Skynet's New Observing Mode: The Campaign Manager
arXiv:2210.08613 · doi:10.1088/1538-3873/ac3f7c
Abstract
Built in 2004, the Skynet robotic telescope network originally consisted of six 0.4 m telescopes located at the Cerro-Tololo Inter-American Observatory in the Chilean Andes. The network was designed to carry out simultaneous multi-wavelength observations of gamma-ray bursts (GRBs) when they are only tens of seconds old. To date, the network has been expanded to ~20 telescopes, including a 20 m radio telescope, that span four continents and five countries. The Campaign Manager (CM) is a new observing mode that has been developed for Skynet. Available to all Skynet observers, the CM semi-autonomously and indefinitely scales and schedules exposures on the observer's behalf while allowing for modification to scaling parameters in real time. The CM is useful for follow up to various transient phenomena including gravitational-wave events, GRB localizations, young supernovae, and eventually, sufficiently bright Argus Optical Array and Large Synoptic Survey Telescope events.
7 pages, 4 figures
References in corpus (11)
- Multi-messenger Observations of a Binary Neutron Star Merger
- A gravitational-wave standard siren measurement of the Hubble constant
- The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
- Evryscope science: exploring the potential of all-sky gigapixel-scale telescopes
- Optical and X-Ray Observations of GRB 060526: A Complex Afterglow Consistent with An Achromatic Jet Break
- GRB 120711A: an intense INTEGRAL burst with long-lasting soft gamma-ray emission and a powerful optical flash
- An empirical limit on the kilonova rate from the DLT40 one day cadence Supernova Survey
- The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125
- Optical follow-up of gravitational wave events during the second advanced LIGO/VIRGO observing run with the DLT40 Survey
- PROMPT Observations of the Early-Time Optical Afterglow of GRB 060607A
- Colour variations in the GRB 120327A afterglow