shape and redshift dependence \|Mao, Wei-Ming, Hu, Chen, et al. \| RAA \| 10-905 \| 2010 \| 2010RAA....10..905M \| http://ui.adsabs.harvard.edu/#abs/2010RAA....10..905M Searching for X-ray emission from AGB stars \|Ramstedt, S., Montez, R., et al. \| A&A \| 543-147 \| 2012 \| 2012A&A...543A.147R \| http://ui.adsabs.harvard.edu/#abs/2012A&A...543A.147R The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L 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 The INTEGRAL High-energy Cut-off Distribution of Type 1 Active Galactic Nuclei \|Malizia, A., Molina, M., et al. \| ApJ \| 782-25 \| 2014 \| 2014ApJ...782L..25M \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...782L..25M 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 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 Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X Interstellar Dust Properties from a Survey of X-Ray Halos \|Valencic, Lynne A., Smith, Randall K., \| ApJ \| 809-66 \| 2015 \| 2015ApJ...809...66V \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...809...66V X-ray spectral parameters for a sample of 95 active galactic nuclei \|Vasylenko, A. A., Zhdanov, V. I., \| Ap&SS \| 360-71 \| 2015 \| 2015Ap&SS.360...71V \| http://ui.adsabs.harvard.edu/#abs/2015Ap&SS.360...71V A hard X-ray view of the soft excess in AGN \|Boissay, Rozenn, Ricci, Claudio, \| A&A \| 588-70 \| 2016 \| 2016A&A...588A..70B \| http://ui.adsabs.harvard.edu/#abs/2016A&A...588A..70B 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 The accretion environment of supergiant fast X-ray transients probed with XMM-Newton \|Bozzo, E., Bernardini, F., et al. \| A&A \| 608-128 \| 2017 \| 2017A&A...608A.128B \| http://ui.adsabs.harvard.edu/#abs/2017A&A...608A.128B Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz, Tobias, \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V 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 Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Ancient Pulsar Wind Nebulae as a natural explanation for unidentified gamma-ray sources \|Kaufmann, S., Tibolla, O., \| NPPP \| 297-91 \| 2018 \| 2018NPPP..297...91K \| http://ui.adsabs.harvard.edu/#abs/2018NPPP..297...91K Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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 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	2006-03-01T04:26:07Z/2006-04-04T00:34:14Z
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	2007-05-31T00:00:00Z
Keywords	"companion star", "companion stellar envelope", "XMM", "additional persistent", "absorbed persistent hmxb", "XMM-Newton", "slow pulsar orbiting", "absorbing column density", "dense circumstellar material", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Roland Walter, 2007, 'A NEW CLASS OF HIGHLY ABSORBED PERSISTENT HMXB', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hxfknyc