Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Nearby Supernova Factory Collaboration"'
Autor:
Chotard, Nicolas
Vers la fin des années 1990, l’utilisation des supernovae de type Ia (SNe Ia) comme indicateurs de distance a permis de mettre en évidence l’expansion accélérée de l’univers. Depuis lors, des campagnes d’observations de grandes envergure
Externí odkaz:
http://www.theses.fr/2011LYO10180/document
Autor:
Chotard, Nicolas
One of the current limitations of type Ia supernovae used as distance indicators is themixing of their different sources of variabilitiy during the empirical standardization of their distance modulus. Using the nearby SNe Ia spectral sample observed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______166::26a2ec6c81c6b37f138e9837142b4484
https://theses.hal.science/tel-00660289v2
https://theses.hal.science/tel-00660289v2
Autor:
Buton, Clément
Il y a près d’une décennie, l'utilisation des supernovae de type Ia comme indicateurs de distances a permis de découvrir l'expansion accélérée de l'univers. Les expériences de seconde génération ont augmenté de manière significative la t
Externí odkaz:
http://www.theses.fr/2009LYO10303/document
Autor:
Buton, Clément
Ten years ago, type Ia supernovae used as distances indicators led to the discovery of the accelerating expansion of the universe. Today, a second generation of surveys has significantly increased the high-redshift type Ia supernovae sample. The low-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______166::f4b62c7a5461f9b1ec93d38d6e448c13
https://theses.hal.science/tel-00465853v2
https://theses.hal.science/tel-00465853v2
Autor:
The Nearby Supernova Factory Collaboration, Aldering, G., Antilogus, P., Bailey, S., Baltay, C., Bauer, A., Blanc, N., Bongard, S., Copin, Y., Gangler, E., Gilles, S., Kessler, R., Kocevski, D., Lee, B. C., Loken, S., Nugent, P., Pain, R., Pecontal, E., Pereira, R., Perlmutter, S., Rabinowitz, D., Rigaudier, G., Scalzo, R., Smadja, G., Thomas, R. C., Wang, L., Weaver, B. A.
Publikováno v:
Astrophys.J.650:510-527,2006
We report Nearby Supernova Factory observations of SN 2005gj, the second confirmed case of a "hybrid" Type Ia/IIn supernova. Our early-phase photometry of SN 2005gj shows that the interaction is much stronger than for the prototype, SN 2002ic. Our fi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606499
Autor:
Stein, George, Seljak, Uros, Buton, C., Copin, Y., Dixon, S., Fouchez, D., Gangler, E., Gupta, R., Hayden, B., Hillebrandt, W., Karmen, M., Kim, A. G., Bohm, Vanessa, Kowalski, M., Kuesters, Daniel, Leget, P. F., Mondon, F., Nordin, J., Pain, R., Pecontal, E., Pereira, R., Perlmutter, S., Ponder, K. A., Aldering, G., Rabinowitz, D., Rigault, M., Rubin, D., Runge, K., Saunders, C., Smadja, G., Suzuki, N., Tao, C., Taubenberger, S., Thomas, R. C., Antilogus, P., Vincenzi, M., Nearby Supernova Factory Collaboration, Aragon, C., Bailey, S., Baltay, C., Bongard, S., Boone, K.
Publikováno v:
Astrophys.J.
Astrophys.J., 2022, 935 (1), pp.5. ⟨10.3847/1538-4357/ac7c08⟩
The astrophysical journal / 2 935(1), 5 (2022). doi:10.3847/1538-4357/ac7c08
Astrophys.J., 2022, 935 (1), pp.5. ⟨10.3847/1538-4357/ac7c08⟩
The astrophysical journal / 2 935(1), 5 (2022). doi:10.3847/1538-4357/ac7c08
The astrophysical journal 935(1), 5 (2022). doi:10.3847/1538-4357/ac7c08
We construct a physically parameterized probabilistic autoencoder (PAE) to learn the intrinsic diversity of Type Ia supernovae (SNe Ia) from a sparse set of spectral time s
We construct a physically parameterized probabilistic autoencoder (PAE) to learn the intrinsic diversity of Type Ia supernovae (SNe Ia) from a sparse set of spectral time s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ebfeb4d8863beac3835c90ee02e3ae12
http://arxiv.org/abs/2207.07645
http://arxiv.org/abs/2207.07645
Autor:
Boone, K., Aldering, G., Fouchez, D., Gangler, E., Gupta, R., Hayden, B., Hillebrandt, W., Kim, A. G., Kowalski, M., Kuesters, Daniel, Léget, P.-F., Mondon, F., Antilogus, P., Nordin, J., Pain, R., Pecontal, E., Pereira, R., Perlmutter, S., Ponder, K. A., Rabinowitz, D., Rigault, M., Rubin, D., Runge, K., Aragon, C., Saunders, C., Smadja, G., Suzuki, N., Tao, C., Taubenberger, S., Thomas, R. C., Vincenzi, M., Nearby Supernova Factory Collaboration, Bailey, S., Baltay, C., Bongard, S., Buton, C., Copin, Y., Dixon, S.
Publikováno v:
Astrophys.J.
Astrophys.J., 2021, 912 (1), pp.70. ⟨10.3847/1538-4357/abec3c⟩
Astrophysical Journal, vol 912, iss 1
The Astrophysical Journal, vol 912, iss 1
The astrophysical journal / 2 912(1), 70 (2021). doi:10.3847/1538-4357/abec3c
Astrophys.J., 2021, 912 (1), pp.70. ⟨10.3847/1538-4357/abec3c⟩
Astrophysical Journal, vol 912, iss 1
The Astrophysical Journal, vol 912, iss 1
The astrophysical journal / 2 912(1), 70 (2021). doi:10.3847/1538-4357/abec3c
The astrophysical journal 912(1), 70 (2021). doi:10.3847/1538-4357/abec3c
We study the spectral diversity of Type Ia supernovae (SNe Ia) at maximum light using high signal-to-noise spectrophotometry of 173 SNe Ia from the Nearby Supernova Factor
We study the spectral diversity of Type Ia supernovae (SNe Ia) at maximum light using high signal-to-noise spectrophotometry of 173 SNe Ia from the Nearby Supernova Factor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::91403f5e077dae0f62d39cd887b552f7
https://hal.science/hal-03235654
https://hal.science/hal-03235654
Autor:
Saunders, Claire, Aldering, G., Chen, J., Chotard, N., Copin, Y., Dixon, S., Fagrelius, P., Fakhouri, H. K., Feindt, U., Fouchez, D., Gangler, E., Hayden, B., Antilogus, P., Hillebrandt, W., Kim, A. G., Kowalski, Marek, Küsters, D., Leget, P.-F., Lombardo, S., Nordin, J., Pain, R., Pecontal, E., Pereira, R., Bailey, S., Perlmutter, S., Rabinowitz, D., Rigault, M., Rubin, D., Runge, K., Smadja, G., Sofiatti, C., Suzuki, N., Tao, C., Taubenberger, S., Baltay, C., Thomas, R. C., Vincenzi, M., Nearby Supernova Factory Collaboration, Barbary, K., Baugh, D., Boone, K., Bongard, S., Buton, C.
Publikováno v:
Astrophys.J.
Astrophys.J., 2018, 869 (2), pp.167. ⟨10.3847/1538-4357/aaec7e⟩
Astrophysical Journal, vol 869, iss 2
The Astrophysical Journal
The astrophysical journal / 1 869(2), 167 (2018). doi:10.3847/1538-4357/aaec7e
The Astrophysical Journal, vol 869, iss 2
Astrophys.J., 2018, 869 (2), pp.167. ⟨10.3847/1538-4357/aaec7e⟩
Astrophysical Journal, vol 869, iss 2
The Astrophysical Journal
The astrophysical journal / 1 869(2), 167 (2018). doi:10.3847/1538-4357/aaec7e
The Astrophysical Journal, vol 869, iss 2
The astrophysical journal 869(2), 167 (2018). doi:10.3847/1538-4357/aaec7e
SN Ia cosmology depends on the ability to fit and standardize observations of supernova magnitudes with an empirical model. We present here a series of new models of SN I
SN Ia cosmology depends on the ability to fit and standardize observations of supernova magnitudes with an empirical model. We present here a series of new models of SN I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a46fdf7e60c6a1a61a346bf5b9ff5261
https://hal.archives-ouvertes.fr/hal-01921643
https://hal.archives-ouvertes.fr/hal-01921643
Autor:
Léget, P.-F., Gangler, E., Mondon, F., Aldering, G., Antilogus, P., Aragon, C., Bailey, S., Baltay, C., Barbary, K., Bongard, S., Boone, K., Buton, C., Chotard, N., Copin, Y., Dixon, S., Fagrelius, P., Feindt, U., Fouchez, D., Hayden, B., Hillebrandt, W.
Publikováno v:
Astronomy & Astrophysics / Astronomie et Astrophysique; Apr2020, Vol. 636, p1-24, 24p
Publikováno v:
Astronomische Nachrichten; Feb2004, Vol. 325 Issue 2, p116-119, 4p