IDENTIFYING BLUE HORIZONTAL BRANCH STARS USING THE z FILTER

In this paper we present a new method for selecting blue horizontal branch (BHB) candidates based on color-color photometry. We make use of the Sloan Digital Sky Survey z band as a surface gravity indicator and show its value for selecting BHB stars from quasars, white dwarfs, and main-sequence A-ty...

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Veröffentlicht in:The Astronomical journal 2012-04, Vol.143 (4), p.1-9
Hauptverfasser: Vickers, John J, Grebel, Eva K, HUXOR, AVON P
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HUXOR, AVON P
description In this paper we present a new method for selecting blue horizontal branch (BHB) candidates based on color-color photometry. We make use of the Sloan Digital Sky Survey z band as a surface gravity indicator and show its value for selecting BHB stars from quasars, white dwarfs, and main-sequence A-type stars. Using the g, r, i, and ; bands, we demonstrate that extraction accuracies on a par with more traditional u, g, and r photometric selection methods may be achieved. We also show that the completeness necessary to probe major Galactic structure may be maintained. Our new method allows us to efficiently select BHB stars from photometric sky surveys that do not include a u-band filter such as the Panoramic Survey Telescope and Rapid Response System.
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subjects ACCURACY
ASTRONOMY
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Bands
COLOR
FILTERS
Galactic structure
GRAVITATION
Horizontal branch stars
MAIN SEQUENCE STARS
MILKY WAY
PHOTOMETRY
PROBES
QUASARS
Sky surveys (astronomy)
Stars
WHITE DWARF STARS
title IDENTIFYING BLUE HORIZONTAL BRANCH STARS USING THE z FILTER
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