DRAFT
2024-03-15 14:32:26
Type: Object/s-Discovery/Classification
ePESSTO+ spectroscopic classification of optical transient AT2024egc
Authors: C. Vogl, S. Taubenberger (MPA/TUM), G. Csoernyei (MPA), S. Blondin (LAM/ESO), J. Terwel (TCD), E. Concepcion, M. Bronikowski (Nova Gorica), T.-W. Chen (NCU), S. Benetti (INAF-OAPd), S. Brennan (Stockholm), J. Anderson (ESO), M. Gromadzki (Warsaw), C. Inserra (Cardiff), E. Kankare (Turku), T. Müller Bravo (ICE), M. Nicholl (QUB), O. Yaron, E. Zimmerman (Weizmann), D. Young (QUB)
Source Group: ePESSTO+
Abstract:
This report includes classifications of one Type IIn SN (AT2024egc).

ePESSTO+, the advanced Public ESO Spectroscopic Survey for Transient Objects (Smartt et al. 2015 2015A&A...579A..40S), reports the following supernova classifications.

The target was supplied by BlackGEM (https://astro.ru.nl/blackgem/).

Observations were performed on the ESO New Technology Telescope (NTT) at La Silla on the night of 2024 March 14, using EFOSC2 and Grism 13 (3985-9315A, 18A resolution). Classifications were done using GELATO (Harutyunyan et al. 2008 2008A&A...488..383H).

The classification spectra and additional details can be obtained from http://www.pessto.org (via WISeREP) and the IAU Transient Name Server.

The classified objects are listed in the Related Objects table below.

Show current TNS values
Catalog Name Reported RA Reported DEC Reported Obj-Type Reported Redshift Host Name Host Redshift Source Phase (days) Remarks TNS RA TNS DEC TNS Obj-Type TNS Redshift
TNS 2024egc [BGEM J191145.30-570804.0] 19:11:45.308 -57:08:04.06 SN IIn 0.01 ESO184-G025 0.01 BlackGEM IIn. Narrow Balmer P-Cygni profiles superimposed on a broader emission component. GELATO provides good matches to the peculiar Type IIn SN 2009ip at 6 days past UV maximum light. Known host redshift z=0.010. 19:11:45.308 -57:08:04.06 SN IIn 0.01014

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