A dataset provided by the European Space Agency

Proposal ID 030276
Title 3-D Structure of Soft X-Ray Background along the Galactic Plane
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302760501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302760801

DOI https://doi.org/10.5270/esa-n6s2tv4
Principal Investigator, PI Dr Sangwook Park
Abstract The 3-dimensional structure of the X-ray emitting hot plasmas along the lines ofsight to make up the observed 0.5-2 keV X-ray background is unknown. The onlyway to unveil the 3-D distribution of the soft X-ray emitting Galactic hotplasmas is to discover and study X-ray shadows cast by dense molecular cloudsat known distances. We have performed such X-ray shadow experiments withXMM-Newton observations awarded in AO2 cycle, but our data were severelycontaminated by the flaring particle background. We therefore request foranother set of X-ray shadow observations, including repeat of the previouslyawarded targets.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-09-18T18:31:36Z/2005-09-22T16:18:28Z
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 2006-10-21T00:00:00Z
Last Update 2025-08-04
Keywords "XMM", "xray shadow experiments", "XMM-Newton", "dimensional structure", "x ray shadows", "kev xray background", "xmm newton", "xray shadow", "soft xray background", "dense molecular clouds", "flaring particle background", "ao2 cycle", "galactic plane"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Sangwook Park, 2006, '3-D Structure of Soft X-Ray Background along the Galactic Plane', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-n6s2tv4