Image Details
Caption: Figure 4.
AT 2016blu was monitored with KAIT, GSP, and AAVSO observers in 2026 March as it approached its expected outburst. When it reached a peak magnitude of 16.6, Chandra ToO observations were triggered, resulting in a total exposure of 100 ks obtained over five epochs. Optical spectra were obtained during this period with Lick/Kast and later with MMT/BCH and LBT/MODS (see Figure 5).
© 2026. The Author(s). Published by the American Astronomical Society.