Zobrazeno 1 - 10
of 6 855
pro vyhledávání: '"Esposito S"'
Autor:
Gholizadeh P, Safari R, Marofi P, Zeinalzadeh E, Pagliano P, Ganbarov K, Esposito S, Khodadadi E, Yousefi M, Samadi Kafil H
Publikováno v:
Journal of Inflammation Research, Vol Volume 13, Pp 285-292 (2020)
Pourya Gholizadeh,1,2 Rohollah Safari,3 Parham Marofi,4 Elham Zeinalzadeh,4 Pasquale Pagliano,5 Khudaverdi Ganbarov,6 Silvano Esposito,5 Ehsaneh Khodadadi,7 Mehdi Yousefi,8 Hossein Samadi Kafil7 1Student Research Committee, Tabriz University of Medic
Externí odkaz:
https://doaj.org/article/415b9e446def41ada92ddc7dfdb65a6d
Publikováno v:
AO4ELT7 proceedings 2023
The upcoming extremely large telescopes will have to deal with the so-called ''pupil fragmentation'' effect: for what concerns the Extremely Large Telescope (ELT), the presence of thick spider legs supporting the secondary mirror may induce unseen ph
Externí odkaz:
http://arxiv.org/abs/2312.12898
Autor:
Crowe, S., Fedriani, R., Tan, J. C., Whittle, M., Zhang, Y., Garatti, A. Caratti o, Farias, J. P., Gautam, A., Telkamp, Z., Rothberg, B., Grudic, M., Andersen, M., Cosentino, G., Garcia-Lopez, R., Rosero, V., Tanaka, K., Pinna, E., Rossi, F., Miller, D., Agapito, G., Plantet, C., Ghose, E., Christou, J., Power, J., Puglisi, A., Briguglio, R., Brusa, G., Taylor, G., Zhang, X., Mazzoni, T., Bonaglia, M., Esposito, S., Veillet, C.
Methods: Broad- and narrow-band imaging of AFGL 5180 was made in the NIR with the LBT, in both seeing-limited ($\sim0.5\arcsec$) and high angular resolution ($\sim0.09\arcsec$) Adaptive Optics (AO) modes, as well as with HST. Archival ALMA continuum
Externí odkaz:
http://arxiv.org/abs/2311.11909
Autor:
Mannucci, F., Scialpi, M., Ciurlo, A., Yeh, S., Marconcini, C., Tozzi, G., Cresci, G., Marconi, A., Amiri, A., Belfiore, F., Carniani, S., Cicone, C., Nardini, E., Pancino, E., Rubinur, K., Severgnini, P., Ulivi, L., Venturi, G., Vignali, C., Volonteri, M., Pinna, E., Rossi, F., Puglisi, A., Agapito, G., Plantet, C., Ghose, E., Carbonaro, L., Xompero, M., Grani, P., Esposito, S., Power, J., Ramon, J. C. Guerra, Lefebvre, M., Cavallaro, A., Davies, R., Riccardi, A., Macintosh, M., Taylor, W., Dolci, M., Baruffolo, A., Feuchtgruber, H., Kravchenko, K., Rau, C., Sturm, E., Wiezorrek, E., Dallilar, Y., Kenworthy, M.
The Gaia-Multi-Peak (GMP) technique can be used to identify large numbers of dual or lensed AGN candidates at sub-arcsec separation, allowing us to study both multiple SMBHs in the same galaxy and rare, compact lensed systems. The observed samples ca
Externí odkaz:
http://arxiv.org/abs/2305.07396
Autor:
Davies, R., Absil, O., Agapito, G., Berbel, A. Agudo, Baruffolo, A., Biliotti, V., Bonaglia, M., Bonse, M., Briguglio, R., Campana, P., Cao, Y., Carbonaro, L., Cortes, A., Cresci, G., Dallilar, Y., Dannert, F., De Rosa, R. J., Deysenroth, M., Di Antonio, I., Di Cianno, A., Di Rico, G., Doelman, D., Dolci, M., Dorn, R., Eisenhauer, F., Esposito, S., Fantinel, D., Ferruzzi, D., Feuchtgruber, H., Finger, G., Schreiber, N. M. Förster, Gao, X., Gemperlein, H., Genzel, R., Gillessen, S., Ginski, C., Glauser, A. M., Glindemann, A., Grani, P., Hartl, M., Hayoz, J., Heida, M., Henry, D., Hofmann, R., Huber, H., Kasper, M., Keller, C., Kenworthy, M., Kravchenko, K., Kuntschner, H., Lacour, S., Lightfoot, J., Lunney, D., Lutz, D., Macintosh, M., Mannucci, F., Marsset, M., Modigliani, A., Neeser, M., de Xivry, G. Orban, Ott, T., Pallanca, L., Patapis, P., Pearson, D., Peña, E., Percheron, I., Puglisi, A., Quanz, S. P., Rabien, S., Rau, C., Riccardi, A., Salasnich, B., Schmid, H. -M., Schubert, J., Serra, B., Shimizu, T., Snik, F., Sturm, E., Tacconi, L., Taylor, W., Valentini, A., Waring, C., Wiezorrek, E., Xompero, M.
ERIS, the Enhanced Resolution Imager and Spectrograph, is an instrument that both extends and enhances the fundamental diffraction limited imaging and spectroscopy capability for the VLT. It replaces two instruments that were being maintained beyond
Externí odkaz:
http://arxiv.org/abs/2304.02343
Autor:
Massi, F., Garatti, A. Caratti o, Cesaroni, R., Sridharan, T. K., Ghose, E., Pinna, E., Beltrán, M. T., Leurini, S., Moscadelli, L., Sanna, A., Agapito, G., Briguglio, R., Christou, J., Esposito, S., Mazzoni, T., Miller, D., Plantet, C., Power, J., Puglisi, A., Rossi, F., Rothberg, B., Taylor, G., Veillet, C.
Publikováno v:
A&A 672, A113 (2023)
We exploit the increased sensitivity of the recently installed AO SOUL at the LBT to obtain new high-spatial-resolution NIR images of the massive young stellar object IRAS20126+4104 and its outflow. We aim to derive the jet proper motions and kinemat
Externí odkaz:
http://arxiv.org/abs/2301.06832
In this paper we will discuss the application of optimal filtering techniques for the adaptive optics system of the LBT telescope. We have studied the application of both Kalman and H$_\infty$ filters to estimate the temporal evolution of the phase p
Externí odkaz:
http://arxiv.org/abs/2301.05165
Autor:
Selva, J., Argyroudis, S., Cotton, F., Esposito, S., Iqbal, S.M., Lorito, S., Stojadinovic, B., Basili, R., Hoechner, A., Mignan, A., Pitilakis, K., Thio, H.K., Giardini, D.
Publikováno v:
In International Journal of Disaster Risk Reduction August 2024 110
Autor:
Loddo, F., Andreazza, A., Arteche, F., Barbero, M.B., Barillon, P., Beccherle, R., Bilei, G.M., Bjalas, W., Bonaldo, S., Bortoletto, D., Calderini, G., Caratelli, A., Christian, D.C., Christiansen, J., Conti, E., Crescioli, F., Daas, M., De Robertis, G., Demaria, N., Deptuch, G.C., Dieter, Y., Dimitrievska, A., Ding, L., Esposito, S., Exarchou, D., Fahim, F., Fioriti, A., Fougeron, D., Gaioni, L., Garcia-Sciveres, M., Gerardin, S., Gnani, D., Grippo, M., Gromov, V., Hamer, M., Havranek, M., Heim, T., Hemperek, T., Hinterkeuser, F., Hoff, J., Huiberts, S., Janssen, J., Jara Casas, L.M., Jirsa, J., John, J.J., Kampkotter, J., Karagounis, M., Khwaira, Y., Kluit, R., Krieger, A., Krueger, H., Lalic, J., Lauritzen, M., Licciulli, F., Lipton, R., Liu, T., Lopez Morillo, E., Lounis, A., Luongo, F., Magazzu, G., Marcisovsky, M., Marconi, S., Marquez Lasso, F., Marzocca, C., Mattiazzo, S., Menouni, M., Minuti, M., Mironova, M., Miryala, S., Monteil, E., Moustakas, K., Muõz Chavero, F., Neue, G., Orfanelli, S., Paccagnella, A., Pacher, L., Palla, F., Palomo Pinto, F.R., Papadopoulou, A., Paterno, A., Petri, A., Placidi, P., Pohl, D., Pradas, A., Prydderch, M.L., Pulli, A., Ratti, L., Re, V., Rehman, A., Rymaszewski, P., Solal, M.C., Standke, M., Stiller, A., Strebler, T., Stugu, B., Thomas, S., Traversi, G., Vogrig, D., Vogt, M., Wang, T., Yang, H., Zdenko, J., Zimmerman, T.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A October 2024 1067
The future large adaptive telescopes will trigger new constraints for the calibration of Adaptive Optics (AO) systems equipped with pre-focal Deformable Mirrors (DM). The image of the DM actuators grid as seen by the Wave-Front Sensor (WFS) may evolv
Externí odkaz:
http://arxiv.org/abs/2104.11261