Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Holczer, T."'
Autor:
Goosmann, R. W., Holczer, T., Mouchet, M., Dumont, A. -M., Behar, E., Godet, O., Goncalves, A. C., Kaspi, S.
We model the observed X-ray spectral continuum shape, ionic column densities, and absorption measure distribution (AMD) of the warm absorber in the Seyfert galaxy NGC 3783. We assume a photo-ionized medium with a uniform total (gas+radiation) pressur
Externí odkaz:
http://arxiv.org/abs/1603.01448
Autor:
Gandolfi, D., Parviainen, H., Deeg, H. J., Lanza, A. F., Fridlund, M., Moroni, P. G. Prada, Alonso, R., Augusteijn, T., Cabrera, J., Evans, T., Geier, S., Hatzes, A. P., Holczer, T., Hoyer, S., Kangas, T., Mazeh, T., Pagano, I., Tal-Or, L., Tingley, B.
Publikováno v:
A&A 576, A11 (2015)
We report the spectroscopic confirmation of the Kepler object of interest KOI-183.01 (Kepler-423b), a half-Jupiter mass planet transiting an old solar-like star every 2.7 days. Our analysis is the first to combine the full Kepler photometry (quarters
Externí odkaz:
http://arxiv.org/abs/1409.8245
Autor:
Steenbrugge, K. C., Kaastra, J. S., Detmers, R. G., Ebrero, J., Ponti, G., Costantini, E., Kriss, G. A., Mehdipour, M., Pinto, C., Branduardi-Raymont, G., Behar, E., Arav, N., Cappi, M., Bianchi, S., Petrucci, P. -O., Ratti, E. M., Holczer, T.
Context. The study of abundances in the nucleus of active galaxies allows us to investigate the evolution of abundance by comparing local and higher redshift galaxies. However, the methods used so far have substantial drawbacks or rather large uncert
Externí odkaz:
http://arxiv.org/abs/1108.2488
Autor:
Detmers, R. G., Kaastra, J. S., Steenbrugge, K. C., Ebrero, J., Kriss, G. A., Arav, N., Behar, E., Costantini, E., Branduardi-Raymont, G., Mehdipour, M., Bianchi, S., Cappi, M., Petrucci, P. -O., Pinto, C., Ratti, E. M., Holczer, T.
We present the results of our 600 ks RGS observation as part of the multiwavelength campaign on Mrk 509. The very high quality of the spectrum allows us to investigate the ionized outflow with an unprecedented accuracy due to the long exposure and th
Externí odkaz:
http://arxiv.org/abs/1107.0658
Autor:
Papadimitratos, P., Buttyan, L., Holczer, T., Schoch, E., Freudiger, J., Raya, M., Ma, Z., Kargl, F., Kung, A., Hubaux, J. -P.
Publikováno v:
IEEE Communcations Magazine, vol. 46, no. 11, pp. 100--109, November 2008
Significant developments have taken place over the past few years in the area of vehicular communication (VC) systems. Now, it is well understood in the community that security and protection of private user information are a prerequisite for the dep
Externí odkaz:
http://arxiv.org/abs/0912.5391
Autor:
Blustin, A. J., Kriss, G. A., Holczer, T., Behar, E., Kaastra, J. S., Page, M. J., Kaspi, S., Branduardi-Raymont, G., Steenbrugge, K. C.
Although AGN feedback through ionised winds is of great importance in models of AGN/galaxy coevolution, the mass and energy output via these winds, even in the nearby universe, is poorly understood. The issue is complicated by the wide range of ionis
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702311
Autor:
Steenbrugge KC, Kaastra JS, Detmers RG, Ebrero J, Ponti G, Costantini E, Kriss GA, Mehdipour M, Pinto C, Branduardi Raymont G, Behar E, Arav N, Cappi M, Petrucci PO, Ratti EM, Holczer T., BIANCHI, STEFANO
Context. The study of abundances in the nucleus of active galaxies allows us to investigate the evolution of the abundance by comparing local and higher redshift galaxies. However, the methods used so far have substantial drawbacks or rather large un
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3668::76d2936b625ed9e6ad098382216aeafb
https://hdl.handle.net/11590/124579
https://hdl.handle.net/11590/124579
Autor:
Detmers RG, Kaastra JS, Steenbrugge KC, Ebrero J, Kriss GA, Arav N, Behar E, Costantini E, Branduardi Raymont G, Mehdipour M, Cappi M, Petrucci P, Ponti G, Pinto C, Ratti EM, Holczer T., BIANCHI, STEFANO
We present the results of our 600 ks RGS observation as part of the multiwavelength campaign on Mrk 509. The very high quality of the spectrum allows us to investigate the ionized outflow with an unprecedented accuracy due to the long exposure and th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3668::dcdbfe55a33875859ee7a48d92abc7b0
https://hdl.handle.net/11590/124577
https://hdl.handle.net/11590/124577
Akademický článek
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Autor:
Blustin, A.J., Kriss, G.A., Holczer, T., Behar, E., Kaastra, J.S., Page, M., Kaspi, S., Branduardi-Raymont, G., Steenbrugge, K.C., Astrophysics, Dep Natuurkunde
Publikováno v:
Astronomy and Astrophysics, 466(1), 107. EDP Sciences
Although AGN feedback through ionised winds is of great importance in models of AGN/galaxy coevolution, the mass and energy output via these winds, even in the nearby universe, is poorly understood. The issue is complicated by the wide range of ionis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::7cf1aae4e5866a97f510c3fd1a2f5bab
https://dspace.library.uu.nl/handle/1874/43654
https://dspace.library.uu.nl/handle/1874/43654