Zobrazeno 1 - 10
of 434
pro vyhledávání: '"Kruehler, T"'
Autor:
Greiner, J., Krühler, T., Bolmer, J., Klose, S., Afonso, P. M. J., Elliott, J., Filgas, R., Graham, J. F., Kann, D. A., Knust, F., Yoldaş, A. Küpcü, Nardini, M., Guelbenzu, A. M. Nicuesa, Estay, F. Olivares, Rossi, A., Schady, P., Schweyer, T., Sudilovsky, V., Varela, K., Wiseman, P.
A dedicated gamma-ray burst (GRB) afterglow observing program was performed between 2007 and 2016 with GROND, a seven-channel optical and near-infrared imager at the 2.2m telescope of the Max-Planck Society at ESO/La Silla. In this first of a series
Externí odkaz:
http://arxiv.org/abs/2410.14441
Autor:
Klose, S., Schmidl, S., Kann, D. A., Guelbenzu, A. Nicuesa, Schulze, S., Greiner, J., Olivares, F., Kruehler, T., Schady, P., Afonso, P. M. J., Filgas, R., Fynbo, J. P. U., Perley, D. A., Rau, A., Rossi, A., Takats, K., Tanga, M., Updike, A. C., Varela, K.
Publikováno v:
A&A 622, A138 (2019)
Twenty years ago, GRB 980425/SN 1998bw revealed that long Gamma-Ray Bursts (GRBs) are physically associated with broad-lined type Ic supernovae. Since then more than 1000 long GRBs have been localized to high angular precision, but only in about 50 c
Externí odkaz:
http://arxiv.org/abs/1808.02710
Autor:
Postigo, A. de Ugarte, Thoene, C. C., Bensch, K., van der Horst, A. J., Kann, D. A., Cano, Z., Izzo, L., Goldoni, P., Martin, S., Filgas, R., Schady, P., Gorosabel, J., Bikmaev, I., Bremer, M., Burenin, R., Castro-Tirado, A. J., Covino, S., Fynbo, J. P. U., Garcia-Appadoo, D., de Gregorio-Monsalvo, I., Jelinek, M., Khamitov, I., Kamble, A., Kouveliotou, C., Kruehler, T., Melnikov, S., Nardini, M., Perley, D. A., Petitpas, G., Pooley, G., Rau, A., Rol, E., Sanchez-Ramirez, R., Starling, R. L. C., Tanvir, N. R., Wiersema, K., Wijers, R. A. M. J., Zafar, T.
Publikováno v:
A&A 620, A190 (2018)
Long gamma-ray bursts give us the chance to study both their extreme physics and the star-forming galaxies in which they form. GRB 100418A, at a z = 0.6239, had a bright optical and radio afterglow, and a luminous star-forming host galaxy. This allow
Externí odkaz:
http://arxiv.org/abs/1807.04281
Autor:
Tanvir, N. R., Fynbo, J. P. U., Postigo, A. de Ugarte, Japelj, J., Wiersema, K., Malesani, D., Perley, D. A., Levan, A. J., Selsing, J., Cenko, S. B., Kann, D. A., Milvang-Jensen, B., Berger, E., Cano, Z., Chornock, R., Covino, S., Cucchiara, A., D'Elia, V., Goldoni, P., Gomboc, A., Heintz, K. E., Hjorth, J., Izzo, L., Jakobsson, P., Kaper, L., Kruehler, T., Laskar, T., Myers, M., Piranomonte, S., Pugliese, G., Sanchez-Ramirez, R., Schulze, S., Sparre, M., Stanway, E. R., Tagliaferri, G., Thoene, C. C., Vergani, S., Vreeswijk, P. M., Wijers, R. A. M. J., Watson, D., Xu, D.
The part played by stars in the ionization of the intergalactic medium remains an open question. A key issue is the proportion of the stellar ionizing radiation that escapes the galaxies in which it is produced. Spectroscopy of gamma-ray burst afterg
Externí odkaz:
http://arxiv.org/abs/1805.07318
Autor:
Anderson, J. P., Dessart, L., Gutiérrez, C. P., Krühler, T., Galbany, L., Jerkstrand, A., Smartt, S. J., Contreras, C., Morrell, N., Phillips, M. M., Stritzinger, M. D., Hsiao, E. Y., González-Gaitán, S., Agliozzo, C., Castellón, S., Chambers, K. C., Chen, T. -W., Flewelling, H., Gonzalez, C., Hosseinzadeh, G., Huber, M., Fraser, M., Inserra, C., Kankare, E., Mattila, S., Magnier, E., Maguire, K., Lowe, T. B., Sollerman, J., Sullivan, M., Young, D. R., Valenti, S.
Red supergiants have been confirmed as the progenitor stars of the majority of hydrogen-rich type II supernovae. However, while such stars are observed with masses >25M$_\odot$, detections of >18M$_\odot$ progenitors remain elusive. Red supergiants a
Externí odkaz:
http://arxiv.org/abs/1805.04434
Autor:
Selsing, J., Malesani, D., Goldoni, P., Fynbo, J. P. U., Krühler, T., Antonelli, L. A., Arabsalmani, M., Bolmer, J., Cano, Z., Christensen, L., Covino, S., D'Avanzo, P., D'Elia, V., De Cia, A., Postigo, A. de Ugarte, Flores, H., Friis, M., Gomboc, A., Greiner, J., Groot, P., Hammer, F., Hartoog, O. E., Heintz, K. E., Hjorth, J., Jakobsson, P., Japelj, J., Kann, D. A., Kaper, L., Ledoux, C., Leloudas, G., Levan, A. J., Maiorano, E., Melandri, A., Milvang-Jensen, B., Palazzi, E., Palmerio, J. T., Perley, D. A., Pian, E., Piranomonte, S., Pugliese, G., Sánchez-Ramírez, R., Savaglio, S., Schady, P., Schulze, S., Sollerman, J., Sparre, M., Tagliaferri, G., Tanvir, N. R., Thöne, C. C., Vergani, S. D., Vreeswijk, P., Watson, D., Wiersema, K., Wijers, R., Xu, D., Zafar, T.
Publikováno v:
A&A 623, A92 (2019)
In this work we present spectra of all $\gamma$-ray burst (GRB) afterglows that have been promptly observed with the X-shooter spectrograph until 31-03-2017. In total, we obtained spectroscopic observations of 103 individual GRBs observed within 48 h
Externí odkaz:
http://arxiv.org/abs/1802.07727
Autor:
Greiner, J., Bolmer, J., Wieringa, M., van der Horst, A. J., Petry, D., Schulze, S., Knust, F., de Bruyn, G., Krühler, T., Wiseman, P., Klose, S., Delvaux, C., Graham, J. F., Kann, D. A., Moin, A., Nicuesa-Guelbenzu, A., Schady, P., Schmidl, S., Schweyer, T., Tanga, M., Tingay, S., van Eerten, H., Varela, K.
Publikováno v:
A&A 614, A29 (2018)
Deriving physical parameters from gamma-ray burst afterglow observations remains a challenge, even now, 20 years after the discovery of afterglows. The main reason for the lack of progress is that the peak of the synchrotron emission is in the sub-mm
Externí odkaz:
http://arxiv.org/abs/1802.01882
Autor:
Krühler, T., Fraser, M., Leloudas, G., Schulze, S., Stone, N. C., van Velzen, S., Amorin, R., Hjorth, J., Jonker, P. G., Kann, D. A., Kim, S., Kuncarayakti, H., Mehner, A., Guelbenzu, A. Nicuesa
Publikováno v:
A&A 610, A14 (2018)
The progenitors of astronomical transients are linked to a specific stellar population and galactic environment, and observing their host galaxies hence constrains the physical nature of the transient itself. Here, we use imaging from the Hubble Spac
Externí odkaz:
http://arxiv.org/abs/1710.01045
Autor:
Sánchez-Menguiano, L., Sánchez, S. F., Pérez, I., Ruiz-Lara, T., Galbany, L., Anderson, J. P., Krühler, T., Kuncarayakti, H., Lyman, J. D.
Publikováno v:
A&A 609, A119 (2018)
We characterise the oxygen abundance radial distribution of a sample of 102 spiral galaxies observed with VLT/MUSE using the O3N2 calibrator. The high spatial resolution of the data allows us to detect 14345 HII regions with the same image quality as
Externí odkaz:
http://arxiv.org/abs/1710.01188
Autor:
Tanga, M., Krühler, T., Schady, P., Klose, S., Graham, J. F., Greiner, J., Kann, D. A., Nardini, M.
Publikováno v:
A&A 615, A136 (2018)
The collapsar model has proved highly successful in explaining the properties of long gamma-ray bursts (GRBs), with the most direct confirmation being the detection of a supernova (SN) coincident with the majority of nearby long GRBs. Within this mod
Externí odkaz:
http://arxiv.org/abs/1708.06270