Zobrazeno 1 - 10
of 118
pro vyhledávání: '"Schahmanèche, K."'
Autor:
Regnault, N., Guyonnet, A., Schahmanèche, K., Guillou, L. Le, Antilogus, P., Astier, P., Barrelet, E., Betoule, M., Bongard, S., Cuillandre, J. -C., Juramy, C., Pain, R., Rocci, P. -F., Tisserand, P., Villa, F.
Publikováno v:
A&A 581, A45 (2015)
We describe the design, operation, and first results of a photometric calibration project, called DICE (Direct Illumination Calibration Experiment), aiming at achieving precise instrumental calibration of optical telescopes. The heart of DICE is an i
Externí odkaz:
http://arxiv.org/abs/1506.08212
Autor:
Betoule, M., Kessler, R., Guy, J., Mosher, J., Hardin, D., Biswas, R., Astier, P., El-Hage, P., Konig, M., Kuhlmann, S., Marriner, J., Pain, R., Regnault, N., Balland, C., Bassett, B. A., Brown, P. J., Campbell, H., Carlberg, R. G., Cellier-Holzem, F., Cinabro, D., Conley, A., D'Andrea, C. B., DePoy, D. L., Doi, M., Ellis, R. S., Fabbro, S., Filippenko, A. V., Foley, R. J., Frieman, J. A., Fouchez, D., Galbany, L., Goobar, A., Gupta, R. R., Hill, G. J., Hlozek, R., Hogan, C. J., Hook, I. M., Howell, D. A., Jha, S. W., Guillou, L. Le, Leloudas, G., Lidman, C., Marshall, J. L., Möller, A., Mourão, A. M., Neveu, J., Nichol, R., Olmstead, M. D., Palanque-Delabrouille, N., Perlmutter, S., Prieto, J. L., Pritchet, C. J., Richmond, M., Riess, A. G., Ruhlmann-Kleider, V., Sako, M., Schahmaneche, K., Schneider, D. P., Smith, M., Sollerman, J., Sullivan, M., Walton, N. A., Wheeler, C. J.
We present cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observations obtained by the SDSS-II and SNLS collaborations. The data set includes several low-redshift samples (z<0.1), all 3 seasons from the SDSS-II (0.05 < z
Externí odkaz:
http://arxiv.org/abs/1401.4064
Autor:
Betoule, M., Marriner, J., Regnault, N., Cuillandre, J. -C., Astier, P., Guy, J., Balland, C., Hage, P. El, Hardin, D., Kessler, R., Guillou, L. Le, Mosher, J., Pain, R., Rocci, P. -F., Sako, M., Schahmaneche, K.
We present a combined photometric calibration of the SNLS and the SDSS supernova survey, which results from a joint effort of the SDSS and the SNLS collaborations. We deliver fluxes calibrated to the HST spectrophotometric star network for large sets
Externí odkaz:
http://arxiv.org/abs/1212.4864
Autor:
Regnault, N., Barrelet, E., Guyonnet, A., Juramy, C., Rocci, P. -F., Guillou, L. Le, Schahmanèche, K., Villa, F.
Dark Energy studies with type Ia supernovae set very tight constraints on the photometric calibration of the imagers used to detect the supernovae and follow up their flux variations. Among the key challenges is the measurement of the shape and norma
Externí odkaz:
http://arxiv.org/abs/1208.6301
Autor:
Amanullah, R., Stanishev, V., Goobar, A., Schahmaneche, K., Astier, P., Balland, C., Ellis, R. S., Fabbro, S., Hardin, D., Hook, I. M., Irwin, M. J., McMahon, R. G., Mendez, J. M., Mouchet, M., Pain, R., Ruiz-Lapuente, P., Walton, N. A.
We present multi-band light curves and distances for five type Ia supernovae at intermediate redshifts, 0.18
Externí odkaz:
http://arxiv.org/abs/0711.1375
Autor:
Balland, C., Mouchet, M., Amanullah, R., Astier, P., Fabbro, S., Folatelli, G., Garavini, G., Goobar, A., Hardin, D., Irwin, M. J., McMahon, R. G., Mourao, A. -M., Nobili, S., Pain, R., Pascoal, R., Raux, J., Sainton, G., Schahmaneche, K., Walton, N. A.
Publikováno v:
2007, A&A 464, 827
We present spectra of six Type Ia and two Type II supernovae obtained in June 2002 at the William Herschel Telescope during a search for Type Ia supernovae (SNIa) at intermediate redshift. Supernova type identification and phase determination are per
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703656
Autor:
Garavini, G., Folatelli, G., Nobili, S., Aldering, G., Amanullah, R., Antilogus, P., Astier, P., Blanc, G., Bronder, J., Burns, M. S., Conley, A., Deustua, S. E., Doi, M., Fabbro, S., Fadeyev, V., Gibbons, R., Goldhaber, G., Goobar, A., Groom, D. E., Hook, I., Howell, D. A., Kashikawa, N., Kim, A. G., Kowalski, M., Kuznetsova, N., Lee, B. C., Lidman, C., Mendez, J., Morokuma, T., Motohara, K., Nugent, P. E., Pain, R., Perlmutter, S., Quimby, R., Raux, J., Regnault, N., Ruiz-Lapuente, P., Sainton, G., Schahmaneche, K., Smith, E., Spadafora, A. L., Stanishev, V., Thomas, R. C., Walton, N. A., Wang, L., Wood-Vasey, W. M., Project, N. Yasuda. The Supernova Cosmology
We develop a method to measure the strength of the absorption features in Type Ia supernova (SN Ia) spectra and use it to make a quantitative comparison between the spectra of Type Ia supernovae at low and high redshifts. In this case study, we apply
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703629
Autor:
Balland, C., Mouchet, M., Pain, R., Walton, N. A., Amanullah, R., Astier, P., Ellis, R. S., Fabbro, S., Goobar, A., Hardin, D., Hook, I. M., Irwin, M. J., McMahon, R. M., Mendez, J. M., Ruiz-Lapuente, P., Sainton, G., Schahmaneche, K., Stanishev, V.
We present spectra of twelve Type Ia supernovae obtained in 1999 at the William Herschel Telescope and the Nordic Optical Telescope during a search for Type Ia supernovae (SN Ia) at intermediate redshift. The spectra range from z=0.178 to z=0.493, in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0507703
Autor:
Project, The Supernova Cosmology, Garavini, G., Aldering, G., Amadon, A., Amanullah, R., Astier, P., Balland, C., Blanc, G., Conley, A., Dahlen, T., Deustua, S. E., Fabbro, R. Ellis S., Fadeyev, V., Fan, X., Folatelli, G., Frye, B., Gates, E. L., Gibbons, R., Goldhaber, G., Goldman, B., Goobar, A., Groom, D. E., Haissinski, J., Hardin, D., Hook, I., Howell, D. A., Kent, S., Kim, A. G., Knop, R. A., Kowalski, M., Kuznetsova, N., Lidman, B. C. Lee C., Mendez, J., Miller, G. J., Moniez, M., Mouchet, M., Mourao, A., Newberg, H., Nobili, S., Nugent, P. E., Pain, R., Perdereau, O., Perlmutter, S., Quimby, R., Regnault, N., Rich, J., Richards, G. T., Ruiz-Lapuente, P., Schaefer, B. E., Schahmaneche, K., Smith, E., Spadafora, A. L., Stanishev, V., Thomas, R. C., Walton, N. A., Wang, L., Wood-Vasey, W. M.
Publikováno v:
Astron.J.130:2278-2292,2005
We present optical spectra of the peculiar Type Ia supernova (SN Ia) 1999ac. The data extend from -15 to +42 days with respect to B-band maximum and reveal an event that is unusual in several respects. Prior to B-band maximum, the spectra resemble th
Externí odkaz:
http://arxiv.org/abs/astro-ph/0507288
Autor:
Project, The Supernova Cosmology, Nobili, S., Amanullah, R., Garavini, G., Goobar, A., Lidman, C., Stanishev, V., Aldering, G., Antilogus, P., Astier, P., Burns, M. S., Conley, A., Deustua, S. E., Ellis, R., Fabbro, S., Fadeyev, V., Folatelli, G., Gibbons, R., Goldhaber, G., Groom, D. E., Hook, I., Howell, D. A., Kim, A. G., Knop, R. A., Nugent, P. E., Pain, R., Perlmutter, S., Quimby, R., Raux, J., Regnault, N., Ruiz-Lapuente, P., Sainton, G., Schahmaneche, K., Smith, E., Spadafora, A. L., Thomas, R. C., Wang, L.
We present a novel technique for fitting restframe I-band light curves on a data set of 42 Type Ia supernovae (SNe Ia). Using the result of the fit, we construct a Hubble diagram with 26 SNe from the subset at 0.01< z<0.1. Adding two SNe at z~0.5 yie
Externí odkaz:
http://arxiv.org/abs/astro-ph/0504139