A full set of flat field calibration files for the NUV MAMA has been generated from pre-flight laboratory data. An iterative technique with 12 passes through each raw flat data image is used to separate the illuminating lamp signature from the high frequency struc-ture of the MAMA flat itself. The set of flats consists of one wavelength independent P-flat that corrects for the high frequency pixel-to-pixel sensitivity variations and 63 L-flats that correct for the lower frequency, wavelength dependent variations. The S/N of the counting statistics of the P-flat is over 300 per MAMA resolution element (2x2 lores pixels.) On-orbit tests are required to confirm the validity of the ground based flats for the reduction of flight data. 1
The first six months of flight data from the Multiband Imaging Photometer for Spitzer (MIPS) were us...
There are consistent problems that occur during the process of capturing astronomical images which c...
International audienceEuclid is an ESA mission to map the geometry of the dark Universe with a plann...
A full set of flat field calibration files for the NUV MAMA has been generated from pre-flight labor...
Abstract. The Space Telescope Imaging Spectrograph (STIS) was designed to achieve a signal-to-noise ...
The Space Telescope Imaging Spectrograph (STIS) is a second generation HST instrument with three 2-d...
One of the goals in any calibration effort for pushbroom imaging radiometers is to flat field the in...
Self-calibration flat fields are compared to super-sky flat fields for simulated JWST images in this...
Recent imaging pushbroom radiometers with up to 30000 detectors per band in multiple modules and wit...
This is the release intended for use during the JWST Cycle 1 call for proposals Updates in this vers...
The National Ecological Observatory Network (NEON) is a continental-scale ecological observation fac...
We describe an archive of high-precision MDI flat fields that can be used to refine most MDI high-re...
In this study, the observations from S-NPP VIIRS Day-Night band (DNB) and Moderate resolution bands ...
We analyse the applicability of the two-flat-test calibration method across wide spatial frequency r...
The effects of the stationary noise patterns and variable pixel responses that commonly occur with u...
The first six months of flight data from the Multiband Imaging Photometer for Spitzer (MIPS) were us...
There are consistent problems that occur during the process of capturing astronomical images which c...
International audienceEuclid is an ESA mission to map the geometry of the dark Universe with a plann...
A full set of flat field calibration files for the NUV MAMA has been generated from pre-flight labor...
Abstract. The Space Telescope Imaging Spectrograph (STIS) was designed to achieve a signal-to-noise ...
The Space Telescope Imaging Spectrograph (STIS) is a second generation HST instrument with three 2-d...
One of the goals in any calibration effort for pushbroom imaging radiometers is to flat field the in...
Self-calibration flat fields are compared to super-sky flat fields for simulated JWST images in this...
Recent imaging pushbroom radiometers with up to 30000 detectors per band in multiple modules and wit...
This is the release intended for use during the JWST Cycle 1 call for proposals Updates in this vers...
The National Ecological Observatory Network (NEON) is a continental-scale ecological observation fac...
We describe an archive of high-precision MDI flat fields that can be used to refine most MDI high-re...
In this study, the observations from S-NPP VIIRS Day-Night band (DNB) and Moderate resolution bands ...
We analyse the applicability of the two-flat-test calibration method across wide spatial frequency r...
The effects of the stationary noise patterns and variable pixel responses that commonly occur with u...
The first six months of flight data from the Multiband Imaging Photometer for Spitzer (MIPS) were us...
There are consistent problems that occur during the process of capturing astronomical images which c...
International audienceEuclid is an ESA mission to map the geometry of the dark Universe with a plann...