English

Mary, a pipeline to aid discovery of optical transients

Instrumentation and Methods for Astrophysics 2017-09-13 v1 High Energy Astrophysical Phenomena Solar and Stellar Astrophysics

Abstract

The ability to quickly detect transient sources in optical images and trigger multi-wavelength follow up is key for the discovery of fast transients. These include events rare and difficult to detect such as kilonovae, supernova shock breakout, and "orphan" Gamma-ray Burst afterglows. We present the Mary pipeline, a (mostly) automated tool to discover transients during high-cadenced observations with the Dark Energy Camera (DECam) at CTIO. The observations are part of the "Deeper Wider Faster" program, a multi-facility, multi-wavelength program designed to discover fast transients, including counterparts to Fast Radio Bursts and gravitational waves. Our tests of the Mary pipeline on DECam images return a false positive rate of ~2.2% and a missed fraction of ~3.4% obtained in less than 2 minutes, which proves the pipeline to be suitable for rapid and high-quality transient searches. The pipeline can be adapted to search for transients in data obtained with imagers other than DECam.

Keywords

Cite

@article{arxiv.1708.04629,
  title  = {Mary, a pipeline to aid discovery of optical transients},
  author = {Igor Andreoni and Colin Jacobs and Sarah Hegarty and Tyler Pritchard and Jeff Cooke and Stuart Ryder},
  journal= {arXiv preprint arXiv:1708.04629},
  year   = {2017}
}

Comments

Accepted for publication in PASA; 15 pages, 7 figures, 3 tables