Add to ORKGResults of tests to demonstrate the very high differential-photometric stability of CCD light sensors are presented. The measurements reported here demonstrate that in a controlled laboratory environment, a front-illuminated CCD can provide differential-photometric measurements with reproducible precision approaching one part in 10(exp 5). Practical limitations to the precision of differential-photometric measurements with CCDs and implications for spaceborne applications are discussed
We describe the development of the fully depleted, back illuminated charge coupled devices for the T...
A front-illuminated development Euclid charge-coupled device (CCD) is tested to observe the CCD poin...
ABSTRACT. This paper summarizes a three-night observing campaign aimed at achieving millimagnitude-p...
Results of tests to demonstrate the very high differential-photometric stability of CCD light sensor...
Characterization of scientific-grade CCDs is extremely important if one hopes to attain very precise...
We have performed end-to-end laboratory and numerical simulations to demonstrate the capability of d...
A common cause of errors in CCD differential photometry is an improper calibration of the array. The...
The accurate measurement of the position of celestial objects is a fundamental step for several astr...
Photometry is the measure of the brightness of an object. When making such measurements on stars, it...
Charge-Coupled-Device (CCD) cameras have opened a new world in astronomy and other related sciences ...
This paper summarizes the introductory presentation for a workshop (held Nov 18,19 2013 at Brookhave...
Differential photometry offers the most precise method for measuring the brightness of astronomical ...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2009.Includes bibliographica...
This book brings together experts in the field of astronomical photometry to discuss how their subfi...
The application of CCDs to star trackers and star mappers is considered. Advantages and disadvantage...
We describe the development of the fully depleted, back illuminated charge coupled devices for the T...
A front-illuminated development Euclid charge-coupled device (CCD) is tested to observe the CCD poin...
ABSTRACT. This paper summarizes a three-night observing campaign aimed at achieving millimagnitude-p...
Results of tests to demonstrate the very high differential-photometric stability of CCD light sensor...
Characterization of scientific-grade CCDs is extremely important if one hopes to attain very precise...
We have performed end-to-end laboratory and numerical simulations to demonstrate the capability of d...
A common cause of errors in CCD differential photometry is an improper calibration of the array. The...
The accurate measurement of the position of celestial objects is a fundamental step for several astr...
Photometry is the measure of the brightness of an object. When making such measurements on stars, it...
Charge-Coupled-Device (CCD) cameras have opened a new world in astronomy and other related sciences ...
This paper summarizes the introductory presentation for a workshop (held Nov 18,19 2013 at Brookhave...
Differential photometry offers the most precise method for measuring the brightness of astronomical ...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2009.Includes bibliographica...
This book brings together experts in the field of astronomical photometry to discuss how their subfi...
The application of CCDs to star trackers and star mappers is considered. Advantages and disadvantage...
We describe the development of the fully depleted, back illuminated charge coupled devices for the T...
A front-illuminated development Euclid charge-coupled device (CCD) is tested to observe the CCD poin...
ABSTRACT. This paper summarizes a three-night observing campaign aimed at achieving millimagnitude-p...