Zobrazeno 1 - 10
of 115
pro vyhledávání: '"Fiaschi, M."'
Autor:
Angeloni, R., Ramos, R. Contreras, Catelan, M., Dékány, I., Gran, F., Alonso-García, J., Hempel, M., Navarrete, C., Andrews, H., Aparicio, A., Beamín, J. C., Berger, C., Borissova, J., Peña, C. Contreras, Cunial, A., de Grijs, R., Espinoza, N., Eyheramendy, S., Lopes, C. E. Ferreira, Fiaschi, M., Hajdu, G., Han, J., Hełminiak, K. G., Hempel, A., Hidalgo, S. L., Ita, Y., Jeon, Y. -B., Jordán, A., Kwon, J., Lee, J. T., Martín, E. L., Masetti, N., Matsunaga, N., Milone, A. P., Minniti, D., Morelli, L., Murgas, F., Nagayama, T., Navarro, C., Ochner, P., Pérez, P., Pichara, K., Rojas-Arriagada, A., Roquette, J., Saito, R. K., Siviero, A., Sohn, J., Sung, H. -I., Tamura, M., Tata, R., Tomasella, L., Townsend, B., Whitelock, P.
Publikováno v:
A&A 567, A100 (2014)
Context. The Vista Variables in the V\'ia L\'actea (VVV) ESO Public Survey is a variability survey of the Milky Way bulge and an adjacent section of the disk carried out from 2010 on ESO Visible and Infrared Survey Telescope for Astronomy (VISTA). VV
Externí odkaz:
http://arxiv.org/abs/1405.4517
Autor:
Spiro, S., Pastorello, A., Pumo, M. L., Zampieri, L., Turatto, M., Smartt, S. J., Benetti, S., Cappellaro, E., Valenti, S., Agnoletto, I., Altavilla, G., Aoki, T., Brocato, E., Corsini, E. M., Di Cianno, A., Elias-Rosa, N., Hamuy, M., Enya, K., Fiaschi, M., Folatelli, G., Desidera, S., Harutyunyan, A., Howell, D. A., Kawka, A., Kobayashi, Y., Leibundgut, B., Minezaki, T., Navasardyan, H., Nomoto, K., Mattila, S., Pietrinferni, A., Pignata, G., Raimondo, G., Salvo, M., Schmidt, B. P., Sollerman, J., Spyromilio, J., Taubenberger, S., Valentini, G., Vennes, S., Yoshii, Y.
We present new data for five under-luminous type II-plateau supernovae (SNe IIP), namely SN 1999gn, SN 2002gd, SN 2003Z, SN 2004eg and SN 2006ov. This new sample of low-luminosity SNe IIP (LL SNe IIP) is analyzed together with similar objects studied
Externí odkaz:
http://arxiv.org/abs/1401.5426
Autor:
Ergon, M., Sollerman, J., Fraser, M., Pastorello, A., Taubenberger, S., Elias-Rosa, N., Bersten, M., Jerkstrand, A., Benetti, S., Botticella, M. T., Fransson, C., Harutyunyan, A., Kotak, R., Smartt, S., Valenti, S., Bufano, F., Cappellaro, E., Fiaschi, M., Howell, A., Kankare, E., Magill, L., Mattila, S., Maund, J., Naves, R., Ochner, P., Ruiz, J., Smith, K., Tomasella, L., Turatto, M.
We present optical and near-infrared (NIR) photometry and spectroscopy of the Type IIb supernova (SN) 2011dh for the first 100 days. We complement our extensive dataset with SWIFT ultra-violet (UV) and Spitzer mid-infrared (MIR) data to build a UV to
Externí odkaz:
http://arxiv.org/abs/1305.1851
Autor:
Maguire, K., Di Carlo, E., Smartt, S. J., Pastorello, A., Tsvetkov, D. Yu., Benetti, S., Spiro, S., Arkharov, A. A., Beccari, G., Botticella, M. T., Cappellaro, E., Cristallo, S., Dolci, M., Elias-Rosa, N., Fiaschi, M., D., Gorshanov, Harutyunyan, A., Larionov, V. M., Navasardyan, H., Pietrinferni, A., Raimondo, G., Di Rico, G., Valenti, S., Valentini, G., Zampieri, L.
We present new optical and near infrared (NIR) photometry and spectroscopy of the type IIP supernova, SN 2004et. In combination with already published data, this provides one of the most complete studies of optical and NIR data for any type IIP SN fr
Externí odkaz:
http://arxiv.org/abs/0912.3111
We present spectroscopic and photometric data of a sample of Type II plateau Supernovae, covering a wide range of properties, from the $^{56}$Ni rich, high luminosity events (e.g. SN 1992am) to the low-luminosity, $^{56}$Ni poor SNe (e.g. SN 1997D).
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310056
Publikováno v:
In Procedia CIRP 2015 33:508-513
Publikováno v:
In Optics and Laser Technology March 2014 56:35-42
Publikováno v:
In CIRP Annals - Manufacturing Technology 2014 63(1):229-232
Publikováno v:
In Optics and Laser Technology July 2012 44(5):1611-1619
Autor:
Munari U., Siviero A., Tamajo E., Fiaschi M., Dallaporta S., Cherini G., Frigo A., Castellani F., Graziani M., Moretti S., Tomaselli S.
Publikováno v:
Open Astronomy, Vol 21, Iss 1-2, Pp 180-183 (2012)
We have collected high precision optical photometry of VV8, so far 782 individual observing runs uniformly distributed over the period 2005 - 2011. This dataset allows us to refine the known long periodicity of VV8 to P = 16.8 yr, with peak-to-valley
Externí odkaz:
https://doaj.org/article/32848ff51dcd48d589a00a51896f87ca