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  * Conversion wavelength - grating position:   * Conversion wavelength - grating position (based on ILT-1) :
     || Band || Order || Filter || wavelength || Grating position ||
     || R1 || 1 || n/a || 210um || 96K ||
     || || || || 100um || 991K ||
     || B2B || 2 || B || 100um || 301K ||
     || || || || 70um || 812K ||
     || B2A || 2 || A || 70um || 812K ||
     || || || || 53um || 1040K ||
     || B3A || 3 || A || 70um || 183K ||
     || || || || 50um || 740K ||

  * Other wavelengths in the PCSS:
    {{{
from spec import *

print wave2GratPos(105., "B2", 8, calVersion="FM_1_0")
print gratPos2Wave(1000000, "B2", 8, calversion="FM_1_0")

    }}}

FM ILT reference numbers

Ge:Ga detector settings

  • Blue
    • par

      value

      comment

      Bias d

      198 mV

      From bias / heater loop test

      Bias r

      10 mV

      Component level value - to be verified on CRE checkout test

      Heater

      1.5 mA

      Result from bias / heater loop test (2.68K/1.84mA) exceeds thermal budget

  • Red
    • par

      value

      comment

      Bias d

      69 mV

      From bias / heater loop test

      Bias r

      10 mV

      Component level value - to be verified on CRE checkout test

Grating

  • Configuration table: CONFGrat. Column : FMILTFast / FMILT_R_Fast for redundant
  • Allowed working range :
    • 45K - 1045K (nominal)
    • 65K - 1065K (redundant)
  • Conversion wavelength - grating position (based on ILT-1) :
    • Band

      Order

      Filter

      wavelength

      Grating position

      R1

      1

      n/a

      210um

      96K

      100um

      991K

      B2B

      2

      B

      100um

      301K

      70um

      812K

      B2A

      2

      A

      70um

      812K

      53um

      1040K

      B3A

      3

      A

      70um

      183K

      50um

      740K

  • Other wavelengths in the PCSS:
    • from spec import *
      
      print wave2GratPos(105., "B2", 8, calVersion="FM_1_0")
      print gratPos2Wave(1000000, "B2", 8, calversion="FM_1_0")

Chopper

  • !!! Do NOT use the chopper in redundant mode !!!
  • Configuration table CONFChopper / column : CSLopt3-600
  • Accessible range : -23500 to +23000
    • At +/- 25000 a field plate limit disables the controller
  • Conversion chopper position - angle on the sky - FPU angle
    • FPU Angle

      Sky Angle

      Chopper pos

      Comment

      -7.6 deg

      -5.8 arcmin

      -21350

      center CS1 (determined from PHOTO FoV map)

      -2.2 deg

      -1.8 arcmin

      -6700

      Photometer chop field A

      0.2 deg

      0 arcmin

      664

      Optical zero - value from Zeiss measurements

      2.7 deg

      1.8 arcmin

      8000

      Photometer chop field B

      7.9 deg

      5.7 arcmin

      +21200

      center CS2 (determined from PHOTO FoV map)

  • Other angles - in the PCSS (release >20070303A) :

    • from all import *
      
      chopPositions = Double1d([-21350.,-6700., 664., 8000., +21200.]) # CS1, PhotLeft, Center, PhotRight, CS2
      
      # Chopper positions to FPU angles (deg)
      print chopPos2FpuAnglePol(chopPositions)
      
      # Chopper positions to Sky angles (arcmin)
      print chopPos2FpuAnglePol(chopPositions-664)*60/80.69
      
      
      # FPU angles (deg) to Chopper positions
      fpuAngles = Double1d([-4, 4])
      print fpuAngle2ChopPosPol(fpuAngles)
      
      # Sky angles (arcmin) to Chopper positions
      skyAngles = Double1d([-3, 3])
      print 664 + fpuAngle2ChopPosPol(skyAngles/60*80.69)
  • Chopper step to move over one pixel - depends on chopper position
    • Chop pos

      Blue phot (3.2")

      Red phot (6.4")

      Spectro (9.4")

      -21350 (CS1)

      163

      325

      476

      -6700

      218

      436

      640

      664

      221

      441

      648

      8000

      209

      417

      614

      21200 (CS2)

      151

      302

      445

  • At other positions - in the PCSS (release >20070303A):

    •        bluePhotSky = 3.2 # Blue photometer pixel on the sky (arcsec)
             fpuAngle = -7.6   # degrees - chopper angle at which to calculate the delta position
             chopPos = fpuAngle2ChopPosPol(Double1d([fpuAngle]))
             offsetChopPos = fpuAngle2ChopPosPol(Double1d([fpuAngle - bluePhotSky * 80.69/3600])
             print offsetChopPos

Filter Wheel PHOT

  • POS A = Long wavelength (Green)
  • POS B = Short wavelength (Blue)

Filter Wheel SPEC

  • POS A = Short wavelength (50-70um)
  • POS B = Long wavelength (70-100um)

Calibration sources

  • CS1
    • 48 Ohm = 55K
    • Chopper position center : -21350
  • CS2
    • 58 Ohm = 60K
    • Chopper position center : +21200

XY stage

  • Scale: 1" on the sky = 0.18mm
  • Spectrometer
    • Focus : +5mm (from FMILT-1, not incompatible with spectro FMILT-2)
    • 1 pixel = 9.4" = 1.692mm
    • Center spectro field :
      • X stage (mm)

        Y stage (mm)

        RED

        -12.7628

        0.938300

        BLUE

        -12.6774

        1.15180

  • Photometer
    • Focus : +5mm (from FMILT-1)
    • 1 blue pixel = 3.2" = 0.576mm
    • 1 red pixel = 6.4" = 1.152mm
    • Center field :
      • x = 4 mm
      • y = 1.5

Herschel: FmIltProc/ReferenceNumbers (last edited 2009-07-15 14:32:37 by localhost)