Early-Time Flux Measurements of SN 2014J Obtained with Small Robotic Telescopes: Extending the AAVSO Light Curve
B. Poppe, T. Plaggenborg, W. Zheng, I. Shivvers, K. Itagaki, A. V., Filippenko, J. Kunz

TL;DR
This study demonstrates the use of small robotic telescopes for early-time photometry of SN 2014J, extending light curves and providing one of the earliest detections of the supernova, with high accuracy and validation against established data.
Contribution
It shows that NASA's small robotic MicroObservatory telescopes can reliably measure early supernova brightness, extending the AAVSO light curve with early detection data.
Findings
Early-time photometry agrees within 0.05 mag around maximum brightness.
Data from small robotic telescopes are comparable to larger observatories.
First detection was less than a day after explosion, providing valuable early data.
Abstract
In this work, early-time photometry of supernova (SN) 2014J is presented, extending the AAVSO CCD database to prediscovery dates. The applicability of NASA's small robotic MicroObservatory Network telescopes for photometric measurements is evaluated. Prediscovery and postdiscovery photometry of SN 2014J is measured from images taken by two different telescopes of the network, and is compared to measurements from the Katzman Automatic Imaging Telescope and the Itagaki Observatory. In the early light-curve phase (which exhibits stable spectral behavior with constant color indices), these data agree with reasonably high accuracy (better than 0.05 mag around maximum brightness, and 0.15 mag at earlier times). Owing to the changing spectral energy distribution of the SN and the different spectral characteristics of the systems used, differences increase after maximum light. We augment light…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Solar and Space Plasma Dynamics
