Zobrazeno 1 - 10
of 111
pro vyhledávání: '"Dilday B"'
Autor:
Baltay, C., Grossman, L., Howard, R., Rabinowitz, D., Arcavi, I., Barbour, N., Burke, J., Contreras, C., Dilday, B., Graham, M., Hiramatsu, D., Hossenzadeh, G., Howell, D. A., McCully, C., McKinnon, R., Ment, K., Montesi, R., Pellegrino, C., Valenti, S.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2021 Apr 01. 133(1022), 1-15.
Externí odkaz:
https://www.jstor.org/stable/27123856
Autor:
Parrent, J. T., Howell, D. A., Fesen, R. A., Parker, S., Bianco, F. B., Dilday, B., Sand, D., Valenti, S., Vinkó, J., Berlind, P., Challis, P., Milisavljevic, D., Sanders, N., Marion, G. H., Wheeler, J. C., Brown, P., Calkins, M. L., Friesen, B., Kirshner, R., Pritchard, T., Quimby, R., Roming, P.
Publikováno v:
2016MNRAS.457.3702P
SN 2012dn is a super-Chandrasekhar mass candidate in a purportedly normal spiral (SAcd) galaxy, and poses a challenge for theories of type Ia supernova diversity. Here we utilize the fast and highly parameterized spectrum synthesis tool, SYNAPPS, to
Externí odkaz:
http://arxiv.org/abs/1603.03868
Autor:
Graham, M. L., Sand, D. J., Valenti, S., Howell, D. A., Parrent, J., Halford, M., Zaritsky, D., Bianco, F., Rest, A., Dilday, B.
We present time series photometric and spectroscopic data for the transient SN 2009ip from the start of its outburst in September 2012 until November 2013. This data was collected primarily with the new robotic capabilities of the Las Cumbres Observa
Externí odkaz:
http://arxiv.org/abs/1402.1765
Autor:
Brown, T. M., Baliber, N., Bianco, F. B., Bowman, M., Burleson, B., Conway, P., Crellin, M., Depagne, É., De Vera, J., Dilday, B., Dragomir, D., Dubberley, M., Eastman, J. D., Elphick, M., Falarski, M., Foale, S., Ford, M., Fulton, B. J., Garza, J., Gomez, E. L., Graham, M., Greene, R., Haldeman, B., Hawkins, E., Haworth, B., Haynes, R., Hidas, M., Hjelstrom, A. E., Howell, D. A., Hygelund, J., Lister, T. A., Lobdill, R., Martinez, J., Mullins, D. S., Norbury, M., Parrent, J., Paulson, R., Petry, D. L., Pickles, A., Posner, V., Rosing, W. E., Ross, R., Sand, D. J., Saunders, E. S., Shobbrook, J., Shporer, A., Street, R. A., Thomas, D., Tsapras, Y., Tufts, J. R., Valenti, S., Horst, K. Vander, Walker, Z., White, G., Willis, M.
Las Cumbres Observatory Global Telescope (LCOGT) is a young organization dedicated to time-domain observations at optical and (potentially) near-IR wavelengths. To this end, LCOGT is constructing a world-wide network of telescopes, including the two
Externí odkaz:
http://arxiv.org/abs/1305.2437
Autor:
Hachinger, S., Mazzali, P. A., Sullivan, M., Ellis, R., Maguire, K., Gal-Yam, A., Howell, D. A., Nugent, P. E., Baron, E., Cooke, J., Arcavi, I., Bersier, D., Dilday, B., James, P. A., Kasliwal, M. M., Kulkarni, S. R., Ofek, E. O., Laher, R. R., Parrent, J., Surace, J., Yaron, O., Walker, E. S.
Radiative transfer studies of Type Ia supernovae (SNe Ia) hold the promise of constraining both the time-dependent density profile of the SN ejecta and its stratification by element abundance which, in turn, may discriminate between different explosi
Externí odkaz:
http://arxiv.org/abs/1208.1267
Autor:
Dilday, B., Howell, D. A., Cenko, S. B., Silverman, J. M., Nugent, P. E., Sullivan, M., Ben-Ami, S., Bildsten, L., Bolte, M., Endl, M., Filippenko, A. V., Gnat, O., Horesh, A., Hsiao, E., Kasliwal, M. M., Kirkman, D., Maguire, K., Marcy, G. W., Moore, K., Pan, Y., Parrent, J. T., Podsiadlowski, P., Quimby, R. M., Sternberg, A., Suzuki, N., Tytler, D. R., Xu, D., Bloom, J. S., Gal-Yam, A., Hook, I. M., Kulkarni, S. R., Law, N. M., Ofek, E. O., Polishook, D., Poznanski, D.
There is a consensus that Type-Ia supernovae (SNe Ia) arise from the thermonuclear explosion of white dwarf stars that accrete matter from a binary companion. However, direct observation of SN Ia progenitors is lacking, and the precise nature of the
Externí odkaz:
http://arxiv.org/abs/1207.1306
Autor:
Maguire, K., Sullivan, M., Ellis, R. S., Nugent, P. E., Howell, D. A., Gal-Yam, A., Cooke, J., Mazzali, P., Pan, Y-C., Dilday, B., Thomas, R. C., Arcavi, I., Ben-Ami, S., Bersier, D., Bianco, F. B., Fulton, B. J., Hook, I., Horesh, A., Hsiao, E., James, P. A., Podsiadlowski, P., Walker, E. S., Yaron, O., Kasliwal, M. M., Laher, R. R., Law, N. M., Ofek, E. O., Poznanski, D., Surace, J.
We present an analysis of the maximum light, near ultraviolet (NUV; 2900-5500 A) spectra of 32 low redshift (0.001
Externí odkaz:
http://arxiv.org/abs/1205.7040
Autor:
Parrent, J. T., Howell, D. A., Friesen, B., Thomas, R. C., Fesen, R. A., Milisavljevic, D., Bianco, F. B., Dilday, B., Nugent, P., Baron, E., Arcavi, I., Ben-Ami, S., Bersier, D., Bildsten, L., Bloom, J., Cao, Y., Cenko, S. B., Filippenko, A. V., Gal-Yam, A., Kasliwal, M. M., Konidaris, N., Kulkarni, S. R., Law, N. M., Levitan, D., Maguire, K., Mazzali, P. A., Ofek, E. O., Pan, Y., Polishook, D., Poznanski, D., Quimby, R. M., Silverman, J. M., Sternberg, A., Sullivan, M., Walker, E. S., Xu, D., Buton, C., Pereira, R.
The nearby Type Ia supernova SN 2011fe in M101 (cz=241 km s^-1) provides a unique opportunity to study the early evolution of a "normal" Type Ia supernova, its compositional structure, and its elusive progenitor system. We present 18 high signal-to-n
Externí odkaz:
http://arxiv.org/abs/1205.6011
Autor:
Leloudas, G., Chatzopoulos, E., Dilday, B., Gorosabel, J., Vinko, J., Gallazzi, A., Wheeler, J. C., Bassett, B., Fischer, J. A., Frieman, J. A., Fynbo, J. P. U., Goobar, A., Jelinek, M., Malesani, D., Nichol, R. C., Nordin, J., Ostman, L., Sako, M., Schneider, D. P., Smith, M., Sollerman, J., Stritzinger, M. D., Thoene, C. C., Postigo, A. de Ugarte
Publikováno v:
Astronomy & Astrophysics 541 (2012) A129
We study SN 2006oz, a newly-recognized member of the class of H-poor, super-luminous supernovae. We present multi-color light curves from the SDSS-II SN Survey, that cover the rise time, as well as an optical spectrum that shows that the explosion oc
Externí odkaz:
http://arxiv.org/abs/1201.5393
Autor:
Lampeitl, H., Nichol, R. C., Seo, H. -J., Giannantonio, T., Shapiro, C., Bassett, B., Percival, W. J., Davis, T. M., Dilday, B., Frieman, J., Garnavich, P., Sako, M., Smith, M., Sollerman, J., Becker, A. C., Cinabro, D., Filippenko, A. V., Foley, R. J., Hogan, C. J., Holtzman, J. A., Jha, S. W., Konishi, K., Marriner, J., Richmond, M. W., Riess, A. G., Schneider, D. P., Stritzinger, M., van der Heyden, K. J., VanderPlas, J. T., Wheeler, J. C., Zheng, C.
Publikováno v:
Mon.Not.Roy.Astron.Soc.401:2331-2342,2009
We present an analysis of the luminosity distances of Type Ia Supernovae from the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey in conjunction with other intermediate redshift (z<0.4) cosmological measurements including redshift-space distor
Externí odkaz:
http://arxiv.org/abs/0910.2193