Results 21 to 30 of about 35,122 (152)
Ultraviolet Diversity of Type Ia Supernovae [PDF]
, 2016 Ultraviolet (UV) observations of Type Ia supernovae (SNe Ia) probe the
outermost layers of the explosion, and UV spectra of SNe Ia are expected to be
extremely sensitive to differences in progenitor composition and the details of
the explosion.Brown, P., Filippenko, A. V., Foley, Ryan J., Fox, O. D., Hillebrandt, W., Kirshner, R. P., Marion, G. H., Milne, P. A., Pan, Yen-Chen, Parrent, J. T., Pignata, G., Stritzinger, M. D. +11 morecore +3 more sourcesNear-infrared and Optical Nebular-phase Spectra of Type Ia Supernovae SN 2013aa and SN 2017cbv in NGC 5643
The Astrophysical Journal, 2023 We present multiwavelength time-series spectroscopy of SN 2013aa and SN 2017cbv, two Type Ia supernovae (SNe Ia) on the outskirts of the same host galaxy, NGC 5643. This work utilizes new nebular-phase near-infrared (NIR) spectra obtained by the Carnegie Sahana Kumar, Eric Y. Hsiao, C. Ashall, M. M. Phillips, N. Morrell, P. Hoeflich, C. R. Burns, L. Galbany, E. Baron, C. Contreras, S. Davis, T. Diamond, F. Förster, M. L. Graham, E. Karamehmetoglu, R. P. Kirshner, B. Koribalski, K. Krisciunas, J. Lu, G. H. Marion, P. J. Pessi, A. L. Piro, M. Shahbandeh, M. D. Stritzinger, N. B. Suntzeff, S. A. Uddin +25 moredoaj +1 more sourceType Ia Supernovae and Cosmology
, 2004 I discuss the use of Type Ia supernovae (SNe Ia) for cosmological distance
determinations. Low-redshift SNe Ia (z < 0.1) demonstrate that the Hubble
expansion is linear with H_0 = 72 +/- 8 km/s/Mpc, and that the properties of
dust in other galaxies are ...A. Balbi, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. G. Riess, A. Gal-Yam, A. Goobar, A. Goobar, A. J. Barber, A. Kim, A. L. Coil, A. N. Aguirre, A. N. Aguirre, A. N. Aguirre, A. Saha, A. Saha, A. Sandage, A. Sandage, A. V. Filippenko, A. V. Filippenko, A. V. Filippenko, A. V. Filippenko, A. V. Filippenko, A. V. Filippenko, A. V. Filippenko, A. V. Filippenko, B. Barris, B. Chaboyer, B. K. Gibson, B. Leibundgut, B. Leibundgut, B. Leibundgut, B. P. Schmidt, B. R. Parodi, B. Williams, C. B. Netterfield, C. H. Ford, C. H. Lineweaver, C. H. Lineweaver, D. Branch, D. Branch, D. Branch, D. Branch, D. Branch, D. Branch, D. Branch, D. C. Leonard, D. C. Leonard, D. E. Groom, D. E. Holz, D. E. Holz, D. Hardin, D. J. Eisenstein, D. Maoz, D. N. Spergel, E. Cappellaro, E. Cappellaro, E. E. Falco, E. E. Salpeter, E. L. Wright, F. Hoyle, F. Matteucci, F. Paerels, G. Aldering, G. Efstathiou, G. Efstathiou, G. Goldhaber, G. Goldhaber, G. Goldhaber, G. Goldhaber, G. Goldhaber, G. Wilson, H. Norgaard-Nielsen, H. Umeda, J. A. Peacock, J. A. Tyson, J. J. Cowan, J. L. Tonry, J. N. Bahcall, J. P. Blakeslee, J. P. Ostriker, J. V. Narlikar, J. Wambsganss, K. Hatano, K. Krisciunas, K. Krisciunas, K. Krisciunas, K. Krisciunas, K. Nomoto, L. R. Yungelson, L. Strolger, M. Davis, M. Hamuy, M. Hamuy, M. Hamuy, M. Hamuy, M. Hamuy, M. Livio, M. M. Phillips, M. M. Phillips, M. M. Phillips, M. Modjaz, M. R. Nolta, M. S. Turner, M. Sullivan, M. Turatto, M. Zaldarriaga, N. A. Bahcall, N. Afshordi, N. Benítez, N. Kaiser, N. Suntzeff, P. Bernardis de, P. Bernardis de, P. Fosalba, P. Garnavich, P. Garnavich, P. Garnavich, P. Höflich, P. Madau, P. Nugent, P. Nugent, P. Nugent, P. Ruiz-Lapuente, P. S. Drell, R. C. Smith, R. G. Gratton, R. J. Foley, R. Kallosh, R. Kantowski, R. Kantowski, R. Knop, R. Pain, R. Pain, R. Pain, R. R. Caldwell, R. R. Caldwell, R. Tripp, R. Tripp, S. Bergh van den, S. Boughn, S. Hanany, S. Hancock, S. M. Carroll, S. M. Carroll, S. Perlmutter, S. Perlmutter, S. Perlmutter, S. Perlmutter, T. D. Oswalt, T. Dahlen, T. Dahlen, T. E. Vaughan, T. Matheson, T. Matheson, V. D. Ivanov, W. Freedman, W. Li, W. Li, W. Li, W. Li, W. Li, W. Li, W. Percival, Y. Wang, Yu. P. Pskovskii, Yu. P. Pskovskii +175 morecore +1 more sourceType Ia Supernova Explosion Models [PDF]
, 2000 Because calibrated light curves of Type Ia supernovae have become a major
tool to determine the local expansion rate of the Universe and also its
geometrical structure, considerable attention has been given to models of these
events over the past couple ...Aldering G, Arnett WD, Beer A, Blinnikov SI, Blinnikov SI, Buchler JR, Buchler JR, Bychkov VV, Cappellaro E, Chandrasekhar S, Damköhler G, Darrieus G, Garcia-Senz D, Greiner J, Hoeflich P, Homeier D, Imshennik VS, Imshennik VS, Ivanova LN, Kercek A, Khokhlov AM, Khokhlov AM, Khokhlov AM, King AR, Kolmogorov AN, Landau LD, Landau LD, Lewis B, Lucy LB, Lundmark K, Lundmark K, Mair G, Mazzali PA, Mazzali PA, Mihalas D, Mochkovitch R, Mochkovitch R, Müller E, Niemeyer JC, Nomoto K, Nomoto K, Paczynski B, Paczynski B, Pakull MW, Pauldrach AWA, Pskovskii IP, Reinecke M, Reinecke M, Saio H, Schoenfelder V, Shigeyama T, Thielemann FK, Tripp R, Van den Heuvel EPJ, Wellstein S, Williams FA, Zeldovich YB +56 morecore +2 more sourcesSN 2021hpr: A Normal Type Ia Supernova Showing Excess Emission in the Early Rising Phase
The Astrophysical JournalWe present extensive optical observations of a nearby Type Ia supernova (SN Ia), SN 2021hpr, located in the spiral galaxy NGC 3147 at a distance of ∼45 Mpc. Our observations cover a phase within ∼1–2 days to ∼290 days after the explosion.Abdusamatjan Iskandar, Xiaofeng Wang, Ali Esamdin, Xiangyun Zeng, Craig Pellegrino, Shengyu Yan, Jialian Liu, Alexei V. Filippenko, D. Andrew Howell, Curtis McCully, Thomas G. Brink, Maokai Hu, Yi Yang, WeiKang Zheng, Guoliang Lü, Jujia Zhang, CuiYing Song, RuiFeng Huang, Rachael C. Amaro, Chunhai Bai, Kyle G. Dettman, Lluís Galbany, Daichi Hiramatsu, Bostroem K. Azalee, Koichi Itagaki, Saurabh W. Jha, Shuguo Ma, David J. Sand, Jennifer E. Andrews, Jacob Jencson, Peter Milne, Jeniveve Pearson, Manisha Shrestha, Nathan Smith, Réka Könyves-Tóth, Samuel Wyatt, Xuan Zhang, Shahidin Yaqup, Letian Wang, Mengfan Zhang +39 moredoaj +1 more sourceCosmology from Type Ia Supernovae [PDF]
, 1998 This presentation reports on first evidence for a
low-mass-density/positive-cosmological-constant universe that will expand
forever, based on observations of a set of 40 high-redshift supernovae.Aldering, G., Boyle, B. J., Couch, W. J., Deustua, S., Ellis, R. S., Fabbro, S., Filippenko, A. V., Fruchter, A. S., Goldhaber, G., Goobar, A., Groom, D. E., Hook, I. M., Irwin, M., Kim, A. G., Kim, M. Y., Knop, R. A., Lidman, C., Matheson, T., McMahon, R. G., Newberg, H. J. M., Nugent, P., Pain, R., Panagia, N., Pennypacker, C. R., Perlmutter, S., Ruiz-Lapuente, P., Schaefer, B., Walton, N. +27 morecore +2 more sourcesA JWST Medium-resolution MIRI Spectrum and Models of the Type Ia Supernova 2021aefx at +415 days
The Astrophysical JournalWe present a JWST MIRI medium-resolution spectrometer spectrum (5–27 μ m) of the Type Ia supernova (SN Ia) SN 2021aefx at +415 days past B -band maximum.C. Ashall, P. Hoeflich, E. Baron, M. Shahbandeh, J. M. DerKacy, K. Medler, B. J. Shappee, M. A. Tucker, E. Fereidouni, T. Mera, J. Andrews, D. Baade, K. A. Bostroem, P. J. Brown, C. R. Burns, A. Burrow, A. Cikota, T. de Jaeger, A. Do, Y. Dong, I. Dominguez, O. Fox, L. Galbany, E. Y. Hsiao, K. Krisciunas, B. Khaghani, S. Kumar, J. Lu, J. R. Maund, P. Mazzali, N. Morrell, F. Patat, C. Pfeffer, M. M. Phillips, J. Schmidt, S. Stangl, C. P. Stevens, M. D. Stritzinger, N. B. Suntzeff, C. M. Telesco, L. Wang, Y. Yang +41 moredoaj +1 more sourceBump Morphology of the CMAGIC Diagram
The Astrophysical Journal, 2023 We apply the color–magnitude intercept calibration method (CMAGIC) to the Nearby Supernova Factory SNe Ia spectrophotometric data set. The currently existing CMAGIC parameters are the slope and intercept of a straight line fit to the linear region in the L. Aldoroty, L. Wang, P. Hoeflich, J. Yang, N. Suntzeff, G. Aldering, P. Antilogus, C. Aragon, S. Bailey, C. Baltay, S. Bongard, K. Boone, C. Buton, Y. Copin, S. Dixon, D. Fouchez, E. Gangler, R. Gupta, B. Hayden, Mitchell Karmen, A. G. Kim, M. Kowalski, D. Küsters, P.-F. Léget, F. Mondon, J. Nordin, R. Pain, E. Pecontal, R. Pereira, S. Perlmutter, K. A. Ponder, D. Rabinowitz, M. Rigault, D. Rubin, K. Runge, C. Saunders, G. Smadja, N. Suzuki, C. Tao, R. C. Thomas, M. Vincenzi +40 moredoaj +1 more source
