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AAS 2013 1/ 13<br />
ROBOSPECT: Automated Equivalent Width<br />
Measurement<br />
Christopher Waters & Julie Krugler Hollek<br />
<strong>Institute</strong> <strong>for</strong> <strong>Astronomy</strong><br />
University of Texas<br />
Long Beach AAS, January 8, 2013
AAS 2013 2/ 13<br />
What does ROBOSPECT do?<br />
◮ Iteratively construct a best-fit<br />
model to an input spectrum.<br />
◮ Model the continuum level.<br />
◮ Identify and fit spectral lines.<br />
◮ Various line models<br />
(Gaussian, Voigt, etc.).<br />
◮ Measure equivalent widths,<br />
line flux.<br />
◮ Deblend closely spaced lines.
AAS 2013 3/ 13<br />
What does ROBOSPECT do?<br />
◮ Iteratively construct a best-fit<br />
model to an input spectrum.<br />
◮ Model the continuum level.<br />
◮ Identify and fit spectral lines.<br />
◮ Various line models<br />
(Gaussian, Voigt, etc.).<br />
◮ Measure equivalent widths,<br />
line flux.<br />
◮ Deblend closely spaced lines.
AAS 2013 4/ 13<br />
What does ROBOSPECT do?<br />
◮ Iteratively construct a best-fit<br />
model to an input spectrum.<br />
◮ Model the continuum level.<br />
◮ Identify and fit spectral lines.<br />
◮ Various line models<br />
(Gaussian, Voigt, etc.).<br />
◮ Measure equivalent widths,<br />
line flux.<br />
◮ Deblend closely spaced lines.
AAS 2013 5/ 13<br />
Does it work on my data?<br />
◮ Reads ascii and fits spectra.<br />
◮ Data can be flux calibrated or<br />
continuum normalized.<br />
◮ Emission and absorption lines<br />
identified and fit.<br />
◮ Not designed <strong>for</strong> highly blended<br />
bands (molecules, high<br />
metallicity stars).
AAS 2013 6/ 13<br />
Does it work on my data?<br />
◮ Reads ascii and fits spectra.<br />
◮ Data can be flux calibrated or<br />
continuum normalized.<br />
◮ Emission and absorption lines<br />
identified and fit.<br />
◮ Not designed <strong>for</strong> highly blended<br />
bands (molecules, high<br />
metallicity stars).
AAS 2013 7/ 13<br />
Does it work on my data?<br />
◮ Reads ascii and fits spectra.<br />
◮ Data can be flux calibrated or<br />
continuum normalized.<br />
◮ Emission and absorption lines<br />
identified and fit.<br />
◮ Not designed <strong>for</strong> highly blended<br />
bands (molecules, high<br />
metallicity stars).
AAS 2013 8/ 13<br />
How accurate is it?<br />
◮ Iterative process reduces<br />
continuum and lines covariance.<br />
◮ Fit quality related to the input<br />
spectrum S/N.<br />
◮ Continuum placement is the<br />
largest source of uncertainty.<br />
◮ Matches measurements done by<br />
hand.
AAS 2013 9/ 13<br />
How accurate is it?<br />
◮ Iterative process reduces<br />
continuum and lines covariance.<br />
◮ Fit quality related to the input<br />
spectrum S/N.<br />
◮ Continuum placement is the<br />
largest source of uncertainty.<br />
◮ Matches measurements done by<br />
hand.
AAS 2013 10/ 13<br />
When can I get it?<br />
◮ Test version <strong>available</strong> from me now (see me at the<br />
Pan-STARRS booth #132).<br />
◮ Public release at<br />
http://www.ifa.hawaii.edu/~watersc1/robospect/.<br />
◮ Paper describing the algorithm and fit quality will be<br />
submitted by the end of the month.<br />
◮ Still writing the manual and documentation to make it easy<br />
<strong>for</strong> other users.
Extra slides<br />
AAS 2013 11/ 13
Extra slides<br />
AAS 2013 12/ 13
Extra slides<br />
AAS 2013 13/ 13