Zobrazeno 1 - 10
of 273
pro vyhledávání: '"Krühler, T."'
Autor:
Michałowski, Michał J., Gentile, G., Kruhler, T., Kuncarayakti, H., Kamphuis, P., Hjorth, J., Berta, S., D'Elia, V., Elliott, J., Galbany, L., Greiner, J., Hunt, L. K., Koprowski, M. P., Floc'h, E. Le, Guelbenzu, A. Nicuesa, Palazzi, E., Rasmussen, J., Rossi, A., Savaglio, S., Postigo, A. de Ugarte, van der Werf, P., Vergani, S. D.
Publikováno v:
A&A 618, A104 (2018)
The potential similarity of the powering mechanisms of relativistic SNe and GRBs allowed us to make a prediction that relativistic SNe are born in environments similar to those of GRBs, that is, ones which are rich in atomic gas. Here we embark on te
Externí odkaz:
http://arxiv.org/abs/1808.00977
Autor:
Lopez-Coba, C., Sanchez, S. F., Cruz-Gonzalez, I., Binette, L., Galbany, L., Kruhler, T., Rodrıguez, L. F., Barrera-Ballesteros, J. K., Sanchez-Menguiano, L., Walcher, C. J., Aquino-Ortız, E., Anderson, J. P.
We report the detection of a highly collimated linear emission-line structure in the spiral galaxy NGC\,232 through the use of integral field spectroscopy data from the All-weather MUse Supernova Integral field Nearby Galaxies (AMUSING) survey. This
Externí odkaz:
http://arxiv.org/abs/1711.02785
Autor:
Smartt, S. J., Chen, T. -W., Jerkstrand, A., Coughlin, M., Kankare, E., Sim, S. A., Fraser, M., Inserra, C., Maguire, K., Chambers, K. C., Huber, M. E., Kruhler, T., Leloudas, G., Magee, M., Shingles, L. J., Smith, K. W., Young, D. R., Tonry, J., Kotak, R., Gal-Yam, A., Lyman, J. D., Homan, D. S., Agliozzo, C., Anderson, J. P., Ashall, C. R. Angus C., Barbarino, C., Bauer, F. E., Berton, M., Botticella, M. T., Bulla, M., Bulger, J., Cannizzaro, G., Cano, Z., Cartier, R., Cikota, A., Clark, P., De Cia, A., Della Valle, M., Denneau, L., Dennefeld, M., Dessart, L., Dimitriadis, G., Elias-Rosa, N., Firth, R. E., Flewelling, H., Flors, A., Franckowiak, A., Frohmaier, C., Galbany, L., Gonzalez-Gaitan, S., Greiner, J., Gromadzki, M., Guelbenzu, A. Nicuesa, Gutierrez, C. P., Hamanowicz, A., Hanlon, L., Harmanen, J., Heintz, K. E., Heinze, A., Hernandez, M. -S., Hodgkin, S. T., Hook, I. M., Izzo, L., James, P. A., Jonker, P. G., Kerzendorf, W. E., Klose, S., Kostrzewa-Rutkowska, Z., Kowalski, M., Kromer, M., Kuncarayakti, H., Lawrence, A., Lowe, T. B., Magnier, E. A., Manulis, I., Martin-Carrillo, A., Mattila, S., McBrien, O., Muller, A., Nordin, J., O'Neill, D., Onori, F., Palmerio, J. T., Pastorello, A., Patat, F., Pignata, G., Podsiadlowski, Ph., Pumo, M. L., Prentice, S. J., Rau, A., Razza, A., Rest, A., Reynolds, T., Roy, R., Ruiter, A. J., Rybicki, K. A., Salmon, L., Schady, P., Schultz, A. S. B., Schweyer, T., Seitenzahl, I. R., Smith, M., Sollerman, J., Stalder, B., Stubbs, C. W., Sullivan, M., Szegedi, H., Taddia, F., Taubenberger, S., Terreran, G., van Soelen, B., Vos, J., Wainscoat, R. J., Walton, N. A., Waters, C., Weiland, H., Willman, M., Wiseman, P., Wright, D. E., Wyrzykowski, L., Yaron, O.
Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to eject material rich in heavy radioactive isotopes that can power an el
Externí odkaz:
http://arxiv.org/abs/1710.05841
Autor:
Brown, G. C., Levan, A. J., Stanway, E. R., Kruhler, T., Tanvir, N. R., Davies, L. J. M., Fruchter, A., Cenko, S. B., Metzger, B. D.
We present late-time follow-up of the relativistic tidal disruption flare candidate Swift J1112.2-8238. We confirm the previously determined redshift of $z=0.8900\pm0.0005$ based on multiple emission line detections. {\em HST} imaging of the host gal
Externí odkaz:
http://arxiv.org/abs/1708.09668
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., Küpcü Yoldaş, A., Nardini, M., Nicuesa Guelbenzu, A. M., Olivares Estay, F., Rossi, A., Schady, P., Schweyer, T., Sudilovsky, V., Varela, K., Wiseman, P.
Publikováno v:
Astronomy & Astrophysics / Astronomie et Astrophysique; 2024, Vol. 691, p1-21, 21p
Autor:
Leloudas, G., Fraser, M., Stone, N. C., van Velzen, S., Jonker, P. G., Arcavi, I., Fremling, C., Maund, J. R., Smartt, S. J., Kruhler, T., Miller-Jones, J. C. A., Vreeswijk, P. M., Gal-Yam, A., Mazzali, P. A., De Cia, A., Howell, D. A., Inserra, C., Patat, F., Postigo, A. de Ugarte, Yaron, O., Ashall, C., Bar, I., Campbell, H., Chen, T. -W., Childress, M., Elias-Rosa, N., Harmanen, J., Hosseinzadeh, G., Johansson, J., Kangas, T., Kankare, E., Kim, S., Kuncarayakti, H., Lyman, J., Magee, M. R., Maguire, K., Malesani, D., Mattila, S., McCully, C. V., Nicholl, M., Prentice, S., Romero-Canizales, C., Schulze, S., Smith, K. W., Sollerman, J., Sullivan, M., Tucker, B. E., Valenti, S., Wheeler, J. C., Young, D. R.
Publikováno v:
Nat. Astron. 1, 0002 (2016)
When a star passes within the tidal radius of a supermassive black hole, it will be torn apart. For a star with the mass of the Sun ($M_\odot$) and a non-spinning black hole with a mass $<10^8 M_\odot$, the tidal radius lies outside the black hole ev
Externí odkaz:
http://arxiv.org/abs/1609.02927
Autor:
Piranomonte, S., Japelj, J., Vergani, S. D., Savaglio, S., Palazzi, E., Covino, S., Flores, H., Goldoni, P., Cupani, G., Kruhler, T., Mannucci, F., Onori, F., Rossi, A., D'Elia, V., Pian, E., D'Avanzo, P., Gomboc, A., Hammer, F., Randich, S., Fiore, F., Stella, L., Tagliaferri, G.
Long gamma-ray bursts (LGRBs) are associated with the death of massive stars. Their host galaxies therefore represent a unique class of objects tracing star formation across the observable Universe. Indeed, recently accumulated evidence shows that GR
Externí odkaz:
http://arxiv.org/abs/1506.07791
Autor:
Cano, Z., Postigo, A. de Ugarte, Perley, D., Kruhler, T., Margutti, R., Friis, M., Malesani, D., Jakobsson, P., Fynbo, J. P. U., Gorosabel, J., Hjorth, J., Sanchez-Ramirez, R., Schulze, S., Tanvir, N. R., Thone, C. C., Xu, D.
Publikováno v:
MNRAS, 452, 1535 (2015)
We present optical and near-infrared photometry of GRB~140606B ($z=0.384$), and optical photometry and spectroscopy of its associated supernova (SN). The results of our modelling indicate that the bolometric properties of the SN ($M_{\rm Ni} = 0.4\pm
Externí odkaz:
http://arxiv.org/abs/1505.03522
Autor:
van der Horst, A. J., Levan, A. J., Pooley, G. G., Wiersema, K., Kruhler, T., Perley, D. A., Starling, R. L. C., Curran, P. A., Tanvir, N. R., Wijers, R. A. M. J., Strom, R. G., Kouveliotou, C., Hartoog, O. E., Xu, D., Fynbo, J. P. U., Jakobsson, P.
Gamma-ray burst (GRB) 111215A was bright at X-ray and radio frequencies, but not detected in the optical or near-infrared (nIR) down to deep limits. We have observed the GRB afterglow with the Westerbork Synthesis Radio Telescope and Arcminute Microk
Externí odkaz:
http://arxiv.org/abs/1408.3923
Autor:
Cano, Z., Postigo, A. de Ugarte, Pozanenko, A., Butler, N., Thone, C. C., Guidorzi, C., Kruhler, T., Gorosabel, J., Jakobsson, P., Leloudas, G., Malesani, D., Hjorth, J., Melandri, A., Mundell, C., Wiersema, K., D'Avanzo, P., Schulze, S., Gomboc, A., Johansson, A., Zheng, W., Kann, D. A., Knust, F., Varela, K., Akerlof, C. W., Bloom, J., Burkhonov, O., Cooke, E., de Diego, J. A., Dhungana, G., Farina, C., Ferrante, F. V., Flewelling, H. A., Fox, O. D., Fynbo, J., Gehrels, N., Georgiev, L., Gonzalez, J. J., Greiner, J., Guver, T., Hartoog, O., Hatch, N., Jelinek, M, Kehoe, R., Klose, S., Klunko, E., Kopac, D., Kutyrev, A., Krugl, Y., Lee, W. H., Levan, A., Linkov, V., Matkin, A., Minikulov, N., Molotov, I., Prochaska, J. Xavier, Richer, M. G., Roman-Zuniga, C. G., Rumyantsev, V., Sanchez-Ramirez, R., Steele, I., Tanvir, N. R., Volnova, A., Watson, A. M., Xu, D., Yuan, F.
Publikováno v:
A&A 568, A19 (2014)
We present optical and near-infrared (NIR) photometry for three gamma-ray burst supernovae (GRB-SNe): GRB 120729A, GRB 130215A / SN 2013ez and GRB 130831A / SN 2013fu. In the case of GRB 130215A / SN 2013ez, we also present optical spectroscopy at t-
Externí odkaz:
http://arxiv.org/abs/1405.3114