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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-ph2008★ 27 cited

Extremely faint high proper motion objects from SDSS stripe 82 - Optical classification spectroscopy of about 40 new objects

R. -D. Scholz, J. Storm, G. R. Knapp +1

(abridged) Deep multi-epoch Sloan Digital Sky Survey data in a 275 square degrees area along the celestial equator (SDSS stripe 82 = S82) allowed us to search for extremely faint (…

astro-ph2008★ 51 cited

Relative distances of Omega Centauri and 47 Tucanae

G. Bono, P. B. Stetson, N. Sanna +18

We present precise optical and near-infrared ground-based photometry of two Globular Clusters (GCs): Omega Cen and 47 Tuc. These photometric catalogs are unbiased in the Red Giant…

astro-ph2008

2XMM J083026+524133: The most X-ray luminous cluster at redshift 1

G. Lamer, M. Hoeft, J. Kohnert +2

In the distant universe X-ray luminous clusters of galaxies are rare objects. Large area surveys are therefore needed to probe the high luminosity end of the cluster population at…

astro-ph2007★ 227 cited

A new calibration of Galactic Cepheid Period-Luminosity relations from B to K bands, and a comparison to LMC PL relations

P. Fouque, P. Arriagada, J. Storm +8

The universality of the Cepheid Period-Luminosity relations has been under discussion since metallicity effects have been assumed to play a role in the value of the intercept and,…

astro-ph2007★ 36 cited

The Araucaria Project. Near-Infrared Photometry of Cepheid Variables in the Sculptor Galaxy NGC 55

W. Gieren, G. Pietrzynski, I. Soszynski +4

We have obtained deep images in the near-infrared J and K filters of four fields in the Sculptor Group spiral galaxy NGC 55 with the ESO VLT and ISAAC camera. For 40 long-period Ce…

astro-ph2006★ 56 cited

The Araucaria Project: Distance to the Local Group Galaxy NGC 3109 from Near-Infrared Photometry of Cepheids

I. Soszynski, W. Gieren, G. Pietrzynski +3

We present near-infrared J- and K-band photometry of 77 Cepheid variables in the Local Group galaxy NGC 3109. Combining our data with the previously published optical V- and I-band…