A dataset provided by the European Space Agency

Name 011007
Title The boundary layer in the disk accreting CV U Gem
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0110070401

DOI 10.5270/esa-s2ol3ln
Author Prof Keith Mason
Description GT- The bright CV U Gem will be studied to identify the location and properties of the boundary layer. Although this is not a pilot observation in the strict sense, if the count rate is above a certain rate, then the EPIC modes will be modified compared to that given in the RPS here. These modification are setout in the attached postscript file.
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High-precision multi-band measurements of the angular clustering of X-ray sources . Ebrero, J., Mateos, S., et all. . A&A . 500-749 . 2009 . 2009A&A...500..749E ,
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New constraints on the X-ray spectral properties of type 1 active galactic nuclei . Scott, A. E., Stewart, G. C., et all. . MNRAS . 417-992 . 2011 . 2011MNRAS.417..992S ,
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 . ...,
The 2XMMi-SDSS Galaxy Cluster Survey. I. The first cluster sample and X-ray luminosity-temperature relation . Takey, A., Schwope, A., . A&A . 534-120 . 2011 . 2011A&A...534A.120T ,
High precision X-ray log N - log S distributions: implications for the obscured AGN population . Mateos, S., Warwick, R. S., et all. . A&A . 492-51 . 2008 . 2008A&A...492...51M ,
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Are Optically Selected Quasars Universally X-Ray Luminous? X-Ray-UV Relations in Sloan Digital Sky Survey Quasars . Gibson, Robert R., Brandt, W. N., . ApJ . 685-773 . 2008 . 2008ApJ...685..773G ,
The XMM-Newton serendipitous survey. VI. The X-ray luminosity function . Ebrero, J., Carrera, F. J., et all. . A&A . 493-55 . 2009 . 2009A&A...493...55E ,
Breaking the sigma8-Omega m Degeneracy Using the Clustering of High-z X-ray Active Galactic Nuclei . Basilakos, Spyros, Plionis, Manolis, . ApJ . 714-185 . 2010 . 2010ApJ...714L.185B ,
Wavelet and R-S analysis of the X-ray flickering of cataclysmic variables . Anzolin, G., Tamburini, F., et all. . A&A . 519-69 . 2010 . 2010A&A...519A..69A ,
An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 . Henley, David B., Shelton, Robin L., . ApJS . 187-388 . 2010 . 2010ApJS..187..388H ,
Deriving an X-ray luminosity function of dwarf novae based on parallax measurements . Byckling, K., Mukai, K., et all. . MNRAS . 408-2298 . 2010 . 2010MNRAS.408.2298B ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
X-ray spectral variations of U Gem from quiescence to outburst . Guver, T., Uluyazi, C., et all. . MNRAS . 372-450 . 2006 . 2006MNRAS.372..450G ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Detectability of low-energy X-ray spectral components in type 1 active galactic nuclei . Scott, A. E., Stewart, G. C., . MNRAS . 423-2633 . 2012 . 2012MNRAS.423.2633S ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey . Pineau, F.-X., Motch, C., et all. . A&A . 527-126 . 2011 . 2011A&A...527A.126P ,
Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 . Ballo, L., Heras, F. J. H., et all. . A&A . 545-66 . 2012 . 2012A&A...545A..66B ,
The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton . De Luca, A., Molendi, S., . A&A . 419-837 . 2004 . 2004A&A...419..837D ,
The Fifth Data Release Sloan Digital Sky Survey-XMM-Newton Quasar Survey . Young, M., Elvis, M., . ApJS . 183-17 . 2009 . 2009ApJS..183...17Y ,
A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys . Brightman, M., Silverman, J. D., et all. . MNRAS . 433-2485 . 2013 . 2013MNRAS.433.2485B ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
The first ultraviolet quasar-stacked spectrum at z ~= 2.4 from WFC3 . Lusso, E., Worseck, G., et all. . MNRAS . 449-4204 . 2015 . 2015MNRAS.449.4204L ,
ERRATUM: "The Fifth Data Release Sloan Digital Sky Survey-XMM-Newton Quasar Survey" (2009, ApJS, 183, 17) . Young, M., Elvis, M., . ApJS . 185-250 . 2009 . 2009ApJS..185..250Y ,
The relationship between [O III]lambda5007 A equivalent width and obscuration in active galactic nuclei . Caccianiga, A., Severgnini, P., . MNRAS . 415-1928 . 2011 . 2011MNRAS.415.1928C ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
Do the spectral energy distributions of type 1 active galactic nuclei show diversity? . Scott, A. E., Stewart, G. C., . MNRAS . 438-2253 . 2014 . 2014MNRAS.438.2253S ,
Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era . Evans, P. A., Osborne, J. P., et all. . MNRAS . 448-2210 . 2015 . 2015MNRAS.448.2210E ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The XMM Cluster Survey: the halo occupation number of BOSS galaxies in X-ray clusters . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 463-1929 . 2016 . 2016MNRAS.463.1929M ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals . Sibeck, David G., Allen, R., et all. . SSRv . 214-79 . 2018 . 2018SSRv..214...79S ,
The XMM Cluster Survey: Present status and latest results . Viana, P. T. P., Mehrtens, N., et all. . AN . 334-462 . 2013 . 2013AN....334..462V ,
The Spectrum of the Universe . Hill, Ryley, Masui, Kiyoshi W., . ApSpe . 72-663 . 2018 . 2018ApSpe..72..663H ,
The evolving X-ray spectrum of active galactic nuclei: Evidence for an increasing reflection fraction with redshift . Avirett-Mackenzie, M. S., Ballantyne, D. R., . MNRAS . 486-3488 . 2019 . 2019MNRAS.486.3488A ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background . Ananna, Tonima Tasnim, Treister, Ezequiel, et all. . ApJ . 889-17 . 2020 . 2020ApJ...889...17A ,
Testing Comptonization as the Origin of the Continuum in Nonmagnetic Cataclysmic Variables: The Photon Index of X-Ray Emission . Maiolino, T., Titarchuk, L., et all. . ApJ . 900-153 . 2020 . 2020ApJ...900..153M ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-04-13T05:13:28Z/2002-04-13T11:36:49Z
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 2003-05-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-05-23T00:00:00Z, 011007, 17.56_20190403_1200. https://doi.org/10.5270/esa-s2ol3ln