Results 11 to 20 of about 64,604 (243)
Post conjunction detection of $\beta$ Pictoris b with VLT/SPHERE [PDF]
, 2018 With an orbital distance comparable to that of Saturn in the solar system,
\bpic b is the closest (semi-major axis $\simeq$\,9\,au) exoplanet that has
been imaged to orbit a star.Abe, L., Antichi, J., Baruffolo, A., Baudino, J.-L., Baudoz, P., Baudrand, J., Bazzon, A., Beust, H., Beuzit, J.-L., Biller, B., Blanchard, P., Boccaletti, A., Bohn, A.J., Bonavita, M., Bonnefoy, M., Buey, T., Cantalloube, F., Carbillet, M., Carle, M., Cascone, E., Charnay, B., Charton, J., Chauvin, G., Cheetham, A., Claudi, R., Costille, A., Cudel, M., D'Orazi, V., Daemgen, S., De Caprio, V., Deboulbe, A., Delorme, P., Desidera, S., Dohlen, K., Dominik, C., Fantinel, D., Feautrier, P., Feldt, M., Fontanive, C., Fusco, T., Galicher, R., Gigan, P., Girard, J., Giro, E., Gisler, D., Gluck, L., Gomez,, Gonzales, C.A., Gratton, R., Gry, C., Hagelberg, J., Henning, T., Hubin, N., Hugot, E., Janson, M., Jaquet, M., Kasper, M., Kenworthy, M., Keppler, M., Koypitova, T., Kral, Q., Lagadec, E., Lagrange, A.-M., Langlois, M., Lannier, J., Le Coroller, H., Le Mignant, D., Ligi, R., Llored, M., Madec, F., Magnard, Y., Maire, A.-L., Martinez, P., Maurel, D., Menard, F., Mesa, D., Messina, S., Meyer, M., Milli, J., Moeller-Nilsson, O., Mordasini, C., Mouillet, D., Moulin, T., Moutou, C., Mueeller, A., Origne, A., Pavlov, A., Peretti, S., Perret, D., Perrot, C., Petit, C., Plas, G. van der, Pragt, J., Rouan, D., Salter, G., Samland, M., Schlieder, J.E., Schmid, H.-M., Schmidt, T., Sissa, E., Szulagyi, J., Turatto, M., Udry, S., Vigan, A., Wildi, F., Zurlo, A. +105 morecore +3 more sourcesSN 2002lt and GRB 021211: a SN/GRB Connection at z = 1 [PDF]
, 2003 We present spectroscopic and photometric observations of the afterglow of GRB
021211 and the discovery of its associated supernova, SN 2002lt. The spectrum
shows a broad feature (FWHM = 150 A), around 3770 A (in the rest-frame of the
GRB), which we ...Antonelli, L. A., Benetti, S., Chincarini, G., Cocozza, G., Covino, S., D'Avanzo, P., Della Valle, M., Fugazza, D., Ghisellini, G., Gilmozzi, R., Hamuy, M., Lazzati, D., Malesani, D., Mason, E., Mazzali, P., Stella, L., Testa, V. +16 morecore +1 more sourceThe GAPS programme with HARPS-N@TNG IV: A planetary system around XO-2S [PDF]
, 2014 We performed an intensive radial velocity monitoring of XO-2S, the wide
companion of the transiting planet-host XO-2N, using HARPS-N at TNG in the
framework of the GAPS programme.Affer, L., Andreuzzi, G., Barbieri, M., Bedin, L. R., Benatti, S., Biazzo, K., Bignamini, A., Bonavita, M., Bonomo, A. S., Borsa, F., Calcidese, P., Christille, J. M., Claudi, R. U., Cosentino, R., Covino, E., Damasso, M., Desidera, S., Esposito, M., Fiorenzano, A. F. Martinez, Gandolfi, D., Giacobbe, P., Gratton, R., Harutyunyan, A., Lanza, A. F., Latham, D., Lattanzi, M., Leto, G., Lodato, G., Lovis, C., Maggio, A., Malavolta, L., Mancini, L., Marzari, F., Micela, G., Molinari, E., Mordasini, C., Munari, U., Nascimbeni, V., Pagano, I., Pedani, M., Pepe, F., Piotto, G., Poretti, E., Rainer, M., Ribas, I., Sanchez, R. Zanmar, Santos, N. C., Scandariato, G., Silvotti, R., Southworth, J., Sozzetti, A. +50 morecore +2 more sourcesMining the XRT archive to probe the X-ray absorber structure in the AGN
population [PDF]
, 2014 One of the key ingredients of the Unified Model of Active Galactic Nuclei
(AGN) is the presence of a torus-like optically thick medium composed by dust
and gas around the putative supermassive black hole.Andreon, S., Ballo, L., Braito, V., Caccianiga, A., Campana, S., Della Ceca, R., Moretti, A., Severgnini, P., Vignali, C. +8 morecore +2 more sourcesSN 2005cs in M51 I. The first month of evolution of a subluminous SN II
plateau [PDF]
, 2006 Early time optical observations of supernova (SN) 2005cs in the Whirlpool
Galaxy (M51), are reported. Photometric data suggest that SN 2005cs is a
moderately under-luminous Type II plateau supernova (SN IIP).A. Harutyunyan, A. Pastorello, Abbott, Arnett, Baron, Benetti, Bresolin, Clocchiatti, Connolly, D. Sauer, Dessart, Dessart, Elmhamdi, Feldmeier, Filippenko, Filippenko, G. Di Rico, G. Valentini, Graham, Grevesse, H. Navasardyan, Hamuy, Hamuy, Hashimoto, Hendry, Hillier, K. Nomoto, K. S. Kawabata, Kloehr, L. Zampieri, Landolt, Leonard, Leonard, Li, Li, Lucy, M. Del Principe, M. Dolci, M. Ragni, M. T. Botticella, Maund, Maund, Mazzali, Mazzali, Mazzali, Mazzali, Menzies, Modjaz, N. Elias-Rosa, Nomoto, Nomoto, Nomoto, P. A. Mazzali, Paczynski, Pastorello, Pastorello, Patat, Phillips, Pozzo, Richmond, Richmond, S. Benetti, S. Gagliardi, S. Taubenberger, Schlegel, Smartt, Sonneborn, Strolger, Sugerman, Sugimoto, T. Iijima, Turatto, Turatto, Utrobin, Van Dyk, Van Dyk, Wheeler, Young, Zampieri, Zampieri +79 morecore +3 more sourcesNeutral Iron Emission Lines From The Day-side Of KELT-9b -- The GAPS
Programme With HARPS-N At TNG XX [PDF]
, 2020 We present the first detection of atomic emission lines from the atmosphere
of an exoplanet. We detect neutral iron lines from the day-side of KELT-9b (Teq
$\sim$ 4, 000 K).Affer, L., Allart, R., Benatti, S., Biazzo, K., Bignamini, A., Bonomo, A. S., Borsa, F., Borsato, L., Brogi, M., Bruno, G., Carleo, I., Claudi, R., Cosentino, R., Covino, E., Damasso, M., Desidera, S., Di Fabrizio, L., Désert, J. M., Ehrenreich, D., Fiorenzano, A., Fossati, L., Frustagli, G., Giacobbe, P., Harutyunyan, A., Hoeijmakers, J., Lanza, A. F., Lavie, B., Leto, G., Line, M., Lovis, C., Magazzù, A., Maggio, A., Malavolta, L., Maldonado, J., Mancini, L., Micela, G., Molinari, E., Nardiello, D., Nascimbeni, V., Pagano, I., Panwar, V., Pedani, M., Pino, L., Piotto, G., Poretti, E., Rainer, M., Scandariato, G., Smareglia, R., Sozzetti, A., Wyttenbach, A. +49 morecore +4 more sourcesSpectroscopy of the hot pulsating star Beta Cephei. Velocities and EWs
from C,N,O and Si lines [PDF]
, 2007 Frequencies in oscillating $\beta$ Cephei stars are usually inferred by means
of radial velocities measured from the SiIII triplet 4552-4574 A. These lines,
relatively insensitive to the variation of Teff through a pulsation cycle, show
small equivalent ...Busa', I., Catanzaro, G., Leone, F., Romano, P. +3 morecore +1 more sourceNIR Follow-Up of the VVDS 02hr Field [PDF]
, 2006 We present a new K-band survey covering 623 arcmin$^2$ in the VVDS 0226-0430
deep field down to a limiting magnitude K$_{\rm{Vega}}$ $\leq$ 20.5. We use the
spectroscopic sample extracted from this new K-band catalogue to assess the
effectiveness of ...Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Bondi, M., Bongiorno, A., Bottini, D., Brinchmann, J., Brun, V. Le, Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Cucciati, O., de la Torre, S., Fevre, O. Le, Foucaud, S., Franzetti, P., Garilli, B., Gavignaud, I., Guzzo, L., Ilbert, O., Iovino, A., Lamareille, F., Maccagni, D., Marano, B., Marinoni, C., Mazure, A., McCracken, H. J., Mellier, Y., Meneux, B., Merighi, R., Merluzzi, P., Paltani, S., Pello, R., Picat, J. -P., Pollo, A., Pozzetti, L., Radovich, M., Scaramella, R., Scodeggio, M., Temporin, S., Tresse, L., Vergani, D., Vettolani, G., Walcher, C. J., Zamorani, G., Zanichelli, A., Zucca, E. +48 morecore +3 more sources
