z-logo
open-access-imgOpen Access
Automated Detection of Short Optical Transients of Astrophysical Origin in Real Time
Author(s) -
M. Sokołowski,
K. Małek,
L. W. Piotrowski,
G. Wrochna
Publication year - 2010
Publication title -
advances in astronomy
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.364
H-Index - 34
eISSN - 1687-7977
pISSN - 1687-7969
DOI - 10.1155/2010/463496
Subject(s) - physics , transient (computer programming) , pipeline (software) , sky , identification (biology) , astronomy , astrophysics , object (grammar) , real time computing , artificial intelligence , computer science , botany , biology , programming language , operating system
The detection of short optical transients of astrophysical origin in real time is an important task for existing robotic telescopes. The faster a new optical transient is detected, the earlier follow-up observations can be started. The sooner the object is identified, the more data can be collected before the source fades away, particularly in the most interesting early period of the transient. In this the real-time pipeline designed for identification of optical flashes with the “Pi of the Sky” project will be presented in detail together with solutions used by other experiments

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom