Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Baskill, D."'
Autor:
Stuhlinger, M., Altieri, B., Baskill, D., Dennerl, K., Esquej, M. P., Freyberg, M., Haberl, F., Herder, J. W. den, Kaastra, J., Kirsch, M. G. F., Metcalfe, L., Pollock, A. M. T., Read, A. M., Saxton, R. D., Sembay, S., Smith, M. J. S., Talavera, A., Vink, J., de Vries, C.
Further achievements of the XMM-Newton cross-calibration - XMM internal as well as with other X-ray missions - are presented. We explain the major changes in the new version SASv6.5 of the XMM-Newton science analysis system. The current status of the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0511395
Autor:
Sembay, S., Abbey, A., Altieri, B., Ambrosi, R., Baskill, D., Ferrando, P., Mukerjee, K., Read, A., Turner, M. J. L.
XMM-Newton was launched into space on a highly eccentric 48 hour orbit on December 10th 1999. XMM-Newton is now in its fifth year of operation and has been an outstanding success, observing the Cosmos with imaging, spectroscopy and timing capabilitie
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407347
We have carried out a thorough analysis of non-magnetic cataclysmic variables observed with ASCA, and have discovered possible periods in three targets: WW Cet, EI UMa and IX Vel. These may be caused by the rotation of the white dwarf at the centre o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0110089
Publikováno v:
Mon.Not.Roy.Astron.Soc. 328 (2001) 71
We present ASCA observations of the dwarf nova Z Camelopardalis during outburst and during a transition from quiescence to another outburst. At the beginning of the transition the X-ray count rate was an order of magnitude higher and the spectrum muc
Externí odkaz:
http://arxiv.org/abs/astro-ph/0108017
Autor:
Kirsch, M. G., Abbey, A., Altieri, B., Baskill, D., Dennerl, K., van Dooren, J., Fauste, J., Freyberg, M. J., Gabriel, C., Haberl, F., Hartmann, H., Hartner, G., Meidinger, N., Metcalfe, L., Olabarri, B., Pollock, A. M., Read, A. M., Rives, S., Sembay, S., Smith, M. J.
Publikováno v:
Proceedings of SPIE; Nov2005 Part 2, Issue 1, p58980S-58980S-12, 12p
Autor:
Barcons, X., Carrera, F. J., Ceballos, M. T., Page, M. J., Bussons-Gordo, J., Corral, A., Ebrero, J., Mateos, S., Tedds, J. A., Watson, M. G., Baskill, D., Birkinshaw, M., Boller, T., Borisov, N., Bremer, M., Bromage, G. E., Brunner, H., Caccianiga, A., Crawford, C. S., Cropper, M. S., Della Ceca, R., Derry, P., Fabian, A. C., Guillout, P., Hashimoto, Y., Hasinger, G., Hassall, B. J. M., Lamer, G., Loaring, N. S., Maccacaro, T., Mason, K. O., McMahon, R. G., Mirioni, L., Mittaz, J. P. D., Motch, C., Negueruela, I., Osborne, J. P., Panessa, F., Pérez-Fournon, I., Pye, J. P., Roberts, T. P., Rosen, S., Schartel, N., Schurch, N., Schwope, A., Severgnini, P., Sharp, R., Stewart, G. C., Szokoly, G., Ullán, A., Ward, M. J., Warwick, R. S., Wheatley, P. J., Webb, N. A., Worrall, D., Yuan, W., Ziaeepour, H., Barcons, X., Carrera, F. J., Ceballos, M. T., Page, M. J., Bussons-Gordo, J., Corral, A., Ebrero, J., Mateos, S., Tedds, J. A., Watson, M. G., Baskill, D., Birkinshaw, M., Boller, T., Borisov, N., Bremer, M., Bromage, G. E., Brunner, H., Caccianiga, A., Crawford, C. S., Cropper, M. S., Della Ceca, R., Derry, P., Fabian, A. C., Guillout, P., Hashimoto, Y., Hasinger, G., Hassall, B. J. M., Lamer, G., Loaring, N. S., Maccacaro, T., Mason, K. O., McMahon, R. G., Mirioni, L., Mittaz, J. P. D., Motch, C., Negueruela, I., Osborne, J. P., Panessa, F., Pérez-Fournon, I., Pye, J. P., Roberts, T. P., Rosen, S., Schartel, N., Schurch, N., Schwope, A., Severgnini, P., Sharp, R., Stewart, G. C., Szokoly, G., Ullán, A., Ward, M. J., Warwick, R. S., Wheatley, P. J., Webb, N. A., Worrall, D., Yuan, W., Ziaeepour, H.
Publikováno v:
Astronomy and Astrophysics; December 2007, Vol. 476 Issue: 3 p1191-1203, 13p
Publikováno v:
NASA Astrophysics Data System
We have carried out a thorough analysis of non-magnetic cataclysmic variables observed with ASCA, and have discovered possible periods in three targets: WW Cet, EI UMa and IX Vel. These may be caused by the rotation of the white dwarf at the centre o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cde13d0dc016c3dec7f2739bbce2df86
https://ui.adsabs.harvard.edu/#abs/2002ASPC..261..465B
https://ui.adsabs.harvard.edu/#abs/2002ASPC..261..465B
Autor:
Stuhlinger, M., Bruno Altieri, Esquej, M. P., Kirsch, M. G. F., Metcalfe, L., Pollock, A. M. T., Saxton, R. D., Smith, M. J. S., Talavera, A., Sembay, S., Read, A. M., Baskill, D., Haberl, F., Freyberg, M., Dennerl, K., Kaastra, J., Den Herder, J. W., Vries, C., Vink, J.
Publikováno v:
NASA Astrophysics Data System
Scopus-Elsevier
Scopus-Elsevier
Further achievements of the XMM-Newton cross-calibration - XMM internal as well as with other X-ray missions - are presented. We explain the major changes in the new version SASv6.5 of the XMM-Newton science analysis system. The current status of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d072d76ddee255f37c256de52525484
https://ui.adsabs.harvard.edu/#abs/2006ESASP.604..937S
https://ui.adsabs.harvard.edu/#abs/2006ESASP.604..937S
Conference
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Akademický článek
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