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HATPI Preperihelion Time-series Photometry of the Interstellar Comet 3I/ATLAS

Abstract:
The Hungarian-made Automated Telescope PI Steradians (HATPI) is a recently commissioned time-domain facility at Las Campanas Observatory, Chile, that uses 64 wide-angle, 9.6 cm diameter lenses and back-illuminated CCDs, yielding a mosaic field-of-view of 7100 square arcdegrees, observing the night sky at a cadence of 45 s and a spatial scale of 19 .″ 7 pixel−1. In this paper, we present moving object time-series photometry with this facility, focusing on the interstellar comet 3I/ATLAS, which was first robustly recovered by HATPI on the night of 2025 July 2 (one night after its discovery) at a Gaia G-band magnitude of G = 17.796 ± 0.082 mag (±0.030 mag systematic uncertainty). The comet then increased in brightness to G = 14.071 ± 0.073 mag ± 0.030 mag by 2025 September 13, after which it became unobservable by HATPI as it approached perihelion. Before 3I/ATLAS achieved a brightness of G = 16.396 ± 0.029 mag ± 0.030 mag on 2025 August 6, it could be detected when stacking all HATPI observations from a single night, while after this date it is sufficiently bright to detect in individual 45 s exposures. We do not detect evidence for significant short-time-scale variations in the brightness of 3I/ATLAS after August 6. Compared to other light curves in the literature, the HATPI photometry exhibits a somewhat steeper rise in brightness with decreasing heliocentric distance, rH. The HATPI magnitudes are well-fit as a power law function of rH, with an exponential index of n = 5.167 ± 0.095, over the range 2.14 au
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-3881/ae4a99

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ORCID:
0000-0001-8732-6166
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ORCID:
0000-0001-7204-6727
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ORCID:
0000-0002-5389-3944
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ORCID:
0000-0001-7442-6926
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ORCID:
0000-0002-8423-0510


Publisher:
IOP Publishing
Journal:
The Astronomical Journal More from this journal
Volume:
171
Issue:
5
Pages:
270
Article number:
270
Publication date:
2026-04-02
Acceptance date:
2026-02-24
DOI:
EISSN:
1538-3881
ISSN:
0004-6256


Language:
English
Keywords:
Pubs id:
2407731
Local pid:
pubs:2407731
Source identifiers:
3913196
Deposit date:
2026-04-02
ARK identifier:
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