Zobrazeno 1 - 10
of 205
pro vyhledávání: '"Temporin S."'
Autor:
Pintos-Castro, I., Povic, M., Sánchez-Portal, M., Cepa, J., Altieri, B., Bongiovanni, Á., Duc, P. A., Ederoclite, A., Oteo, I., García, A. M. Pérez, Martínez, R. Pérez, Polednikova, J., Ramón-Pérez, M., Temporin, S.
Publikováno v:
A&A 592, A108 (2016)
The study of the evolution of the morphological distribution of galaxies in different environments can provide important information about the effects of the environment and the physical mechanisms responsible for the morphological transformations. A
Externí odkaz:
http://arxiv.org/abs/1604.08850
Autor:
Valtchanov, Ivan, Altieri, B., Berta, S., Chapin, E., Coia, D., Conversi, L., Dannerbauer, H., Domínguez-Sánchez, H., Rawle, T. D., Sánchez-Portal, M., Santos, J. S., Temporin, S.
We report the serendipitous detection of a significant overdensity of Herschel-SPIRE 250 micron sources in the vicinity of MRC1138-26. We use an adaptive kernel density estimate to quantify the significance, including a comparison with other fields.
Externí odkaz:
http://arxiv.org/abs/1309.4223
Autor:
Sánchez-Portal, M., Cepa, J., Pintos-Castro, I., Pérez-Martínez, R., Smail, I., Alfaro, E., Altieri, B., Aragón-Salamanca, A., Balkowski, C., Balogh, M., Biviano, A., Bongiovanni, A., Bremer, M., Castander, F., Castañeda, H., Castro-Rodríguez, N., Coia, D., Duc, P. A., Geach, J., González-Serrano, I., Haines, C., McBreen, B., Metcalfe, L., Pérez-Fournón, I., García, A. M. Pérez, Poggianti, B., Rodríguez-Espinosa, J. M., Smith, G. P., Temporin, S., Valtchanov, I.
Aimed at understanding the evolution of galaxies in clusters, the GLACE survey is mapping a set of optical lines ([OII]3727, [OIII]5007, Hbeta and Halpha/[NII] when possible) in several galaxy clusters at redshift around 0.40, 0.63 and 0.86, using th
Externí odkaz:
http://arxiv.org/abs/1012.1750
Autor:
Cucciati, O., Marinoni, C., Iovino, A., Bardelli, S., Adami, C., Mazure, A., Scodeggio, M., Maccagni, D., Temporin, S., Zucca, E., De Lucia, G., Blaizot, J., Garilli, B., Meneux, B., Zamorani, G., Fèvre, O. Le, Cappi, A., Guzzo, L., Bottini, D., Brun, V. Le, Tresse, L., Vettolani, G., Zanichelli, A., Arnouts, S., Bolzonella, M., Charlot, S., Ciliegi, P., Contini, T., Foucaud, S., Franzetti, P., Gavignaud, I., Ilbert, O., Lamareille, F., McCracken, H. J., Marano, B., Merighi, R., Paltani, S., Pellò, R., Pollo, A., Pozzetti, L., Vergani, D., Pérez-Montero, E.
[Abridged] We present a homogeneous and complete catalogue of optical groups identified in the purely flux limited (17.5<=I<=24.0) VIMOS-VLT Deep Survey (VVDS). We use mock catalogues extracted from the MILLENNIUM simulation, to correct for potential
Externí odkaz:
http://arxiv.org/abs/0911.3740
Compact groups of galaxies are in particular good laboratories for studying galaxy interactions and their effects on the evolution of galaxies due to their high density and low velocity dispersion. SCG0018-4854 is a remarkably high galaxy density and
Externí odkaz:
http://arxiv.org/abs/0910.4978
Autor:
Scodeggio, M., Vergani, D., Cucciati, O., Iovino, A., Franzetti, P., Garilli, B., Lamareille, F., Bolzonella, M., Pozzetti, L., Abbas, U., Marinoni, C., Contini, T., Bottini, D., Brun, V. Le, Fevre, O. Le, Maccagni, D., Scaramella, R., Tresse, L., Vettolani, G., Zanichelli, A., Adami, C., Arnouts, S., Bardelli, S., Cappi, A., Charlot, S., Ciliegi, P., Foucaud, S., Gavignaud, I., Guzzo, L., Ilbert, O., McCracken, H. J., Marano, B., Mazure, A., Meneux, B., Merighi, R., Paltani, S., Pello, R., Pollo, A., Radovich, M., Zamorani, G., Zucca, E., Bondi, M., Bongiorno, A., Brinchmann, J., de la Torre, S., de Ravel, L., Gregorini, L., Memeo, P., Perez-Montero, E., Mellier, Y., Temporin, S., Walcher, C. J.
Hierarchical models of galaxy formation predict that the properties of a dark matter halo depend on the large-scale environment surrounding the halo. As a result of this correlation, we expect massive haloes to be present in larger number in overdens
Externí odkaz:
http://arxiv.org/abs/0903.0271
Autor:
Pastorello, A., Valenti, S., Zampieri, L., Navasardyan, H., Taubenberger, S., Smartt, S. J., Arkharov, A. A., Baernbantner, O., Barwig, H., Benetti, S., Birtwhistle, P., Botticella, M. T., Cappellaro, E., Del Principe, M., Di Mille, F., Di Rico, G., Dolci, M., Elias-Rosa, N., Efimova, N. V., Fiedler, M., Harutyunyan, A., Hoeflich, P. A., Kloehr, W., Larionov, V. M., Lorenzi, V., Maund, J. R., Napoleone, N., Ragni, M., Richmond, M., Ries, C., Spiro, S., Temporin, S., Turatto, M., Wheeler, J. C.
We present the results of the one year long observational campaign of the type II-plateau SN 2005cs, which exploded in the nearby spiral galaxy M51 (the Whirlpool Galaxy). This extensive dataset makes SN 2005cs the best observed low-luminosity, 56Ni-
Externí odkaz:
http://arxiv.org/abs/0901.2075
Autor:
Marinoni, C., Guzzo, L., Cappi, A., Fevre, O. Le, Mazure, A., Meneux, B., Pollo, A., Iovino, A., McCracken, H. J., Scaramella, R., de la Torre, S., Virey, J. M., Bottini, D., Garilli, B., Brun, V. Le, Maccagni, D., Picat, J. P., Scodeggio, M., Tresse, L., Vettolani, G., Zanichelli, A., Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Charlot, S., Ciliegi, P., Contini, T., Foucaud, S., Franzetti, P., Gavignaud, I., Ilbert, O., Lamareille, F., Marano, B., Mathez, G., Merighi, R., Paltani, S., Pellò, R., Pozzetti, L., Radovich, M., Vergani, D., Zamorani, G., Zucca, E., Abbas, U., Bondi, M., Bongiorno, A., Brinchmann, J., Buzzi, A., Cucciati, O., de Ravel, L., Gregorini, L., Mellier, Y., Merluzzi, P., Perez-Montero, E., Taxil, P., Temporin, S., Walcher, C. J.
We study the evolution of the low-order moments of the galaxy overdensity distribution over the redshift interval 0.7
Externí odkaz:
http://arxiv.org/abs/0811.2358
Autor:
Bardelli, S., Zucca, E., Bolzonella, M., Ciliegi, P., Gregorini, L., Zamorani, G., Bondi, M., Zanichelli, A., Tresse, L., Vergani, D., Gavignaud, I., Bongiorno, A., Bottini, D., Garilli, B., Brun, V. Le, Fevre, O. Le, Maccagni, D., Scaramella, R., Scodeggio, M., Vettolani, G., Adami, C., Arnouts, S., Cappi, A., Charlot, S., Contini, T., Foucaud, S., Franzetti, P., Guzzo, L., Ilbert, O., Iovino, A., Lamareille, F., McCracken, H. J., Marano, B., Marinoni, C., Mazure, A., Meneux, B., Merighi, R., Paltani, S., Pello`, R., Pollo, A., Pozzetti, L., Radovich, M., Abbas, U., Brinchmann, J., Cucciati, O., de la Torre, S., de Ravel, L., Memeo, P., Perez-Montero, E., Mellier, Y., Merluzzi, P., Temporin, S., De Ruiter, H. R., Parma, P.
(abridged) We use the 1.4 GHz VIMOS-VLA Deep Survey and the optical VVDS and the CFHT-LS to compare the properties of radio loud galaxies with respect to the whole population of optical galaxies. The availability of multiband photometry and high qual
Externí odkaz:
http://arxiv.org/abs/0811.1653
We present an investigation of the dust-enshrouded activity in a sample of X-ray selected clusters drawn from the XMM-LSS survey in the redshift range z ~ 0.05 - 1.05. By taking advantage of the contiguous mid-IR coverage of the XMM-LSS field by the
Externí odkaz:
http://arxiv.org/abs/0810.5499