Zobrazeno 1 - 10
of 5 135
pro vyhledávání: '"Šivo, A."'
We design and implement from scratch a new fuzzer called SIVO that refines multiple stages of grey-box fuzzing. First, SIVO refines data-flow fuzzing in two ways: (a) it provides a new taint inference engine that requires only logarithmic in the inpu
Externí odkaz:
http://arxiv.org/abs/2102.02394
Autor:
Marsh, Herbert W., Hau, Kit-Tai
Publikováno v:
The Journal of Experimental Education, 1998 Apr 01. 66(3), 274-285.
Externí odkaz:
https://www.jstor.org/stable/20152566
Autor:
Conod, Uriel, Jackson, Kate, Turri, Paolo, Chapman, Scott, Lardière, Olivier, Lamb, Masen, Correia, Carlos, Sivo, Gaetano, Sivanandam, Suresh, Véran, Jean-Pierre
Publikováno v:
Publications of the Astronomical Society of the Pacific, Volume 135, Number 1052, 2023
The Gemini Infrared Multi-Object Spectrograph (GIRMOS) will be a near-infrared, multi-object, medium spectral resolution, integral field spectrograph (IFS) for Gemini North Telescope, designed to operate behind the future Gemini North Adaptive Optics
Externí odkaz:
http://arxiv.org/abs/2310.15338
Akademický článek
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Autor:
Calore, Francesca, Carenza, Pierluca, Eckner, Christopher, Giannotti, Maurizio, Lucente, Giuseppe, Mirizzi, Alessandro, Sivo, Francesco
Publikováno v:
Phys. Rev. D 109, 043010 (2024)
A future Galactic Supernova (SN) explosion can lead to a gamma-ray signal induced by ultralight Axion-Like Particles (ALPs) thermally produced in the SN core and converted into high-energy photons in the Galactic magnetic field. The detection of such
Externí odkaz:
http://arxiv.org/abs/2306.03925
Akademický článek
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Autor:
Sivo, Gaetano, Scharwächter, Julia, Lazo, Manuel, Blain, Célia, Goodsell, Stephen, van Dam, Marcos, Tschimmel, Martin, Roe, Henry, Lotz, Jennifer, Tomassino-Reed, Kim, Rambold, William, Raich, Courtney, Cardenes, Ricardo, Ebbers, Angelic, Gaggstatter, Tim, Gigoux, Pedro, Schneider, Thomas, Cavedoni, Charles, Kang, Stacy, Karewicz, Stanislas, Carr, Heather, Ball, Jesse, Hirst, Paul, Chirre, Emmanuel, White, John, Magill, Lindsay, Grogan, Molly, Jordan, Anne, Sivanandam, Suresh, Lamb, Masen, Muzzin, Adam, Marin, Eduardo, Chapman, Scott, Dunn, Jennifer, Kerley, Dan, Véran, Jean-Pierre, Andersen, Morten, Marchis, Franck, Diaz, Ruben, Blakeslee, John, Pierce, Michael, Carrasco, Rodrigo, Kim, Hwyhyun, Feldmeier-Krause, Anja, McConnachie, Alan, Jee, James, Fraser, Wesley, Ammons, Mark, Packham, Christopher, Bally, John, Dupuy, Trent, Huber, Daniel, Lemoine-Busserole, Marie, Puzia, Thomas, Turri, Paolo, Trujillo, Chadwick, Lee, Janice
The Gemini North Adaptive Optics (GNAO) facility is the upcoming AO facility for Gemini North providing a state-of-the-art AO system for surveys and time domain science in the era of JWST and Rubin operations. GNAO will be optimized to feed the Gemin
Externí odkaz:
http://arxiv.org/abs/2208.14519
Autor:
CAPPELLETTI, FRANCESCA
Publikováno v:
The Burlington Magazine, 2012 Jan 01. 154(1306), 46-47.
Externí odkaz:
https://www.jstor.org/stable/41418905
Autor:
Calore, Francesca, Carenza, Pierluca, Eckner, Christopher, Fischer, Tobias, Giannotti, Maurizio, Jaeckel, Joerg, Kotake, Kei, Kuroda, Takami, Mirizzi, Alessandro, Sivo, Francesco
Axion-like particles (ALPs) may be abundantly produced in core-collapse (CC) supernovae (SNe), hence the cumulative signal from all past SN events can create a diffuse flux peaked at energies of about 25~MeV. We improve upon the modeling of the ALPs
Externí odkaz:
http://arxiv.org/abs/2110.03679