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An optimized Hβ index for disentangling stellar population ages |
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Chemical Properties of Star-Forming Dwarf Galaxies |
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Post-AGB stars with hot circumstellar dust: binarity of the low-amplitude pulsators |
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The Luminosity-Size and Mass-Size Relations of Galaxies out to z ~ 3 |
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IRAC Mid-Infrared Imaging of the Hubble Deep Field-South: Star Formation Histories and Stellar Masses of Red Galaxies at z>2 |
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The structure of galactic disks. Studying late-type spiral galaxies using SDSS |
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The Size Evolution of Galaxies since z~3: Combining SDSS, GEMS, and FIRES |
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Strong size evolution of the most massive galaxies since z ~ 2 |
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Exploring the Evolutionary Paths of the Most Massive Galaxies since z ~ 2 |
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Size Evolution of the Most Massive Galaxies at 1.7 < z < 3 from GOODS NICMOS Survey Imaging |
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A Photometric Diagnostic to Aid in the Identification of Transiting Extrasolar Planets |
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X-ray spectral properties of active galactic nuclei in the Chandra Deep Field South |
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Measuring Solar Magnetic Fields with Artificial Neural Networks |
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On the Diagnostic Potential of Hα for Chromospheric Magnetism |
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Feature Extraction Techniques for the Analysis of Spectral Polarization Profiles |
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Strategies for Spectral Profile Inversion Using Artificial Neural Networks |
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Spinor: Visible and Infrared Spectro-Polarimetry at the National Solar Observatory |
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Spectral Line Selection for HMI: A Comparison of Fe I 6173 Å and Ni I 6768 Å |
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The Horizontal Magnetic Flux of the Quiet-Sun Internetwork as Observed with the Hinode Spectro-Polarimeter |
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Determining the spectroscopic mass ratio in interacting binaries: application to X-Ray Nova Sco 1994 |
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The formation and evolution of hydrogen-deficient post-AGB white dwarfs: The emerging chemical profile and the expectations for the PG 1159-DB-DQ evolutionary connection |
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Early universe constraints on time variation of fundamental constants |
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WMAP 5-year constraints on time variation of α and m in a detailed recombination scenario |
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Spatial relation between the 1908 Messina Straits earthquake slip and recent earthquake distribution |
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A dark jet dominates the power output of the stellar black hole Cygnus X-1 |
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