Light Curve for Type Ia Supernova Candidate AT 2018we
T. Willamo, J. Ala-K\"onni, J. Arvo, I. Pippa, T. Salo

TL;DR
This paper reports photometric observations of the supernova candidate AT 2018we, confirming its classification as a Type Ia supernova and estimating its distance at approximately 43 Mpc based on the constructed light curve.
Contribution
The study provides the first detailed light curve of AT 2018we, confirming its Type Ia classification and estimating its distance, based on follow-up observations from Gaia alerts.
Findings
Confirmed Type Ia supernova classification.
Estimated host galaxy distance at ~43 Mpc.
Constructed detailed light curve from observations.
Abstract
We present photometric follow-up observations of the supernova candidate AT 2018we, which was discovered by the Gaia photometric alerts system. The first Gaia detection of the object was made Feb 12, 2018. Our observations, made in Cousins R and Johnson B band, range from Feb 20 to May 5, 2018. From our observations, we have constructed a light curve, which supports the initial prediction of type Ia, included in the Gaia alert. Based on this classification, we have also estimated the distance to its assumed host galaxy, which was found to be around 43 Mpc.
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research
