A dataset provided by the European Space Agency

Name: The chemistry of interstellar dust through the scattering halo of Cyg X-2
Published: 2006-10-28T00:00:00Z

Proposal ID	030328
Title	The chemistry of interstellar dust through the scattering halo of Cyg X-2
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303280101
DOI	https://doi.org/10.5270/esa-fhcnfq5
Principal Investigator, PI	Dr Elisa Costantini
Abstract	We propose to observe the bright X-ray source Cyg X-2 as an ideal candidate tostudy the chemistry of the diffuse Interstellar Medium (ISM). We will study thetwo phases of ISM (gas and dust) through spectroscopy of the absorbed spectrumand the spectral and spatial analysis of the X-ray dust scattering halo. Thestudy of the scattering halo of Cyg X-2 unveiled for the first time featuresfrom the ID constituents. To perform a quantitative measurement of the chemistryof the Interstellar Dust (ID) grains a large collective area, a large field ofview, and a broad band coverage, like the one provided by XMM, is needed.
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 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 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 The Spitzer Mid-infrared Active Galactic Nucleus Survey. I. Optical and Near-infrared Spectroscopy of Obscured Candidates and Normal Active Galactic Nuclei Selected in the Mid-infrared \|Lacy M. Ridgway S. E. et al. \| ApJS \| 208-24 \| 2013 \| 2013ApJS..208...24L \| http://ui.adsabs.harvard.edu/#abs/2013ApJS..208...24L 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-Zeldovich 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 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 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 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 Oxygen and iron in interstellar dust: An X-ray investigation \|Psaradaki I. Costantini E. et al. \| A&A \| 670-30 \| 2023 \| 2023A&A...670A..30P \| http://ui.adsabs.harvard.edu/#abs/2023A&A...670A..30P Elemental Abundances in the Diffuse Interstellar Medium from Joint Far-ultraviolet and X-Ray Spectroscopy: Iron Oxygen Carbon and Sulfur \|Psaradaki I. Corrales L. et al. \| AJ \| 167-217 \| 2024 \| 2024AJ....167..217P \| http://ui.adsabs.harvard.edu/#abs/2024AJ....167..217P 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	2005-06-14T13:49:56Z/2005-06-14T22:40:05Z
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	2006-10-28T00:00:00Z
Last Update	2025-01-27
Keywords	"spatial analysis", "id constituents", "interstellar dust", "cyg x", "broad band coverage", "scattering halo", "absorbed spectrum", "XMM", "ism gas", "ideal candidate"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Elisa Costantini, 2006, 'The chemistry of interstellar dust through the scattering halo of Cyg X-2', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-fhcnfq5