Zobrazeno 1 - 10
of 1 580
pro vyhledávání: '"Federici M"'
Publikováno v:
Clinical Interventions in Aging, Vol Volume 13, Pp 1237-1244 (2018)
Alessia Valentini,1 Massimo Federici,1 Maria Assunta Cianfarani,1 Umberto Tarantino,2 Aldo Bertoli1 1Department of Systems Medicine, University of Rome “Tor Vergata”, Rome, Italy; 2Department of Orthopaedics and Traumatology, University of Rome
Externí odkaz:
https://doaj.org/article/214d5d610ea4487db7ac8fc866a04608
Publikováno v:
Clinical Interventions in Aging, Vol Volume 12, Pp 335-341 (2017)
Aldo Bertoli,1 Alessia Valentini,1 Maria Assunta Cianfarani,1 Elena Gasbarra,2 Umberto Tarantino,2 Massimo Federici1 1Department of Systems Medicine, University of Rome “Tor Vergata”, Rome, Italy; 2Department of Orthopaedics and Traumatology, Uni
Externí odkaz:
https://doaj.org/article/69b0fc632342481687af36c4a5d446fd
Autor:
Lotti, S., Cea, D., Macculi, C., Mineo, T., Natalucci, L., Perinati, E., Piro, L., Federici, M., Martino, B.
Publikováno v:
A&A 569, A54 (2014)
Methods.There are no experimental data about the background experienced by microcalorimeters in the L2 orbit, and thus the particle background levels were calculated by means of Monte Carlo simulations: we considered the original design configuration
Externí odkaz:
http://arxiv.org/abs/1410.3373
Autor:
Fiocchi, M., Natalucci, L., Chenevez, J., Bazzano, A., Tarana, A., Ubertini, P., Brandt, S., Beckmann, V., Federici, M., Galis, R., Hudec, R.
Publikováno v:
Astrophys.J.693:333-339,2009
We report on the results of INTEGRAL observations of the neutron star low mass X-ray binary SAX J1810.8-2609 during its latest active phase in August 2007. The current outburst is the first one since 1998 and the derived luminosity is 1.1-2.6x10^36 e
Externí odkaz:
http://arxiv.org/abs/0811.1128
Autor:
Del Santo, M., Sidoli, L., Romano, P., Bazzano, A., Tarana, A., Ubertini, P., Federici, M., Mereghetti, S.
Publikováno v:
AIP Conf.Proc.1010:162-164,2008
In 2005 March 22nd, the INTEGRAL satellite caught a type-I X-ray burst from the unidentified source XMMU J174716.1-281048, serendipitously discovered with XMM-Newton in 2003. Based on the type-I X-ray burst properties, we derived the distance of the
Externí odkaz:
http://arxiv.org/abs/0803.1750
Autor:
Del Santo, M., Bazzano, A., Bezayiff, N., Smith, D. M., Ubertini, P., De Cesare, G., Federici, M.
The microquasar 1E 1740.7-2942 is one of the most appealing source of the Galactic Centre region. The high energy feature detected once by SIGMA has been searched in the last years by INTEGRAL, but never confirmed. Classified as a persistent source,
Externí odkaz:
http://arxiv.org/abs/0710.0335
The INTEGRAL/IBIS survey was performed collecting all the GPS and GCDE data together with all the available public data . The second catalogue, published in 2006 by Bird et al., is dominated by detection of 113 X-ray binaries, with 38 being high-mass
Externí odkaz:
http://arxiv.org/abs/0710.0298
\integral and \sax observations of the neutron-star LMXB 4U~1705--44 have been analysed to deeply investigate the spectral state transitions nature. Its energy spectrum can be described as the sum of one or two blackbody, a 6.4-keV Fe line and a comp
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610319
The 4-200 keV spectral and temporal behaviour of the low mass X-ray binary 4U 1820-30 has been studied with INTEGRAL during 2003-2005. This source as been observed in both the soft (banana) and hard (island) spectral states. A high energy tail above
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610328
Recent INTEGRAL observations and archival BeppoSAX data have been analyzed to deeply investigate the hard X-ray behavior of the neutron star, atoll type, low mass X-ray Binary 4U1636-53. Our investigation in three different periods outline three corr
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610320