A dataset provided by the European Space Agency

Name: Soft X-ray Absorption Edges in LMXBs
Published: 2004-05-15T00:00:00Z

Proposal ID	015104
Title	Soft X-ray Absorption Edges in LMXBs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0151040201
DOI	https://doi.org/10.5270/esa-dglndkd
Principal Investigator, PI	Dr Norbert S. Schulz
Abstract	We propose a survey of RGS observations of bright X-ray binaries in thewavelength range between 14 and 25 A in order to measure optical depthsof photo-electric absorption edges of Ne, Fe, O, and possibly N and determineprecise values for column densities. We will also model the structureof observed edges and compare them with most recent laboratory measurements.From the measurement of the equivalent widths of the 1s-2p absorption ofmono-atomic oxygen in the ISM and the measurement of the O K edge depthwe can conclude on the distribution of oxygen in the ISM and/or determinesource intrinsic absorption properties. The relative strengths of allmeasured edges will be used to test proposed abundance distributions for the ISM
Publications	Spectral Analysis of LMC-X2 with XMM/Newton \|Lavagetto, G., Iaria, R., et al. \| ChJAS \| 8-325 \| 2008 \| 2008ChJAS...8..325L \| http://ui.adsabs.harvard.edu/#abs/2008ChJAS...8..325L Spectral analysis of LMC X-2 with XMM/Newton: unveiling the emission process in the extragalactic Z-source \|Lavagetto, G., Iaria, R., et al. \| A&A \| 478-181 \| 2008 \| 2008A&A...478..181L \| http://ui.adsabs.harvard.edu/#abs/2008A&A...478..181L 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 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 The Chandra Small Magellanic Cloud Wing Survey - the search for X-ray binaries \|McGowan, K. E., Coe, M. J., et al. \| MNRAS \| 383-330 \| 2008 \| 2008MNRAS.383..330M \| http://ui.adsabs.harvard.edu/#abs/2008MNRAS.383..330M 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
Instrument	EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2003-04-21T20:21:23Z/2003-04-22T03:22:54Z
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	2004-05-15T00:00:00Z
Keywords	"bright xray binary", "optical depths", "abundance distributions", "column densities", "mono atomic oxygen", "relative strengths", "laboratory measurements", "edge depth", "wavelength range", "precise values", "equivalent widths", "absorption properties", "1s 2p absorption"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Norbert S. Schulz, 2004, 'Soft X-ray Absorption Edges in LMXBs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-dglndkd