A dataset provided by the European Space Agency

Name: Diagnosing intracluster hot gas with resonance absorption lines
Published: 2003-11-14T00:00:00Z

Proposal ID	014227
Title	Diagnosing intracluster hot gas with resonance absorption lines
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0142270101
DOI	https://doi.org/10.5270/esa-oso6kcy
Principal Investigator, PI	Dr Xavier Barcons
Abstract	We propose an RGS observation of the BL Lac object 4U 0543-31 (z=0.069) whoseline of sight crosses the cluster A S549(z=0.04) in order to study the physical properties of the hot gas in that cluster via resonance absorption lines. Weexpecto to measure intracluster gas coronal temperature and relative abundancesof various elements, densities as well as measure or otherwise constrainturbulent velocities of which very little is known. If the cluster emission canbe disentangled from that of the BL Lac in the EPIC images, we shall be able toestimate the distance to the cluster. This proposal is a pioneering experiment that will be a pathfinder for future studies of the diffuse warm or hot intergalactic medium.
Publications	Tentative detection of warm intervening gas towards PKS 0548-322 with XMM-Newton \|Barcons X. Paerels F. B. S. et al. \| MNRAS \| 359-1549 \| 2005 \| 2005MNRAS.359.1549B \| http://ui.adsabs.harvard.edu/#abs/2005MNRAS.359.1549B 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 Detection of Intra-day Variability Timescales of Four High-energy Peaked Blazars with XMM-Newton \|Gaur Haritma Gupta Alok C. et al. \| ApJ \| 718-279 \| 2010 \| 2010ApJ...718..279G \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...718..279G Fractal dimension and thermodynamic fluctuation properties of IDV light curves \|Leung Chun-Sing Wei Jian-Yan et al. \| RAA \| 11-1031 \| 2011 \| 2011RAA....11.1031L \| http://ui.adsabs.harvard.edu/#abs/2011RAA....11.1031L 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 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 Chandra monitoring observations of the ultraluminous X-ray source NGC 5204 X-1 \|Roberts T. P. Kilgard R. E. et al. \| MNRAS \| 371-1877 \| 2006 \| 2006MNRAS.371.1877R \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.371.1877R X-ray variability of 104 active galactic nuclei. XMM-Newton power-spectrum density profiles \|Gonzalez-Martin O. Vaughan S. \| A&A \| 544-80 \| 2012 \| 2012A&A...544A..80G \| http://ui.adsabs.harvard.edu/#abs/2012A&A...544A..80G 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 The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page M. J. Brindle C. et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi J. A. Albacete Colombo J. F. et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C High spectral resolution X-ray observations of AGN \|Kaastra J. S. \| AN \| 329-162 \| 2008 \| 2008AN....329..162K \| http://ui.adsabs.harvard.edu/#abs/2008AN....329..162K 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 Discussing the physical meaning of the absorption feature at 2.1 keV in 4U 1538-52 \|Rodes-Roca J. J. Torrejon J. M. et al. \| AN \| 335-804 \| 2014 \| 2014AN....335..804R \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..804R 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 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. Guainazzi M. \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S 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 Nitrogen X-ray absorption in the local ISM \|Gatuzz Efrain Garcu00eda Javier A. \| MNRAS \| 504-4460 \| 2021 \| 2021MNRAS.504.4460G \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.504.4460G Study of X-Ray Intraday Variability of HBL Blazars Based on Observations Obtained with XMM-Newton \|Devanand P. U. Gupta Alok C. et al. \| ApJ \| 939-80 \| 2022 \| 2022ApJ...939...80D \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...939...80D 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	2002-10-11T12:16:16Z/2002-10-12T14:31:17Z
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	2003-11-14T00:00:00Z
Last Update	2025-01-27
Keywords	"sight crosses", "EPIC", "pioneering experiment", "resonance absorption lines", "epic images", "hot intergalactic medium", "relative abundance", "diffuse warm", "physical properties", "cluster emission", "hot gas", "bl lac"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Xavier Barcons, 2003, 'Diagnosing intracluster hot gas with resonance absorption lines', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-oso6kcy