Zobrazeno 1 - 10
of 35
pro vyhledávání: '"Cabanac, Rémi"'
Autor:
Rojas, Karina, Collett, Thomas E., Ballard, Daniel, Magee, Mark R., Birrer, Simon, Buckley-Geer., Elizabeth, Chan, James H. H., Clément, Benjamin, Diego, José M., Gentile, Fabrizio, González, Jimena, Joseph, Rémy, Mastache, Jorge, Schuldt, Stefan, Tortora, Crescenzo, Verdugo, Tomás, Verma, Aprajita, Daylan, Tansu, Millon, Martin, Jackson, Neal, Dye, Simon, Melo, Alejandra, Mahler, Guillaume, Ogando, Ricardo L. C., Courbin, Frédéric, Fritz, Alexander, Herle, Aniruddh, Barroso, Javier A. Acevedo, Cañameras, Raoul, Cornen, Claude, Dhanasingham, Birendra, Glazebrook, Karl, Martinez, Michael N., Ryczanowski, Dan, Savary, Elodie, Góis-Silva, Filipe, Ureña-López, L. Arturo, Wiesner, Matthew P., Wilde, Joshua, Calçada, Gabriel Valim, Cabanac, Rémi, Pan, Yue, Sierra, Isaac, Despali, Giulia, Cavalcante-Gomes, Micaele V., Macmillan, Christine, Maresca, Jacob, Grudskaia, Aleksandra, O'Donnell, Jackson H., Paic, Eric, Niemiec, Anna, de la Bella, Lucia F., Bromley, Jane, Williams, Devon M., More, Anupreeta, Levine, Benjamin C.
We investigate the ability of human 'expert' classifiers to identify strong gravitational lens candidates in Dark Energy Survey like imaging. We recruited a total of 55 people that completed more than 25$\%$ of the project. During the classification
Externí odkaz:
http://arxiv.org/abs/2301.03670
Autor:
Metcalf, R. Benton, Meneghetti, M., Avestruz, Camille, Bellagamba, Fabio, Bom, Clécio R., Bertin, Emmanuel, Cabanac, Rémi, Courbin, F., Davies, Andrew, Decencière, Etienne, Flamary, Rémi, Gavazzi, Raphael, Geiger, Mario, Hartley, Philippa, Huertas-Company, Marc, Jackson, Neal, Jullo, Eric, Kneib, Jean-Paul, Koopmans, Léon V. E., Lanusse, François, Li, Chun-Liang, Ma, Quanbin, Makler, Martin, Li, Nan, Lightman, Matthew, Petrillo, Carlo Enrico, Serjeant, Stephen, Schäfer, Christoph, Sonnenfeld, Alessandro, Tagore, Amit, Tortora, Crescenzo, Tuccillo, Diego, Valentín, Manuel B., Velasco-Forero, Santiago, Kleijn, Gijs A. Verdoes, Vernardos, Georgios
Publikováno v:
A&A 625, A119 (2019)
Large scale imaging surveys will increase the number of galaxy-scale strong lensing candidates by maybe three orders of magnitudes beyond the number known today. Finding these rare objects will require picking them out of at least tens of millions of
Externí odkaz:
http://arxiv.org/abs/1802.03609
Autor:
Ibata, Rodrigo, McConnachie, Alan, Cuillandre, Jean-Charles, Fantin, Nicholas, Haywood, Misha, Martin, Nicolas F., Bergeron, Piere, Beckmann, Volker, Bernard, Edouard, Bonifacio, Piercarlo, Caffau, Elisabetta, Carlberg, Raymond, Côté, Patrick, Cabanac, Rémi, Chapman, Scott, Duc, Pierre-Alain, Durret, Florence, Famaey, Benoît, Frabbro, Sébastien, Gwyn, Stephen, Hammer, Francois, Hill, Vanessa, Hudson, Michael J., Lançon, Ariane, Lewis, Geraint, Malhan, Khyati, di Matteo, Paola, McCracken, Henry, Mei, Simona, Mellier, Yannick, Navarro, Julio, Pires, Sandrine, Pritchet, Chris, Reylé, Celine, Richer, Harvey, Robin, Annie C., Jannsen, Rubén Sánchez, Sawicki, Marcin, Scott, Douglas, Scottez, Vivien, Spekkens, Kristine, Starkenburg, Else, Thomas, Guillaume, Venn, Kim
We present the chemical distribution of the Milky Way, based on 2,900$\, {\rm deg^2}$ of $u$-band photometry taken as part of the Canada-France Imaging Survey. When complete, this survey will cover 10,000$\, {\rm deg^2}$ of the Northern sky. By combi
Externí odkaz:
http://arxiv.org/abs/1708.06359
Autor:
Ibata, Rodrigo, McConnachie, Alan, Cuillandre, Jean-Charles, Fantin, Nicholas, Haywood, Misha, Martin, Nicolas F., Bergeron, Piere, Beckmann, Volker, Bernard, Edouard, Bonifacio, Piercarlo, Caffau, Elisabetta, Carlberg, Raymond, Côté, Patrick, Cabanac, Rémi, Chapman, Scott, Duc, Pierre-Alain, Durret, Florence, Famaey, Benoît, Frabbro, Sébastien, Gwyn, Stephen, Hammer, Francois, Hill, Vanessa, Hudson, Michael J., Lançon, Ariane, Lewis, Geraint, Malhan, Khyati, di Matteo, Paola, McCracken, Henry, Mei, Simona, Mellier, Yannick, Navarro, Julio, Pires, Sandrine, Pritchet, Chris, Reylé, Celine, Richer, Harvey, Robin, Annie C., Jannsen, Rubén Sánchez, Sawicki, Marcin, Scott, Douglas, Scottez, Vivien, Spekkens, Kristine, Starkenburg, Else, Thomas, Guillaume, Venn, Kim
The Canada-France Imaging Survey (CFIS) will map the northern high Galactic latitude sky in the $u$-band ("CFIS-u", 10,000$\, {\rm deg^2}$) and in the $r$-band ("CFIS-r", 5,000$\, {\rm deg^2}$), enabling a host of stand-alone science investigations,
Externí odkaz:
http://arxiv.org/abs/1708.06356
Telescopes with unobstructed pupil are known to deliver clean point spread function (PSF) to their focal plane, in contrast to traditional telescopes with obstructed pupil. Recent progress in the manufacturing aspheric surfaces and mounting accuracy
Externí odkaz:
http://arxiv.org/abs/1403.2879
Autor:
More, Anupreeta, Cabanac, Remi, More, Surhud, Alard, Christophe, Limousin, Marceau, Kneib, Jean-Paul, Gavazzi, Raphael, Motta, Veronica
We present the Strong Lensing Legacy Survey - ARCS (SARCS) sample compiled from the final T0006 data release of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) covering a total non-overlapping area of 159 sq.deg. We adopt a semi-automatic m
Externí odkaz:
http://arxiv.org/abs/1109.1821
Autor:
Limousin, Marceau, Jullo, Eric, Richard, Johan, Cabanac, Remi, Suyu, Sherry H., Halkola, Aleksi, Kneib, Jean-Paul, Gavazzi, Raphael, Soucail, Genevieve
Precise modelling of strong lensing systems can be affected by external mass distributions, e.g. the group or cluster within which the lens is embedded. In this article, we propose to turn this limitation to our advantage and to use precise strong le
Externí odkaz:
http://arxiv.org/abs/0906.4118
We recently reported the discovery of FORJ0332-3557, a lensed Lyman-break galaxy at z=3.77 in a remarkable example of strong galaxy-galaxy gravitational lensing. We present here a medium-resolution rest-frame UV spectrum of the source, which appears
Externí odkaz:
http://arxiv.org/abs/0803.0679
Publikováno v:
Astrophys.J. 631 (2005) 252-261
We present high-resolution observations of Henize 2-10 in Ks (2.2um), L' (3.8um), M' (4.8um) bands. These allow for the first time to track accurately the structures at the heart of the galaxy from the optical to the radio. All radio knots previously
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506042