DRAFT
2024-04-12 14:40:42
Type: Object/s-Data/Analysis
Monitoring of AT 2024ggi (ATLAS24fsk) with Mephisto facilities
Authors: Brajesh Kumar, Xin-Lei Chen, Weikang Lin, Yuan Fang, Guowang Du, Xinzhong Er, Xiangkun Liu, Yangwei Zhang, Tianyu Zhang, Yuxi Bao, Xingzhu Zou, Yu Pan, Jinghua Zhang, Kaushik Chatterjee, Chenxu Liu, Yuan-Pei Yang, Xiaowei Liu (SWIFAR, YNU)
Keywords: Supernova
Abstract:
We observed AT 2024ggi (ATLAS24fsk) with the Mephisto facilities (50 cm array and 1.6m) located at the Lijiang observatory. The preliminary analysis of 1.6m images indicates that the SN has brightened ~0.3 and ~0.15 mag in Mephisto u and r bands during UT 15:24 - 16:54, 2024-04-11. Further monitoring is planned, and analysis is in progress.

Simultaneous multi-band (uvgriz) photometric observations of AT 2024ggi (ATLAS24fsk) (AstroNotes 2024-100, Srivastav et al., 2024-101, Killestein et al., 2024-102, Chen et al., 2024-103, Hoogendam et al., 2024-104, Zhai et al., 2024-105, Yang et al., 2024-107, Pérez-Fournon et al.) field were performed under moderate sky conditions (seeing ~1.3”) starting from 14:57 UT, 2024-04-11 (~11.6 hr after the ATLAS discovery, AstroNotes 2024-100). The observations were acquired using the Multi-channel Photometric Survey Telescope (Mephisto) of Yunnan University at Lijiang Observatory (IAU code: 044) of Yunnan Astronomical Observatories, Chinese Academy of Sciences. As the source was at a lower altitude, the observations began with 50 cm twin telescopes (g, r, i, z bands), and later, 1.6m was also utilized. The pre-processing and preliminary photometry of the images were done with automatic data reduction and photometry pipeline developed for the Mephisto. Here, we note that the Mephisto filter system (u, v, g, r, I, and z) mean transmission wavelengths are 345, 385, 530, 630, 837, and 945 nm, and the effective band widths are 38, 37, 79, 102, 109 and 71 nm.

SourceURL:file:///home/brajesh/Documents/Circular-SN2024ggi.docx

The preliminary photometric magnitudes of initial frames are below:

u = 16.12 +/- 0.02,

v = 16.07 +/- 0.01,

g = 16.04 +/- 0.01,

r = 15.94 +/- 0.01,

i = 16.12 +/- 0.02,

z = 16.13 +/- 0.02 mag.

The expected Galactic foreground extinction and the host contamination have not been removed from the estimated magnitudes. Further analysis is in progress, and monitoring will be continued in the upcoming nights.

Mephisto (Multi-channel Photometric Survey Telescope) is a 1.6-m wide-field multi-channel telescope, the first of its type in the world, capable of imaging the same field of view in three optical bands simultaneously. It provides real-time, high-quality colors of stellar objects. The on-site telescope assemblage and commissioning were carried out in September 2022. The first light in all three channels was achieved on 2023 December 21.

Show current TNS values
Catalog Name Reported RA Reported DEC Reported Obj-Type Reported Redshift Host Name Host Redshift Remarks TNS RA TNS DEC TNS Obj-Type TNS Redshift
TNS 2024ggi [ATLAS24fsk] 11:18:22.104 -32:50:15.14 SN II 0.002435 11:18:22.087 -32:50:15.27 SN II 0.002435

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