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pro vyhledávání: '"MANNI, L."'
Astrometric microlensing will offer in the next future a new channel for investigating the nature of both lenses and sources involved in a gravitational microlensing event. The effect, corresponding to the shift of the position of the multiple image
Externí odkaz:
http://arxiv.org/abs/1705.01767
Publikováno v:
2017, ApJ, 837, 66
We present a sample of $X$-ray selected candidate black holes in 51 low mass galaxies with $z\le 0.055$ {and mass up to $10^{10}$ M$_{\odot}$} obtained by cross-correlating the NASA-SLOAN Atlas with the 3XMM catalogue. {We have also searched in the a
Externí odkaz:
http://arxiv.org/abs/1704.03182
Autor:
CAPOSSELA, L., GRAGLIA, B., FERRETTI, S., DI SARNO, L., GATTO, A., CALCAGNI, M. L., DI GIUDA, D., COCCIOLILLO, F., ROMEO, D. M., MANNI, L., SOLIGO, M., STACCIOLI, S., NAPOLI, E., CHIARETTI, A.
Publikováno v:
European Review for Medical & Pharmacological Sciences; Sep2024, Vol. 28 Issue 18, p4302-4312, 11p
In gravitational microlensing, binary systems may act as lenses or sources. Identifying lens binarity is generally easy especially in events characterized by caustic crossing since the resulting light curve exhibits strong deviations from smooth sing
Externí odkaz:
http://arxiv.org/abs/1606.02062
Autor:
Antoniucci, S., Nucita, A. A., Giannini, T., Lorenzetti, D., Stelzer, B., Gerardi, D., Rose, S. Delle, Di Paola, A., Giordano, M., Manni, L., Strafella, F.
Publikováno v:
A&A 584, A21 (2015)
V1180 Cas is a young variable that has shown strong photometric fluctuations (Delta_I~6mag) in the recent past, which have been attributed to events of enhanced accretion. The source has entered a new high-brightness state in Sept.2013, which we have
Externí odkaz:
http://arxiv.org/abs/1509.07730
We present the results of the analysis of deep archival \sat\ observations towards the dwarf spheroidal galaxies Draco, Leo I, Ursa Major II and Ursa Minor in the Milky Way neighbourhood. The X-ray source population is characterized and cross-correla
Externí odkaz:
http://arxiv.org/abs/1509.01076
Autor:
DI SARNO, L., EFTIMIADI, G., CHIARETTI, A., MANNI, L., GENOVESE, O., SOLIGO, M., CURATOLA, A., MORENA, T. C., GATTO, A., PIASTRA, M., SFERRAZZA, G., PANSINI, V., CONTI, G.
Publikováno v:
European Review for Medical & Pharmacological Sciences; Jun2024, Vol. 28 Issue 11, p3787-3795, 9p
Autor:
Nucita, A. A., Stefanelli, S., De Paolis, F., Masetti, N., Ingrosso, G., Del Santo, M., Manni, L.
Symbiotic X-ray binaries form a subclass of low-mass X-ray binary systems consisting of a neutron star accreting material from a red giant donor star via stellar wind or Roche lobe overflow. Only a few confirmed members are currently known; 4U 1700+2
Externí odkaz:
http://arxiv.org/abs/1401.2053
We report the results of a deep archive XMM-Newton observation of the Fornax spheroidal galaxy that we analyzed with the aim of fully characterizing the X-ray source population (in most of the cases likely to be background active galactic nuclei) det
Externí odkaz:
http://arxiv.org/abs/1301.0190
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