Photometry of Type II Supernova SN 2023ixf with a Worldwide Citizen Science Network
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Published:2023-07-06
Issue:7
Volume:7
Page:141
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ISSN:2515-5172
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Container-title:Research Notes of the AAS
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language:
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Short-container-title:Res. Notes AAS
Author:
Sgro Lauren A.ORCID, Esposito Thomas M.ORCID, Blaclard GuillaumeORCID, Gomez SebastianORCID, Marchis FranckORCID, Filippenko Alexei V.ORCID, Peluso Daniel O’ConnerORCID, Lawrence Stephen S.ORCID, Verveen Aad, Wagner Andreas, Nardi Anouchka, Wiart Barbara, Mirwald Benjamin, Christensen Bill, Eramia Bob, Parker BruceORCID, Guillet BrunoORCID, Kim Byungki, Logan Chelsey A.ORCID, Kyba Christopher C. M.ORCID, Toulmin Christopher, Vantaggiato Claudio G., Adhis Dana, Gary Dave, Goodey Dave, Dickinson David, Koster David, Martin Davy, Bonilla EliudORCID, Chung Enner, Miny Eric, Mortecrette FabriceORCID, Saibi FadiORCID, Gagnon Francois O.ORCID, Simard Franois, Vacon Gary, Simard Georges, Dreise Gerrit, Funakoshi Hiromi, Vacon Janet, Yaniz James, Le Tarnec Jean-CharlesORCID, Laugier Jean-MarieORCID, Siders Jennifer L. W., Sweitzer Jim, Dvoracek Jiri, Archer JohnORCID, Deitz John, Bradley John K., Fukui KeiichiORCID, Sibbernsen KendraORCID, Borrot Kevin, Cross Kevin, Heider KevinORCID, Yamaguchi Koichi, Hirsch Lea A.ORCID, Leroux LioubaORCID, Billiani MarioORCID, Lorber Markus, Smallen Martin J., Shimizu Masao, Nishimura Masayoshi, Ryno MatthewORCID, Cunningham Michael, Gagnon Michael, Primm MichaelORCID, Rushton Michael, Sibbernsen MichaelORCID, Mitchell Mike, Yoblonsky Neil, Leroux Niniane, Clerget Olivier, Stojanović OzrenORCID, Unique Patrice, Huth PatrickORCID, Ang Raymund JohnORCID, Santoni Regis, Foster Robert, Poggiali Roberto, Xu RuyiORCID, Kukita RyuichiORCID, Šćepanović Sanja, Saibi SophieORCID, Will StefanORCID, Latour Stephan, Haythornthwaite Stephen, Cadieux Sylvain, Müller ThoralfORCID, Chung Tze YangORCID, Watanabe Yoshiya, Arnaud Yvan
Abstract
Abstract
We present highly sampled photometry of the supernova (SN) 2023ixf, a Type II SN in M101, beginning 2 days before its first known detection. To gather these data, we enlisted the global Unistellar Network of citizen scientists. These 252 observations from 115 telescopes show the SN’s rising brightness associated with shock emergence followed by gradual decay. We measure a peak M
V
= − 18.18 ± 0.09 mag at 2023 May 25 21:37 UTC in agreement with previously published analyses.
Publisher
American Astronomical Society
Cited by
1 articles.
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