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About

M. Nysewander has established a notable research presence at the intersection of time-domain astronomy, gamma-ray burst (GRB) science, and stellar astrophysics. Central to their work is the development and application of the PROMPT (Panchromatic Robotic Optical Monitoring and Polarimetry Telescopes) array — a suite of six 0.41-meter Ritchey-Chrétien telescopes at Cerro Tololo Inter-American Observatory in Chile, constructed with over $1.2 million in grants and donations. This robotic facility, capable of responding to GRB alerts within seconds, has proven transformative for capturing the earliest moments of GRB optical afterglows. Nysewander's detailed multiwavelength light curve of GRB 060607A, beginning just tens of seconds post-burst, exemplifies this capability and has garnered over 30 citations. Beyond GRBs, their work extends to stellar variability, including the discovery of large-amplitude oscillations in the hot subdwarf B star CS 1246 (25 citations) and pulsation studies of EC 22221-3152, alongside variable star monitoring in globular clusters like NGC 1851. With a cumulative citation impact exceeding 150 across their key works, Nysewander's contributions have meaningfully advanced rapid-response observational astronomy.