Based in part on observations made at Observatoire de Haute Provence (CNRS), France, with the MISTRAL instrument. This research has also made use of the MISTRAL database, operated at CeSAM (LAM), Marseille, France. We acknowledge the excellent support from Observatoire de Haute-Provence, in particular Jerome Schmitt, Jean Claude Brunel, Francois Huppert, Jean Balcaen, Yoann Degot-Longhi, Stephane Favard, and Jean-Pierre Troncin. We thank the OHP direction for the allocations of two DDT observing slots. The operation of FRAM telescopes is supported by the grants of the Ministry of Education of the Czech Republic LM2023032 and LM2023047, as well as EU/MEYS grants CZ.02.1.01/0.0/0.0/16_013/0001403, CZ.02.1.01/0.0/0.0/18_046/0016007, CZ.02.1.01/0.0/0.0/16_019/0000754 and CZ.02.01.01/00/22_008/0004632. The work of F.,N., is supported by NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The work of W. Corradi is supported by Laboratório Nacional de Astrofísica - LNA, through project numbers P-003, P-011, I-004 and I-013 from OPD. The work of N. Sasaki is supported by Universidade do Estado do Amazonas - UEA and LNA through project numbers P-003, P-008 and I-004 and I-007. The work of L. de Almeida is supported by Laboratório Nacional de Astrofísica (LNA) through project numbers: I-009, I-022, I-027 and P-008 from OPD. The work of K. Noysena and M. Tanasan is based on observations made with the Thai Robotic Telescope under program ID TRTC11A_003, which is operated by the National Astronomical Research Institute of Thailand (Public Organization). The work is supported by CNRS-MITI and Programme National des Hautes Energies (PNHE). The Unistellar Network and T. M. Esposito are partially supported by generous contributions from the Gordon and Betty Moore Foundation and Frédéric Gastaldo. C.~Andrade and M.~W.~Coughlin acknowledge support from the National Science Foundation with grant numbers PHY-2308862 and PHY-2117997. This publication was made possible through the support of Grant 62192 from the John Templeton Foundation to LSST-DA. The opinions expressed in this publication are those of the author(s) and do not necessarily reflect the views of LSST-DA or the John Templeton Foundation.

Andrade, Cristina et al.-- Full list of authors: Andrade, Cristina; Duverne, Pierre-Alexandre; Liu, Jialian; Navarete, Felipe; Abdelaziz, Abdelaziz E.; Abdelkareem, Mohamed; Abdi, Ilmah; Aboueisha, Mohamed; Adami, Christophe; Agayeva, Shabnam; Aivazyan, Vova; de Almeida, Leandro; Akl, Dalya; Antier, Sarah; Arnaud, Yvan; Ata, Saad A.; Badawy, Wageeh A.; Bai, Chunhai; Bendary, Reda; Benkhaldoun, Zouhair; Borrot, Kevin; Broens, Eric; Cai, Yongzhi; Clerget, Olivier; Corradi, Wagner; Coughlin, Michael W.; Delaunoy, Nicolas; Dubois, Franky; Ducoin, Jean-Grégoire; Elhosseiny, Eslam; Esposito, Thomas M.; Esamdin, Ali; Foulon, Pascal; Foulon, Roland; Freeberg, Michael; Galdies, Charles; Gokuldass, Priyadarshini; Guillet, Bruno; Hamed, Gamal M.; Haremza, Bruno; Hello, Patrice; Hendy, Yasser; Huth, Patrick; Inasaridze, Raguli; Iskandar, Abdusamatjan; Kaeouach, Aziz; Kamel, Tarek M.; Karpov, Sergey; Kneip, Raymond; Kochiashvili, Nino; Kuossari, Petri; Li, Liping; Li, Xin; Liu, Jinzhong; Lorber, Markus; Mabrouk, Raouf H.; Marchais, Denis; Maris, Elisabeth; Márquez, Isabel; Mašek, Martin; Ménard, Roger; Meneghelli, Nicola; Mitchell, Mike; Noysena, Kanthanakorn; Odeh, Mohammad; Ono, Wataru; Parent, Gérard; Parker, Bruce; Peloton, Julien; Popowicz, Adam; Pradier, Thierry; Price, Stephen; Pyshna, Oleksandra; Rajabov, Yodgor; Saibi, Fadi; Saibi, Sophie; Saint-Gelais, Denis; Sasaki, Nelio; Serrau, Marc; Shimizu, Masao; Shokry, Ahmed; Simon, Andrii; Sokoliuk, Oleksii; Takey, Ali; Tanasan, Manasanun; Tillayev, Yusuf; Di Tommaso, Giuseppe; Tosta e Melo, Iara; Turpin, Damien; Wang, Xiaofeng; Wang, Zhenyu; Zead, Ibrahim; Zhang, Jujia

First detected on 2023 November 4 by the Gravitational-wave Optical Transient Observer, SN 2023wrk is a Type Ia Supernova at 40¿Mpc, with significant unburned carbon in the outer ejecta. In this note, we present photometric and spectroscopic observations and analysis conducted by the Global Rapid Advanced Network Devoted to the Multi-messenger Addict over a 115¿days period, which includes 78¿days of measurements. The observations were contributed by both amateur and professional astronomers. J. Liu et al. analyzed the physical processes involved, and compared the evolution of color and spectral lines. We conclude that SN¿2023wrk is the second 1999aa-like object with strong carbon absorption lines that has ever been found, which enriches our understanding of the subclass of 1999aa-like SNe. © 2024 The Author(s).