Zobrazeno 1 - 10
of 52
pro vyhledávání: '"S. Baumont"'
Autor:
Monique S. Baumont, Caity S. Dekker, Nina Rabinovitch Blecker, Christy Turlington Burns, Nan E. Strauss
Publikováno v:
American Journal of Obstetrics and Gynecology. 228:S954-S964
Autor:
Matthieu Roman, Mark Sullivan, P. Astier, M. Betoule, A. Conley, Christopher J. Pritchet, Anais Möller, R. Pain, Christophe Balland, Dominique Fouchez, V. Arsenijevic, Sebastien Fabbro, Rowan Ellis, Ayan Mitra, V. Ruhlmann-Kleider, A. Mourao, P. El-Hage, S. Baumont, Julien Guy, F. Cellier-Holzem, Dale Andrew Howell, Nicolas Regnault, Raymond G. Carlberg, D. Hardin, C. Lidman, J. Neveu, Isobel Hook
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 614, pp.A134. ⟨10.1051/0004-6361/201731924⟩
Astron.Astrophys.
Astron.Astrophys., 2018, 614, pp.A134. ⟨10.1051/0004-6361/201731924⟩
Astronomy and Astrophysics-A&A, 2018, 614, pp.A134. ⟨10.1051/0004-6361/201731924⟩
NASA Astrophysics Data System
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 614, pp.A134. ⟨10.1051/0004-6361/201731924⟩
Astron.Astrophys.
Astron.Astrophys., 2018, 614, pp.A134. ⟨10.1051/0004-6361/201731924⟩
Astronomy and Astrophysics-A&A, 2018, 614, pp.A134. ⟨10.1051/0004-6361/201731924⟩
NASA Astrophysics Data System
We aim to present 70 spectra of 68 new high-redshift type Ia supernovae (SNeIa) measured at ESO's VLT during the final two years of operation (2006-2008) of the Supernova Legacy Survey (SNLS). We use the full five year SNLS VLT spectral set to invest
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b28be48875e5c933781166bef7f4435
https://hal.archives-ouvertes.fr/hal-01833671
https://hal.archives-ouvertes.fr/hal-01833671
Autor:
Franz E. Bauer, Lluís Galbany, Ting-Wan Chen, Stuart A. Sim, Avishay Gal-Yam, Jesper Sollerman, D. Bersier, David Rabinowitz, Brian P. Schmidt, Francesco Taddia, U. Feindt, Giorgos Leloudas, Matt Nicholl, M. T. Botticella, David Young, Anders Jerkstrand, L. Le Guillou, Cosimo Inserra, J. Polshaw, Kate Maguire, Erkki Kankare, Michel Dennefeld, K. W. Smith, Mark Sullivan, Stefano Benetti, Paolo A. Mazzali, Steve Schulze, S. Baumont, M. J. Childress, C. Baltay, M. Della Valle, Nancy Elias-Rosa, E. Hadjiyska, Stefano Valenti, Fang Yuan, Stephen J. Smartt, Ryan McKinnon, Morgan Fraser, Richard Scalzo, S. Rostami
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Nicholl, M, Smartt, S J, Jerkstrand, A, Inserra, C, Sim, S A, Chen, T-W, Benetti, S, Fraser, M, Gal-Yam, A, Kankare, E, Maguire, K, Smith, K, Sullivan, M, Valenti, S, Young, D R, Baltay, C, Bauer, F E, Baumont, S, Bersier, D, Botticella, M-T, Childress, M, Dennefeld, M, Della Valle, M, Elias-Rosa, N, Feindt, U, Galbany, L, Hadjiyska, E, Le Guillou, L, Leloudas, G, Mazzali, P, McKinnon, R, Polshaw, J, Rabinowitz, D, Rostami, S, Scalzo, R, Schmidt, B P, Schulze, S, Sollerman, J, Taddia, F & Yuan, F 2015, ' On the diversity of superluminous supernovae: ejected mass as the dominant factor ', Monthly Notices of the Royal Astronomical Society, vol. 452, no. 4, pp. 3869-3893 . https://doi.org/10.1093/mnras/stv1522
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Nicholl, M, Smartt, S J, Jerkstrand, A, Inserra, C, Sim, S A, Chen, T-W, Benetti, S, Fraser, M, Gal-Yam, A, Kankare, E, Maguire, K, Smith, K, Sullivan, M, Valenti, S, Young, D R, Baltay, C, Bauer, F E, Baumont, S, Bersier, D, Botticella, M-T, Childress, M, Dennefeld, M, Della Valle, M, Elias-Rosa, N, Feindt, U, Galbany, L, Hadjiyska, E, Le Guillou, L, Leloudas, G, Mazzali, P, McKinnon, R, Polshaw, J, Rabinowitz, D, Rostami, S, Scalzo, R, Schmidt, B P, Schulze, S, Sollerman, J, Taddia, F & Yuan, F 2015, ' On the diversity of superluminous supernovae: ejected mass as the dominant factor ', Monthly Notices of the Royal Astronomical Society, vol. 452, no. 4, pp. 3869-3893 . https://doi.org/10.1093/mnras/stv1522
We assemble a sample of 24 hydrogen-poor super-luminous supernovae (SLSNe). Parameterizing the light curve shape through rise and decline timescales shows that the two are highly correlated. Magnetar-powered models can reproduce the correlation, with
Autor:
P. Ripoche, Melissa L. Graham, Stephen D. J. Gwyn, Stéphane Basa, S. Baumont, Julien Guy, Tianmeng Zhang, A. Conley, Kathy Perrett, Nicolas Regnault, D. Hardin, James D. Neill, Emma S. Walker, Christopher J. Pritchet, Christophe Balland, Dominique Fouchez, Pierre Astier, D. Balam, Saul Perlmutter, C. Lidman, Raymond G. Carlberg, Eric Hsiao, D. A. Howell, Mark Sullivan, I. M. Hook, J. Le Du, Nao Suzuki, Reynald Pain
Publikováno v:
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2008, 135, pp.1343-1349. ⟨10.1088/0004-6256/135/4/1343⟩
The Astronomical Journal, 2008, 135, pp.1343-1349. ⟨10.1088/0004-6256/135/4/1343⟩
The Astronomical Journal, American Astronomical Society, 2008, 135, pp.1343-1349. ⟨10.1088/0004-6256/135/4/1343⟩
The Astronomical Journal, 2008, 135, pp.1343-1349. ⟨10.1088/0004-6256/135/4/1343⟩
The Canada-France-Hawaii Telescope Supernova Legacy Survey (SNLS) has created a large homogeneous database of intermediate redshift (0.2 < z < 1.0) type Ia supernovae (SNe Ia). The SNLS team has shown that correlations exist between SN Ia rates, prop
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::41eed4983c78c4055871cbeeb58a469a
https://ora.ox.ac.uk/objects/uuid:c2057478-734c-41e9-a6c2-2bcaca09371e
https://ora.ox.ac.uk/objects/uuid:c2057478-734c-41e9-a6c2-2bcaca09371e
Autor:
Julien Guy, Christopher J. Pritchet, A. Conley, D. Fouchez, Stéphane Basa, Saul Perlmutter, V. Ruhlmann-Kleider, James D. Neill, P. Ripoche, S. Baumont, D. A. Howell, D. Hardin, David D. Balam, I. M. Hook, C. Lidman, Nathalie Palanque-Delabrouille, Mark Sullivan, Nicolas Regnault, Raymond G. Carlberg, Emma S. Walker, Christophe Balland, Santiago González-Gaitán, Kathy Perrett, Pierre Astier, J. Rich, Reynald Pain
Publikováno v:
The Astronomical Journal
The Astronomical Journal, 2012, 144, pp.59. ⟨10.1088/0004-6256/144/2/59⟩
The Astronomical Journal, American Astronomical Society, 2012, 144, pp.59. ⟨10.1088/0004-6256/144/2/59⟩
The Astronomical Journal, 2012, 144, pp.59. ⟨10.1088/0004-6256/144/2/59⟩
The Astronomical Journal, American Astronomical Society, 2012, 144, pp.59. ⟨10.1088/0004-6256/144/2/59⟩
We present a measurement of the volumetric Type Ia supernova (SN Ia) rate (SNR_Ia) as a function of redshift for the first four years of data from the Canada-France-Hawaii Telescope (CFHT) Supernova Legacy Survey (SNLS). This analysis includes 286 sp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e9c77cda57172c67bac50a5b3da7e00c
https://ora.ox.ac.uk/objects/uuid:8c83d0a9-7f81-4506-aa01-8885892b32b2
https://ora.ox.ac.uk/objects/uuid:8c83d0a9-7f81-4506-aa01-8885892b32b2
Autor:
Reynald Pain, Sebastien Fabbro, C. Lidmam, N. Fourmanoit, Melissa L. Graham, Jeffrey A. Rich, Richard S. Ellis, S. Baumont, K. Perrett, Nao Suzuki, Julien Guy, Mark Sullivan, Nicolas Regnault, Michael J. Hudson, A. Mourao, D. Hardin, C. Balland, D. Fouchez, E. S. Walker, Pierre Astier, James D. Neill, Saul Perlmutter, David D. Balam, C. J. Pritchet, N. Palanque-Delabrouille, T. Kronborg, H. K. Fakhouri, Alex Conley, Santiago González-Gaitán, P. Ripoche, V. Ruhlmann-Kleider, S. Basa, I. M. Hook, Raymond G. Carlberg, Eric Hsiao, D. A. Howell
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2011, 737, pp.102. ⟨10.1088/0004-637X/737/2/102⟩
The Astrophysical Journal, American Astronomical Society, 2011, 737, pp.102. ⟨10.1088/0004-637X/737/2/102⟩
The Astrophysical Journal, 2011, 737, pp.102. ⟨10.1088/0004-637X/737/2/102⟩
The Astrophysical Journal, American Astronomical Society, 2011, 737, pp.102. ⟨10.1088/0004-637X/737/2/102⟩
We present observational constraints on the nature of dark energy using the Supernova Legacy Survey three year sample (SNLS3) of Guy et al. (2010) and Conley et al. (2011). We use the 472 SNe Ia in this sample, accounting for recently discovered corr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7fcb00ff8116f83d350b531b0ef5a971
https://doi.org/10.1088/0004-637x/737/2/102
https://doi.org/10.1088/0004-637x/737/2/102
Autor:
Sebastien Fabbro, Hélène M. Courtois, P. Antilogus, A. Mourao, J. Bronder, V. Arsenijevic, Dominique Fouchez, Julien Guy, S. Basa, D. Guide, Richard Taillet, A. C. Gonçalves, Christopher J. Pritchet, Charling Tao, Saul Perlmutter, David D. Balam, Reynald Pain, D. Hardin, M. Filiol, Nathalie Palanque-Delabrouille, James D. Neill, Christophe Balland, Éric Aubourg, Nicolas Regnault, M. Mouchet, Richard G. McMahon, J. Rich, H. Lafoux, Ariel Goobar, Mark Sullivan, V. Lusset, Nicholas A. Walton, S. Baumont, Pierre Astier, I. M. Hook, D. A. Howell, Greg Aldering, K. Perrett, Raymond G. Carlberg, Rowan Ellis, C. Lidman, P. Ripoche
Publikováno v:
Astronomy & Astrophysics. 447:31-48
We present distance measurements to 71 high redshift type Ia supernovae discovered during the first year of the 5-year Supernova Legacy Survey (SNLS). These events were detected and their multi-color light-curves measured using the MegaPrime/MegaCam
Autor:
T. W. Chen, M. Della Valle, M. Sullivan, M. Dennefeld, Nancy Elias-Rosa, Stephen J. Smartt, Jesper Sollerman, S. Rostami, E. Hadjiyska, L. Le Guillou, Brian P. Schmidt, Kate Maguire, Ryan McKinnon, Matt Nicholl, Morgan Fraser, K. W. Smith, Stefano Valenti, S. Baumont, Franz E. Bauer, U. Feindt, Fang Yuan, Lluís Galbany, Paolo A. Mazzali, J. Polshaw, C. Baltay, D. Rabinowitz, D. Bersier, F. Taddia, M. J. Childress, Richard Scalzo, S. Benetti, Stuart A. Sim, Avishay Gal-Yam, Anders Jerkstrand, Cosimo Inserra, Steve Schulze, David Young, M. T. Botticella, Erkki Kankare, Giorgos Leloudas
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 457:2514-2515
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Astronomy & Astrophysics. 388:661-666
We present CCD photometric observations of Centaurs 2000 QC243 and 2001 PT13. For 2000 QC243 ,a large amplitude period is found at 4:57 h 0:05 h, which likely corresponds to half the rotation period of the body, or coincides with the full rotation pe