MILLIMETER TRANSIENT POINT SOURCES IN THE SPTpol 100 SQUARE DEGREE SURVEY
2016
The
millimetertransient sky is largely unexplored, with measurements limited to follow-up of objects detected at other wavelengths. High-
angular-resolutiontelescopes, designed for measurement of the
cosmic microwave background(CMB), offer the possibility to discover new, unknown transient sources in this band—particularly the
afterglowsof unobserved
gamma-ray bursts(GRBs). Here, we use the 10 m
millimeter-wave
South Pole Telescope, designed for the primary purpose of observing the CMB at arcminute and larger angular scales, to conduct a search for such objects. During the 2012–2013 season, the telescope was used to continuously observe a 100 deg^2 patch of sky centered at R.A. 23h30m and decl. −55° using the polarization-sensitive SPTpol camera in two bands centered at 95 and 150 GHz. These 6000 hr of observations provided continuous monitoring for day- to month-scale
millimeter-wave transient sources at the 10 mJy level. One candidate object was observed with properties broadly consistent with a GRB
afterglow, but at a statistical significance too low (p = 0.01) to confirm detection.
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