WIYN 0.9-m Observatory
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 OBSERVING INFORMATION



  All the information necessary for observing at the 0.9m telescope is listed below.

     
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Acknowledgement

S2KB CCD Information

  • Technical Specifications

  • Date: 4/10/97 
    CCD NAME : S2KB 
    CCD SN : 1383BR03-01 
    PIXEL SIZE : 21x21 microns
    PIXEL SCALE : 0.60 arcsec/pixel
    CHIP SIZE : 2048 x 2048 
    DIGITAL LIMITATION : 65,534 
    BIAS LEVEL : ~750 (gain=#3)    
    MICROCODE : "Harcon1009" 
    PREFLASH, e- : none 
    NOISE,    e-/RMS : 14 9 8 7 
    GAIN, e-/ADU : 7.5 5.0 3.0 2.0 1.0  
    GAIN, DETPARS#: 1 2 3 4 5 
    LINEARITY,0.1%,e-: ~210,000 
    LINEARITY,1.0%,e-: ~230,000   
    COLUMN SPILLOVER, e- : ~240,000 
    INTERNAL RADIATION EVENT RATE, EVENTS/HR : ~2700    
    CONTROL TEMP. deg C (thermocouple) : ~-107 
    COMPUTER TEMP. deg C (ccdinfo) :    ~-109 
    DARK CURRENT, e-/hr/pix : ~5-10 
    DEAD COLUMNS : 
    HOT COLUMNS : [1571:1571,1134:2048] bias 
                                    : [2066:2066,1:2048] in overscan region, see comment below
    LOW COLUMNS : [1103:1103,744:2048] flat field
  • The quantum efficiency of S2KB is given in this figure. The abscissa is wavelength in nanometers and the ordinate is dQE (%).

  • Here are examples of the original calibration frames for S2KB. Click on the link to display the (BIG) image.

  • There is a hot column in the overscan region, [2066:2066,1:2048]. Check for the presence and position of this column in your data. You will probably NOT want to use the default BIASSEC in CCDPROC, but rather set BIASSEC to [2053:2064,1:2048] or a similar region of your choosing.

  • More recently, S2KB has developed an enhanced bias level in one corner amounting to a peak of ~1500 ADU above an overall level of ~965 ADU. Here is a bias exposure which shows this effect. The enhancement is limited to the region X < ~240 pix and Y> ~1800 pix.

  • You can estimate exposure times for S2KB using the CCDTIME package in IRAF v2.11.3 which should still have the necessary information in its ccdtime$kpno.dat database file. If it does not, here is the kpno.dat file.

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