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Home > Information for Researchers > 1st Generation Instruments > Guider Cameras

1st Generation Instruments
HAWC High-resolution Airborne Wideband Camera
EXES
Echelon-Cross -Echelle Spectrograph
FIFI LS Field Imaging Far-Infrared Line Spectrometer
FORCAST Faint Object InfraRed CAmera for the SOFIA Telescope
GREAT German Receiver for Astronomy at Terahertz Frequencies
FLITECAM First Light Infrared Test Experiment CAMera
HIPO High-speed Imaging Photometer for Occultations
GUIDERS Guider cameras
WV MONITOR Water Vapor Monitor

Guider Cameras

SOFIA has three acquisition/guider/tracking cameras, the Wide Field Imager (WFI), the Fine Field Imager (FFI),and the Focal Plane Imager (FPI), which are designed to determine where the telescope is pointed on the sky and provide telescope pointing corrections via optical tracking on guide stars. The WFI and FFI are mounted on the telescope head ring and can be seen in the photograph below. The FPI images the telescope focal plane via a dichroic and a second tertiary mirror. All three cameras operate at optical wavelengths. The properties of the imagers are given in the table below.

 

Parameter

FPI

FFI

WFI

notes

Optics description:

main 3.5m TA (Cassegrain) + 8x reduction

Schmidt-Cass + field expander

F/2 Petzval lens

FPI has ±60 cm focus range, reticle, reimaging optics

aperture diameter:

2500 mm

254 mm

68 mm

 

FOV:

9’ diam.

67’ x 67’

6.0° x 6.0°

 

image scale (arc—sec/pixel):

0.55 ”/pxl

4.1 ”/pxl

21 ”/pxl

FPI scale varies 10% over focus range

star image size:

(80% Enc Energy)

7 ”

13 ”

~1.2 ’

FPI seeing-limited;

FFI, WFI optics limited

R-band sensitivity:

(S/N = 10 in 1 s)

13

11

9

 

centroid precision:

(S/N = 10)

~0.05 ”

~1 ”

~8 ”

 

Filters available:

  • 3 ND’s
  • red (day)
  • clear
  • blankoff
  • 3 ND’s
  • red (day)
  • clear
  • blankoff
  • 3 ND’s
  • red (day)
  • clear
  • blankoff

ND T: 8% - 75%

“red” = Schott RG1000

( l > 900 nm)


All three imagers use the same model Proscan "High Speed Slow-Scan" camera, containing a Thomson 7888A frame transfer CCD. The basic (nominal) properties of this CCD are given here:

Parameter

Value or range

Notes

Array dimensions:

1024 x 1024 image area

frame transfer readout

Pixel size:

14 microns

 

Binning options:

1x1, 2x2, 4x4

4x4 done off chip

Integration time:

10 – 10,000 ms

 

Data format:

14-bit or 8-bit

2 MHz or 5 MHz rate

Maximum frame rate:

8 frames / s

2x2 binning, 5 MHz

Peak Q. E.:

18% at l 550 nm

electronic shutter, fill factor

Read noise:

60 e - = 5 DN

 

Dark current (25 °C):

12500 e -/s

No FPI cooling, CCD ~at cabin temperature in flight

Dark current (-20 °C):

200 e -/s

Likely for WFI, FFI

Gain (14-bit mode)

12 e - / DN

~600 e -/ DN in 8-bit mode

saturation

170,000 – 200,000 e -

 

The imagers acquire star field frames and on-board control software correlates the star positions with star catalogues to determine the attitude of the telescope with respect to the sky. The guider camera images can also be captured during flight and saved as FITS files; they will be archived along with the science instrument data. The two image pairs shown here provide a comparison between images acquired with the WFI during tests in the summer of 2004 and star charts for the associated fields. Initial tests indicate that the WFI should perform quite well during SOFIA science missions.

 

 

Page Last Updated: July 15, 2011

 

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