A dataset provided by the European Space Agency

Name 030328
Title The chemistry of interstellar dust through the scattering halo of Cyg X-2
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303280101

DOI 10.5270/esa-fhcnfq5
Author Dr Elisa Costantini
Description We propose to observe the bright X-ray source Cyg X-2 as an ideal candidate to study the chemistry of the diffuse Interstellar Medium (ISM). We will study the two phases of ISM (gas and dust) through spectroscopy of the absorbed spectrum and the spectral and spatial analysis of the X-ray dust scattering halo. The study of the scattering halo of Cyg X-2 unveiled for the first time features from the ID constituents. To perform a quantitative measurement of the chemistry of the Interstellar Dust (ID) grains a large collective area, a large field of view, and a broad band coverage, like the one provided by XMM, is needed.
Publication The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 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 ,
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 all. . ApJS . 208-24 . 2013 . 2013ApJS..208...24L ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years o...
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-10-28T00:00:00Z, 030328, 17.56_20190403_1200. https://doi.org/10.5270/esa-fhcnfq5