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Your search keyword '"Thöne, C."' showing total 37 results
Start Over Author "Thöne, C." Journal monthly notices of the royal astronomical society
37 results on '"Thöne, C."'

1. Correction to: Comparing emission- and absorption-based gas-phase metallicities in GRB host galaxies at z = 2−4 using JWST

Author

Schady, P, primary, Yates, R M, additional, Christensen, L, additional, De Cia, A, additional, Rossi, A, additional, D’Elia, V, additional, Heintz, K E, additional, Jakobsson, P, additional, Laskar, T, additional, Levan, A, additional, Salvaterra, R, additional, Starling, R L C, additional, Tanvir, N R, additional, Thöne, C C, additional, Vergani, S, additional, Wiersema, K, additional, Arabsalmani, M, additional, Chen, H -W, additional, De Pasquale, M, additional, Fruchter, A, additional, Fynbo, J P U, additional, García-Benito, R, additional, Gompertz, B, additional, Hartmann, D, additional, Kouveliotou, C, additional, Milvang-Jensen, B, additional, Palazzi, E, additional, Perley, D A, additional, Piranomonte, S, additional, Pugliese, G, additional, Savaglio, S, additional, Sbarufatti, B, additional, Schulze, S, additional, Tagliaferri, G, additional, de Ugarte Postigo, A, additional, Watson, D, additional, and Wiseman, P, additional

Published
2024
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2. Multi-band analyses of the bright GRB 230812B and the associated SN2023pel

Author

Hussenot-Desenonges, T, primary, Wouters, T, additional, Guessoum, N, additional, Abdi, I, additional, Abulwfa, A, additional, Adami, C, additional, Fernández, J F Agüí, additional, Ahumada, T, additional, Aivazyan, V, additional, Akl, D, additional, Anand, S, additional, Andrade, C M, additional, Antier, S, additional, Ata, S A, additional, D’Avanzo, P, additional, Azzam, Y A, additional, Baransky, A, additional, Basa, S, additional, Blazek, M, additional, Bendjoya, P, additional, Beradze, S, additional, Boumis, P, additional, Bremer, M, additional, Brivio, R, additional, Buat, V, additional, Bulla, M, additional, Burkhonov, O, additional, Burns, E, additional, Cenko, S B, additional, Coughlin, M W, additional, Corradi, W, additional, Daigne, F, additional, Dietrich, T, additional, Dornic, D, additional, Ducoin, J-G, additional, Duverne, P-A, additional, Elhosseiny, E G, additional, Elnagahy, F I, additional, El-Sadek, M A, additional, Ferro, M, additional, Le Floc’h, E, additional, Freeberg, M, additional, Fynbo, J P U, additional, Götz, D, additional, Gurbanov, E, additional, Hamed, G M, additional, Hasanov, E, additional, Healy, B F, additional, Heintz, K E, additional, Hello, P, additional, Inasaridze, R, additional, Iskandar, A, additional, Ismailov, N, additional, Izzo, L, additional, Jhawar, S, additional, du Laz, T Jegou, additional, Kamel, T M, additional, Karpov, S, additional, Klotz, A, additional, Koulouridis, E, additional, Kuin, N P, additional, Kochiashvili, N, additional, Leonini, S, additional, Lu, K-X, additional, Malesani, D B, additional, Mašek, M, additional, Mao, J, additional, Melandri, A, additional, Mihov, B M, additional, Natsvlishvili, R, additional, Navarete, F, additional, Nedora, V, additional, Nicolas, J, additional, Odeh, M, additional, Palmerio, J, additional, Pang, P T H, additional, De Pasquale, M, additional, Peng, H W, additional, Pormente, S, additional, Peloton, J, additional, Pradier, T, additional, Pyshna, O, additional, Rajabov, Y, additional, Rakotondrainibe, N A, additional, Rivet, J-P, additional, Rousselot, L, additional, Saccardi, A, additional, Sasaki, N, additional, Schneider, B, additional, Serrau, M, additional, Shokry, A, additional, Slavcheva-Mihova, L, additional, Simon, A, additional, Sokoliuk, O, additional, Srinivasaragavan, G, additional, Strausbaugh, R, additional, Takey, A, additional, Tanvir, N R, additional, Thöne, C C, additional, Tillayev, Y, additional, Melo, I Tosta e, additional, Turpin, D, additional, de Ugarte Postigo, A, additional, Vasylenko, V, additional, Vergani, S D, additional, Vidadi, Z, additional, Xu, D, additional, Wang, L T, additional, Wang, X F, additional, Winters, J M, additional, Zhang, X-L, additional, and Zhu, Z, additional

Published
2024
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3. Comparing emission- and absorption-based gas-phase metallicities in GRB host galaxies at z = 2−4 using JWST

Author

Schady, P, primary, Yates, R M, additional, Christensen, L, additional, De Cia, A, additional, Rossi, A, additional, D’Elia, V, additional, Heintz, K E, additional, Jakobsson, P, additional, Laskar, T, additional, Levan, A, additional, Salvaterra, R, additional, Starling, R L C, additional, Tanvir, N R, additional, Thöne, C C, additional, Vergani, S, additional, Wiersema, K, additional, Arabsalmani, M, additional, Chen, H -W, additional, De Pasquale, M, additional, Fruchter, A, additional, Fynbo, J P U, additional, García-Benito, R, additional, Gompertz, B, additional, Hartmann, D, additional, Kouveliotou, C, additional, Milvang-Jensen, B, additional, Palazzi, E, additional, Perley, D A, additional, Piranomonte, S, additional, Pugliese, G, additional, Savaglio, S, additional, Sbarufatti, B, additional, Schulze, S, additional, Tagliaferri, G, additional, Postigo, A de Ugarte, additional, Watson, D, additional, and Wiseman, P, additional

Published
2024
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4. GRB 160410A: The first chemical study of the interstellar medium of a short GRB

Author

Agüí Fernández, J F, primary, Thöne, C C, additional, Kann, D A, additional, de Ugarte Postigo, A, additional, Selsing, J, additional, Schady, P, additional, Yates, R M, additional, Greiner, J, additional, Oates, S R, additional, Malesani, D B, additional, Xu, D, additional, Klotz, A, additional, Campana, S, additional, Rossi, A, additional, Perley, D A, additional, Blažek, M, additional, D’Avanzo, P, additional, Giunta, A, additional, Hartmann, D, additional, Heintz, K E, additional, Jakobsson, P, additional, Kirkpatrick IV, C C, additional, Kouveliotou, C, additional, Melandri, A, additional, Pugliese, G, additional, Salvaterra, R, additional, Starling, R L C, additional, Tanvir, N R, additional, Vergani, S D, additional, and Wiersema, K, additional

Published
2023
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5. Multiwavelength analysis of short GRB 201221D and its comparison with other high & low redshift short GRBs.

Author

Dimple, Misra, K, Kann, D A, Arun, K G, Ghosh, A, Gupta, R, Resmi, L, Agüí Fernández, J F, Thöne, C C, de Ugarte Postigo, A, Pandey, S B, and Yadav, L

Subjects
SPECTRAL energy distribution, GAMMA ray bursts, REDSHIFT
Abstract

We present a detailed analysis of short GRB 201221D lying at redshift |$\mathit{ z}$|  = 1.045. We analyse the high-energy data of the burst and compare it with the sample of short gamma-ray bursts (SGRBs). The prompt emission characteristics are typical of those seen in the case of other SGRBs except for the peak energy (E p), which lies at the softer end (generally observed in the case of long bursts). We estimate the host galaxy properties by utilizing the Python -based software Prospector to fit the spectral energy distribution of the host. The burst lies at a high redshift relative to the SGRB sample with a median redshift of |$\mathit{ z}$|  = 0.47. We compare the burst characteristics with other SGRBs with known redshifts along with GRB 200826A (SGRB originated from a collapsar). A careful examination of the characteristics of SGRBs at different redshifts reveals that some of the SGRBs lying at high redshifts have properties similar to long GRBs indicating they might have originated from collapsars. Further study of these GRBs can help to explore the broad picture of progenitor systems of SGRBs. [ABSTRACT FROM AUTHOR]

Published
2022
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6. Low frequency view of GRB 190114C reveals time varying shock micro-physics

Author

Misra, K, primary, Resmi, L, additional, Kann, D A, additional, Marongiu, M, additional, Moin, A, additional, Klose, S, additional, Bernardi, G, additional, Postigo, A de Ugarte, additional, Jaiswal, V K, additional, Schulze, S, additional, Perley, D A, additional, Ghosh, A, additional, Dimple, Dimple, additional, Kumar, H, additional, Gupta, R, additional, Michałowski, M J, additional, Martín, S, additional, Cockeram, A, additional, Cherukuri, S V, additional, Bhalerao, V, additional, Anderson, G E, additional, Pandey, S B, additional, Anupama, G C, additional, Thöne, C C, additional, Barway, S, additional, Wieringa, M H, additional, Fynbo, J P U, additional, and Habeeb, N, additional

Published
2021
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7. GRANDMA observations of advanced LIGO’s and advanced Virgo’s third observational campaign

Author

Antier, S, primary, Agayeva, S, additional, Almualla, M, additional, Awiphan, S, additional, Baransky, A, additional, Barynova, K, additional, Beradze, S, additional, Blažek, M, additional, Boër, M, additional, Burkhonov, O, additional, Christensen, N, additional, Coleiro, A, additional, Corre, D, additional, Coughlin, M W, additional, Crisp, H, additional, Dietrich, T, additional, Ducoin, J-G, additional, Duverne, P-A, additional, Marchal-Duval, G, additional, Gendre, B, additional, Gokuldass, P, additional, Eggenstein, H B, additional, Eymar, L, additional, Hello, P, additional, Howell, E J, additional, Ismailov, N, additional, Kann, D A, additional, Karpov, S, additional, Klotz, A, additional, Kochiashvili, N, additional, Lachaud, C, additional, Leroy, N, additional, Lin, W L, additional, Li, W X, additional, Mašek, M, additional, Mo, J, additional, Menard, R, additional, Morris, D, additional, Noysena, K, additional, Orange, N B, additional, Prouza, M, additional, Rattanamala, R, additional, Sadibekova, T, additional, Saint-Gelais, D, additional, Serrau, M, additional, Simon, A, additional, Stachie, C, additional, Thöne, C C, additional, Tillayev, Y, additional, Turpin, D, additional, Postigo, A de Ugarte, additional, Vasylenko, V, additional, Vidadi, Z, additional, Was, M, additional, Wang, X F, additional, Zhang, J J, additional, Zhang, T M, additional, and Zhang, X H, additional

Published
2020
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8. The first six months of the Advanced LIGO’s and Advanced Virgo’s third observing run with GRANDMA

Author

Antier, S, primary, Agayeva, S, primary, Aivazyan, V, primary, Alishov, S, primary, Arbouch, E, primary, Baransky, A, primary, Barynova, K, primary, Bai, J M, primary, Basa, S, primary, Beradze, S, primary, Bertin, E, primary, Berthier, J, primary, Blažek, M, primary, Boër, M, primary, Burkhonov, O, primary, Burrell, A, primary, Cailleau, A, primary, Chabert, B, primary, Chen, J C, primary, Christensen, N, primary, Coleiro, A, primary, Cordier, B, primary, Corre, D, primary, Coughlin, M W, primary, Coward, D, primary, Crisp, H, primary, Delattre, C, primary, Dietrich, T, primary, Ducoin, J-G, primary, Duverne, P-A, primary, Marchal-Duval, G, primary, Gendre, B, primary, Eymar, L, primary, Fock-Hang, P, primary, Han, X, primary, Hello, P, primary, Howell, E J, primary, Inasaridze, R, primary, Ismailov, N, primary, Kann, D A, primary, Kapanadze, G, primary, Klotz, A, primary, Kochiashvili, N, primary, Lachaud, C, primary, Leroy, N, primary, Le Van Su, A, primary, Lin, W L, primary, Li, W X, primary, Lognone, P, primary, Marron, R, primary, Mo, J, primary, Moore, J, primary, Natsvlishvili, R, primary, Noysena, K, primary, Perrigault, S, primary, Peyrot, A, primary, Samadov, D, primary, Sadibekova, T, primary, Simon, A, primary, Stachie, C, primary, Teng, J P, primary, Thierry, P, primary, Thöne, C C, primary, Tillayev, Y, primary, Turpin, D, primary, de Ugarte Postigo, A, primary, Vachier, F, primary, Vardosanidze, M, primary, Vasylenko, V, primary, Vidadi, Z, primary, Wang, X F, primary, Wang, C J, primary, Wei, J, primary, Yan, S Y, primary, Zhang, J C, primary, Zhang, J J, primary, and Zhang, X H, primary

Published
2019
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9. GRB 171010A/SN 2017htp: a GRB-SN at z = 0.33

Author

Melandri, A, primary, Malesani, D B, additional, Izzo, L, additional, Japelj, J, additional, Vergani, S D, additional, Schady, P, additional, Sagués Carracedo, A, additional, de Ugarte Postigo, A, additional, Anderson, J P, additional, Barbarino, C, additional, Bolmer, J, additional, Breeveld, A, additional, Calissendorff, P, additional, Campana, S, additional, Cano, Z, additional, Carini, R, additional, Covino, S, additional, D’Avanzo, P, additional, D’Elia, V, additional, della Valle, M, additional, De Pasquale, M, additional, Fynbo, J P U, additional, Gromadzki, M, additional, Hammer, F, additional, Hartmann, D H, additional, Heintz, K E, additional, Inserra, C, additional, Jakobsson, P, additional, Kann, D A, additional, Kotilainen, J, additional, Maguire, K, additional, Masetti, N, additional, Nicholl, M, additional, Olivares E, F, additional, Pugliese, G, additional, Rossi, A, additional, Salvaterra, R, additional, Sollerman, J, additional, Stone, M B, additional, Tagliaferri, G, additional, Tomasella, L, additional, Thöne, C C, additional, Xu, D, additional, and Young, D R, additional

Published
2019
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10. The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies, and redshifts with 12 optical filters

Author

Mendes de Oliveira, C, primary, Ribeiro, T, additional, Schoenell, W, additional, Kanaan, A, additional, Overzier, R A, additional, Molino, A, additional, Sampedro, L, additional, Coelho, P, additional, Barbosa, C E, additional, Cortesi, A, additional, Costa-Duarte, M V, additional, Herpich, F R, additional, Hernandez-Jimenez, J A, additional, Placco, V M, additional, Xavier, H S, additional, Abramo, L R, additional, Saito, R K, additional, Chies-Santos, A L, additional, Ederoclite, A, additional, Lopes de Oliveira, R, additional, Gonçalves, D R, additional, Akras, S, additional, Almeida, L A, additional, Almeida-Fernandes, F, additional, Beers, T C, additional, Bonatto, C, additional, Bonoli, S, additional, Cypriano, E S, additional, Vinicius-Lima, E, additional, de Souza, R S, additional, Fabiano de Souza, G, additional, Ferrari, F, additional, Gonçalves, T S, additional, Gonzalez, A H, additional, Gutiérrez-Soto, L A, additional, Hartmann, E A, additional, Jaffe, Y, additional, Kerber, L O, additional, Lima-Dias, C, additional, Lopes, P A A, additional, Menendez-Delmestre, K, additional, Nakazono, L M I, additional, Novais, P M, additional, Ortega-Minakata, R A, additional, Pereira, E S, additional, Perottoni, H D, additional, Queiroz, C, additional, Reis, R R R, additional, Santos, W A, additional, Santos-Silva, T, additional, Santucci, R M, additional, Barbosa, C L, additional, Siffert, Beatriz B, additional, Sodré, L, additional, Torres-Flores, S, additional, Westera, P, additional, Whitten, D D, additional, Alcaniz, J S, additional, Alonso-García, Javier, additional, Alencar, S, additional, Alvarez-Candal, A, additional, Amram, P, additional, Azanha, L, additional, Barbá, R H, additional, Bernardinelli, P H, additional, Borges Fernandes, M, additional, Branco, V, additional, Brito-Silva, D, additional, Buzzo, M L, additional, Caffer, J, additional, Campillay, A, additional, Cano, Z, additional, Carvano, J M, additional, Castejon, M, additional, Cid Fernandes, R, additional, Dantas, M L L, additional, Daflon, S, additional, Damke, G, additional, de la Reza, R, additional, de Melo de Azevedo, L J, additional, De Paula, D F, additional, Diem, K G, additional, Donnerstein, R, additional, Dors, O L, additional, Dupke, R, additional, Eikenberry, S, additional, Escudero, Carlos G, additional, Faifer, Favio R, additional, Farías, H, additional, Fernandes, B, additional, Fernandes, C, additional, Fontes, S, additional, Galarza, A, additional, Hirata, N S T, additional, Katena, L, additional, Gregorio-Hetem, J, additional, Hernández-Fernández, J D, additional, Izzo, L, additional, Jaque Arancibia, M, additional, Jatenco-Pereira, V, additional, Jiménez-Teja, Y, additional, Kann, D A, additional, Krabbe, A C, additional, Labayru, C, additional, Lazzaro, D, additional, Lima Neto, G B, additional, Lopes, Amanda R, additional, Magalhães, R, additional, Makler, M, additional, de Menezes, R, additional, Miralda-Escudé, J, additional, Monteiro-Oliveira, R, additional, Montero-Dorta, A D, additional, Muñoz-Elgueta, N, additional, Nemmen, R S, additional, Nilo Castellón, J L, additional, Oliveira, A S, additional, Ortíz, D, additional, Pattaro, E, additional, Pereira, C B, additional, Quint, B, additional, Riguccini, L, additional, Rocha Pinto, H J, additional, Rodrigues, I, additional, Roig, F, additional, Rossi, S, additional, Saha, Kanak, additional, Santos, R, additional, Schnorr Müller, A, additional, Sesto, Leandro A, additional, Silva, R, additional, Smith Castelli, Analia V, additional, Teixeira, R, additional, Telles, E, additional, Thom de Souza, R C, additional, Thöne, C, additional, Trevisan, M, additional, de Ugarte Postigo, A, additional, Urrutia-Viscarra, F, additional, Veiga, C H, additional, Vika, M, additional, Vitorelli, A Z, additional, Werle, A, additional, Werner, S V, additional, and Zaritsky, D, additional

Published
2019
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11. The fraction of ionizing radiation from massive stars that escapes to the intergalactic medium

Author

Tanvir, N R, primary, Fynbo, J P U, additional, de Ugarte Postigo, A, additional, Japelj, J, additional, Wiersema, K, additional, Malesani, D, additional, Perley, D A, additional, Levan, A J, additional, Selsing, J, additional, Cenko, S B, additional, Kann, D A, additional, Milvang-Jensen, B, additional, Berger, E, additional, Cano, Z, additional, Chornock, R, additional, Covino, S, additional, Cucchiara, A, additional, D’Elia, V, additional, Gargiulo, A, additional, Goldoni, P, additional, Gomboc, A, additional, Heintz, K E, additional, Hjorth, J, additional, Izzo, L, additional, Jakobsson, P, additional, Kaper, L, additional, Krühler, T, additional, Laskar, T, additional, Myers, M, additional, Piranomonte, S, additional, Pugliese, G, additional, Rossi, A, additional, Sánchez-Ramírez, R, additional, Schulze, S, additional, Sparre, M, additional, Stanway, E R, additional, Tagliaferri, G, additional, Thöne, C C, additional, Vergani, S, additional, Vreeswijk, P M, additional, Wijers, R A M J, additional, Watson, D, additional, and Xu, D, additional

Published
2018
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12. Highly ionized metals as probes of the circumburst gas in the natal regions of gamma-ray bursts

Author

Heintz, K E, primary, Watson, D, additional, Jakobsson, P, additional, Fynbo, J P U, additional, Bolmer, J, additional, Arabsalmani, M, additional, Cano, Z, additional, Covino, S, additional, D’Elia, V, additional, Gomboc, A, additional, Japelj, J, additional, Kaper, L, additional, Krogager, J-K, additional, Pugliese, G, additional, Sánchez-Ramírez, R, additional, Selsing, J, additional, Sparre, M, additional, Tanvir, N R, additional, Thöne, C C, additional, de Ugarte Postigo, A, additional, and Vergani, S D, additional

Published
2018
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14. The luminous, massive and solar metallicity galaxy hosting the Swift γ-ray burst GRB 160804A at z = 0.737

Author

Heintz, K E, primary, Malesani, D, additional, Wiersema, K, additional, Jakobsson, P, additional, Fynbo, J P U, additional, Savaglio, S, additional, Cano, Z, additional, Covino, S, additional, D'Elia, V, additional, Gomboc, A, additional, Hammer, F, additional, Kaper, L, additional, Milvang-Jensen, B, additional, Møller, P, additional, Piranomonte, S, additional, Selsing, J, additional, Rhodin, N H P, additional, Tanvir, N R, additional, Thöne, C C, additional, de Ugarte Postigo, A, additional, Vergani, S D, additional, and Watson, D, additional

Published
2017
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15. Cosmic evolution and metal aversion in superluminous supernova host galaxies

Author

Schulze, S., primary, Krühler, T., additional, Leloudas, G., additional, Gorosabel, J., additional, Mehner, A., additional, Buchner, J., additional, Kim, S., additional, Ibar, E., additional, Amorín, R., additional, Herrero-Illana, R., additional, Anderson, J. P., additional, Bauer, F. E., additional, Christensen, L., additional, de Pasquale, M., additional, de Ugarte Postigo, A., additional, Gallazzi, A., additional, Hjorth, J., additional, Morrell, N., additional, Malesani, D., additional, Sparre, M., additional, Stalder, B., additional, Stark, A. A., additional, Thöne, C. C., additional, and Wheeler, J. C., additional

Published
2017
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16. The MUSE view of the host galaxy of GRB 100316D

Author

Izzo, L., primary, Thöne, C. C., additional, Schulze, S., additional, Mehner, A., additional, Flores, H., additional, Cano, Z., additional, de Ugarte Postigo, A., additional, Kann, D. A., additional, Amorín, R., additional, Anderson, J. P., additional, Bauer, F. E., additional, Bensch, K., additional, Christensen, L., additional, Covino, S., additional, Della Valle, M., additional, Fynbo, J. P. U., additional, Jakobsson, P., additional, Klose, S., additional, Kuncarayakti, H., additional, Leloudas, G., additional, Milvang-Jensen, B., additional, Møller, P., additional, Puech, M., additional, Rossi, A., additional, Sánchez-Ramírez, R., additional, and Vergani, S. D., additional

Published
2017
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17. GRB 110715A: the peculiar multiwavelength evolution of the first afterglow detected by ALMA

Author

Sánchez-Ramírez, R., primary, Hancock, P. J., additional, Jóhannesson, G., additional, Murphy, Tara, additional, de Ugarte Postigo, A., additional, Gorosabel, J., additional, Kann, D. A., additional, Krühler, T., additional, Oates, S. R., additional, Japelj, J., additional, Thöne, C. C., additional, Lundgren, A., additional, Perley, D. A., additional, Malesani, D., additional, de Gregorio Monsalvo, I., additional, Castro-Tirado, A. J., additional, D'Elia, V., additional, Fynbo, J. P. U., additional, Garcia-Appadoo, D., additional, Goldoni, P., additional, Greiner, J., additional, Hu, Y.-D., additional, Jelínek, M., additional, Jeong, S., additional, Kamble, A., additional, Klose, S., additional, Kuin, N. P. M., additional, Llorente, A., additional, Martín, S., additional, Nicuesa Guelbenzu, A., additional, Rossi, A., additional, Schady, P., additional, Sparre, M., additional, Sudilovsky, V., additional, Tello, J. C., additional, Updike, A., additional, Wiersema, K., additional, and Zhang, B.-B., additional

Published
2016
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18. The optical identification of events with poorly defined locations: the case of the Fermi GBM GRB 140801A

Author

Lipunov, V. M., primary, Gorosabel, J., additional, Pruzhinskaya, M. V., additional, Postigo, A. de Ugarte, additional, Pelassa, V., additional, Tsvetkova, A. E., additional, Sokolov, I. V., additional, Kann, D. A., additional, Xu, Dong, additional, Gorbovskoy, E. S., additional, Krushinski, V. V., additional, Kornilov, V. G., additional, Balanutsa, P. V., additional, Boronina, S. V., additional, Budnev, N. M., additional, Cano, Z., additional, Castro-Tirado, A. J., additional, Chazov, V. V., additional, Connaughton, V., additional, Delvaux, C., additional, Frederiks, D. D., additional, Fynbo, J. F. U., additional, Gabovich, A. V., additional, Goldstein, A., additional, Greiner, J., additional, Gress, O. A., additional, Ivanov, K. I., additional, Jakobsson, P., additional, Klose, S., additional, Knust, F., additional, Komarova, V. N., additional, Konstantinov, E., additional, Krylov, A. V., additional, Kuvshinov, D. A., additional, Kuznetsov, A. S., additional, Lipunova, G.V., additional, Moskvitin, A. S., additional, Pal'shin, V. D., additional, Pandey, S. B., additional, Poleshchuk, V. A., additional, Schmidl, S., additional, Sergienko, Yu. P., additional, Sinyakov, E. V., additional, Schulze, S., additional, Sokolov, V. V., additional, Sokolova, T. N., additional, Sparre, M., additional, Thöne, C. C., additional, Tlatov, A. G., additional, Tyurina, N. V., additional, Ulanov, M. V., additional, Yazev, S. A., additional, and Yurkov, V. V., additional

Published
2015
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19. GRB 140606B/iPTF14bfu: detection of shock-breakout emission from a cosmological γ-ray burst?

Author

Cano, Zach, primary, de Ugarte Postigo, A., additional, Perley, D., additional, Krühler, T., additional, Margutti, R., additional, Friis, M., additional, Malesani, D., additional, Jakobsson, P., additional, Fynbo, J. P. U., additional, Gorosabel, J., additional, Hjorth, J., additional, Sánchez-Ramírez, R., additional, Schulze, S., additional, Tanvir, N. R., additional, Thöne, C. C., additional, and Xu, D., additional

Published
2015
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20. The warm, the excited, and the molecular gas: GRB 121024A shining through its star-forming galaxy★

Author

Friis, M., primary, De Cia, A., additional, Krühler, T., additional, Fynbo, J. P. U., additional, Ledoux, C., additional, Vreeswijk, P. M., additional, Watson, D. J., additional, Malesani, D., additional, Gorosabel, J., additional, Starling, R. L. C., additional, Jakobsson, P., additional, Varela, K., additional, Wiersema, K., additional, Drachmann, A. P., additional, Trotter, A., additional, Thöne, C. C., additional, de Ugarte Postigo, A., additional, D'Elia, V., additional, Elliott, J., additional, Maturi, M., additional, Goldoni, P., additional, Greiner, J., additional, Haislip, J., additional, Kaper, L., additional, Knust, F., additional, LaCluyze, A., additional, Milvang-Jensen, B., additional, Reichart, D., additional, Schulze, S., additional, Sudilovsky, V., additional, Tanvir, N., additional, and Vergani, S. D., additional

Published
2015
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21. Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies

Author

Leloudas, G., primary, Schulze, S., additional, Krühler, T., additional, Gorosabel, J., additional, Christensen, L., additional, Mehner, A., additional, de Ugarte Postigo, A., additional, Amorín, R., additional, Thöne, C. C., additional, Anderson, J. P., additional, Bauer, F. E., additional, Gallazzi, A., additional, Hełminiak, K. G., additional, Hjorth, J., additional, Ibar, E., additional, Malesani, D., additional, Morrell, N., additional, Vinko, J., additional, and Wheeler, J. C., additional

Published
2015
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22. The luminous, massive and solar metallicity galaxy hosting the Swift γ-ray burst GRB160804A at ɀ = 0.737.

Author

Heintz, K. E., Malesani, D., Wiersema, K., Jakobsson, P., Fynbo, J. P. U., Savaglio, S., Cano, Z., Covino, S., D'Elia, V., Gomboc, A., Hammer, F., Kaper, L., Milvang-Jensen, B., Møller, P., Piranomonte, S., Selsing, J., Rhodin, N. H. P., Tanvir, N. R., Thöne, C. C., and de Ugarte Postigo, A.

Subjects
GAMMA ray bursts, GAMMA ray astronomy, X-ray bursts, GALAXIES, STAR formation, AFTERGLOW (Physics)
Abstract

We here present the spectroscopic follow-up observations with VLT/X-shooter of the Swift long-duration gamma-ray burst GRB160804A at ɀ=0.737. Typically, GRBs are found in lowmass, metal-poor galaxies that constitute the sub-luminous population of star-forming galaxies. For the host galaxy of the GRB presented here, we derive a stellar mass of log (M*/M⨀) = 9.80 ± 0.07, a roughly solar metallicity (12 + log (O/H) = 8.74 ± 0.12) based on emission line diagnostics, and an infrared luminosity of M3.6/(1 + ɀ) = -21.94 mag, but find it to be dust-poor (E(B -- V) < 0.05 mag). This establishes the galaxy hosting GRB160804A as one of the most luminous, massive and metal-rich GRB hosts at ɀ < 1.5. Furthermore, the gasphase metallicity is found to be representative of the physical conditions of the gas close to the explosion site of the burst. The high metallicity of the host galaxy is also observed in absorption, where we detect several strong Fe II transitions as well as MgII and MgI. Although host galaxy absorption features are common in GRB afterglow spectra, we detect absorption from strong metal lines directly in the host continuum (at a time when the afterglow was contributing to <15 per cent). Finally, we discuss the possibility that the geometry and state of the absorbing and emitting gas are indicative of a galactic scale outflow expelled at the final stage of two merging galaxies. [ABSTRACT FROM AUTHOR]

Published
2018
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24. The optical counterpart of the bright X-ray transient Swift J1745−26

Author

Muñoz-Darias, T., primary, de Ugarte Postigo, A., additional, Russell, D. M., additional, Guziy, S., additional, Gorosabel, J., additional, Casares, J., additional, Armas Padilla, M., additional, Charles, P. A., additional, Fender, R. P., additional, Belloni, T. M., additional, Lewis, F., additional, Motta, S., additional, Castro-Tirado, A., additional, Mundell, C. G., additional, Sánchez-Ramírez, R., additional, and Thöne, C. C., additional

Published
2013
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25. GRB 110715A: the peculiar multiwavelength evolution of the first afterglow detected by ALMA.

Author

Sánchez-Ramírez, R., Hancock, P. J., Jóhannesson, G., Murphy, Tara, de Ugarte Postigo, A., Gorosabel, J., Kann, D. A., Krühler, T., Oates, S. R., Japelj, J., Thöne, C. C., Lundgren, A., Perley, D. A., Malesani, D., de Gregorio Monsalvo, I., Castro-Tirado, A. J., D'Elia, V., Fynbo, J. P. U., Garcia-Appadoo, D., and Goldoni, P.

Subjects
WAVELENGTHS, NEAR infrared spectroscopy, X-ray astronomy, RADIO frequency, IONIZATION (Atomic physics)
Abstract

We present the extensive follow-up campaign on the afterglowof GRB 110715A at 17 different wavelengths, from X-ray to radio bands, starting 81 s after the burst and extending up to 74 d later. We performed for the first time aGRBafterglowobservationwith theALMAobservatory. We find that the afterglow of GRB 110715A is very bright at optical and radio wavelengths. We use the optical and near-infrared spectroscopy to provide further information about the progenitor's environment and its host galaxy. The spectrum shows weak absorption features at a redshift z = 0.8225, which reveal a host-galaxy environment with low ionization, column density, and dynamical activity. Late deep imaging shows a very faint galaxy, consistent with the spectroscopic results. The broad-band afterglow emission is modelled with synchrotron radiation using a numerical algorithm and we determine the best-fitting parameters using Bayesian inference in order to constrain the physical parameters of the jet and the medium in which the relativistic shock propagates. We fitted our data with a variety of models, including different density profiles and energy injections. Although the general behaviour can be roughly described by thesemodels, none of them are able to fully explain all data points simultaneously. GRB 110715A shows the complexity of reproducing extensive multiwavelength broad-band afterglow observations, and the need of good sampling in wavelength and time and more complex models to accurately constrain the physics of GRB afterglows. [ABSTRACT FROM AUTHOR]

Published
2017
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26. GRB 100219A with X-shooter – abundances in a galaxy at z =4.7

Author

Thöne, C. C., primary, Fynbo, J. P. U., additional, Goldoni, P., additional, de Ugarte, A. Postigo, additional, Campana, S., additional, Vergani, S. D., additional, Covino, S., additional, Krühler, T., additional, Kaper, L., additional, Tanvir, N., additional, Zafar, T., additional, D’Elia, V., additional, Gorosabel, J., additional, Greiner, J., additional, Groot, P., additional, Hammer, F., additional, Jakobsson, P., additional, Klose, S., additional, Levan, A. J., additional, Milvang-Jensen, B., additional, Nicuesa, A. Guelbenzu, additional, Palazzi, E., additional, Piranomonte, S., additional, Tagliaferri, G., additional, Watson, D., additional, Wiersema, K., additional, and Wijers, R. A. M. J., additional

Published
2012
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27. OGLE-2008-BLG-510: first automated real-time detection of a weak microlensing anomaly - brown dwarf or stellar binary?★

Author

Bozza, V., primary, Dominik, M., additional, Rattenbury, N. J., additional, Jørgensen, U. G., additional, Tsapras, Y., additional, Bramich, D. M., additional, Udalski, A., additional, Bond, I. A., additional, Liebig, C., additional, Cassan, A., additional, Fouqué, P., additional, Fukui, A., additional, Hundertmark, M., additional, Shin, I.-G., additional, Lee, S. H., additional, Choi, J.-Y., additional, Park, S.-Y., additional, Gould, A., additional, Allan, A., additional, Mao, S., additional, Wyrzykowski, Ł., additional, Street, R. A., additional, Buckley, D., additional, Nagayama, T., additional, Mathiasen, M., additional, Hinse, T. C., additional, Novati, S. Calchi, additional, Harpsøe, K., additional, Mancini, L., additional, Scarpetta, G., additional, Anguita, T., additional, Burgdorf, M. J., additional, Horne, K., additional, Hornstrup, A., additional, Kains, N., additional, Kerins, E., additional, Kjaergaard, P., additional, Masi, G., additional, Rahvar, S., additional, Ricci, D., additional, Snodgrass, C., additional, Southworth, J., additional, Steele, I. A., additional, Surdej, J., additional, Thöne, C. C., additional, Wambsganss, J., additional, Zub, M., additional, Albrow, M. D., additional, Batista, V., additional, Beaulieu, J.-P., additional, Bennett, D. P., additional, Caldwell, J. A. R., additional, Cole, A. A., additional, Cook, K. H., additional, Coutures, C., additional, Dieters, S., additional, Prester, D. Dominis, additional, Donatowicz, J., additional, Greenhill, J., additional, Kane, S. R., additional, Kubas, D., additional, Marquette, J.-B., additional, Martin, R., additional, Menzies, J., additional, Pollard, K. R., additional, Sahu, K. C., additional, Williams, A., additional, Szymański, M. K., additional, Kubiak, M., additional, Pietrzyński, G., additional, Soszyński, I., additional, Poleski, R., additional, Ulaczyk, K., additional, DePoy, D. L., additional, Dong, Subo, additional, Han, C., additional, Janczak, J., additional, Lee, C.-U., additional, Pogge, R. W., additional, Abe, F., additional, Furusawa, K., additional, Hearnshaw, J. B., additional, Itow, Y., additional, Kilmartin, P. M., additional, Korpela, A. V., additional, Lin, W., additional, Ling, C. H., additional, Masuda, K., additional, Matsubara, Y., additional, Miyake, N., additional, Muraki, Y., additional, Ohnishi, K., additional, Perrott, Y. C., additional, Saito, To., additional, Skuljan, L., additional, Sullivan, D. J., additional, Sumi, T., additional, Suzuki, D., additional, Sweatman, W. L., additional, Tristram, P. J., additional, Wada, K., additional, Yock, P. C. M., additional, Gulbis, A., additional, Hashimoto, Y., additional, Kniazev, A., additional, and Vaisanen, P., additional

Published
2012
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28. Variable Lyα sheds light on the environment surrounding GRB 090426

Author

Thöne, C. C., primary, Campana, S., additional, Lazzati, D., additional, de Ugarte Postigo, A., additional, Fynbo, J. P. U., additional, Christensen, L., additional, Levan, A. J., additional, Aloy, M. A., additional, Hjorth, J., additional, Jakobsson, P., additional, Levesque, E. M., additional, Malesani, D., additional, Milvang-Jensen, B., additional, Roming, P. W. A., additional, Tanvir, N. R., additional, Wiersema, K., additional, Gladders, M., additional, Wuyts, E., additional, and Dahle, H., additional

Published
2011
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29. Discovery of the nearby long, soft GRB 100316D with an associated supernova

Author

Starling, R. L. C., primary, Wiersema, K., additional, Levan, A. J., additional, Sakamoto, T., additional, Bersier, D., additional, Goldoni, P., additional, Oates, S. R., additional, Rowlinson, A., additional, Campana, S., additional, Sollerman, J., additional, Tanvir, N. R., additional, Malesani, D., additional, Fynbo, J. P. U., additional, Covino, S., additional, D'Avanzo, P., additional, O'Brien, P. T., additional, Page, K. L., additional, Osborne, J. P., additional, Vergani, S. D., additional, Barthelmy, S., additional, Burrows, D. N., additional, Cano, Z., additional, Curran, P. A., additional, De Pasquale, M., additional, D'Elia, V., additional, Evans, P. A., additional, Flores, H., additional, Fruchter, A. S., additional, Garnavich, P., additional, Gehrels, N., additional, Gorosabel, J., additional, Hjorth, J., additional, Holland, S. T., additional, van der Horst, A. J., additional, Hurkett, C. P., additional, Jakobsson, P., additional, Kamble, A. P., additional, Kouveliotou, C., additional, Kuin, N. P. M., additional, Kaper, L., additional, Mazzali, P. A., additional, Nugent, P. E., additional, Pian, E., additional, Stamatikos, M., additional, Thöne, C. C., additional, and Woosley, S. E., additional

Published
2010
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32. High-precision photometry by telescope defocussing - II. The transiting planetary system WASP-4

Author

Southworth, John, primary, Hinse, T. C., additional, Burgdorf, M. J., additional, Dominik, M., additional, Hornstrup, A., additional, Jørgensen, U. G., additional, Liebig, C., additional, Ricci, D., additional, Thöne, C. C., additional, Anguita, T., additional, Bozza, V., additional, Novati, S. Calchi, additional, Harpsøe, K., additional, Mancini, L., additional, Masi, G., additional, Mathiasen, M., additional, Rahvar, S., additional, Scarpetta, G., additional, Snodgrass, C., additional, Surdej, J., additional, and Zub, M., additional

Published
2009
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33. High-precision photometry by telescope defocusing - I. The transiting planetary system WASP-5

Author

Southworth, John, primary, Hinse, T. C., additional, Jørgensen, U. G., additional, Dominik, M., additional, Ricci, D., additional, Burgdorf, M. J., additional, Hornstrup, A., additional, Wheatley, P. J., additional, Anguita, T., additional, Bozza, V., additional, Novati, S. Calchi, additional, Harpsøe, K., additional, Kjaergaard, P., additional, Liebig, C., additional, Mancini, L., additional, Masi, G., additional, Mathiasen, M., additional, Rahvar, S., additional, Scarpetta, G., additional, Snodgrass, C., additional, Surdej, J., additional, Thöne, C. C., additional, and Zub, M., additional

Published
2009
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34. Numerical models of blackbody-dominated gamma-ray bursts-II. Emission properties.

Author

MartÍnez, C. Cuesta, Aloy, M. A., Mimica, P., Thöne, C., and de Ugarte Postigo, A.

Subjects
GAMMA rays, BLACK body (Physics), GALAXIES, LARGE scale structure (Astronomy), ASTRONOMICAL surveys, INTEGRAL field spectroscopy, ASTRONOMICAL observations
Abstract

Blackbody-dominated (BBD) gamma-ray bursts (GRBs) are events characterized by long durations and the presence of a significant thermal component following the prompt emission, as well as by the absence of a typical afterglow. GRB 101225A is the most prominent member of this class. A plausible progenitor system for it and for BBD-GRBs is the merger a neutron star and a helium core of an evolved, massive star. Using relativistic hydrodynamic simulations we model the propagation of ultrarelativistic jets through the environments created by such mergers. In a previous paper we showed that the thermal emission in BBD-GRBs is linked to the interaction of an ultrarelativistic jet with the ejected envelope of the secondary star of the binary. Here we focus on explaining the emission properties of BBD-GRBs computing the whole radiative signature (both thermal and non-thermal) of the jet dynamical evolution. The non-thermal emission of the forward shock of the jet is dominant during the early phases of the evolution, when that shock is moderately relativistic. Our models do not produce a classical afterglow because the quick deceleration of the jet results primarily from the mass entrainment in the beam, and not from the process of plowing mass from the external medium in front of the GRBB ejecta. The contribution of the reverse shock is of the same magnitude than that of the forward shock during the first 80 min after the GRB. Later, it quickly fades because the jet/environment interaction chocks the ultrarelativistic jet beam and effectively dumps the reverse shock. In agreement with observations, we obtain rather flat light curves during the first 2 d after the GRB, and a spectral evolution consistent with the observed reddening of the system. [ABSTRACT FROM AUTHOR]

Published
2015
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35. The host of the SN-less GRB 060505 in high resolution★.

Author

Thöne, C. C., Christensen, L., Prochaska, J. X., Bloom, J. S., Gorosabel, J., Fynbo, J. P. U., Jakobsson, P., and Fruchter, A. S.

Subjects
*GAMMA ray bursts, *HIGH resolution spectroscopy, *GALACTIC dynamics, *KINEMATICS, *ANGULAR momentum (Mechanics)
Abstract

The spiral host galaxy of the Swift GRB 060505 at z = 0.089 was the site of a puzzling long duration burst without an accompanying supernova. Studies of the burst environment by Thöne et al. suggested that this Gamma-ray Burst (GRB) came from the collapse of a massive star and that the GRB site was a region with properties different from the rest of the galaxy. We reobserved the galaxy in high spatial resolution using the VIMOS integral-field unit at the VLT with a spaxel size of 0.67 arcsec. Furthermore, we use long-slit high-resolution data from HIRES/Keck at two different slit positions covering the GRB site, the centre of the galaxy and an H ii region next to the GRB region. We compare the properties of different H ii regions in the galaxy with the GRB site and study the global and local kinematic properties of this galaxy. The resolved data show that the GRB site has the lowest metallicity in the galaxy with ∼1/3 Z⊙, but its specific star formation rate (SSFR) of 7.4 M⊙ yr−1/L/L* and age (determined by the Hα EW) are similar to other H ii regions in the host. The galaxy shows a gradient in metallicity and SSFR from the bulge to the outskirts as it is common for spiral galaxies. This gives further support to the theory that GRBs prefer regions of higher star formation and lower metallicity, which, in S-type galaxies, are more easily found in the spiral arms than in the centre. Kinematic measurements of the galaxy do not show evidence for large perturbations but a minor merger in the past cannot be excluded. This study confirms the collapsar origin of GRB 060505 but reveals that the properties of the H ii region surrounding the GRB were not unique to that galaxy. Spatially resolved observations are key to know the implications and interpretations of unresolved GRB hosts observations at higher redshifts. [ABSTRACT FROM AUTHOR]

Published
2014
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36. GRB 100219A with X-shooter – abundances in a galaxy at z =4.7.

Author

Thöne, C. C., Fynbo, J. P. U., Goldoni, P., de Ugarte, A. Postigo, Campana, S., Vergani, S. D., Covino, S., Krühler, T., Kaper, L., Tanvir, N., Zafar, T., D’Elia, V., Gorosabel, J., Greiner, J., Groot, P., Hammer, F., Jakobsson, P., Klose, S., Levan, A. J., and Milvang-Jensen, B.

Subjects
*COSMIC abundances, *REDSHIFT, *QUASARS, *GAMMA ray bursts, *WAVELENGTHS
Abstract

Abundances of galaxies at redshifts z > 4 are difficult to obtain from damped Lyα (DLA) systems in the sightlines of quasars (QSOs) due to the Lyα forest blanketing and the low number of high-redshift QSOs known to date. Gamma-ray bursts (GRBs) with their higher luminosity are well suited to study galaxies out to the formation of the first stars at z > 10. The large wavelength coverage of the X-shooter spectrograph makes it an excellent tool to study the interstellar medium of high-redshift galaxies, in particular if the redshift is not known beforehand. In this paper, we determine the properties of a GRB host at z = 4.667 23 from absorption lines combined with X-ray and optical imaging data. This is one of the highest redshifts where a detailed analysis with medium-resolution data is possible. We measure a relatively high metallicity of [S/H] = −1.1 ± 0.2 for a galaxy at this redshift. Assuming ultraviolet pumping as origin for the fine-structure lines, the material observed is between 0.3 and 1.0 kpc from the GRB. The extinction determined by the spectral slope from X-rays to the infrared shows a moderate value of AV = 0.13 ± 0.05 mag and relative abundances point to a warm disc extinction pattern. Low- and high-ionization as well as fine-structure lines show a complicated kinematic structure probably pointing to a merger in progress. We also detect one intervening system at z = 2.18. GRB-DLAs have a shallower evolution of metallicity with redshift than QSO absorbers and no evolution in their H i column density or ionization fraction. GRB hosts at high redshifts seem to continue the trend of the metallicity–luminosity relation towards lower metallicities but the sample is still too small to draw a definite conclusion. While the detection of GRBs at z > 4 with current satellites is still difficult, they are very important for our understanding of the early epochs of star and galaxy formation. [ABSTRACT FROM AUTHOR]

Published
2013

37. The X-ray absorbing column densities of Swift gamma-ray bursts.

Author

Campana, S., Thöne, C. C., de Ugarte Postigo, A., Tagliaferri, G., Moretti, A., and Covino, S.

Subjects
*GAMMA ray bursts, *GAMMA ray astronomy, *HYDROGEN, *ASTRONOMY, *REDSHIFT
Abstract

Long gamma-ray bursts (GRBs) are associated with the explosion of massive stars in star-forming regions. A large fraction of GRBs show intrinsic absorption as detected in optical spectra but absorption signatures are also detectable in the afterglow X-ray spectra. We present here a comprehensive analysis of the full sample of 93 GRBs with known redshift promptly observed by the Swift X-Ray Telescope (XRT) up to 2009 June. The distribution of X-ray column densities clearly shows that GRBs are heavily absorbed indicating that they indeed occur in dense environments. Furthermore, there is a lack of heavily absorbed GRBs at low redshift that might therefore be candidates for the missing ‘dark’ GRB population. However, there is no statistically significant correlation between the amount of X-ray absorption and the ‘darkness’ of a GRB. Finally, we compare the hydrogen column densities derived in the optical with those derived from X-ray absorption. The two distributions are different, with the optical column densities being lower than the X-ray ones, which is even more apparent when correcting for metallicity effects. The most likely explanation is photoionization of hydrogen in the circumburst material caused by the radiation field of the burst. [ABSTRACT FROM AUTHOR]

Published
2010
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