Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-28T01:23:13.317Z Has data issue: false hasContentIssue false
  • English
  • Français

The SED Machine - Fast classification of transient objects

Published online by Cambridge University Press:  06 January 2014

Andreas Ritter ,
N. Konidaris ,
C. C. Ngeow ,
R. Quimby  and
S. Ben-Ami
Andreas Ritter
Affiliation:
Graduate Department of Astronomy, National Central University, email: [email protected]
N. Konidaris
Affiliation:
California Institute of Technology, CA, USA
C. C. Ngeow
Affiliation:
Graduate Department of Astronomy, National Central University, email: [email protected]
R. Quimby
Affiliation:
University of Tokyo, Japan
S. Ben-Ami
Affiliation:
The Weizmann Institute of Science, Israel
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The field of time-domain astronomy is expected to enjoy a golden age during this decade. However, the traditional method for the classification of transient candidates using spectra obtained with medium- to large-aperture telescopes is extremely time consuming and struggling to keep up with the discovery rate. The Spectral Energy Distribution (SED) Machine uses a new approach in order to overcome this shortcoming.

Keywords

instrumentation: spectrographstechniques: photometrictechniques: spectroscopictelescopesstars: novaegamma rays: bursts
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S298: Setting the scene for Gaia and LAMOST , May 2013 , pp. 435
Copyright
Copyright © International Astronomical Union 2014