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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

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