A dataset provided by the European Space Agency

Name: Improved Shadowing Observations of the Galactic Halo with XMM-Newton
Published: 2014-02-23T00:00:00Z

Proposal ID	069050
Title	Improved Shadowing Observations of the Galactic Halo with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690500101
DOI	https://doi.org/10.5270/esa-7at9i3p
Principal Investigator, PI	Dr David Henley
Abstract	We are proposing shadowing observations of the hot gas in the Galactic halo.Unlike recent shadowing observations, we are proposing to observe compact cloudsfor which on- and off-cloud spectra can be extracted from a single XMM field.This technique is the only way to ensure that the time-variable contribution dueto solar system X-rays is the same in the on- and off-cloud spectra. From thesedata, we will determine the halos X-ray spectrum and measure its temperatureand emission measure. This information will help constrain models for the hothalos origin.
Publications	XMM-Newton Measurement of the Galactic Halo X-Ray Emission using a Compact Shadowing Cloud \|Henley David B. Shelton Robin L. et al. \| ApJ \| 799-117 \| 2015 \| 2015ApJ...799..117H \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...799..117H 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 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 Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earths Magnetosphere to the Solar Wind Proton Flux \|Zhang Yingjie Sun Tianran et al. \| ApJ \| 948-69 \| 2023 \| 2023ApJ...948...69Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z 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 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	2013-02-04T23:34:53Z/2013-02-06T01:00:10Z
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	2014-02-23T00:00:00Z
Keywords	"cloud spectra", "proposing shadowing", "hot halo", "improved shadowing", "constrain models", "XMM", "xray spectrum", "xmm newton", "hot gas", "compact clouds", "single xmm field", "galactic halo", "XMM-Newton", "time variable", "solar system xray"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr David Henley, 2014, 'Improved Shadowing Observations of the Galactic Halo with XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7at9i3p