Omega Prime - Technical Characteristics
and Astronomical Performance


Calar Alto
Homepage 
MPIA
Homepage 

Array Type Rockwell 1024 x 1024 pixel HAWAII array: 
HgCdTe detector + Si MOSFET non-destructive readout 
Pixel scale 0.3961±0.0004 arcsec/pixel
Field of View 405.6 arcsec square (6.76 arcmin square) 
Wavelenth range 1.0 µm - 2.5 µm 
Telescope Calar Alto 3.5m (prime focus)

Sensitivity:
For point sources to the 5 sigma level (i.e. the brightest pixel in the centre of the star is at 5 times the background noise), with two minutes integration time (not including any overheads for detector read out etc.), and with a seeing of 1 arcsec FWHM.
 

K' = 17.5 mag H = 18.1 mag J = 19.2 mag

Filter options:
All filter data determined at 77 Kelvin! A tracing of the filter transmission curve (sorry for the low-quality) can be found by clicking on the filter name (please, note that the transmission curve have been determined in parallel beam).
Last update: Jan 2002

A. Guijarro
 
Filter Central
Wavelength
(µm)
FWHM
Width
(µm)
Tpeak
(%)
cut on
50% T
(µm)
cut off
50% T
(µm)
Thickness
(mm)
Status
J 1.275  0.290  82  1.130  1.420  in 
H 1.646  0.305  80  1.493  1.798  in 
Km =K' 2.118  0.348  96  1.944  2.292  in 
Ks 2.196  0.388  85  2.002  2.390  in 
K 2.215  0.419  81  2.008  2.427  in 
H-short 1.564  0.145  84  1.491  1.636  in 
H-long 1.775  0.218  90  1.672  1.878  in 
BDS
short end K
2.080  0.257  91  1.951  2.208  in 
BDL
long end K
2.281  0.263  95  2.150  2.413  N/A 
NB1.644
FeII
in 
NB2.122
H2 1-0 S(1)
2.125  0.0206
(0.97%)
82  in 
NB2.144
K Cont.
2.143  0.0227
(1.06%)
85  in 
NB2.166
Bracket gamma
2.170  0.0219
(1.01%)
74  2.159  2.182  1.9  in 
NB2.248
H2 2-1 S(1)
in 
NB2.295
CO
2.291  0.0215
(0.94%)
65  2.281  2.302  1.9  in 

A Schematic diagram [17 kB] of Omega-prime is also available.

Click here to return to the Omega-Prime Home Page


Peter Bizenberger Dave Thompson
E-mail: Peter E-mail: Dave
Phone: +49 (6221) 528-311