A dataset provided by the European Space Agency

Name: Spectro-Imaging of Dust Scattering Haloes
Published: 2005-04-20T00:00:00Z

Proposal ID	011136
Title	Spectro-Imaging of Dust Scattering Haloes
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111360101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111360201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111360301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111360401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111360501
DOI	https://doi.org/10.5270/esa-k6kqw74
Principal Investigator, PI	Dr Bernd Aschenbach
Abstract	Bright and absorbed galactic X-ray sources are surrounded by haloes of radiationscattered on interstellar dust grains. It is proposed to study the physical andchemical properties of these grains, in particular whether or not grains havesilicate cores surrounded by organic mantles. The refractive index of both andtherefore the scattering cross sections are substantially different. Therfore,the shape of a spectrally resolved halo could be dominated either by onecomponent or the other. Cyg X-2 and GX 339-4 have been selected because theyhave bright haloes but are not too absorbed in order to get sufficient intensityeven at lower energies. Another observation of GX 339-4 in timing mode (Wilms etal.) is devoted to the properties of the central source only.
Publications	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 Absorption and scattering by interstellar dust: an XMM-Newton observation of Cyg X-2 \|Costantini, E., Freyberg, M. J., \| A&A \| 444-187 \| 2005 \| 2005A&A...444..187C \| http://ui.adsabs.harvard.edu/#abs/2005A&A...444..187C Rapid X-Ray Variability of Seyfert 1 Galaxies \|Vaughan, S., Fabian, A. C., \| Ap&SS \| 300-119 \| 2005 \| 2005Ap&SS.300..119V \| http://ui.adsabs.harvard.edu/#abs/2005Ap&SS.300..119V 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 Magnetic coupling of a rotating black hole with advection-dominated accretion flows \|Ye, Yong-Chun, Wang, Ding-Xiong, \| NewA \| 12-471 \| 2007 \| 2007NewA...12..471Y \| http://ui.adsabs.harvard.edu/#abs/2007NewA...12..471Y 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 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 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 XMM-Newton/Reflection Grating Spectrometer detection of the missing interstellar O VII Kalpha absorption line in the spectrum of Cyg X-2 \|Cabot, Samuel H. C., Wang, Q. Daniel, \| MNRAS \| 431-511 \| 2013 \| 2013MNRAS.431..511C \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.431..511C 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 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 Tracing the Reverberation Lag in the Hard State of Black Hole X-Ray Binaries \|De Marco, B., Ponti, G., et al. \| ApJ \| 814-50 \| 2015 \| 2015ApJ...814...50D \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...814...50D Oxygen, neon, and iron X-ray absorption in the local interstellar medium \|Gatuzz, Efrain, Garcia, Javier A., et al. \| A&A \| 588-111 \| 2016 \| 2016A&A...588A.111G \| http://ui.adsabs.harvard.edu/#abs/2016A&A...588A.111G On the detectability of CO molecules in the interstellar medium via X-ray spectroscopy \|Joachimi, Katerine, Gatuzz, Efrain, et al. \| MNRAS \| 461-352 \| 2016 \| 2016MNRAS.461..352J \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.461..352J The Chandra ACIS Timing Survey Project: glimpsing a sample of faint X-ray pulsators \|Israel, G. L., Esposito, P., et al. \| MNRAS \| 462-4371 \| 2016 \| 2016MNRAS.462.4371I \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.462.4371I 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 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 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 Interstellar oxygen along the line of sight of Cygnus X-2 \|Psaradaki, I., Costantini, E., et al. \| A&A \| 642-208 \| 2020 \| 2020A&A...642A.208P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...642A.208P 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 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	2002-06-03T08:14:01Z/2004-02-18T11:28:42Z
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	2005-04-20T00:00:00Z
Keywords	"silicate cores surrounded", "bright haloes", "radiation scattered", "mode wilms", "lower energies", "dust scattering haloes", "spectrally resolved halo", "organic mantles", "cyg x", "chemical properties", "interstellar dust grains", "refractive index", "gx 339", "spectro imaging", "central source", "scattering cross sections"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Bernd Aschenbach, 2005, 'Spectro-Imaging of Dust Scattering Haloes', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-k6kqw74