A dataset provided by the European Space Agency

Name: New ROSAT discovered Intermediate Polars in the Galactic Plane TS_30
Published: 2005-11-01T00:00:00Z

Proposal ID	010546
Title	New ROSAT discovered Intermediate Polars in the Galactic Plane TS_30
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460801
DOI	https://doi.org/10.5270/esa-vd8c7y9
Principal Investigator, PI	Dr Bernd Aschenbach
Abstract	GT-XMM observations of newly discovered intermediate polars (IPs) are proposed.Broad band pulse phase resolved spectroscopy will allow to investigate thedifferent emission components observed in the X-ray spectra of IPs. The largecollecting area and high spectral resolution of the EPIC detectors will providehigh quality spectra for a detailed modeling to get insight into the accretionprocess close to the surface of the white dwarf. RXJ1914.4+2456 is of particularinterest. It was proposed as candidate for a soft IP or might be the firstdouble-degenerate polar in which case the 569 s period would indicate theorbital period. We propose a 2nd observation about one year after that ofK. Mason to follow the period history.
Publications	X-ray and optical observations of 1RXS J154814.5-452845: A new intermediate polar with soft X-ray emission \|Haberl, F., Motch, C., \| A&A \| 387-201 \| 2002 \| 2002A&A...387..201H \| http://ui.adsabs.harvard.edu/#abs/2002A&A...387..201H The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M 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 XMM-Newton and Chandra observations of the ultra-compact binary RX J1914 + 24 \|Ramsay, Gavin, Cropper, Mark, \| MNRAS \| 367-62 \| 2006 \| 2006MNRAS.367L..62R \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367L..62R The X-ray spectrum of RX J1914.4+2456 revisited \|Ramsay, Gavin, \| MNRAS \| 384-687 \| 2008 \| 2008MNRAS.384..687R \| http://ui.adsabs.harvard.edu/#abs/2008MNRAS.384..687R A new search strategy for microquasar candidates using NVSS/2MASS and XMM-Newton data \|Combi, J. A., Albacete-Colombo, J. F., \| A&A \| 477-125 \| 2008 \| 2008A&A...477..125C \| http://ui.adsabs.harvard.edu/#abs/2008A&A...477..125C Identifying XMM-Newton observations affected by solar wind charge exchange. Part I \|Carter, J. A., Sembay, S., \| A&A \| 489-837 \| 2008 \| 2008A&A...489..837C \| http://ui.adsabs.harvard.edu/#abs/2008A&A...489..837C Why Do Some Intermediate Polars Show Soft X-Ray Emission? A Survey of XMM-Newton Spectra \|Evans, P. A., Hellier, Coel, \| ApJ \| 663-1277 \| 2007 \| 2007ApJ...663.1277E \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...663.1277E Wavelet and R/S analysis of the X-ray flickering of cataclysmic variables \|Anzolin, G., Tamburini, F., et al. \| A&A \| 519-69 \| 2010 \| 2010A&A...519A..69A \| http://ui.adsabs.harvard.edu/#abs/2010A&A...519A..69A An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog \|Georgakakis, A. E., Chavushyan, V., et al. \| MNRAS \| 367-1017 \| 2006 \| 2006MNRAS.367.1017G \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G 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 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 An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H The XMM-Newton serendipitous source catalogue \|Watson, M. G., Pye, J. P., et al. \| AN \| 324-89 \| 2003 \| 2003AN....324...89W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...89W The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca, A., Molendi, S., \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D 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 GEMINI Spectroscopy of the Ultracompact Binary Candidate V407 Vulpeculae \|Steeghs, D., Marsh, T. R., et al. \| ApJ \| 649-382 \| 2006 \| 2006ApJ...649..382S \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...649..382S 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 The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 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 Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals \|Sibeck, David G., Allen, R., et al. \| SSRv \| 214-79 \| 2018 \| 2018SSRv..214...79S \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S 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 The Spectrum of the Universe \|Hill, Ryley, Masui, Kiyoshi W., \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H X-Ray Observations of an Intermediate Polar V2400 Oph \|Joshi, Arti, Pandey, J. C., \| AJ \| 158-11 \| 2019 \| 2019AJ....158...11J \| http://ui.adsabs.harvard.edu/#abs/2019AJ....158...11J 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 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 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 An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q Comptonization as an Origin of the Continuum in Intermediate Polars \|Maiolino, T., Titarchuk, L., et al. \| ApJ \| 911-80 \| 2021 \| 2021ApJ...911...80M \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...911...80M 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 The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q A Study on White Dwarf Masses in Cataclysmic Variables Based on XMM-Newton and Suzaku Observations \|Yu, Zhuo-Li, Xu, Xiao-Jie, \| RAA \| 22-45003 \| 2022 \| 2022RAA....22d5003Y \| http://ui.adsabs.harvard.edu/#abs/2022RAA....22d5003Y Measuring the ICM velocity structure in the Ophiuchus cluster \|Gatuzz, Efrain, Sanders, J. S., et al. \| MNRAS \| 522-2325 \| 2023 \| 2023MNRAS.522.2325G \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.522.2325G Measuring the hot ICM velocity structure function using XMM-Newton observations \|Gatuzz, Efrain, Mohapatra, R., et al. \| MNRAS \| 524-2945 \| 2023 \| 2023MNRAS.524.2945G \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.524.2945G Chemical enrichment of ICM within the Ophiuchus cluster I: radial profiles \|Gatuzz, Efrain, Sanders, J. S., et al. \| MNRAS \| 526-396 \| 2023 \| 2023MNRAS.526..396G \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526..396G 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	2000-09-07T10:02:37Z/2004-10-02T06:21:54Z
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	2005-11-01T00:00:00Z
Keywords	"accretion process close", "emission components", "intermediate polars ips", "period history", "XMM", "galactic plane ts_30", "double degenerate polar", "soft ip", "epic detectors", "intermediate polars", "white dwarf", "spectral resolution", "EPIC", "xray spectra", "ROSAT", "orbital period", "quality spectra"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Bernd Aschenbach, 2005, 'New ROSAT discovered Intermediate Polars in the Galactic Plane TS_30', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vd8c7y9