Zobrazeno 1 - 10
of 942
pro vyhledávání: '"P. Kotak"'
Autor:
Warwick, B., Lyman, J., Pursiainen, M., Coppejans, D. L., Galbany, L., Jones, G. T., Killestein, T. L., Kumar, A., Oates, S. R., Ackley, K., Anderson, J. P., Aryan, A., Breton, R. P., Chen, T. W., Clark, P., Dhillon, V. S., Dyer, M. J., Gal-Yam, A., Galloway, D. K., Gutiérrez, C. P., Gromadzki, M., Inserra, C., Jiménez-Ibarra, F., Kelsey, L., Kotak, R., Kravtsov, T., Kuncarayakti, H., Magee, M. R., Matilainen, K., Mattila, S., Müller-Bravo, T. E., Nicholl, M., Noysena, K., Nuttall, L. K., O'Brien, P., O'Neill, D., Pallé, E., Pessi, T., Petrushevska, T., Pignata, G., Pollacco, D., Ragosta, F., Ramsay, G., Sahu, A., Sahu, D. K., Singh, A., Sollerman, J., Stanway, E., Starling, R., Steeghs, D., Teja, R. S., Ulaczyk, K.
SN 2023tsz is a Type Ibn supernova (SNe Ibn) discovered in an extremely low-mass host. SNe Ibn are an uncommon subtype of stripped-envelope core-collapse SNe. They are characterised by narrow helium emission lines in their spectra and are believed to
Externí odkaz:
http://arxiv.org/abs/2409.14147
Autor:
Gutiérrez, Claudia P., Mattila, Seppo, Lundqvist, Peter, Dessart, Luc, González-Gaitán, Santiago, Jonker, Peter G., Dong, Subo, Coppejans, Deanne, Chen, Ping, Charalampopoulos, Panos, Elias-Rosa, Nancy, Reynolds, Thomas, Kochanek, Christopher, Fraser, Morgan, Pastorello, Andrea, Gromadzki, Mariusz, Neustadt, Jack, Benetti, Stefano, Kankare, Erkki, Kangas, Tuomas, Kotak, Rubina, Stritzinger, Maximilian D., Wevers, Thomas, Zhang, Bing, Bersier, David, Bose, Subhash, Buckley, David A. H., Dastidar, Raya, Gangopadhyay, Anjasha, Hamanowicz, Aleksandra, Kollmeier, Juna, Mao, Jirong, Misra, Kuntal, Potter, Stephen B., Prieto, Jose L., Romero-Colmenero, Encarni, Singh, Mridweeka, Somero, Auni, Terreran, Giacomo, Vaisanen, Petri, Wyrzykowski, Lukasz
We present ultraviolet, optical and near-infrared photometric and optical spectroscopic observations of the luminous, fast blue optical transient (LFBOT), CSS161010:045834-081803 (CSS161010). The transient was found in a low-redshift (z=0.033) dwarf
Externí odkaz:
http://arxiv.org/abs/2408.04698
Autor:
Valerin, G., Pastorello, A., Mason, E., Reguitti, A., Benetti, S., Cai, Y. -Z., Chen, T. -W., Eappachen, D., Elias-Rosa, N., Fraser, M., Gangopadhyay, A., Hsiao, E. Y., Howell, D. A., Inserra, C., Izzo, L., Jencson, J., Kankare, E., Kotak, R., Lundqvist, P., Mazzali, P. A., Misra, K., Pignata, G., Prentice, S. J., Sand, D. J., Smartt, S. J., Stritzinger, M. D., Tartaglia, L., Valenti, S., Anderson, J. P., Andrews, J. E., Amaro, R. C., Barbarino, C., Brennan, S., Bufano, F., Callis, E., Cappellaro, E., Dastidar, R., Della Valle, M., Fiore, A., Fulton, M. D., Galbany, L., Gromadzki, M., Heikkilä, T., Hiramatsu, D., Karamehmetoglu, E., Kuncarayakti, H., Leloudas, G., Limongi, M., Lundquist, M., McCully, C., Müller-Bravo, T. E., Nicholl, M., Ochner, P., Gonzalez, E. Padilla, Paraskeva, E., Pellegrino, C., Rau, A., Reichart, D. E., Reynolds, T. M., Roy, R., Salmaso, I., Shahbandeh, M., Singh, M., Sollerman, J., Turatto, M., Tomasella, L., Wyatt, S., Young, D. R.
We investigate the spectroscopic characteristics of Intermediate Luminosity Red Transients (ILRTs), a class of elusive objects with peak luminosity between that of classical novae and standard supernovae. We present the extensive optical and near-inf
Externí odkaz:
http://arxiv.org/abs/2407.21733
Autor:
Valerin, G., Pastorello, A., Reguitti, A., Benetti, S., Cai, Y. -Z., Chen, T. -W., Eappachen, D., Elias-Rosa, N., Fraser, M., Gangopadhyay, A., Hsiao, E. Y., Howell, D. A., Inserra, C., Izzo, L., Jencson, J., Kankare, E., Kotak, R., Mazzali, P. A., Misra, K., Pignata, G., Prentice, S. J., Sand, D. J., Smartt, S. J., Stritzinger, M. D., Tartaglia, L., Valenti, S., Anderson, J. P., Andrews, J. E., Amaro, R. C., Brennan, S., Bufano, F., Callis, E., Cappellaro, E., Dastidar, R., Della Valle, M., Fiore, A., Fulton, M. D., Galbany, L., Heikkilä, T., Hiramatsu, D., Karamehmetoglu, E., Kuncarayakti, H., Leloudas, G., Lundquist, M., McCully, C., Müller-Bravo, T. E., Nicholl, M., Ochner, P., Gonzalez, E. Padilla, Paraskeva, E., Pellegrino, C., Reichart, D. E., Reynolds, T. M., Roy, R., Salmaso, I., Singh, M., Turatto, M., Tomasella, L., Wyatt, S., Young, D. R.
We investigate the photometric characteristics of a sample of Intermediate Luminosity Red Transients (ILRTs), a class of elusive objects with peak luminosity between that of classical novae and standard supernovae. We present the multi-wavelength pho
Externí odkaz:
http://arxiv.org/abs/2407.21671
Autor:
O'Neill, David, Lyman, Joseph, Ackley, Kendall, Steeghs, Danny, Galloway, Duncan, Dhillon, Vik, O'Brien, Paul, Ramsay, Gavin, Noysena, Kanthanakorn, Kotak, Rubina, Breton, Rene, Nuttall, Laura, Pallé, Enric, Pollacco, Don, Ulaczyk, Krzysztof, Dyer, Martin, Jiménez-Ibarra, Felipe, Killestein, Tom, Kumar, Amit, Kelsey, Lisa, Godson, Ben, Jarvis, Dan
The search for the electromagnetic counterparts to gravitational wave (GW) events has been rapidly gathering pace in recent years thanks to the increasing number and capabilities of both gravitational wave detectors and wide field survey telescopes.
Externí odkaz:
http://arxiv.org/abs/2407.18642
Autor:
Dyer, Martin J., Ackley, Kendall, Jiménez-Ibarra, Felipe, Lyman, Joseph, Ulaczyk, Krzysztof, Steeghs, Danny, Galloway, Duncan K., Dhillon, Vik S., O'Brien, Paul, Ramsay, Gavin, Noysena, Kanthanakorn, Kotak, Rubina, Breton, Rene, Nuttall, Laura, Pallé, Enric, Pollacco, Don, Killestein, Tom, Kumar, Amit, O'Neill, David, Kelsey, Lisa, Godson, Ben, Jarvis, Dan
The Gravitational-wave Optical Transient Observer (GOTO) is a project dedicated to identifying optical counter-parts to gravitational-wave detections using a network of dedicated, wide-field telescopes. After almost a decade of design, construction,
Externí odkaz:
http://arxiv.org/abs/2407.17176
Autor:
Killestein, T. L., Kelsey, L., Wickens, E., Nuttall, L., Lyman, J., Krawczyk, C., Ackley, K., Dyer, M. J., Jiménez-Ibarra, F., Ulaczyk, K., O'Neill, D., Kumar, A., Steeghs, D., Galloway, D. K., Dhillon, V. S., O'Brien, P., Ramsay, G., Noysena, K., Kotak, R., Breton, R. P., Pallé, E., Pollacco, D., Awiphan, S., Belkin, S., Chote, P., Clark, P., Coppejans, D., Duffy, C., Eyles-Ferris, R., Godson, B., Gompertz, B., Graur, O., Irawati, P., Jarvis, D., Julakanti, Y., Kennedy, M. R., Kuncarayakti, H., Levan, A., Littlefair, S., Magee, M., Mandhai, S., Sánchez, D. Mata, Mattila, S., McCormac, J., Mullaney, J., Munday, J., Patel, M., Pursiainen, M., Rana, J., Sawangwit, U., Stanway, E., Starling, R., Warwick, B., Wiersema, K.
Time-domain astrophysics continues to grow rapidly, with the inception of new surveys drastically increasing data volumes. Democratised, distributed approaches to training sets for machine learning classifiers are crucial to make the most of this tor
Externí odkaz:
http://arxiv.org/abs/2406.02334
Autor:
Moran, S., Kotak, R., Fraser, M., Pastorello, A., Cai, Y. -Z., Valerin, G., Mattila, S., Cappellaro, E., Kravtsov, T., Gutiérrez, C. P., Elias-Rosa, N., Reguitti, A., Lundqvist, P., Brink, T. G., Filippenko, A. V., Wang, X. -F.
We present results from a five-month-long observing campaign of the unusual transient AT 2022fnm, which displays properties common to both luminous red novae (LRNe) and intermediate-luminosity red transients (ILRTs). Although its photometric evolutio
Externí odkaz:
http://arxiv.org/abs/2406.02816
Autor:
Elias-Rosa, Nancy, Brennan, Seán J., Benetti, Stefano, Cappellaro, Enrico, Pastorello, Andrea, Kozyreva, Alexandra, Lundqvist, Peter, Fraser, Morgan, Anderso, Joseph P., Cai, Yong-Zhi, Chen, Ting-Wan, Dennefeld, Michel, Gromadzki, Mariusz, Gutiérrez, Claudia P., Ihanec, Nada, Inserra, Cosimo, Kankare, Erkki, Kotak, Rubina, Mattila, Seppo, Moran, Shane, Müller-Bravo, Tomás E., Pessi, Priscila J., Pignata, Giuliano, Reguitti, Andrea, Reynolds, Thomas M., Smartt, Stephen J., Smith, Ken, Tartaglia, Leonardo, Valerin, Giorgio, de Boer, Thomas, Chambers, Kenneth, Gal-Yam, Avishay, Gao, Hua, Geier, Stefan, Mazzali, Paolo A., Nicholl, Matt, Ragosta, Fabio, Rest, Armin, Yaron, Ofer, Young, David R.
Publikováno v:
A&A 686, A13 (2024)
We present photometric and spectroscopic data sets for SN 2020pvb, a Type IIn-P supernova (SN) similar to SNe 1994W, 2005cl, 2009kn and 2011ht, with a precursor outburst detected (PS1 w-band ~ -13.8 mag) around four months before the B-band maximum l
Externí odkaz:
http://arxiv.org/abs/2402.02924
Autor:
Kangas, Tuomas, Kuncarayakti, Hanindyo, Nagao, Takashi, Kotak, Rubina, Kankare, Erkki, Fraser, Morgan, Stevance, Heloise, Mattila, Seppo, Maeda, Kei'ichi, Stritzinger, Maximilian, Lundqvist, Peter, Elias-Rosa, Nancy, Ferrari, Lucía, Folatelli, Gastón, Frohmaier, Christopher, Galbany, Lluís, Kawabata, Miho, Koutsiona, Eleni, Müller-Bravo, Tomás E., Piscarreta, Lara, Pursiainen, Miika, Singh, Avinash, Taguchi, Kenta, Teja, Rishabh Singh, Valerin, Giorgio, Pastorello, Andrea, Benetti, Stefano, Cai, Yong-Zhi, Charalampopoulos, Panos, Gutiérrez, Claudia P., Kravtsov, Timo, Reguitti, Andrea
Publikováno v:
A&A 689, A182 (2024)
We present optical and near-infrared photometry and spectroscopy of SN 2023aew and our findings on its remarkable properties. This event, initially resembling a Type IIb supernova (SN), rebrightens dramatically $\sim$90 d after the first peak, at whi
Externí odkaz:
http://arxiv.org/abs/2401.17423