Search

Your search keyword '"Hafizov, B."' showing total 11 results
Start Over Author "Hafizov, B."
11 results on '"Hafizov, B."'

1. Timing of AB And eclipses

Author

Kozyreva, V. S., Ibrahimov, M. A., Gaynullina, E. R., Karimov, R. G., Hafizov, B. M., Satovskii, B. L., Krushevska, V. N., Kuznyetsova, Yu. G., Bogomazov, A. I., Irsmambetova, T. R., and Tutukov, A. V.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

This study aims timing the eclipses of the short period low mass binary star AB And. The times of minima are taken from the literature and from our observations in October 2013 (22 times of minima) and in August 2014 (23 times of minima). We find and discuss an inaccuracy in the determination of the types of minima in the previous investigation by \citet{li2014}. We study the secular evolution of the central binary's orbital period and the possibility of the existence of third and fourth companions in the system., Comment: 14 pages, 3 figures, 3 tables, accepted by New Astronomy

Published
2017
Full Text
View/download PDF

2. The Afterglows of Swift-era Gamma-Ray Bursts. I. Comparing pre-Swift and Swift era Long/Soft (Type II) GRB Optical Afterglows

Author

Kann, D. A., Klose, S., Zhang, B., Malesani, D., Nakar, E., Pozanenko, A., Wilson, A. C., Butler, N. R., Jakobsson, P., Schulze, S., Andreev, M., Antonelli, L. A., Bikmaev, I. F., Biryukov, V., Böttcher, M., Burenin, R. A., Cerón, J. M. Castro, Castro-Tirado, A. J., Chincarini, G., Cobb, B. E., Covino, S., D'Avanzo, P., D'Elia, V., Della Valle, M., Postigo, A. de Ugarte, Efimov, Yu., Ferrero, P., Fugazza, D., Fynbo, J. P. U., Gålfalk, M., Grundahl, F., Gorosabel, J., Gupta, S., Guziy, S., Hafizov, B., Hjorth, J., Holhjem, K., Ibrahimov, M., Im, M., Israel, G. L., Jeĺinek, M., Jensen, B. L., Karimov, R., Khamitov, I. M., Kızıloǧlu, Ü., Klunko, E., Kubánek, P., Kutyrev, A. S., Laursen, P., Levan, A. J., Mannucci, F., Martin, C. M., Mescheryakov, A., Mirabal, N., Norris, J. P., Ovaldsen, J. -E., Paraficz, D., Pavlenko, E., Piranomonte, S., Rossi, A., Rumyantsev, V., Salinas, R., Sergeev, A., Sharapov, D., Sollerman, J., Stecklum, B., Stella, L., Tagliaferri, G., Tanvir, N. R., Telting, J., Testa, V., Updike, A. C., Volnova, A., Watson, D., Wiersema, K., and Xu, D.

Subjects
Astrophysics
Abstract

We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ray burst (GRB) afterglows including GRBs up to September 2009, for a total of 76 GRBs, and present an additional three pre-Swift GRBs not included in an earlier sample. Furthermore, we publish 840 additional new photometry data points on a total of 42 GRB afterglows, including large data sets for GRBs 050319, 050408, 050802, 050820A, 050922C, 060418, 080413A and 080810. We analyzed the light curves of all GRBs in the sample and derived spectral energy distributions for the sample with the best data quality, allowing us to estimate the host galaxy extinction. We transformed the afterglow light curves into an extinction-corrected z=1 system and compared their luminosities with a sample of pre-Swift afterglows. The results of a former study, which showed that GRB afterglows clustered and exhibited a bimodal distribution in luminosity space, is weakened by the larger sample. We found that the luminosity distribution of the two afterglow samples (Swift-era and pre-Swift) are very similar, and that a subsample for which we were not able to estimate the extinction, which is fainter than the main sample, can be explained by assuming a moderate amount of line-of-sight host extinction. We derived bolometric isotropic energies for all GRBs in our sample, and found only a tentative correlation between the prompt energy release and the optical afterglow luminosity at one day after the GRB in the z=1 system. A comparative study of the optical luminosities of GRB afterglows with echelle spectra (which show a high number of foreground absorbing systems) and those without reveals no indication that the former are statistically significantly more luminous. (abridged), Comment: ApJ, in press; 65 pages in journal format; 20 pages main text, 18 pages Appendix, 5 pages references, 6 tables (21 pages), 9 figures, 840 original data points; v4: Updated references and acknowledgements, corrected mistake in table 1

Published
2007
Full Text
View/download PDF

3. Timing of AB And eclipses

Author

Kozyreva, V. S, primary, Ibrahimov, M. A, additional, Gaynullina, E. R, additional, Karimov, R. G, additional, Hafizov, B. M, additional, Satovskii, B. L, additional, Krushevska, V. N, additional, Kuznyetsova, Yu. G, additional, Bogomazov, A. I, additional, Irsmambetova, T. R, additional, and Tutukov, A. V, additional

Published
2018
Full Text
View/download PDF

4. The afterglows of Swift-era gamma-ray bursts. I. Comparing pre-Swift and Swift-era long/soft (type II) GRB optical afterglows

Author

Kann D., Klose S., Zhang B., Malesani D., Nakar E., Pozanenko A., Wilson A., Butler N., Jakobsson P., Schulze S., Andreev M., Antonelli L., Bikmaev I., Biryukov V., Böttcher M., Burenin R., Cerón J., Castro-Tirado A., Chincarini G., Cobb B., Covino S., D'Avanzo P., D'Elia V., Valle M., De Ugarte Postigo A., Efimov Y., Ferrero P., Fugazza D., Fynbo J., Gålfalk M., Grundahl F., Gorosabel J., Gupta S., Guziy S., Hafizov B., Hjorth J., Holhjem K., Ibrahimov M., Im M., Israel G., Jelainek M., Jensen B., Karimov R., Khamitov I., Kiziloǧlu U., Klunko E., Kubánek P., Kutyrev A., Laursen P., Levan A., Mannucci F., Martin C., Mescheryakov A., Mirabal N., Norris J., Ovaldsen J., Paraficz D., Pavlenko E., Piranomonte S., Rossi A., Rumyantsev V., Salinas R., Sergeev A., Sharapov D., Sollerman J., Stecklum B., Stella L., Tagliaferri G., Tanvir N., Telting J., Testa V., Updike A., Volnova A., Watson D., Wiersema K., and Xu D.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics, Dust, extinction, general [Gamma-ray burst]
Abstract

We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ray burst (GRB) afterglows including GRBs up to 2009 September, for a total of 76 GRBs, and present an additional three pre-Swift GRBs not included in an earlier sample. Furthermore, we publish 840 additional new photometry data points on a total of 42 GRB afterglows, including large data sets for GRBs 050319, 050408, 050802, 050820A, 050922C, 060418, 080413A, and 080810. We analyzed the light curves of all GRBs in the sample and derived spectral energy distributions for the sample with the best data quality, allowing us to estimate the host-galaxy extinction. We transformed the afterglow light curves into an extinction-corrected z = 1 system and compared their luminosities with a sample of pre-Swift afterglows. The results of a former study, which showed that GRB afterglows clustered and exhibited a bimodal distribution in luminosity space, are weakened by the larger sample. We found that the luminosity distribution of the two afterglow samples (Swift-era and pre-Swift) is very similar, and that a subsample for which we were not able to estimate the extinction, which is fainter than the main sample, can be explained by assuming a moderate amount of line-of-sight host extinction. We derived bolometric isotropic energies for all GRBs in our sample, and found only a tentative correlation between the prompt energy release and the optical afterglow luminosity at 1 day after the GRB in the z = 1 system. A comparative study of the optical luminosities of GRB afterglows with echelle spectra (which show a high number of foreground absorbing systems) and those without, reveals no indication that the former are statistically significantly more luminous. Furthermore, we propose the existence of an upper ceiling on afterglow luminosities and study the luminosity distribution at early times, which was not accessible before the advent of the Swift satellite. Most GRBs feature afterglows that are dominated by the forward shock from early times on. Finally, we present the first indications of a class of long GRBs, which form a bridge between the typical highluminosity, high-redshift events and nearby low-luminosity events (which are also associated with spectroscopic supernovae) in terms of energetics and observed redshift distribution, indicating a continuous distribution overall. © 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.

Published
2010

5. THE AFTERGLOWS OF SWIFT-ERA GAMMA-RAY BURSTS. I. COMPARING PRE-SWIFT AND SWIFT-ERA LONG/SOFT (TYPE II) GRB OPTICAL AFTERGLOWS

Author

Kann, D. A., Klose, S., Zhang, B., Malesani, D., Nakar, E., Pozanenko, A., Wilson, A. C., Butler, N. R., Jakobsson, P., Schulze, S., Andreev, M., Antonelli, L. A., Bikmaev, I. F., Biryukov, V., Boettcher, M., Burenin, R. A., Castro Ceron, J. M., Castro-Tirado, A. J., Chincarini, G., Cobb, B. E., Covino, S., D'Avanzo, P., D'Elia, V., Della Valle, M., Postigo, A. de Ugarte, Efimov, Yu., Ferrero, P., Fugazza, D., Fynbo, J. P. U., Gålfalk, Magnus, Grundahl, F., Gorosabel, J., Gupta, S., Guziy, S., Hafizov, B., Hjorth, J., Holhjem, K., Ibrahimov, M., Im, M., Israel, G. L., Jelinek, M., Jensen, B. L., Karimov, R., Khamitov, I. M., Kiziloglu, Ue, Klunko, E., Kubanek, P., Kutyrev, A. S., Laursen, P., Levan, A. J., Mannucci, F., Martin, C. M., Mescheryakov, A., Mirabal, N., Norris, J. P., Ovaldsen, J. -E, Paraficz, D., Pavlenko, E., Piranomonte, S., Rossi, A., Rumyantsev, V., Salinas, R., Sergeev, A., Sharapov, D., Sollerman, Jesper, Stecklum, B., Stella, L., Tagliaferri, G., Tanvir, N. R., Telting, J., Testa, V., Updike, A. C., Volnova, A., Watson, D., Wiersema, K., Xu, D., Kann, D. A., Klose, S., Zhang, B., Malesani, D., Nakar, E., Pozanenko, A., Wilson, A. C., Butler, N. R., Jakobsson, P., Schulze, S., Andreev, M., Antonelli, L. A., Bikmaev, I. F., Biryukov, V., Boettcher, M., Burenin, R. A., Castro Ceron, J. M., Castro-Tirado, A. J., Chincarini, G., Cobb, B. E., Covino, S., D'Avanzo, P., D'Elia, V., Della Valle, M., Postigo, A. de Ugarte, Efimov, Yu., Ferrero, P., Fugazza, D., Fynbo, J. P. U., Gålfalk, Magnus, Grundahl, F., Gorosabel, J., Gupta, S., Guziy, S., Hafizov, B., Hjorth, J., Holhjem, K., Ibrahimov, M., Im, M., Israel, G. L., Jelinek, M., Jensen, B. L., Karimov, R., Khamitov, I. M., Kiziloglu, Ue, Klunko, E., Kubanek, P., Kutyrev, A. S., Laursen, P., Levan, A. J., Mannucci, F., Martin, C. M., Mescheryakov, A., Mirabal, N., Norris, J. P., Ovaldsen, J. -E, Paraficz, D., Pavlenko, E., Piranomonte, S., Rossi, A., Rumyantsev, V., Salinas, R., Sergeev, A., Sharapov, D., Sollerman, Jesper, Stecklum, B., Stella, L., Tagliaferri, G., Tanvir, N. R., Telting, J., Testa, V., Updike, A. C., Volnova, A., Watson, D., Wiersema, K., and Xu, D.

Abstract

We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ray burst (GRB) afterglows including GRBs up to 2009 September, for a total of 76 GRBs, and present an additional three pre-Swift GRBs not included in an earlier sample. Furthermore, we publish 840 additional new photometry data points on a total of 42 GRB afterglows, including large data sets for GRBs 050319, 050408, 050802, 050820A, 050922C, 060418, 080413A, and 080810. We analyzed the light curves of all GRBs in the sample and derived spectral energy distributions for the sample with the best data quality, allowing us to estimate the host-galaxy extinction. We transformed the afterglow light curves into an extinction-corrected z = 1 system and compared their luminosities with a sample of pre-Swift afterglows. The results of a former study, which showed that GRB afterglows clustered and exhibited a bimodal distribution in luminosity space, are weakened by the larger sample. We found that the luminosity distribution of the two afterglow samples (Swift-era and pre-Swift) is very similar, and that a subsample for which we were not able to estimate the extinction, which is fainter than the main sample, can be explained by assuming a moderate amount of line-of-sight host extinction. We derived bolometric isotropic energies for all GRBs in our sample, and found only a tentative correlation between the prompt energy release and the optical afterglow luminosity at 1 day after the GRB in the z = 1 system. A comparative study of the optical luminosities of GRB afterglows with echelle spectra (which show a high number of foreground absorbing systems) and those without, reveals no indication that the former are statistically significantly more luminous. Furthermore, we propose the existence of an upper ceiling on afterglow luminosities and study the luminosity distribution at early times, which was not accessible before the advent of the Swift satellite. Most GRBs feature aftergl, authorCount :76

Published
2010
Full Text
View/download PDF

6. THE AFTERGLOWS OFSWIFT-ERA GAMMA-RAY BURSTS. I. COMPARING PRE-SWIFTANDSWIFT-ERA LONG/SOFT (TYPE II) GRB OPTICAL AFTERGLOWS

Author

Kann, D. A., primary, Klose, S., additional, Zhang, B., additional, Malesani, D., additional, Nakar, E., additional, Pozanenko, A., additional, Wilson, A. C., additional, Butler, N. R., additional, Jakobsson, P., additional, Schulze, S., additional, Andreev, M., additional, Antonelli, L. A., additional, Bikmaev, I. F., additional, Biryukov, V., additional, Böttcher, M., additional, Burenin, R. A., additional, Castro Cerón, J. M., additional, Castro-Tirado, A. J., additional, Chincarini, G., additional, Cobb, B. E., additional, Covino, S., additional, D'Avanzo, P., additional, D'Elia, V., additional, Della Valle, M., additional, de Ugarte Postigo, A., additional, Efimov, Yu., additional, Ferrero, P., additional, Fugazza, D., additional, Fynbo, J. P. U., additional, Gålfalk, M., additional, Grundahl, F., additional, Gorosabel, J., additional, Gupta, S., additional, Guziy, S., additional, Hafizov, B., additional, Hjorth, J., additional, Holhjem, K., additional, Ibrahimov, M., additional, Im, M., additional, Israel, G. L., additional, Jeĺinek, M., additional, Jensen, B. L., additional, Karimov, R., additional, Khamitov, I. M., additional, Kiziloǧlu, Ü., additional, Klunko, E., additional, Kubánek, P., additional, Kutyrev, A. S., additional, Laursen, P., additional, Levan, A. J., additional, Mannucci, F., additional, Martin, C. M., additional, Mescheryakov, A., additional, Mirabal, N., additional, Norris, J. P., additional, Ovaldsen, J.-E., additional, Paraficz, D., additional, Pavlenko, E., additional, Piranomonte, S., additional, Rossi, A., additional, Rumyantsev, V., additional, Salinas, R., additional, Sergeev, A., additional, Sharapov, D., additional, Sollerman, J., additional, Stecklum, B., additional, Stella, L., additional, Tagliaferri, G., additional, Tanvir, N. R., additional, Telting, J., additional, Testa, V., additional, Updike, A. C., additional, Volnova, A., additional, Watson, D., additional, Wiersema, K., additional, and Xu, D., additional

Published
2010
Full Text
View/download PDF

8. The afterglows of Swift-era gamma-ray bursts. I. Comparing pre-Swift and Swift-era long/soft (type II) GRB optical afterglows

Author

Kann D., Klose S., Zhang B., Malesani D., Nakar E., Pozanenko A., Wilson A., Butler N., Jakobsson P., Schulze S., Andreev M., Antonelli L., Bikmaev I., Biryukov V., Böttcher M., Burenin R., Cerón J., Castro-Tirado A., Chincarini G., Cobb B., Covino S., D'Avanzo P., D'Elia V., Valle M., De Ugarte Postigo A., Efimov Y., Ferrero P., Fugazza D., Fynbo J., Gålfalk M., Grundahl F., Gorosabel J., Gupta S., Guziy S., Hafizov B., Hjorth J., Holhjem K., Ibrahimov M., Im M., Israel G., Jelainek M., Jensen B., Karimov R., Khamitov I., Kiziloǧlu U., Klunko E., Kubánek P., Kutyrev A., Laursen P., Levan A., Mannucci F., Martin C., Mescheryakov A., Mirabal N., Norris J., Ovaldsen J., Paraficz D., Pavlenko E., Piranomonte S., Rossi A., Rumyantsev V., Salinas R., Sergeev A., Sharapov D., Sollerman J., Stecklum B., Stella L., Tagliaferri G., Tanvir N., Telting J., Testa V., Updike A., Volnova A., Watson D., Wiersema K., Xu D., Kann D., Klose S., Zhang B., Malesani D., Nakar E., Pozanenko A., Wilson A., Butler N., Jakobsson P., Schulze S., Andreev M., Antonelli L., Bikmaev I., Biryukov V., Böttcher M., Burenin R., Cerón J., Castro-Tirado A., Chincarini G., Cobb B., Covino S., D'Avanzo P., D'Elia V., Valle M., De Ugarte Postigo A., Efimov Y., Ferrero P., Fugazza D., Fynbo J., Gålfalk M., Grundahl F., Gorosabel J., Gupta S., Guziy S., Hafizov B., Hjorth J., Holhjem K., Ibrahimov M., Im M., Israel G., Jelainek M., Jensen B., Karimov R., Khamitov I., Kiziloǧlu U., Klunko E., Kubánek P., Kutyrev A., Laursen P., Levan A., Mannucci F., Martin C., Mescheryakov A., Mirabal N., Norris J., Ovaldsen J., Paraficz D., Pavlenko E., Piranomonte S., Rossi A., Rumyantsev V., Salinas R., Sergeev A., Sharapov D., Sollerman J., Stecklum B., Stella L., Tagliaferri G., Tanvir N., Telting J., Testa V., Updike A., Volnova A., Watson D., Wiersema K., and Xu D.

Abstract

We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ray burst (GRB) afterglows including GRBs up to 2009 September, for a total of 76 GRBs, and present an additional three pre-Swift GRBs not included in an earlier sample. Furthermore, we publish 840 additional new photometry data points on a total of 42 GRB afterglows, including large data sets for GRBs 050319, 050408, 050802, 050820A, 050922C, 060418, 080413A, and 080810. We analyzed the light curves of all GRBs in the sample and derived spectral energy distributions for the sample with the best data quality, allowing us to estimate the host-galaxy extinction. We transformed the afterglow light curves into an extinction-corrected z = 1 system and compared their luminosities with a sample of pre-Swift afterglows. The results of a former study, which showed that GRB afterglows clustered and exhibited a bimodal distribution in luminosity space, are weakened by the larger sample. We found that the luminosity distribution of the two afterglow samples (Swift-era and pre-Swift) is very similar, and that a subsample for which we were not able to estimate the extinction, which is fainter than the main sample, can be explained by assuming a moderate amount of line-of-sight host extinction. We derived bolometric isotropic energies for all GRBs in our sample, and found only a tentative correlation between the prompt energy release and the optical afterglow luminosity at 1 day after the GRB in the z = 1 system. A comparative study of the optical luminosities of GRB afterglows with echelle spectra (which show a high number of foreground absorbing systems) and those without, reveals no indication that the former are statistically significantly more luminous. Furthermore, we propose the existence of an upper ceiling on afterglow luminosities and study the luminosity distribution at early times, which was not accessible before the advent of the Swift satellite. Most GRBs feature aftergl

9. The afterglows of Swift-era gamma-ray bursts. I. Comparing pre-Swift and Swift-era long/soft (type II) GRB optical afterglows

Author

Kann D., Klose S., Zhang B., Malesani D., Nakar E., Pozanenko A., Wilson A., Butler N., Jakobsson P., Schulze S., Andreev M., Antonelli L., Bikmaev I., Biryukov V., Böttcher M., Burenin R., Cerón J., Castro-Tirado A., Chincarini G., Cobb B., Covino S., D'Avanzo P., D'Elia V., Valle M., De Ugarte Postigo A., Efimov Y., Ferrero P., Fugazza D., Fynbo J., Gålfalk M., Grundahl F., Gorosabel J., Gupta S., Guziy S., Hafizov B., Hjorth J., Holhjem K., Ibrahimov M., Im M., Israel G., Jelainek M., Jensen B., Karimov R., Khamitov I., Kiziloǧlu U., Klunko E., Kubánek P., Kutyrev A., Laursen P., Levan A., Mannucci F., Martin C., Mescheryakov A., Mirabal N., Norris J., Ovaldsen J., Paraficz D., Pavlenko E., Piranomonte S., Rossi A., Rumyantsev V., Salinas R., Sergeev A., Sharapov D., Sollerman J., Stecklum B., Stella L., Tagliaferri G., Tanvir N., Telting J., Testa V., Updike A., Volnova A., Watson D., Wiersema K., Xu D., Kann D., Klose S., Zhang B., Malesani D., Nakar E., Pozanenko A., Wilson A., Butler N., Jakobsson P., Schulze S., Andreev M., Antonelli L., Bikmaev I., Biryukov V., Böttcher M., Burenin R., Cerón J., Castro-Tirado A., Chincarini G., Cobb B., Covino S., D'Avanzo P., D'Elia V., Valle M., De Ugarte Postigo A., Efimov Y., Ferrero P., Fugazza D., Fynbo J., Gålfalk M., Grundahl F., Gorosabel J., Gupta S., Guziy S., Hafizov B., Hjorth J., Holhjem K., Ibrahimov M., Im M., Israel G., Jelainek M., Jensen B., Karimov R., Khamitov I., Kiziloǧlu U., Klunko E., Kubánek P., Kutyrev A., Laursen P., Levan A., Mannucci F., Martin C., Mescheryakov A., Mirabal N., Norris J., Ovaldsen J., Paraficz D., Pavlenko E., Piranomonte S., Rossi A., Rumyantsev V., Salinas R., Sergeev A., Sharapov D., Sollerman J., Stecklum B., Stella L., Tagliaferri G., Tanvir N., Telting J., Testa V., Updike A., Volnova A., Watson D., Wiersema K., and Xu D.

Abstract

We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ray burst (GRB) afterglows including GRBs up to 2009 September, for a total of 76 GRBs, and present an additional three pre-Swift GRBs not included in an earlier sample. Furthermore, we publish 840 additional new photometry data points on a total of 42 GRB afterglows, including large data sets for GRBs 050319, 050408, 050802, 050820A, 050922C, 060418, 080413A, and 080810. We analyzed the light curves of all GRBs in the sample and derived spectral energy distributions for the sample with the best data quality, allowing us to estimate the host-galaxy extinction. We transformed the afterglow light curves into an extinction-corrected z = 1 system and compared their luminosities with a sample of pre-Swift afterglows. The results of a former study, which showed that GRB afterglows clustered and exhibited a bimodal distribution in luminosity space, are weakened by the larger sample. We found that the luminosity distribution of the two afterglow samples (Swift-era and pre-Swift) is very similar, and that a subsample for which we were not able to estimate the extinction, which is fainter than the main sample, can be explained by assuming a moderate amount of line-of-sight host extinction. We derived bolometric isotropic energies for all GRBs in our sample, and found only a tentative correlation between the prompt energy release and the optical afterglow luminosity at 1 day after the GRB in the z = 1 system. A comparative study of the optical luminosities of GRB afterglows with echelle spectra (which show a high number of foreground absorbing systems) and those without, reveals no indication that the former are statistically significantly more luminous. Furthermore, we propose the existence of an upper ceiling on afterglow luminosities and study the luminosity distribution at early times, which was not accessible before the advent of the Swift satellite. Most GRBs feature aftergl

10. THE AFTERGLOWS OF SWIFT-ERA GAMMA-RAY BURSTS. I. COMPARING PRE-SWIFT AND SWIFT-ERA LONG/SOFT (TYPE II) GRB OPTICAL AFTERGLOWS

Author

Kann, D. A., Klose, S., Zhang, B., Malesani, D., Nakar, E., Pozanenko, A., Wilson, A. C., Butler, N. R., Jakobsson, P., Schulze, S., Andreev, M., Antonelli, L. A., Bikmaev, I. F., Biryukov, V., B¨ottcher, M., Burenin, R. A., Castro Cer´on, J. M., Castro-Tirado, A. J., Chincarini, G., Cobb, B. E., Covino, S., D’Avanzo, P., D’Elia, V., Della Valle, M., de Ugarte Postigo, A., Efimov, Yu, Ferrero, P., Fugazza, D., Fynbo, J. P.U., Gålfalk, M., Grundahl, F., Gorosabel, J., Gupta, S., Guziy, S., Hafizov, B., Hjorth, J., Holhjem, K., Ibrahimov, M., Im, M., Israel, G. L., Je´linek, M., Jensen, B. L., Karimov, R., Khamitov, I. M., Kizilogˇlu, U., Klunko, E., Kuba´nek, P., Kutyrev, A. S., Laursen, P., Levan, A. J., Mannucci, F., Martin, C. M., Mescheryakov, A., Mirabal, N., Norris, J. P., Ovaldsen, J. -E., Paraficz, D., Pavlenko, E., Piranomonte, S., Rossi, A., Rumyantsev, V., Salinas, R., Sergeev, A., Sharapov, D., Sollerman, J., Stecklum, B., Stella, L., Tagliaferri, G., Tanvir, N. R., Telting, J., Testa, V., Updike, Adria, Volnova, A., Watson, D., Wiersema, K., Xu, D., Kann, D. A., Klose, S., Zhang, B., Malesani, D., Nakar, E., Pozanenko, A., Wilson, A. C., Butler, N. R., Jakobsson, P., Schulze, S., Andreev, M., Antonelli, L. A., Bikmaev, I. F., Biryukov, V., B¨ottcher, M., Burenin, R. A., Castro Cer´on, J. M., Castro-Tirado, A. J., Chincarini, G., Cobb, B. E., Covino, S., D’Avanzo, P., D’Elia, V., Della Valle, M., de Ugarte Postigo, A., Efimov, Yu, Ferrero, P., Fugazza, D., Fynbo, J. P.U., Gålfalk, M., Grundahl, F., Gorosabel, J., Gupta, S., Guziy, S., Hafizov, B., Hjorth, J., Holhjem, K., Ibrahimov, M., Im, M., Israel, G. L., Je´linek, M., Jensen, B. L., Karimov, R., Khamitov, I. M., Kizilogˇlu, U., Klunko, E., Kuba´nek, P., Kutyrev, A. S., Laursen, P., Levan, A. J., Mannucci, F., Martin, C. M., Mescheryakov, A., Mirabal, N., Norris, J. P., Ovaldsen, J. -E., Paraficz, D., Pavlenko, E., Piranomonte, S., Rossi, A., Rumyantsev, V., Salinas, R., Sergeev, A., Sharapov, D., Sollerman, J., Stecklum, B., Stella, L., Tagliaferri, G., Tanvir, N. R., Telting, J., Testa, V., Updike, Adria, Volnova, A., Watson, D., Wiersema, K., and Xu, D.

Abstract

Published in: Astrophysical Journal, Volume 720, 2010

11. THE AFTERGLOWS OF SWIFT-ERA GAMMA-RAY BURSTS. I. COMPARING PRE-SWIFT AND SWIFT-ERA LONG/SOFT (TYPE II) GRB OPTICAL AFTERGLOWS

Author

Kann, D. A., Klose, S., Zhang, B., Malesani, D., Nakar, E., Pozanenko, A., Wilson, A. C., Butler, N. R., Jakobsson, P., Schulze, S., Andreev, M., Antonelli, L. A., Bikmaev, I. F., Biryukov, V., B¨ottcher, M., Burenin, R. A., Castro Cer´on, J. M., Castro-Tirado, A. J., Chincarini, G., Cobb, B. E., Covino, S., D’Avanzo, P., D’Elia, V., Della Valle, M., de Ugarte Postigo, A., Efimov, Yu, Ferrero, P., Fugazza, D., Fynbo, J. P.U., Gålfalk, M., Grundahl, F., Gorosabel, J., Gupta, S., Guziy, S., Hafizov, B., Hjorth, J., Holhjem, K., Ibrahimov, M., Im, M., Israel, G. L., Je´linek, M., Jensen, B. L., Karimov, R., Khamitov, I. M., Kizilogˇlu, U., Klunko, E., Kuba´nek, P., Kutyrev, A. S., Laursen, P., Levan, A. J., Mannucci, F., Martin, C. M., Mescheryakov, A., Mirabal, N., Norris, J. P., Ovaldsen, J. -E., Paraficz, D., Pavlenko, E., Piranomonte, S., Rossi, A., Rumyantsev, V., Salinas, R., Sergeev, A., Sharapov, D., Sollerman, J., Stecklum, B., Stella, L., Tagliaferri, G., Tanvir, N. R., Telting, J., Testa, V., Updike, Adria, Volnova, A., Watson, D., Wiersema, K., Xu, D., Kann, D. A., Klose, S., Zhang, B., Malesani, D., Nakar, E., Pozanenko, A., Wilson, A. C., Butler, N. R., Jakobsson, P., Schulze, S., Andreev, M., Antonelli, L. A., Bikmaev, I. F., Biryukov, V., B¨ottcher, M., Burenin, R. A., Castro Cer´on, J. M., Castro-Tirado, A. J., Chincarini, G., Cobb, B. E., Covino, S., D’Avanzo, P., D’Elia, V., Della Valle, M., de Ugarte Postigo, A., Efimov, Yu, Ferrero, P., Fugazza, D., Fynbo, J. P.U., Gålfalk, M., Grundahl, F., Gorosabel, J., Gupta, S., Guziy, S., Hafizov, B., Hjorth, J., Holhjem, K., Ibrahimov, M., Im, M., Israel, G. L., Je´linek, M., Jensen, B. L., Karimov, R., Khamitov, I. M., Kizilogˇlu, U., Klunko, E., Kuba´nek, P., Kutyrev, A. S., Laursen, P., Levan, A. J., Mannucci, F., Martin, C. M., Mescheryakov, A., Mirabal, N., Norris, J. P., Ovaldsen, J. -E., Paraficz, D., Pavlenko, E., Piranomonte, S., Rossi, A., Rumyantsev, V., Salinas, R., Sergeev, A., Sharapov, D., Sollerman, J., Stecklum, B., Stella, L., Tagliaferri, G., Tanvir, N. R., Telting, J., Testa, V., Updike, Adria, Volnova, A., Watson, D., Wiersema, K., and Xu, D.

Abstract

Published in: Astrophysical Journal, Volume 720, 2010

Catalog

Books, media, physical & digital resources
See catalog results