Gain
1.74 e-/adu
Readnoise
~13.0 e- with T_CCD = -10 deg C
Bias
Level
100 adu = 174 e-
Dark Count
Rate
0.95 adu/sec = 1.65 e-/sec
Full-well
capacity
180000 e- , 65535 adu - bias level and dark count
Pixel
size
20 micron x 20 micron
Pixel
scale
0.809"/pix
Size of
Science CCD
512 pix x 512 pix
Science CCD Field of
View 6.9' x 6.9'
Size of Tracking
CCD
190 pix x 162 pix
Tracking CCD Field of
View 2.6' x 2.2'
Imaging
Mode:
ST-8E CCD
Gain 2.68 e-/aduDispersion 4.1 Angstrom/mm = 0.37 Angstrom/pix
Readnoise 18.6 e- with T_ccd = -10 C
Full-well capacity 16383 adu (unbinned), 32500 adu (2 x 2 binning)
Pixel size 9 micron x 9 micron (unbinned)
Size of Detector 1534 pix x 1020 pix (unbinned)
Pixel scale 0.728"/pix (2 x 2 binning)
Field of View 9.3 arcmin x 6.2 arcmin (2 x 2 binning)Imaging Mode:
Photometric calibration of the telescope + ST8 CCD + BVRI filters was performed on Nov 13, 1999 when 12 standard stars in 4 Landolt fields were observed. From 32 to 42 separate observations were made in each filter. The derived calibration equations listed below convert instrumental magnitudes (bvri) to standard magnitudes (BVRI). They are valid for stars with -0.04 < (B-V) < 1.06 and 1.20 < airmasses < 1.73. Note that the zeropoint of 25 mag corresponds to a flux of 1 adu/sec = 2.68 e-/sec.
v = V + 5.479 (+/- 0.033) + 0.023 (+/- 0.049) * (B-V) + 0.397 (+/- 0.086) * (X-1.25)
b = B + 6.263 (+/- 0.028) - 0.209 (+/- 0.038) * (B-V) + 0.610 (+/- 0.072) * (X-1.25)
r = R + 5.064 (+/- 0.014) + 0.065 (+/- 0.020) * (B-V) + 0.359 (+/- 0.036) * (X-1.25)
i = I + 5.919 (+/- 0.014) - 0.018 (+/- 0.019) * (V-I) + 0.225 (+/- 0.032) * (X-1.25)Filter Average Flux (e-/sec) Surface Brightness of the Night Sky for New Moon Phase
from an M=15 mag star (mag/arcsec^2) (e-/pix/sec)U 15. 16.5 5.9
B 125. 17.9 13.9
V 158. 17.5 29.9
R 229. 17.0 65.5
I 111. 14.8 249.0The New SBIG Self-Guiding Spectrograph (w/o binning):
Dispersion 1.067 Angstrom/pix = 0.1186 Angstrom/micron
Resolution TBD
Wavelength Coverage 1637 AngstromThe Old Spectrograph (w/o binning):
ST-7 XE ABG CCD used w/ the 8" Meade Telescopes
Gain ~ 2.3 e-/aduST-6 CCD used on the Finder/Guider Telescope
Gain 6.7 e-/adu
Readnoise 30 e-
Full-well capacity 400000 e- = 65535 adu
Pixel size 23 micron x 27 micron
Pixel scale 4.0 "/pix x 4.75 "/pix
Size of Detector 375 pix x 242 pix
Field of View 25.0 arcmin x 19.2 arcmin
ST-6 CCD used on the 24" Telescope
Gain 6.7 e-/adu
Readnoise 30 e-
Full-well capacity 400000 e- = 65535 adu
Pixel size 23 micron x 27 micron
Pixel scale 0.98" x 1.1"
Size of Detector 375 pix x 242 pix
Field of View 6.1 arcmin x 4.6 arcminThe following photometric data were determined from observations of 10 standard stars in the Landolt SA 92 field on August 28, 1996:
Filter Average Flux (e-/sec) Surface Brightness of the Night Sky for Full Moon Phase
from an M=15 star (mag/arcsec^2) (e-/pix/sec)B 174 18.81 5.84
V 235 18.23 13.4
R 260 17.40 31.9