Selection of wavelength calibration features for automatic format recovery in astronomical spectrographs

Details Selection of wavelength calibration features for automatic format recovery in astronomical spectrographs Selection of wavelength calibration features for automatic format recovery in astronomical spectrographs

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008spie.7014e.195b&link_type=abstract

Ground-based and Airborne Instrumentation for Astronomy II. Edited by McLean, Ian S.; Casali, Mark M. Proceedings of the SPI

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Automated wavelength calibration requires line lists that are free of blended or unstable features at the resolution of the spectrograph in order to avoid false matches. We present a procedure that will identify isolated features suitable for use as wavelength standards. The procedure takes into account the expected signal to noise level and the degree of uncertainty in the spectral format that defines how isolated the spectral features must be. Our goal is to produce a customised list of features that can be unambiguously matched to observed features.

Affiliated with

Also associated with

No associations

Rating

Selection of wavelength calibration features for automatic format recovery in astronomical spectrographs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Selection of wavelength calibration features for automatic format recovery in astronomical spectrographs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Selection of wavelength calibration features for automatic format recovery in astronomical spectrographs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1060560