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19962026
most citedBVRI Light Curves for 22 Type Ia Supernovae

758 citations · 5.6k across the 93 of their papers we have counts for

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astro-ph2005

Near-Infrared Observations of RR Lyrae Variables in Centauri

M. Del Principe, A. M. Piersimoni, J. Storm +6

We present Near-Infrared (NIR) and -band observations for 181 RR Lyrae stars in the Galactic Globular Cluster Cen. The comparison between predicted and empirical slope…

astro-ph2005

How good are RR Lyrae and Cepheids really as Distance Indicators? The observational approach

Jesper Storm

A number of recent technical developments, including the Hipparcos satellite, the Hubble Space Telescope fine guidance sensors and long base line near-IR interferometry has made it…

astro-ph2005★ 1 cited

Distances to six Cepheids in the LMC cluster NGC1866 from the near-IR surface-brightness method

J. Storm, W. Gieren, P. Fouque +2

We derive individual distances to six Cepheids in the young populous star cluster NGC1866 in the Large Magellanic Cloud employing the near-IR surface brightness technique. With six…

astro-ph2005

Evidence for a Universal Slope of the Period-Luminosity Relation from Direct Distances to Cepheids in the LMC

Wolfgang Gieren, Jesper Storm, Thomas G. Barnes +3

We have applied the infrared surface brightness (ISB) technique to derive distances to 13 Cepheid variables in the LMC which have periods from 3-42 days. The corresponding absolute…

astro-ph2005

Infrared Surface Brightness Distances to Cepheids

Thomas G. Barnes, Jesper Storm, William H. Jefferys +2

Bayesian statistical calculations and linear-bisector calculations for obtaining Cepheid distances and radii by the infrared surface brightness method have been compared for a set…

astro-ph2005★ 20 cited

The near-IR Surface Brightness Method applied to six Cepheids in the young LMC cluster NGC1866

Jesper Storm, Wolfgang P. Gieren, Pascal Fouque +2

We present new near-IR light curves for six Cepheids in the young blue LMC cluster NGC1866 as well as high precision radial velocity curves for ten Cepheids in NGC1866 and two in N…