A dataset provided by the European Space Agency

Name: Mapping the chemistry of interstellar dust through the halo of 4U1820-30
Published: 2010-04-22T00:00:00Z

Proposal ID	055134
Title	Mapping the chemistry of interstellar dust through the halo of 4U1820-30
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551340201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551340301
DOI	https://doi.org/10.5270/esa-4yl680b
Principal Investigator, PI	Dr Elisa Costantini
Abstract	We propose to observe the bright X-ray source 4U1820-30 as optimal candidate tomap the chemistry of the diffuse Galactic Interstellar Medium (ISM). Using theunique XMM-Newton performances, we will study the two phases of ISM (gas anddust) focusing on O, Fe, Mg, and Si. The observation of 4U1820-30 will provide arobust and quantitative estimate on how homogeneous the distribution of theseelements are in the diffuse ISM. The simultaneous analysis of scattering andabsorption has been already successful for another XMM-Newton target (Cyg X-2,Costantini et al. 2005), unveiling for the first time features from the IDconstituents.
Publications	XMM-Newton observation of 4U 1820-30. Broad band spectrum and the contribution of the cold interstellar medium \|Costantini, E., Pinto, C., et al. \| A&A \| 539-32 \| 2012 \| 2012A&A...539A..32C \| http://ui.adsabs.harvard.edu/#abs/2012A&A...539A..32C The Second Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars \|Abdo, A. A., Ajello, M., et al. \| ApJS \| 208-17 \| 2013 \| 2013ApJS..208...17A \| http://ui.adsabs.harvard.edu/#abs/2013ApJS..208...17A 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 hot interstellar medium towards 4U 1820-30: a Bayesian analysis \|Rogantini, D., Costantini, E., et al. \| A&A \| 645-98 \| 2021 \| 2021A&A...645A..98R \| http://ui.adsabs.harvard.edu/#abs/2021A&A...645A..98R 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 Exploring X-ray variability with unsupervised machine learning. I. Self-organizing maps applied to XMM-Newton data \|Kova\\u010devi\\u0107, M., Pasquato, M., et al. \| A&A \| 659-66 \| 2022 \| 2022A&A...659A..66K \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..66K Properties of Milky Way globular clusters associated with X-ray sources \|Botev, Svetoslav, Nedialkov, Petko, \| BlgAJ \| 40-59 \| 2024 \| 2024BlgAJ..40...59B \| http://ui.adsabs.harvard.edu/#abs/2024BlgAJ..40...59B 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	2009-04-02T11:22:55Z/2009-04-03T00:42:52Z
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	2010-04-22T00:00:00Z
Keywords	"interstellar dust", "dust focusing", "XMM", "id constituents", "diffuse ism", "optimal candidate", "xmm newton performances", "ism gas", "XMM-Newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Elisa Costantini, 2010, 'Mapping the chemistry of interstellar dust through the halo of 4U1820-30', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-4yl680b