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pro vyhledávání: '"Faccioli, Lorenzo"'
Autor:
Kosiba, Matej, Lieu, Maggie, Altieri, Bruno, Clerc, Nicolas, Faccioli, Lorenzo, Kendrew, Sarah, Valtchanov, Ivan, Sadibekova, Tatyana, Pierre, Marguerite, Hroch, Filip, Werner, Norbert, Burget, Lukáš, Garrel, Christian, Koulouridis, Elias, Gaynullina, Evelina, Molham, Mona, Ramos-Ceja, Miriam E., Khalikova, Alina
Galaxy clusters appear as extended sources in XMM-Newton images, but not all extended sources are clusters. So, their proper classification requires visual inspection with optical images, which is a slow process with biases that are almost impossible
Externí odkaz:
http://arxiv.org/abs/2006.05998
Autor:
Faccioli, Lorenzo, Smith, Martin C., Yuan, H. -B., Zhang, H. -H., Liu, X. -W., Zhao, H. -B., Yao, J. -S.
We present a catalog of RR Lyrae stars (RRLs) observed by the Xuyi Schmidt Telescope Photometric Survey (XDSS). The area we consider is located in the North Galactic Cap, covering 376.75 sq deg at RA $\approx$ 150 deg and Dec $\approx$ 27 deg down to
Externí odkaz:
http://arxiv.org/abs/1404.6318
Autor:
Sadibekova, Tatyana, Pierre, Marguerite, Clerc, Nicolas, Faccioli, Lorenzo, Gastaud, Rene, Fevre, Jean-Paul Le, Rozo, Eduardo, Rykoff, Eli S.
We performed a detailed and, for a large part interactive, analysis of the matching output between the X-CLASS and redMaPPer cluster catalogues. The overlap between the two catalogues has been accurately determined and possible cluster positional err
Externí odkaz:
http://arxiv.org/abs/1403.4100
Autor:
Pilachowski, Caty, Badenes, Carles, Bailey, Stephen, Barth, Aaron, Beaton, Rachel, Bell, Eric, Bernstein, Rebecca, Bian, Fuyan, Blanton, Michael, Blum, Robert, Bolton, Adam, Bond, Howard, Brodwin, Mark, Bullock, James, Carlin, Jeff, Chary, Ranga-Ram, Cinabro, David, Cooper, Michael, Cota, Jorge L. C., Davis, Marc, Dawson, Kyle, Dey, Arjun, Donahue, Megan, Drake, Jeremy, Ellingson, Erica, Faccioli, Lorenzo, Fan, Xiaohui, Ferguson, Harry, Gawiser, Eric, Geha, Marla, Giavalisco, Mauro, Gonzalez, Anthony, Griest, Kim, Grossan, Bruce, Guhathakurta, Raja, Harding, Paul, Heap, Sara R., Ho, Shirley, Howell, Steve, Jannuzi, Buell, Kalirai, Jason, Keeney, Brian, Kewley, Lisa, Kong, Xu, Lampton, Michael, Lin, Wei-Peng, de la Macorra, Axel, Macri, Lucas, Majewski, Steve, Martini, Paul, Massey, Phil, McSwain, Virginia, Miller, Adam A., Minniti, Dante, Modjaz, Maryam, Morrison, Heather, Moustakas, John, Myers, Adam, Najita, Joan, Newman, Jeffrey, Norman, Dara, Olsen, Knut, Pierce, Michael, Pope, Alexandra, Prescott, Moire, Reddy, Naveen, Reil, Kevin, Rest, Armin, Rhode, Katherine, Rockosi, Connie, Rudnick, Greg, Saha, Abhijit, Salzer, John, Sanders, David, Schlegel, David, Sesar, Branimir, Shields, Joseph, Silverman, Jeffrey, Simon, Josh, Stanford, Adam, Stern, Daniel, Storrie-Lombardi, Lisa, Suntzeff, Nicholas, Surace, Jason, Szalay, Alex, Ulmer, Melville, Weiner, Ben, Willman, Beth, Windhorst, Rogier, Wood-Vasey, Michael
This document summarizes the results of a community-based discussion of the potential science impact of the Mayall+BigBOSS highly multiplexed multi-object spectroscopic capability. The KPNO Mayall 4m telescope equipped with the DOE- and international
Externí odkaz:
http://arxiv.org/abs/1211.0285
Publikováno v:
ApJ, 672:604, 2008 January 1
We present results from a study of the orbits of eclipsing binary stars (EBs) in the Magellanic Clouds. The samples comprise 4510 EBs found in the Large Magellanic Cloud (LMC) by the MACHO project, 2474 LMC EBs found by the OGLE-II project (of which
Externí odkaz:
http://arxiv.org/abs/0711.1633
Autor:
Faccioli, Lorenzo, Alcock, Charles, Cook, Kem, Prochter, Gabriel E., Protopapas, Pavlos, Syphers, David
Publikováno v:
Astron.J.134:1963-1993,2007
We present a new sample of 4634 eclipsing binary stars in the Large Magellanic Cloud (LMC), expanding on a previous sample of 611 objects and a new sample of 1509 eclipsing binary stars in the Small Magellanic Cloud (SMC), that were identified in the
Externí odkaz:
http://arxiv.org/abs/0711.1617
The light curve of a blue variable in the MACHO LMC database (FTS ID 78.5979.72) appeared nearly unvarying for ~4 years (quasi-flat segment) but then rapidly changed to become periodic with noisy minima for the remaining 4 years (periodic segment); t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0503090
Autor:
Faccioli, Lorenzo
Publikováno v:
Faccioli, Lorenzo. (2011). Reducing Zero-point Systematics in Dark Energy Supernova Experiments. Lawrence Berkeley National Laboratory. Lawrence Berkeley National Laboratory: Lawrence Berkeley National Laboratory. Retrieved from: http://www.escholarship.org/uc/item/7nd338dj
We study the effect of filter zero-point uncertainties on future supernova dark energy missions. Fitting for calibration parameters using simultaneous analysis of all Type Ia supernova standard candles achieves a significant improvement over more tra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::abeb90a61cd43d482d0576de7beb90ad
http://www.escholarship.org/uc/item/7nd338dj
http://www.escholarship.org/uc/item/7nd338dj
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