D2 Artikkeli ammatillisessa kokoomateoksessa
Spectroscopic classification of SN 2017hro with NOT
Tekijät: C. Babooram, J. Jormanainen, S. Wagner, F. Wierda, H. Kuncarayakti, G. Fedorets, S. Dyrbye
Kustantaja: R. E. Rutledge
Julkaisuvuosi: 2017
Kokoomateoksen nimi: Astronomer's Telegram
Tietokannassa oleva lehden nimi: The Astronomer's Telegram
Sarjan nimi: Astronomer's Telegram
Numero sarjassa: 10917
Verkko-osoite: https://www.astronomerstelegram.org/?read=10917
Tiivistelmä
We report the spectroscopic classification of supernova SN 2017hro (ATLAS17mwv) in host galaxy 2MASX J22161573+4003267. The observations were performed with the 2.56 m Nordic Optical Telescope equipped with ALFOSC (range 350-950 nm; resolution 1.6 nm) on 2017-11-01.8 UT. Survey Name | IAU Name | Discovery (UT) | Discovery mag | Observation (UT) | Redshift | Type | Phase | Notes ATLAS17mwv | SN 2017hro | 2017-10-28.3 | 18.765 | 2017-11-01.8 | 0.015 | II | around maximum | (1) (1) SN redshift is obtained from host emission lines and consistent with that derived from the SN spectrum.
We report the spectroscopic classification of supernova SN 2017hro (ATLAS17mwv) in host galaxy 2MASX J22161573+4003267. The observations were performed with the 2.56 m Nordic Optical Telescope equipped with ALFOSC (range 350-950 nm; resolution 1.6 nm) on 2017-11-01.8 UT. Survey Name | IAU Name | Discovery (UT) | Discovery mag | Observation (UT) | Redshift | Type | Phase | Notes ATLAS17mwv | SN 2017hro | 2017-10-28.3 | 18.765 | 2017-11-01.8 | 0.015 | II | around maximum | (1) (1) SN redshift is obtained from host emission lines and consistent with that derived from the SN spectrum.
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