A dataset provided by the European Space Agency

Name 004874
Title XMM Study of the bright ultrasoft narrow-line quasar NAB 0205+024
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0048740101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0048740201

DOI 10.5270/esa-xn95h4q
Author Dr Thomas Boller
Description We propose to perform spectral and timing measurements of the ultrasoft narrow- line quasar NAB 0205+024 with XMM. NAB 0205+024 is an extension of the class of ultrasoft narrow-line Seyfert 1 galaxies towards higher luminosities. The proposed observations are expected to build upon our guaranteed time observa- tions on NLS1. XMM spectra will allow (1) precision fitting of the soft X-ray excess and hard X-ray power law, (2) study of broad and ionized iron K line emission, (3) study of ionized gas along the line of sight, and (4) measure- ments of the Compton reflection continuum. XMM light curves will allow (1) studies of X-ray variability, (2) power spectrum analyses, (3) measurements of spectral variability.
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 ,
The XMM-Newton Wide Angle Survey (XWAS): the X-ray spectrum of type-1 AGN . Mateos, S., Carrera, F. J., et all. . A&A . 510-35 . 2010 . 2010A&A...510A..35M ,
Average Fe Kalpha emission from distant AGN . Corral, A., Page, M. J., et all. . A&A . 492-71 . 2008 . 2008A&A...492...71C ,
X-ray absorption in distant type II QSOs . Krumpe, M., Lamer, G., et all. . A&A . 483-415 . 2008 . 2008A&A...483..415K ,
The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project . Fassbender, R., Bohringer, H., et all. . NJPh . 13-125014 . 2011 . 2011NJPh...13l5014F ,
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 ,
Investigating the nature of narrow-line Seyfert 1 galaxies with high-energy spectral complexity . Gallo, L. C., . MNRAS . 368-479 . 2006 . 2006MNRAS.368..479G ,
Th...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-07-23T05:38:48Z/2002-07-23T20:23:40Z
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 2003-08-14T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-08-14T00:00:00Z, 004874, 17.56_20190403_1200. https://doi.org/10.5270/esa-xn95h4q