Zobrazeno 1 - 6
of 6
pro vyhledávání: '"M. T. Ceballos"'
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2022, 134, 024504
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Transition Edge Sensors detector devices, like the core of the X-IFU instrument that will be on-board the Athena X-ray Observatory, produce current pulses as a response to the incident X-ray photons. The reconstruction of these pulses has been tradit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5384a145e929eb3f8f11a3e7e68c1c51
https://hdl.handle.net/10902/28467
https://hdl.handle.net/10902/28467
Autor:
X. Barcons, F. J. Carrera, M. T. Ceballos, M. J. Page, J. Bussons-Gordo, A. Corral, J. Ebrero, S. Mateos, J. A. Tedds, M. G. Watson, D. Baskill, M. Birkinshaw, T. Boller, N. Borisov, M. Bremer, G. E. Bromage, H. Brunner, A. Caccianiga, C. S. Crawford, M. S. Cropper, R. Della Ceca, P. Derry, A. C. Fabian, P. Guillout, Y. Hashimoto, G. Hasinger, B. J. M. Hassall, G. Lamer, N. S. Loaring, T. Maccacaro, K. O. Mason, R. G. McMahon, L. Mirioni, J. P. D. Mittaz, C. Motch, I. Negueruela, J. P. Osborne, F. Panessa, I. Pérez-Fournon, J. P. Pye, T. P. Roberts, S. Rosen, N. Schartel, N. Schurch, A. Schwope, P. Severgnini, R. Sharp, G. C. Stewart, G. Szokoly, A. Ullán, M. J. Ward, R. S. Warwick, P. J. Wheatley, N. A. Webb, D. Worrall, W. Yuan, H. Ziaeepour
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2007, 476 (3), pp.1191-1203. ⟨10.1051/0004-6361:20077606⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & astrophysics, 2007, Vol.476(3), pp.1191-1203 [Peer Reviewed Journal]
Astronomy and Astrophysics-A&A, EDP Sciences, 2007, 476 (3), pp.1191-1203. ⟨10.1051/0004-6361:20077606⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & astrophysics, 2007, Vol.476(3), pp.1191-1203 [Peer Reviewed Journal]
[Aims] X-ray sources at intermediate fluxes (a few x 10-14 erg cm-2 s-1) with a sky density of ~100 deg-2 are responsible for a significant fraction of the cosmic X-ray background at various energies below 10 keV. The aim of this paper is to provide
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f403877ea7c9c491409e5c4f7e194a2a
https://doi.org/10.1051/0004-6361:20077606
https://doi.org/10.1051/0004-6361:20077606
Publikováno v:
Symposium - International Astronomical Union. 201:400-407
We review the use of the X-ray background (XRB) as a cosmological tool with emphasis on three techniques: multipole analysis, autocorrelation functions and excess fluctuations. Although these methods of analysis of XRB fluctuations, and in particular
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e2da3293c29ebee0668f3ae3cb5d73d2
https://doi.org/10.1017/s0074180900216501
https://doi.org/10.1017/s0074180900216501
Autor:
A. Nebot Gómez-Morán, C. Motch, X. Barcons, F. J. Carrera, M. T. Ceballos, M. Cropper, N. Grosso, P. Guillout, O. Hérent, S. Mateos, L. Michel, J. P. Osborne, M. Pakull, F.-X. Pineau, J. P. Pye, T. P. Roberts, S. R. Rosen, A. D. Schwope, M. G. Watson, N. Webb
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics, 2013, 553, A12
Astronomy & astrophysics, 2013, Vol.553, pp.A12 [Peer Reviewed Journal]
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
instname
Astronomy and Astrophysics, 2013, 553, A12
Astronomy & astrophysics, 2013, Vol.553, pp.A12 [Peer Reviewed Journal]
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
Many different classes of X-ray sources contribute to the Galactic landscape at high energies. Although the nature of the most luminous X-ray emitters is now fairly well understood, the population of low-to-medium X-ray luminosity (LX = 1027-34 erg s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::97de6502ebcfc484cfc4fa2673b36961
http://hdl.handle.net/10261/109200
http://hdl.handle.net/10261/109200
Autor:
M. T. Ceballos, J. R. Rodón, A. Ibarra, R. Álvarez, C. Gabriel, D. Tapiador, P. Orviz, I. Campos
Publikováno v:
Astrophysics and Space Science Proceedings ISBN: 9783642112492
The processing of data obtained by the XMM–Newton observatory of the European Space Agency (ESA) is done using the SAS (Software Analysis System) tools provided by the ESA XMM Science Operations Centre (SOC). In order to be operative, these tools m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::135062e65991eba2c69c851f082b346a
https://doi.org/10.1007/978-3-642-11250-8_136
https://doi.org/10.1007/978-3-642-11250-8_136
Autor:
M, Bernácer Borja, P, Llerena Achútegui, E, Castillo Benítez, M T, Ceballos Sainz de Cenzano, E, Fernández Paredes
Publikováno v:
Anales espanoles de pediatria. 12(12)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::4fa9fcdb87289ac83d9a1858a243c96f
https://pubmed.ncbi.nlm.nih.gov/533060
https://pubmed.ncbi.nlm.nih.gov/533060