Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Paolo Ochner"'
Publikováno v:
Aerospace, Vol 11, Iss 9, p 693 (2024)
In recent years, interest in the Moon has grown exponentially, thanks mainly to space programs with strong international cooperation, such as the NASA Artemis program. Several scientific committees have identified the lunar south pole as the region o
Externí odkaz:
https://doaj.org/article/a3aa010e31fc4c5db33fb66eba20cc97
Autor:
K. Azalee Bostroem, Jeniveve Pearson, Manisha Shrestha, David J. Sand, Stefano Valenti, Saurabh W. Jha, Jennifer E. Andrews, Nathan Smith, Giacomo Terreran, Elizabeth Green, Yize Dong, Michael Lundquist, Joshua Haislip, Emily T. Hoang, Griffin Hosseinzadeh, Daryl Janzen, Jacob E. Jencson, Vladimir Kouprianov, Emmy Paraskeva, Nicolas E. Meza Retamal, Daniel E. Reichart, Iair Arcavi, Alceste Z. Bonanos, Michael W. Coughlin, Ross Dobson, Joseph Farah, Lluís Galbany, Claudia Gutiérrez, Suzanne Hawley, Leslie Hebb, Daichi Hiramatsu, D. Andrew Howell, Takashi Iijima, Ilya Ilyin, Kiran Jhass, Curtis McCully, Sean Moran, Brett M. Morris, Alessandra C. Mura, Tomás E. Müller-Bravo, James Munday, Megan Newsome, Maria Th. Pabst, Paolo Ochner, Estefania Padilla Gonzalez, Andrea Pastorello, Craig Pellegrino, Lara Piscarreta, Aravind P. Ravi, Andrea Reguitti, Laura Salo, József Vinkó, Kellie de Vos, J. C. Wheeler, G. Grant Williams, Samuel Wyatt
Publikováno v:
The Astrophysical Journal Letters, Vol 956, Iss 1, p L5 (2023)
We present the optical spectroscopic evolution of SN 2023ixf seen in subnight cadence spectra from 1.18 to 15 days after explosion. We identify high-ionization emission features, signatures of interaction with material surrounding the progenitor star
Externí odkaz:
https://doaj.org/article/4770225259c04e39bbbf9c2988c9bbb1
Autor:
Costantino Sigismondi, Paolo Ochner
Publikováno v:
The Sixteenth Marcel Grossmann Meeting.
Autor:
Costantino Sigismondi, Paolo Ochner
Publikováno v:
The Sixteenth Marcel Grossmann Meeting.
Autor:
Costantino Sigismondi, Paolo Ochner
Publikováno v:
The Sixteenth Marcel Grossmann Meeting.
Autor:
Jules Bourdelle de Micas, Sonia Fornasier, Marco Delbo, Chrysa Avdellidou, Gerard Van Belle, Paolo Ochner
Asteroids, along with other small bodies, are what is left over of the original planetesimal disk from the planet-formation era. Therefore, these objects are considered the best tracers for the processes that occurred during the earliest history of o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b4304174c7b11a97b6e2202708ce9d9a
https://doi.org/10.5194/epsc2022-440
https://doi.org/10.5194/epsc2022-440
Autor:
Virginio Oldani, Federico Manzini, Paolo Ochner, Andrea Reguitti, Luigi R. Bedin, Raoul Behrend, Jean Gabriel Bosch
Publikováno v:
Icarus. 395:115451
Autor:
Luca Zampieri, Sandro Mereghetti, Roberto Turolla, Giampiero Naletto, Paolo Ochner, Aleksandr Burtovoi, Michele Fiori, Cristiano Guidorzi, Luciano Nicastro, Eliana Palazzi, Maura Pilia, Andrea Possenti
In September 2021 the magnetar SGR J1935+2154 entered a stage of burst/flaring activity in the hard X-ray band. On September 10, 2021 we observed SGR J1935+2154 with the fiber-fed fast optical photon counter IFI+Iqueye, mounted at the 1.22 m Galileo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1348729b7c4e4bb619c217a13ee84df
http://hdl.handle.net/20.500.12386/31999
http://hdl.handle.net/20.500.12386/31999
Introduction Within the NEOROCKS project, we are performing a spectroscopic investigation of NEOs in the visible region, in particular, when available, of PHAs, with the Asiago Observatory telescopes (1.80m and 1.20m). Potentially Hazardous Objects a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1cccd5732abbe400c966d8e919a34b9e
https://doi.org/10.5194/epsc2021-387
https://doi.org/10.5194/epsc2021-387
Autor:
Monica Lazzarin, Fiorangela La Forgia, Alessandro Siviero, Paolo Ochner, Elisa Frattin, Petr Pravec, Petr Fatka
With an estimated diameter of about 2200m (http://neo.ssa.esa.int/), and a MOID (minimum orbital intersection distance) of 0.0154 au (6 Lunar Distances LD), (52768) 1998 OR2 is one of the largest known Potentially Hazardous Asteroid. On 29 April 2020
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c9f4aec417c979adda45afad64260c89
https://doi.org/10.5194/epsc2020-974
https://doi.org/10.5194/epsc2020-974