SN 2018bsz: a Type I superluminous supernova with aspherical circumstellar material

Autor: M. Pursiainen, G. Leloudas, E. Paraskeva, A. Cikota, J. P. Anderson, C. R. Angus, S. Brennan, M. Bulla, E. Camacho-Iñiguez, P. Charalampopoulos, T.-W. Chen, M. Delgado Mancheño, M. Fraser, C. Frohmaier, L. Galbany, C. P. Gutiérrez, M. Gromadzki, C. Inserra, J. Maund, T. E. Müller-Bravo, S. Muñoz Torres, M. Nicholl, F. Onori, F. Patat, P. J. Pessi, R. Roy, J. Spyromilio, P. Wiseman, D. R. Young

Publikováno v: Pursiainen, M, Leloudas, G, Paraskeva, E, Cikota, A, Anderson, J P, Angus, C R, Brennan, S, Bulla, M, Camacho-Iniguez, E, Charalampopoulos, P, Chen, T-W, Delgado Mancheno, M, Fraser, M, Frohmaier, C, Galbany, L, Gutierrez, C P, Gromadzki, M, Inserra, C, Maund, J, Mueller-Bravo, T E, Munoz Torres, S, Nicholl, M, Onori, F, Patat, F, Pessi, P J, Roy, R, Spyromilio, J, Wiseman, P & Young, D R 2022, ' SN 2018bsz : A Type I superluminous supernova with aspherical circumstellar material ', Astronomy and Astrophysics, vol. 666, A30 . https://doi.org/10.1051/0004-6361/202243256
Pursiainen, M, Leloudas, G, Paraskeva, E, Cikota, A, Anderson, J P, Angus, C R, Brennan, S, Bulla, M, Camacho-Iniguez, E, Charalampopoulos, P, Chen, T-W, Delgado Mancheno, M, Fraser, M, Frohmaier, C, Galbany, L, Gutierrez, C P, Gromadzki, M, Inserra, C, Maund, J, Mueller-Bravo, T E, Munoz Torres, S, Nicholl, M, Onori, F, Patat, F, Pessi, P J, Roy, R, Spyromilio, J, Wiseman, P & Young, D R 2022, ' SN 2018bsz : A Type I superluminous supernova with aspherical circumstellar material ', Astronomy & Astrophysics, vol. 666, A30 . https://doi.org/10.1051/0004-6361/202243256

We present a spectroscopic analysis of the most nearby Type I superluminous supernova (SLSN-I), SN 2018bsz. The photometric evolution of SN 2018bsz has several surprising features, including an unusual pre-peak plateau and evidence for rapid formatio

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fde134c94bc0d0804b942ede4651a581

The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science

Autor: D Steeghs, D K Galloway, K Ackley, M J Dyer, J Lyman, K Ulaczyk, R Cutter, Y-L Mong, V Dhillon, P O’Brien, G Ramsay, S Poshyachinda, R Kotak, L K Nuttall, E Pallé, R P Breton, D Pollacco, E Thrane, S Aukkaravittayapun, S Awiphan, U Burhanudin, P Chote, A Chrimes, E Daw, C Duffy, R Eyles-Ferris, B Gompertz, T Heikkilä, P Irawati, M R Kennedy, T Killestein, H Kuncarayakti, A J Levan, S Littlefair, L Makrygianni, T Marsh, D Mata-Sanchez, S Mattila, J Maund, J McCormac, D Mkrtichian, J Mullaney, K Noysena, M Patel, E Rol, U Sawangwit, E R Stanway, R Starling, P Strøm, S Tooke, R West, D J White, K Wiersema

Publikováno v: Monthly Notices of the Royal Astronomical Society, 511, 2, pp. 2405-2422
Monthly Notices of the Royal Astronomical Society, 511, 2405-2422

The Gravitational-wave Optical Transient Observer (GOTO) is an array of wide-field optical telescopes, designed to exploit new discoveries from the next generation of gravitational wave detectors (LIGO, Virgo, KAGRA), study rapidly evolving transient

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::23a8922e993e393105e21cfdf38ccd63
http://arxiv.org/abs/2110.05539

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