output
19942026
most citedFinal Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant

3.3k citations

Showing 2012Show all

27 papers · 1 filter

astro-ph.IM2012★ 321 cited

Science with the Murchison Widefield Array

Judd D. Bowman, Iver Cairns, David L. Kaplan +58

Significant new opportunities for astrophysics and cosmology have been identified at low radio frequencies. The Murchison Widefield Array is the first telescope in the Southern Hem…

astro-ph.GA2012★ 17 cited

The Young Open Clusters King 12, NGC 7788, and NGC 7790: Pre-Main Sequence Stars and Extended Stellar Halos

T. J. Davidge

The stellar contents of the open clusters King 12, NGC 7788, and NGC 7790 are investigated using MegaCam images. Comparisons with isochrones yield an age < 20 Myr for King 12, 20--…

astro-ph.SR2012★ 40 cited

Variable stars in the Globular Cluster NGC 2808

Andrea Kunder, Peter B. Stetson, Marcio Catelan +2

The first calibrated broadband BVI time-series photometry is presented for the variable stars in NGC 2808, with observations spanning a range of twenty-eight years. We have also re…

astro-ph.CO2012★ 56 cited

PAndAS in the mist: The stellar and gaseous mass within the halos of M31 and M33

Geraint F. Lewis, Robert Braun, Alan W. McConnachie +12

Large scale surveys of the prominent members of the Local Group have provided compelling evidence for the hierarchical formation of massive galaxies, revealing a wealth of substruc…

astro-ph.SR2012★ 16 cited

The Horizontal Branch of NGC 1851: Constraints from its RR Lyrae Variables

Andrea Kunder, Maurizio Salaris, Santi Cassisi +5

We use the pulsational properties of the RR Lyrae variables in the globular cluster NGC 1851 to obtain detailed constraints of the various sub-stellar populations present along its…

astro-ph.SR2012★ 6 cited

A catalogue of Paschen-line profiles in standard stars

Wenjin Huang, George Wallerstein, Myra Stone

We have assembled an atlas of line profiles of the Paschen Delta line at 10,049 angstroms for the use of stellar modelling. For a few stars we have substituted the Paschen Gamma li…