Primary and secondary mirror manufacturing for COLIBRI ground follow-up telescope of the SVOM mission

Autor: Kjetil Dohlen, Didier Dubreuil, F. A. Uribe, S. Cuevas Cardona, C. Meessen, S. Basa, J. Boy, B. Cordier, D. Corre, Emmanuel Hugot, P. Gallais, F. Quirós, J. Platzer, Alan M. Watson, H. Valentin, Jorge Fuentes-Fernández, Liliana Figueroa, W. H. Lee, J-L. Atteia, A. Le Van Suu, Rosalía Langarica Lebre, P. E. Blanc, E. Jimenez-Bailon, O. Boulade, E. Cadena, J. Floriot, J. F. Le Borgne, A. F. Simon, F. Dolon, R. Mathon, Samuel Ronayette, Marc Ferrari, M. Ageron, E. Pallier, J. L. Ochoa, Damien Dornic, Michel Marcos, P. Ambert, A. Klotz

Publikováno v: Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation III.

COLIBRI is one of the two robotic ground follow-up telescopes for the SVOM (Space Variable Object Monitor) mission dedicated to the study of gamma-ray bursts, allowing determination of precise celestial coordinates of the detected bursts. COLIBRI tel

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::3167f5fef5fc2a394fce011502bf44e5
https://doi.org/10.1117/12.2311656

Engulfing a radio pulsar: the case of PSR J1023+0038

Autor: P. Goldoni, T. Munoz-Darias, H. Otí-Floranes, F. G. Ramón-Fox, N. Masetti, Rob Fender, P. D'Avanzo, Sergio Campana, Eliana Palazzi, Stefano Covino, E. Jimenez Bailon, F. Coti Zelati, Maria Cristina Baglio

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 444 (2), pp.1783-1792. ⟨10.1093/mnras/stu1552⟩
Monthly Notices of the Royal Astronomical Society, 2014, 444 (2), pp.1783-1792. ⟨10.1093/mnras/stu1552⟩

The binary millisecond radio pulsar PSR J1023+0038 has been recently the subject of multiwavelength monitoring campaigns which revealed that an accretion disc has formed around the neutron star (since 2013 June). We present here the results of X-ray

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::25c351b434a74da17802897f257cb455
https://doi.org/10.1093/mnras/stu1552

Fossil Groups Origins III. Characterization of the sample and observational properties of fossil systems

Autor: M. Lozada Muoz, Nicola R. Napolitano, J. A. L. Aguerri, C. del Burgo, José M. Vílchez, Marisa Girardi, Enrico Maria Corsini, N. Castro-Rodríguez, W. Boschin, Cristina Catalán-Torrecilla, E. Jimenez Bailon, R. Barrena, N. Herrera-Ruiz, Jairo Méndez-Abreu, S. Zarattini, Rubén Sánchez-Janssen, Jorge Iglesias-Páramo, Elena D'Onghia

Publikováno v: E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid

(Abridged) Fossil systems are group- or cluster-sized objects whose luminosity is dominated by a very massive central galaxy. In the current cold dark matter scenario, these objects formed hierarchically at an early epoch of the Universe and then slo

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::43280ba135138b5e6a5d1289aee1d788
http://arxiv.org/abs/1403.0588

XMM-NEWTONVIEW OF THE MULTIPHASE WARM ABSORBER IN SEYFERT 1 GALAXY NGC 985

Autor: Luc Binette, Fabrizio Nicastro, Mercedes Andrade-Velazquez, Yair Krongold, Nancy Brickhouse, Smita Mathur, Martin Elvis, Maria Santos-Lleo, E. Jimenez-Bailon

Publikováno v: The Astrophysical Journal. 690:773-782

We present an analysis of an XMM-Newton observation of the Seyfert 1 Galaxy NGC 985. The EPIC spectra present strong residuals to a single power-law model, indicating the presence of ionized absorbing gas and a soft excess. A broad-band fit to the EP

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::61a8c4da3b13a5b1caa20adc59587209
https://doi.org/10.1088/0004-637x/690/1/773

The XMM-Newton/INTEGRAL monitoring campaign of IGR J16318-4848

Autor: Giorgio Matt, Fabrizio Nicastro, E. Jimenez-Bailon, Erik Kuulkers, R. Walter, Matteo Guainazzi, Jerome Rodriguez, A. Ibarra

Publikováno v: Astronomy & Astrophysics. 465:501-507

IGR J16318-4848 is the prototype and one of the more extreme examples of the new class of highly obscured Galactic X-ray sources discovered by INTEGRAL. A monitoring campaign on this source has been carried out by XMM-Newton and INTEGRAL, consisting

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c2980e1e12e9584b7d96b27a6e726ca
https://doi.org/10.1051/0004-6361:20066225