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20042009
most citedThe Milky Way Tomography with SDSS: II. Stellar Metallicity

573 citations

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9 papers · 1 filter

astro-ph200880 cited

Biases and Uncertainties in Physical Parameter Estimates of Lyman Break Galaxies from Broad-band Photometry

Seong-Kook Lee, Rafal Idzi, Henry C. Ferguson +3

We investigate the biases and uncertainties in estimates of physical parameters of high-redshift Lyman break galaxies (LBGs), such as stellar mass, mean stellar population age, and…

astro-ph200835 cited

A High Yield of New Sightlines for the Study of Intergalactic Helium: Far-UV-Bright Quasars from SDSS, GALEX, and HST

David Syphers, Scott F. Anderson, Wei Zheng +6

Investigations of He II Ly-alpha (304 A rest) absorption toward a half-dozen quasars at z~3-4 have demonstrated the great potential of helium studies of the IGM, but the current cr…

astro-ph2008573 cited

The Milky Way Tomography with SDSS: II. Stellar Metallicity

Zeljko Ivezic, Branimir Sesar, Mario Juric +50

Using effective temperature and metallicity derived from SDSS spectra for ~60,000 F and G type main sequence stars (0.2<g-r<0.6), we develop polynomial models for estimating these…

astro-ph2008

UV and FUV spectroscopy of the hybrid PG 1159-type central star NGC 7094

M. Ziegler, T. Rauch, E. Reiff +3

Previous studies aiming at the iron-abundance determination in three PG 1159 stars (K 1-16, PG 1159-035, NGC 7094) and a [WC]-PG 1159 transition star (Abell 78) have revealed that…

astro-ph2007

Spectral Analysis of Central Stars of Planetary Nebulae

Thomas Rauch, Klaus Werner, Marc Ziegler +2

Spectral analysis by means of NLTE model atmospheres has presently arrived at a high level of sophistication. High-resolution spectra of central stars of planetary nebulae can be r…

astro-ph200719 cited

A new superwind galaxy: XMM-Newton observations of NGC 6810

David K. Strickland

We present the first imaging X-ray observation of the highly inclined (i = 78 deg) Sab Seyfert 2 galaxy NGC 6810 using XMM-Newton, which reveals soft X-ray emission that extends ou…