Zobrazeno 1 - 10
of 62
pro vyhledávání: '"Dilday, Benjamin"'
Autor:
Nugent, Peter E., Sullivan, Mark, Cenko, S. Bradley, Thomas, Rollin C., Kasen, Daniel, Howell, D. Andrew, Bersier, David, Bloom, Joshua S., Kulkarni, S. R., Kandrashoff, Michael T., Filippenko, Alexei V., Silverman, Jeffrey M., Marcy, Geoffrey W., Howard, Andrew W., Isaacson, Howard T., Maguire, Kate, Suzuki, Nao, Tarlton, James E., Pan, Yen-Chen, Bildsten, Lars, Fulton, Benjamin J., Parrent, Jerod T., Sand, David, Podsiadlowski, Philipp, Bianco, Federica B., Dilday, Benjamin, Graham, Melissa L., Lyman, Joe, James, Phil, Kasliwal, Mansi M., Law, Nicholas M., Quimby, Robert M., Hook, Isobel M., Walker, Emma S., Mazzali, Paolo, Pian, Elena, Ofek, Eran O., Gal-Yam, Avishay, Poznanski, Dovi
Type Ia supernovae (SNe Ia) have been used empirically as standardized candles to reveal the accelerating universe even though fundamental details, such as the nature of the progenitor system and how the star explodes, remained a mystery. There is co
Externí odkaz:
http://arxiv.org/abs/1110.6201
Autor:
Smith, Mathew, Nichol, Robert C, Dilday, Benjamin, Marriner, John, Kessler, Richard, Bassett, Bruce, Cinabro, David, Frieman, Joshua, Garnavich, Peter, Jha, Saurabh W, Lampeitl, Hubert, Sako, Masao, Schneider, Donald P, Sollerman, Jesper
Using data from the Sloan Digital Sky Supernova Survey-II, we measure the rate of Type Ia Supernovae (SNe Ia) as a function of galaxy properties at intermediate redshift. A sample of 342 SNe Ia with 0.05
Externí odkaz:
http://arxiv.org/abs/1108.4923
Autor:
Sako, Masao, Bassett, Bruce, Connolly, Brian, Dilday, Benjamin, Campbell, Heather, Frieman, Joshua, Gladney, Larry, Kessler, Richard, Lampeitl, Hubert, Marriner, John, Miquel, Ramon, Nichol, Robert, Schneider, Donald, Smith, Mathew, Sollerman, Jesper
We analyze the three-year SDSS-II Superernova (SN) Survey data and identify a sample of 1070 photometric SN Ia candidates based on their multi-band light curve data. This sample consists of SN candidates with no spectroscopic confirmation, with a sub
Externí odkaz:
http://arxiv.org/abs/1107.5106
Autor:
Hayden, Brian T., Garnavich, Peter M., Kasen, Daniel, Dilday, Benjamin, Frieman, Joshua A., Jha, Saurabh W., Lampeitl, Hubert, Nichol, Robert C., Sako, Masao, Schneider, Donald P., Smith, Mathew, Sollerman, Jesper, Wheeler, J. Craig
Publikováno v:
The Astrophysical Journal, Volume 722, Issue 2, pp. 1691-1698 (2010)
From the set of nearly 500 spectroscopically confirmed type~Ia supernovae and around 10,000 unconfirmed candidates from SDSS-II, we select a subset of 108 confirmed SNe Ia with well-observed early-time light curves to search for signatures from shock
Externí odkaz:
http://arxiv.org/abs/1008.4797
Autor:
Lampeitl, Hubert, Smith, Mathew, Nichol, Robert C., Bassett, Bruce, Cinabro, David, Dilday, Benjamin, Foley, Ryan J., Frieman, Joshua A., Garnavich, Peter M., Goobar, Ariel, Im, Myungshin, Jha, Saurabh W., Marriner, John, Miquel, Ramon, Nordin, Jakob, Östman, Linda, Riess, Adam G., Sako, Masao, Schneider, Donald P., Sollerman, Jesper, Stritzinger, Maximilian
Publikováno v:
Astrophys.J.722:566-576,2010
We present an analysis of the host galaxy dependencies of Type Ia Supernovae (SNe Ia) from the full three year sample of the SDSS-II Supernova Survey. We rediscover, to high significance, the strong correlation between host galaxy typeand the width o
Externí odkaz:
http://arxiv.org/abs/1005.4687
A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey
Autor:
Dilday, Benjamin, Bassett, Bruce, Becker, Andrew, Bender, Ralf, Castander, Francisco, Cinabro, David, Frieman, Joshua A., Galbany, Lluís, Garnavich, Peter, Goobar, Ariel, Hopp, Ulrich, Ihara, Yutaka, Jha, Saurabh W., Kessler, Richard, Lampeitl, Hubert, Marriner, John, Miquel, Ramon, Mollá, Mercedes, Nichol, Robert C., Nordin, Jakob, Riess, Adam G., Sako, Masao, Schneider, Donald P., Smith, Mathew, Sollerman, Jesper, Wheeler, J. Craig, Östman, Linda, Bizyaev, Dmitry, Brewington, Howard, Malanushenko, Elena, Malanushenko, Viktor, Oravetz, Dan, Pan, Kaike, Simmons, Audrey, Snedden, Stephanie
Publikováno v:
Astrophys.J.715:1021-1035,2010
ABRIDGED We present measurements of the Type Ia supernova (SN) rate in galaxy clusters based on data from the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. The cluster SN Ia rate is determined from 9 SN events in a set of 71 C4 clusters at
Externí odkaz:
http://arxiv.org/abs/1003.1521
Autor:
Dilday, Benjamin, Smith, Mathew, Bassett, Bruce, Becker, Andrew, Bender, Ralf, Castander, Francisco, Cinabro, David, Filippenko, Alexei V., Frieman, Joshua A., Galbany, Lluis, Garnavich, Peter M., Goobar, Ariel, Hopp, Ulrich, Ihara, Yutaka, Jha, Saurabh W., Kessler, Richard, Lampeitl, Hubert, Marriner, John, Miquel, Ramon, Molla, Mercedes, Nichol, Robert C., Nordin, Jakob, Riess, Adam G., Sako, Masao, Schneider, Donald P., Sollerman, Jesper, Wheeler, J. Craig, Ostman, Linda, Bizyaev, Dmitry, Brewington, Howard, Malanushenko, Elena, Malanushenko, Viktor, Oravetz, Dan, Pan, Kaike, Simmons, Audrey, Snedden, Stephanie
Publikováno v:
Astrophys.J.713:1026-1036,2010
We present a measurement of the volumetric Type Ia supernova (SN Ia) rate based on data from the Sloan Digital Sky Survey II (SDSS-II) Supernova Survey. The adopted sample of supernovae (SNe) includes 516 SNe Ia at redshift z \lesssim 0.3, of which 2
Externí odkaz:
http://arxiv.org/abs/1001.4995
Autor:
Hayden, Brian T., Garnavich, Peter M., Kessler, Richard, Frieman, Joshua A., Jha, Saurabh W., Cinabro, David, Dilday, Benjamin, Kasen, Daniel, Marriner, John, Nichol, Robert C., Riess, Adam G., Sako, Masao, Schneider, Donald P., Smith, Mathew, Sollerman, Jesper, Bassett, Bruce
Publikováno v:
Astrophys.J.712:350-366,2010
We analyze the rise and fall times of type Ia supernova (SN Ia) light curves discovered by the SDSS-II Supernova Survey. From a set of 391 light curves k-corrected to the rest frame B and V bands, we find a smaller dispersion in the rising portion of
Externí odkaz:
http://arxiv.org/abs/1001.3428
Autor:
Kessler, Richard, Cinabro, David, Bassett, Bruce, Dilday, Benjamin, Frieman, Joshua A., Garnavich, Peter M., Jha, Saurabh, Marriner, John, Nichol, Robert C., Sako, Masao, Smith, Mathew, Bernstein, Joseph P., Bizyaev, Dmitry, Goobar, Ariel, Kuhlmann, Stephen, Schneider, Donald P., Stritzinger, Maximilian
Publikováno v:
Astrophys.J.717:40-57,2010
Large planned photometric surveys will discover hundreds of thousands of supernovae (SNe), outstripping the resources available for spectroscopic follow-up and necessitating the development of purely photometric methods to exploit these events for co
Externí odkaz:
http://arxiv.org/abs/1001.0738
Autor:
LSST Science Collaboration, Abell, Paul A., Allison, Julius, Anderson, Scott F., Andrew, John R., Angel, J. Roger P., Armus, Lee, Arnett, David, Asztalos, S. J., Axelrod, Tim S., Bailey, Stephen, Ballantyne, D. R., Bankert, Justin R., Barkhouse, Wayne A., Barr, Jeffrey D., Barrientos, L. Felipe, Barth, Aaron J., Bartlett, James G., Becker, Andrew C., Becla, Jacek, Beers, Timothy C., Bernstein, Joseph P., Biswas, Rahul, Blanton, Michael R., Bloom, Joshua S., Bochanski, John J., Boeshaar, Pat, Borne, Kirk D., Bradac, Marusa, Brandt, W. N., Bridge, Carrie R., Brown, Michael E., Brunner, Robert J., Bullock, James S., Burgasser, Adam J., Burge, James H., Burke, David L., Cargile, Phillip A., Chandrasekharan, Srinivasan, Chartas, George, Chesley, Steven R., Chu, You-Hua, Cinabro, David, Claire, Mark W., Claver, Charles F., Clowe, Douglas, Connolly, A. J., Cook, Kem H., Cooke, Jeff, Cooray, Asantha, Covey, Kevin R., Culliton, Christopher S., de Jong, Roelof, de Vries, Willem H., Debattista, Victor P., Delgado, Francisco, Dell'Antonio, Ian P., Dhital, Saurav, Di Stefano, Rosanne, Dickinson, Mark, Dilday, Benjamin, Djorgovski, S. G., Dobler, Gregory, Donalek, Ciro, Dubois-Felsmann, Gregory, Durech, Josef, Eliasdottir, Ardis, Eracleous, Michael, Eyer, Laurent, Falco, Emilio E., Fan, Xiaohui, Fassnacht, Christopher D., Ferguson, Harry C., Fernandez, Yanga R., Fields, Brian D., Finkbeiner, Douglas, Figueroa, Eduardo E., Fox, Derek B., Francke, Harold, Frank, James S., Frieman, Josh, Fromenteau, Sebastien, Furqan, Muhammad, Galaz, Gaspar, Gal-Yam, A., Garnavich, Peter, Gawiser, Eric, Geary, John, Gee, Perry, Gibson, Robert R., Gilmore, Kirk, Grace, Emily A., Green, Richard F., Gressler, William J., Grillmair, Carl J., Habib, Salman, Haggerty, J. S., Hamuy, Mario, Harris, Alan W., Hawley, Suzanne L., Heavens, Alan F., Hebb, Leslie, Henry, Todd J., Hileman, Edward, Hilton, Eric J., Hoadley, Keri, Holberg, J. B., Holman, Matt J., Howell, Steve B., Infante, Leopoldo, Ivezic, Zeljko, Jacoby, Suzanne H., Jain, Bhuvnesh, Jedicke, Jee, M. James, Jernigan, J. Garrett, Jha, Saurabh W., Johnston, Kathryn V., Jones, R. Lynne, Juric, Mario, Kaasalainen, Mikko, Styliani, Kafka, Kahn, Steven M., Kaib, Nathan A., Kalirai, Jason, Kantor, Jeff, Kasliwal, Mansi M., Keeton, Charles R., Kessler, Richard, Knezevic, Zoran, Kowalski, Adam, Krabbendam, Victor L., Krughoff, K. Simon, Kulkarni, Shrinivas, Kuhlman, Stephen, Lacy, Mark, Lepine, Sebastien, Liang, Ming, Lien, Amy, Lira, Paulina, Long, Knox S., Lorenz, Suzanne, Lotz, Jennifer M., Lupton, R. H., Lutz, Julie, Macri, Lucas M., Mahabal, Ashish A., Mandelbaum, Rachel, Marshall, Phil, May, Morgan, McGehee, Peregrine M., Meadows, Brian T., Meert, Alan, Milani, Andrea, Miller, Christopher J., Miller, Michelle, Mills, David, Minniti, Dante, Monet, David, Mukadam, Anjum S., Nakar, Ehud, Neill, Douglas R., Newman, Jeffrey A., Nikolaev, Sergei, Nordby, Martin, O'Connor, Paul, Oguri, Masamune, Oliver, John, Olivier, Scot S., Olsen, Julia K., Olsen, Knut, Olszewski, Edward W., Oluseyi, Hakeem, Padilla, Nelson D., Parker, Alex, Pepper, Joshua, Peterson, John R., Petry, Catherine, Pinto, Philip A., Pizagno, James L., Popescu, Bogdan, Prsa, Andrej, Radcka, Veljko, Raddick, M. Jordan, Rasmussen, Andrew, Rau, Arne, Rho, Jeonghee, Rhoads, James E., Richards, Gordon T., Ridgway, Stephen T., Robertson, Brant E., Roskar, Rok, Saha, Abhijit, Sarajedini, Ata, Scannapieco, Evan, Schalk, Terry, Schindler, Rafe, Schmidt, Samuel, Schmidt, Sarah, Schneider, Donald P., Schumacher, German, Scranton, Ryan, Sebag, Jacques, Seppala, Lynn G., Shemmer, Ohad, Simon, Joshua D., Sivertz, M., Smith, Howard A., Smith, J. Allyn, Smith, Nathan, Spitz, Anna H., Stanford, Adam, Stassun, Keivan G., Strader, Jay, Strauss, Michael A., Stubbs, Christopher W., Sweeney, Donald W., Szalay, Alex, Szkody, Paula, Takada, Masahiro, Thorman, Paul, Trilling, David E., Trimble, Virginia, Tyson, Anthony, Van Berg, Richard, Berk, Daniel Vanden, VanderPlas, Jake, Verde, Licia, Vrsnak, Bojan, Walkowicz, Lucianne M., Wandelt, Benjamin D., Wang, Sheng, Wang, Yun, Warner, Michael, Wechsler, Risa H., West, Andrew A., Wiecha, Oliver, Williams, Benjamin F., Willman, Beth, Wittman, David, Wolff, Sidney C., Wood-Vasey, W. Michael, Wozniak, Przemek, Young, Patrick, Zentner, Andrew, Zhan, Hu
A survey that can cover the sky in optical bands over wide fields to faint magnitudes with a fast cadence will enable many of the exciting science opportunities of the next decade. The Large Synoptic Survey Telescope (LSST) will have an effective ape
Externí odkaz:
http://arxiv.org/abs/0912.0201