Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Barris, Brian J."'
Autor:
Barris, Brian J.
Thesis (Ph. D.)--University of Hawaii at Manoa, 2004.
Includes bibliographical references.
Includes bibliographical references.
Autor:
Silverman, Jeffrey M., Foley, Ryan J., Filippenko, Alexei V., Ganeshalingam, Mohan, Barth, Aaron J., Chornock, Ryan, Griffith, Christopher V., Kong, Jason J., Lee, Nicholas, Leonard, Douglas C., Matheson, Thomas, Miller, Emily G., Steele, Thea N., Barris, Brian J., Bloom, Joshua S., Cobb, Bethany E., Coil, Alison L., Desroches, Louis-Benoit, Gates, Elinor L., Ho, Luis C., Jha, Saurabh W., Kandrashoff, Michael T., Li, Weidong, Mandel, Kaisey S., Modjaz, Maryam, Moore, Matthew R., Mostardi, Robin E., Papenkova, Marina S., Park, Sung, Perley, Daniel A., Poznanski, Dovi, Reuter, Cassie A., Scala, James, Serduke, Franklin J. D., Shields, Joseph C., Swift, Brandon J., Tonry, John L., Van Dyk, Schuyler D., Wang, Xiaofeng, Wong, Diane S.
In this first paper in a series we present 1298 low-redshift (z\leq0.2) optical spectra of 582 Type Ia supernovae (SNe Ia) observed from 1989 through 2008 as part of the Berkeley SN Ia Program (BSNIP). 584 spectra of 199 SNe Ia have well-calibrated l
Externí odkaz:
http://arxiv.org/abs/1202.2128
Autor:
Wang, Xiaofeng, Wang, Lifan, Filippenko, Alexei V., Baron, Eddie, Kromer, Markus, Jack, Dennis, Zhang, Tianmeng, Aldering, Greg, Antilogus, Pierre, Arnett, David, Baade, Dietrich, Barris, Brian J., Benetti, Stefano, Bouchet, Patrice, Burrows, Adam S., Canal, Ramon, Cappellaro, Enrico, Carlberg, Raymond, di Carlo, Elisa, Challis, Peter, Crotts, Arlin, Danziger, John I., Della Valle, Massimo, Fink, Michael, Foley, Ryan J., Fransson, Claes, Gal-Yam, Avishay, Garnavich, Peter, Gerardy, Chris L., Goldhaber, Gerson, Hamuy, Mario, Hillebrandt, Wolfgang, Hoeflich, Peter A., Holland, Stephen T., Holz, Daniel E., Hughes, John P., Jeffery, David J., Jha, Saurabh W., Kasen, Dan, Khokhlov, Alexei M., Kirshner, Robert P., Knop, Robert, Kozma, Cecilia, Krisciunas, Kevin, Lee, Brian C., Leibundgut, Bruno, Lentz, Eric J., Leonard, Douglas C., Lewin, Walter H. G., Li, Weidong, Livio, Mario, Lundqvist, Peter, Maoz, Dan, Matheson, Thomas, Mazzali, Paolo, Meikle, Peter, Miknaitis, Gajus, Milne, Peter, Mochnacki, Stefan, Nomoto, Ken'Ichi, Nugent, Peter E., Oran, Elaine, Panagia, Nino, Perlmutter, Saul, Phillips, Mark M., Pinto, Philip, Poznanski, Dovi, Pritchet, Christopher J., Reinecke, Martin, Riess, Adam, Ruiz-Lapuente, Pilar, Scalzo, Richard, Schlegel, Eric M., Schmidt, Brian, Siegrist, James, Soderberg, Alicia M., Sollerman, Jesper, Sonneborn, George, Spadafora, Anthony, Spyromilio, Jason, Sramek, Richard A., Starrfield, Sumner G., Strolger, Louis G., Suntzeff, Nicholas B., Thomas, Rollin, Tonry, John L., Tornambe, Amedeo, Truran, James W., Turatto, Massimo, Turner, Michael, Van Dyk, Schuyler D., Weiler, Kurt, Wheeler, J. Craig, Wood-Vasey, Michael, Woosley, Stan, Yamaoka, Hitoshi
Publikováno v:
Astrophys.J.749:126-142,2012
We present ultraviolet (UV) spectroscopy and photometry of four Type Ia supernovae (SNe 2004dt, 2004ef, 2005M, and 2005cf) obtained with the UV prism of the Advanced Camera for Surveys on the Hubble Space Telescope. This dataset provides unique spect
Externí odkaz:
http://arxiv.org/abs/1110.5809
Autor:
Barris, Brian J., Tonry, John L.
Publikováno v:
Astrophys.J.637:427-438,2006
We derive the rates of Type Ia supernovae (SNIa) over a wide range of redshifts using a complete sample from the IfA Deep Survey. This sample of more than 100 SNIa is the largest set ever collected from a single survey, and therefore uniquely powerfu
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509655
Publikováno v:
Astron.J.130:2272-2277,2005
We present a new method for optimally extracting point-source time variability information from a series of images. Differential photometry is generally best accomplished by subtracting two images separated in time, since this removes all constant ob
Externí odkaz:
http://arxiv.org/abs/astro-ph/0507584
Autor:
Barris, Brian J., Tonry, John L.
Publikováno v:
Astrophys.J. 613 (2004) L21-L24
We describe a procedure for accurately determining luminosity distances to Type Ia supernovae (SNe Ia) without knowledge of redshift. This procedure, which may be used as an extension of any of the various distance determination methods currently in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408097
Autor:
Barris, Brian J., Tonry, John, Blondin, Stephane, Challis, Peter, Chornock, Ryan, Clocchiatti, Alejandro, Filippenko, Alexei, Garnavich, Peter, Holland, Stephen, Jha, Saurabh, Kirshner, Robert, Krisciunas, Kevin, Leibundgut, Bruno, Li, Weidong, Matheson, Thomas, Miknaitis, Gajus, Riess, Adam, Schmidt, Brian, Smith, R. Chris, Sollerman, Jesper, Spyromilio, Jason, Stubbs, Christopher, Suntzeff, Nicholas, Aussel, H., Chambers, K. C., Connelley, M. S., Donovan, D., Henry, J. P., Kaiser, N., Liu, M. C., Martin, E. L., Wainscoat, R. J.
Publikováno v:
Astrophys.J. 602 (2004) 571-594
We present photometric and spectroscopic observations of 23 high redshift supernovae spanning a range of z=0.34-1.03, 9 of which are unambiguously classified as Type Ia. These supernovae were discovered during the IfA Deep Survey, which began in Sept
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310843
Autor:
Jensen, Joseph B., Tonry, John L., Barris, Brian J., Thompson, Rodger I., Liu, Michael C., Rieke, Marcia J., Ajhar, Edward A., Blakeslee, John P.
Publikováno v:
Astrophys.J.583:712-726,2003
To empirically calibrate the IR surface brightness fluctuation (SBF) distance scale and probe the properties of unresolved stellar populations, we measured fluctuations in 65 galaxies using NICMOS on the Hubble Space Telescope. The early-type galaxie
Externí odkaz:
http://arxiv.org/abs/astro-ph/0210129
Autor:
Blakeslee, John P., Lucey, John R., Tonry, John L., Hudson, Michael J., Narayanan, Vijay K., Barris, Brian J.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 330 (2002) 443
We compare two methods for deriving distances to early-type galaxies: fundamental plane (FP) and surface brightness fluctuations (SBF) distances for 170 galaxies. A third set of distances is provided by predictions derived from the density field of t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0111183
Publikováno v:
Mon.Not.Roy.Astron.Soc. 327 (2001) 1004
We perform a series of comparisons between distance-independent photometric and spectroscopic properties used in the surface brightness fluctuations (SBF) and fundamental plane (FP) methods of early-type galaxy distance estimation. The data are taken
Externí odkaz:
http://arxiv.org/abs/astro-ph/0108194