We continue our series of papers describing the results of a photometric survey of open star clusters, primarily in the southern hemisphere, taken in the u'g'r'i'z' filter system. The entire observed sample covered more than 100 clusters, but here we present data only on NGC 188, which is one of the oldest open clusters known in the Milky Way. We fit the Padova theoretical isochrones to our data. Assuming a solar metallicity for NGC 188, we find a distance of 1700+/-100 pc, an age of 7.5+/-0.7 Gyr, and a reddening E(B-V) of 0.025+/-0.005. This yields a distance modulus of 11.23+/-0.14
We have used the Canada-France-Hawaii Telescope to obtain deep and accurate multi-colour photometry...
We determine the relative ages of the open cluster NGC 188 and selected Hipparcos field stars by iso...
Context. An earlier analysis of the Milky Way Star Cluster (MWSC) catalogue revealed an apparent lac...
The authors continue the series of papers describing the results of a photometric survey of open sta...
We present high-precision UBVRI CCD photometry of the old open cluster NGC 188. Our color-magnitude ...
Photometric UBVI CCD photometry is presented for NGC 188 and Berkeley 17. Color-magnitude diagrams (...
This paper provides a detailed comparison of the differences in parameters derived for a star cluste...
We present initial results of a photometric survey of open star clusters, primarily in the southern ...
We have employed precise and carefully calibrated V - and I - band photometry of NGC 188 at WIYN Obs...
This is the published version. Copyright © 2014. The American Astronomical Society. All rights reser...
This is the published version. Copyright © 2014. The American Astronomical Society. All rights reser...
We present a UBVI and Hα photometric study of the young open cluster NGC 1893 in the HII region W8 (...
In this paper, we present the first BV I CCD photometry of six overlooked old open clusters (Berkele...
We present analysis of deep CCD photometry for the very rich, old open star cluster NGC 6819. These ...
We have used the Canada-France-Hawaii Telescope to obtain deep and accurate multi-colour photometry...
We have used the Canada-France-Hawaii Telescope to obtain deep and accurate multi-colour photometry...
We determine the relative ages of the open cluster NGC 188 and selected Hipparcos field stars by iso...
Context. An earlier analysis of the Milky Way Star Cluster (MWSC) catalogue revealed an apparent lac...
The authors continue the series of papers describing the results of a photometric survey of open sta...
We present high-precision UBVRI CCD photometry of the old open cluster NGC 188. Our color-magnitude ...
Photometric UBVI CCD photometry is presented for NGC 188 and Berkeley 17. Color-magnitude diagrams (...
This paper provides a detailed comparison of the differences in parameters derived for a star cluste...
We present initial results of a photometric survey of open star clusters, primarily in the southern ...
We have employed precise and carefully calibrated V - and I - band photometry of NGC 188 at WIYN Obs...
This is the published version. Copyright © 2014. The American Astronomical Society. All rights reser...
This is the published version. Copyright © 2014. The American Astronomical Society. All rights reser...
We present a UBVI and Hα photometric study of the young open cluster NGC 1893 in the HII region W8 (...
In this paper, we present the first BV I CCD photometry of six overlooked old open clusters (Berkele...
We present analysis of deep CCD photometry for the very rich, old open star cluster NGC 6819. These ...
We have used the Canada-France-Hawaii Telescope to obtain deep and accurate multi-colour photometry...
We have used the Canada-France-Hawaii Telescope to obtain deep and accurate multi-colour photometry...
We determine the relative ages of the open cluster NGC 188 and selected Hipparcos field stars by iso...
Context. An earlier analysis of the Milky Way Star Cluster (MWSC) catalogue revealed an apparent lac...