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Thirty-Five New Pulsating Da White Dwarf Stars

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TLDR
In this article, the authors presented 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Digital Sky Survey (SDSS) and the Hamburg Quasar Survey (HQS).
Abstract
We present 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Digital Sky Survey (SDSS) and the Hamburg Quasar Survey (HQS). We have acquired high-speed time series photometry of preselected DA white dwarfs with a prime focus CCD photometer on the 2.1 m telescope at McDonald Observatory over 15 months. We selected these stars on the basis of prior photometric and spectroscopic observations by the SDSS and HQS. For the homogeneous SDSS sample, we achieve a success rate of 80% for finding new variables at a detection threshold of 0.1%-0.3%. With 35 newly discovered DA variable white dwarfs, we almost double the current sample of 39.

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Journal ArticleDOI

Pulsating White Dwarf Stars and Precision Asteroseismology

TL;DR: In the 40 years since their discovery, pulsating white dwarf stars have moved from side-show curiosities to center stage as important tools for unraveling the deep mysteries of the Universe as discussed by the authors.
Journal ArticleDOI

Evolutionary and pulsational properties of white dwarf stars

TL;DR: A detailed review of the physics of white dwarfs can be found in this paper, with a focus on the physical processes that lead to the formation of the stars and the different energy sources responsible for chemical abundance changes that occur along their evolution.
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The Pulsating White Dwarf Stars

TL;DR: In this paper, the authors present a summary of what is currently known about the three distinct families of isolated pulsating white dwarfs, including the GW Vir stars, V777 Her stars, and ZZ Ceti stars.
References
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Journal ArticleDOI

The Sloan Digital Sky Survey: Technical Summary

Donald G. York
- 27 Jun 2000 - 
TL;DR: The Sloan Digital Sky Survey (SDSS) as mentioned in this paper provides the data to support detailed investigations of the distribution of luminous and non-luminous matter in the Universe: a photometrically and astrometrically calibrated digital imaging survey of pi steradians above about Galactic latitude 30 degrees in five broad optical bands.
Journal ArticleDOI

The Sloan Digital Sky Survey: Technical summary

Donald G. York, +151 more
TL;DR: The Sloan Digital Sky Survey (SDSS) as discussed by the authors provides the data to support detailed investigations of the distribution of luminous and non-luminous matter in the universe: a photometrically and astrometrically calibrated digital imaging survey of π sr above about Galactic latitude 30° in five broad optical bands to a depth of g' ~ 23 mag.
Journal ArticleDOI

Studies in astronomical time series analysis. II - Statistical aspects of spectral analysis of unevenly spaced data

TL;DR: This paper studies the reliability and efficiency of detection with the most commonly used technique, the periodogram, in the case where the observation times are unevenly spaced to retain the simple statistical behavior of the evenly spaced case.
Journal ArticleDOI

The Sloan digital sky survey photometric system

TL;DR: In this paper, the Sloan Digital Sky Survey photometric system, a new five-color (u' g' r' i' z') wide-band CCD system with wavelength coverage from 3000 to 11 000 A.
Journal ArticleDOI

Sloan digital sky survey: Early data release

Chris Stoughton, +212 more
TL;DR: The Sloan Digital Sky Survey (SDSS) is an imaging and spectroscopic survey that will eventually cover approximately one-quarter of the celestial sphere and collect spectra of ≈106 galaxies, 100,000 quasars, 30,000 stars, and 30, 000 serendipity targets as discussed by the authors.
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