User Tools

Site Tools


vatt:instrumentation_and_computers

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
vatt:instrumentation_and_computers [2021/03/31 12:54]
paul [VATT CCD Spectrograph - VATTSpec]
vatt:instrumentation_and_computers [2021/03/31 21:23] (current)
paul [Instrument Interface (a.k.a. the Guider Box)]
Line 6: Line 6:
  
   * [[vatt:vatt4k|VATT4k]]   * [[vatt:vatt4k|VATT4k]]
-  * A replacement STA0500A back illuminated 4K CCD, ITL serial number 8301, was installed March 2017, and updated 26 January 2018. 
-  * It is similar to the September 2007 one, including its QE. 
-  * Pixels: 4096x4096, 15x15 microns 
-  * Gain:1.9 e/DN 
-  * Full well: ADC limited (65k DN) = ~120,000 electrons unbinned 
-  * Noise: ~3.9 electrons 
-  * Photon Transfer Curve 
-  * Gain Curve 
-  * FOV: 12.5 arcmin square 
-  * pixel scale: 0.188 arcsec/pixel 
-  * wavelength range: 300 - 1000 nm, peak 96% at 450 nm 
-  * Preamplifiers added October 2008 inside the dewar. These give faster readout and lower noise. 
    
  
Line 25: Line 13:
   * Field of view on VATT, 3 arcmin with current focal reducer.   * Field of view on VATT, 3 arcmin with current focal reducer.
   * On loan from NUI Galway, currently until June 2011.   * On loan from NUI Galway, currently until June 2011.
-  * Consult Richard Boyle for technical details, and see the NUI Galway "Brown Dwarfs and Substellar Objects" group.+  * Consult Richard Boyle for technical details, and see the [[http://astro.nuigalway.ie/astro/research/cool_stars_brown_dwarfs_exoplanets/|NUI Galway "Brown Dwarfs and Substellar Objects" group]].
    
  
Line 31: Line 19:
  
   * [[vatt:vattspec|VATT Spectrograph]]   * [[vatt:vattspec|VATT Spectrograph]]
-  * This optical region spectrograph has AR coated refractive optics, with a beam size at its camera of 125 mm, giving ... 
-  * slit length: 30 arcsec 
-  * wavelength range: 360 - 950 nm 
-  * spectral coverage: 100 nm at 0.1 nm resolution 
-  * spectral resolutions: 0.1, 0.2, and 0.4 nm with 1 arcsec wide slit 
-  * detector: back illuminated, low noise CCD STA0520A, with very nice cosmetics. 
- 
-     ITL Serial Number 8228 
-     2688x512 pixels, 15x15 microns 
-     Detector operating temperature -110C 
-     Gain: 1.3 e/DN with setting 10; 2.6 e/DN with setting 5 
-     Full well, both gains: ADC limited (65k DN) = 85,000 or 170,000 electrons 
-     Noise: 3.4 electrons (3.2 in overscan region) 
-     QE Curve 
- 
-  * [[VATT:vatt-vattspec_efficiency|efficiency]]: determined by Mark Wagner for telescope plus spectrograph 
-  * further details are under the [[vatt:vattspec-gen-instructions|Instructions for use of the VATT Spectrograph]]. 
-  * bandpass filters available: S8612 (red blocking); GG-400, GG-475, OG-550 (cut-offs to the blue in nm). 
- 
 ===== Instrument Interface (a.k.a. the Guider Box) ===== ===== Instrument Interface (a.k.a. the Guider Box) =====
  
Line 55: Line 24:
   * effective back focal distance, from guide box to focal surface, is 2.000".   * effective back focal distance, from guide box to focal surface, is 2.000".
   * contains two filter wheels, each holding four 3.48" square filters. Adapters to accommodate 2" and 3" square filters are available.   * contains two filter wheels, each holding four 3.48" square filters. Adapters to accommodate 2" and 3" square filters are available.
-  * UBVRI, uvby, Vilnius, Sloan, ECAS, and Order Blocking filters are currently provided.+  * UBVRI, uvby, Vilnius, Sloan, ECAS, and Order Blocking [[vatt:filters|filters]] are currently provided.
   * integrating sphere with continuum and calibration lamps.   * integrating sphere with continuum and calibration lamps.
vatt/instrumentation_and_computers.1617220492.txt.gz ยท Last modified: 2021/03/31 12:54 by paul