The New Milky Way: a wide-field survey of optical transients near the Galactic plane
Kirill Sokolovsky, Stanislav Korotkiy, and Alexandr Lebedev

TL;DR
This paper presents a cost-effective, automated wide-field survey system designed to detect optical transients, including novae, near the Galactic plane within hours, enabling rapid follow-up observations and discovery of fast-evolving astronomical events.
Contribution
The authors developed and demonstrated a low-cost, automated wide-field survey system capable of detecting optical transients in near real-time, significantly reducing detection latency for fast-evolving phenomena.
Findings
Discovered Nova Sagittarii 2012 No. 1 using the system.
Detected two X-ray emitting cataclysmic variables.
Enabled rapid follow-up observations within 22 hours of nova discovery.
Abstract
Currently, it may take days for a bright nova outburst to be detected. With the few exceptions, little is known about novae behaviour prior to maximum light. A theoretically-predicted population of ultra-fast novae with t2<1d is evading observational discovery because it is not possible to routinely organize fast follow-up observations of nova candidates. With the aim of brining the detection time of novae and other bright (V<13.5) optical transients from days down to hours or less, we develop an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. The system is built using low-cost mass-produced components and the transient detection pipeline is based on the open source VaST software. We describe the instrument design and report results of the first observations conducted in October-November 2011 and…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astrophysical Phenomena and Observations · Stellar, planetary, and galactic studies
