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2. Multiband analyses of the bright GRB 230812B and the associated SN2023pel

Author

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

Published
2024

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Books, media, physical & digital resources
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3. Fires in the deep:The luminosity distribution of early-time gamma-ray-burst afterglows in light of the Gamow Explorer sensitivity requirements

Author

Kann, D. A., White, N. E., Ghirlanda, G., Oates, S. R., Melandri, A., Jelínek, M., De Ugarte Postigo, A., Levan, A. J., Martin-carrillo, A., Paek, G. S.-h., Izzo, L., Blazek, M., Thöne, C. C., Agüí Fernández, J. F., Salvaterra, R., Tanvir, N. R., Chang, T.-c., O’brien, P., Rossi, A., Perley, D. A., Im, M., Malesani, D. B., Antonelli, A., Covino, S., Choi, C., D’avanzo, P., D’elia, V., Dichiara, S., Fausey, H. M., Fugazza, D., Gomboc, A., Gorski, K. M., Granot, J., Guidorzi, C., Hanlon, L., Hartmann, D. H., Hudec, R., Jun, H. D., Kim, J., Kim, Y., Klose, S., Kluźniak, W., Kobayashi, S., Kouveliotou, C., Lidz, A., Marongiu, M., Martone, R., Meintjes, P., Mundell, C. G., Murphy, D., Nalewajko, K., Park, W.-k., Szécsi, D., Smith, R. J., Stecklum, B., Steele, I. A., Štrobl, J., Sung, H.-i, Updike, A., Urata, Y., Van Der Horst, A. J., Kann, D. A., White, N. E., Ghirlanda, G., Oates, S. R., Melandri, A., Jelínek, M., De Ugarte Postigo, A., Levan, A. J., Martin-carrillo, A., Paek, G. S.-h., Izzo, L., Blazek, M., Thöne, C. C., Agüí Fernández, J. F., Salvaterra, R., Tanvir, N. R., Chang, T.-c., O’brien, P., Rossi, A., Perley, D. A., Im, M., Malesani, D. B., Antonelli, A., Covino, S., Choi, C., D’avanzo, P., D’elia, V., Dichiara, S., Fausey, H. M., Fugazza, D., Gomboc, A., Gorski, K. M., Granot, J., Guidorzi, C., Hanlon, L., Hartmann, D. H., Hudec, R., Jun, H. D., Kim, J., Kim, Y., Klose, S., Kluźniak, W., Kobayashi, S., Kouveliotou, C., Lidz, A., Marongiu, M., Martone, R., Meintjes, P., Mundell, C. G., Murphy, D., Nalewajko, K., Park, W.-k., Szécsi, D., Smith, R. J., Stecklum, B., Steele, I. A., Štrobl, J., Sung, H.-i, Updike, A., Urata, Y., and Van Der Horst, A. J. more...

Published
2024

4. Multiband analyses of the bright GRB 230812B and the associated SN2023pel

Author

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

Published
2024

5. Multiband analyses of the bright GRB 230812B and the associated SN2023pel

Author

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

Published
2024

6. Varying linear polarisation in the dust-free gamma-ray burst 210610B.

Author

Agüí Fernández, J. F., de Ugarte Postigo, A., Thöne, C. C., Kobayashi, S., Rossi, A., Toma, K., Jelínek, M., Kann, D. A., Covino, S., Wiersema, K., Hartmann, D., Jakobsson, P., Martin-Carrillo, A., Melandri, A., De Pasquale, M., Pugliese, G., Savaglio, S., Starling, R. L. C., Štrobl, J., and Della Valle, M. more...

Subjects
*SPECTRAL energy distribution, *VERY large telescopes, *INTERSTELLAR medium, *LIGHT curves, *OPTICAL spectroscopy, *GAMMA ray bursts
Abstract

Context. Long gamma-ray bursts (GRBs) are produced by the collapse of some very massive stars, that emit ultra-relativistic jets. When the jets collide with the interstellar medium they decelerate and generate the so-called afterglow emission, which has been observed to be polarised. Aims. We study the polarimetric evolution of the GRB 210610B afterglow, at z = 1.1341. This allows us to evaluate the role of geometric and/or magnetic mechanisms in the GRB afterglow polarisation. Methods. We observed GRB 210610B using imaging polarimetry with CAFOS on the 2.2 m Calar Alto Telescope and FORS2 on the 4 × 8.1 m Very Large Telescope. Complementary optical spectroscopy was obtained with OSIRIS on the 10.4 m Gran Telescopio Canarias. We studied the GRB light-curve from X-rays to the optical bands and the Spectral Energy Distribution (SED). This allowed us to strongly constrain the line-of-sight extinction. Finally, we studied the GRB host galaxy using optical to NIR data to fit the SED and derive its integrated properties. Results. GRB 210610B had a bright afterglow with a negligible line-of-sight extinction. Polarimetry was obtained at three epochs: during an early plateau phase, at the time when the light curve breaks, and after the light curve steepened. We observe an initial polarisation of ∼4% that goes to zero at the time of the break, and it then again increases to ∼2%, with a change in the position angle of 54 ± 9 deg. The spectrum shows features with very low equivalent widths. This indicate a small amount of material in the line of sight within the host. Conclusions. The lack of dust and the low amount of material in the line of sight to GRB 210610B allowed us to study the intrinsic polarisation of the GRB optical afterglow. The GRB polarisation signals are consistent with ordered magnetic fields in refreshed shock or/and hydrodynamics-scale turbulent fields in the forward shock. [ABSTRACT FROM AUTHOR] more...

Published
2024
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7. The host of GRB 171205A in 3D: A resolved multiwavelength study of a rare grand-design spiral GRB host.

Author

Thöne, C. C., de Ugarte Postigo, A., Izzo, L., Michalowski, M. J., Levan, A. J., Leung, J. K., Agüí Fernández, J. F., Géron, T., Friesen, R., Christensen, L., Covino, S., D'Elia, V., Hartmann, D. H., Jakobsson, P., De Pasquale, M., Pugliese, G., Rossi, A., Schady, P., Wiersema, K., and Zafar, T. more...

Subjects
INTEGRAL field spectroscopy, SPIRAL galaxies, STAR formation, STELLAR populations, GALACTIC dynamics
Abstract

Long GRB hosts at z < 1 are usually low-mass, low-metallicity star-forming galaxies. Here we present the most detailed, spatially resolved study of the host of GRB 171205A so far, a grand-design barred spiral galaxy at z = 0.036. Our analysis includes MUSE integral field spectroscopy complemented with high-spatial-resolution UV/VIS HST imaging and CO(1−0) and H I 21 cm data. The GRB is located in a small star-forming region in a spiral arm of the galaxy at a deprojected distance of ∼8 kpc from the center. The galaxy shows a smooth negative metallicity gradient and the metallicity at the GRB site is half solar, slightly below the mean metallicity at the corresponding distance from the center. Star formation in this galaxy is concentrated in a few H II regions between 5 and 7 kpc from the center and at the end of the bar, inwards from the GRB region; however the H II region hosting the GRB is in the top 10% of the regions with the highest specific star-formation rate. The stellar population at the GRB site has a very young component (< 5 Myr) that contributes a significant part of the light. Ionized and molecular gas show only minor deviations at the end of the bar. A parallel study found an asymmetric H I distribution and some additional gas near the position of the GRB, which might explain the star-forming region of the GRB site. Our study shows that long GRBs can occur in many types of star-forming galaxies; however the actual GRB sites have consistently low metallicity, high star formation rates, and a young population. Furthermore, gas inflow or interactions triggering the star formation producing the GRB progenitor might not be evident in ionized or even molecular gas but only in H I. [ABSTRACT FROM AUTHOR] more...

Published
2024
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8. 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 more...

Published
2023
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9. 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] more...

Published
2022
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