Abstract There is a scale error, i.e., a systematic dm which is a function of magnitude, in the CCD photometry of NGC7790, NGC4147 and NGC7006 published by Odewahn et al. The scale error also exists in the CCD photometry of NGC7790 by Petrov et al. The reason why this kind of error, which may only exist in photographic photometry, appears in a linear detector such as a CCD, is not immediately clear. If the CCD systems used by Odewahn et al. and Petrov et al. are really linear, maybe it is related to their use of the variable aperture technique in the former and the reduction method in the latter. Key words: techniques: photometric — CC
peer reviewedThe role of star observations is advocated in the photometric calibration of the low sp...
Abstract. Calibration of the CCD camera of the 1m telescope at the Vainu Bappu Observatory, Kavalur,...
We present a catalogue of aperture photometry of galaxies, in UBVRI, assembled from three different ...
There is a scale error, i.e., a systematic dm which is a function of magnitude, in the CCD photometr...
A common cause of errors in CCD differential photometry is an improper calibration of the array. The...
Abstract. The accuracy of new CCD photometry in the Vilnius sys-tem of the M 67 cluster is analyzed....
The accuracy of new CCD photometry in the Vilnius system of the M67 cluster is analyzed. The observa...
The importance of determining the error of the flat field in CCD photometry is detailed and our meth...
We have undertaken CCD observations of field standard stars with Hβ photometric system to investigat...
Using a CCD camera, deep BVI photometric sequences in the magnitude range V = 12-22 are obtained in ...
Photometric U and I standard sequences in the field of the open cluster NGC 7790 are presented. The ...
Context. Understanding the source of systematic errors in photometry is essential for their calibrat...
International audienceMeeting the science goals for many current and future ground-based optical lar...
CCD surface photometry for 232 E and S0 galaxies is presented. The galaxies are observed in Gunn r a...
The field of direct imaging is experiencing a considerable growth in the number of available CCD mos...
peer reviewedThe role of star observations is advocated in the photometric calibration of the low sp...
Abstract. Calibration of the CCD camera of the 1m telescope at the Vainu Bappu Observatory, Kavalur,...
We present a catalogue of aperture photometry of galaxies, in UBVRI, assembled from three different ...
There is a scale error, i.e., a systematic dm which is a function of magnitude, in the CCD photometr...
A common cause of errors in CCD differential photometry is an improper calibration of the array. The...
Abstract. The accuracy of new CCD photometry in the Vilnius sys-tem of the M 67 cluster is analyzed....
The accuracy of new CCD photometry in the Vilnius system of the M67 cluster is analyzed. The observa...
The importance of determining the error of the flat field in CCD photometry is detailed and our meth...
We have undertaken CCD observations of field standard stars with Hβ photometric system to investigat...
Using a CCD camera, deep BVI photometric sequences in the magnitude range V = 12-22 are obtained in ...
Photometric U and I standard sequences in the field of the open cluster NGC 7790 are presented. The ...
Context. Understanding the source of systematic errors in photometry is essential for their calibrat...
International audienceMeeting the science goals for many current and future ground-based optical lar...
CCD surface photometry for 232 E and S0 galaxies is presented. The galaxies are observed in Gunn r a...
The field of direct imaging is experiencing a considerable growth in the number of available CCD mos...
peer reviewedThe role of star observations is advocated in the photometric calibration of the low sp...
Abstract. Calibration of the CCD camera of the 1m telescope at the Vainu Bappu Observatory, Kavalur,...
We present a catalogue of aperture photometry of galaxies, in UBVRI, assembled from three different ...