Index of /ogle/ogle2/var_stars/smc/cep/socep
This directory contains paper and data on single mode second overtone
Cepheid candidates in the SMC.
***WARNING***
The content of this archive was revised on Apr. 1, 2000 due to revised
calibration of the OGLE photometric data. A small systematic effect in
the original calibration was found, mapped, and applied to the data.
This effect, caused by some scattered light in the instrument resulting
in non-perfect flat-fielding, affected only East/West edges of the
frames and amounted to 0.08 mag in the I-band and 0.05 mag in the B and
V-bands at the very edges of the field. On average the effect was very
small - of the order of 0.01-0.02 mag.
We are very grateful to Dr. D.S. Graff (Ohio State University) for
pointing out to us this systematic effect.
*************
pap.ps.gz -- Paper: "The Optical Gravitational Lensing Experiment.
Cepheids in the Magellanic Clouds. II. Single-Mode
Second Overtone Cepheids in the Small Magellanic Cloud."
A. Udalski, I. Soszynski, M. Szymanski, M. Kubiak,
G. Pietrzynski, P. Wozniak, and K. Zebrun,
Acta Astron. 1999, 49, 45.
fig[1-5].ps.gz -- Full size Figures 1-5.
tab1.txt -- Table with basic data on candidates (ASC-II format).
phot.tar -- tar archive of phot/ subdirectory.
subdirectory phot/ -- photometry of individual objects:
subdirectory I/ -- photometry in the I-band
subdirectory V/ -- photometry in the V-band
subdirectory B/ -- photometry in the B-band
The file name is object_id.dat.gz in each of these
subdirectories. Each file contains 3 columns:
Hel JD, magnitude, error.