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Handbook for the SX remote control Spectrograph    Issue 1, 17/8/20 

 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
The T2 thread is part of a removable barrel that is normally locked into a fine-focus sleeve by an M4 setscrew (accessible 
when the box cover is removed). The fine focus sleeve is itself driven by the large ring gear, which is seen surrounding the 
T2 adaptor. One rotation of this ring, moves the camera in or out by 0.75 mm, and permits the accurate focussing of the 
spectrum onto the camera sensor. 
 
As the spectrum is too long to be completely imaged with a typical CCD sensor, the focus assembly may be moved along 
the spectrum, by rotating the drive screw gearbox that is seen at the right hand end of the cross slide. This function is pro-
vided in the Spectrograph control software. 
 
As the grating is designed for a compact optical system, the available back focal distance for the imaging camera, is some-
what limited. It is typically about 20 mm maximum, and this is sufficient for most compact astronomical CCD cameras, but 
not for a DSLR. We recommend using either the SX-694 or SX-814 mono cameras for high resolution imaging with good 
sensitivity. Almost complete colour spectra may be recorded with an SX-M25C. The camera is screwed onto the T2 adaptor 
and the correct spectral orientation achieved by loosening the focus lock screw and rotating the T2 adaptor. The approxi-
mately correct focal position can also be achieved by setting the T2 adaptor extension and fixing it with the lock screw. Fine 
focusing is done via the spectrograph control software. 
 

Summary of Contents for SX Spectrograph PRO

Page 1: ...automated most of the spectrograph functions The remote spectrograph allows you to change slits adjust the imaging camera focus and wavelength setting and switch on a calibration lamp or flat field l...

Page 2: ...es a Lodestar X2 guide camera which observes the image field via a 10 90 beam splitter cube The slit is not directly visible in the field but its position co ordinates are provided and marked by a cur...

Page 3: ...the wavelengths of the lines from any external source A typical calibration spectrum imaged with an M25C colour camera A spectrum with wavelength markers is provided in the appendix The optical input...

Page 4: ...d of the cross slide This function is pro vided in the Spectrograph control software As the grating is designed for a compact optical system the available back focal distance for the imaging camera is...

Page 5: ...Handbook for the SX remote control Spectrograph Issue 1 17 8 20 A general view of the optical and mechanical layout...

Page 6: ...bottom info strip The spectrograph is automatically started with the slit set to the highest resolution position Number 1 20 microns wide x 1 mm high This is usually the best setting for general purpo...

Page 7: ...have the Lodestar drivers and software installed please follow these instructions To install the Lodestar driver use the supplied stick to copy the appropriate driver files to a convenient folder on y...

Page 8: ...size of the spectrograph slit assuming that the 1 mm x 20 uM slit is in use The slit cursor position will probably need adjusting to match your spectrograph The nominal setting will be provided on a l...

Page 9: ...ee several stars when using a 1 or 2 second exposure and be able to refine the focus until the stars are sharply defined If you have a test target in mind slew to this object and find a good bright gu...

Page 10: ...ry slew ing the scope slightly East or West before taking another image The Adjust lock position in the Tools menu of PHD2 is good for this If the brightness falls off for both directions then the sli...

Page 11: ...e such as RSpec see below These simple instructions are sufficient for capturing a spectrum but you will probably want to identify spectral lines and perhaps perform further analysis of the data To th...

Page 12: ...the calibration chart The small double peak at the right is caused by sodium light pollution and is not in the calibration chart You can see that the spectrum is quite linear and matches the referenc...

Page 13: ...lected slit The slit widths available 1 20uM x 1mm 2 30uM x 2mm 3 55uM x 2mm 4 115uM x 2mm 5 325uM x 2mm 6 3mm diameter clear aperture For maximum light input with point sources stars or small nebulae...

Page 14: ...with the angle to achieve a different spectral width or line shape The theoretical best angle is marked by a groove in the floor of the spectrograph but a varia tion of two or three degrees in either...

Page 15: ...2 mm Position 5 325 uM x 2 mm Position 6 3mm x 3 mm circular Input Output Female T2 thread 42 x 0 75 mm input Male T2 thread output Input back focal distance approximately 37 mm Output back focal dist...

Page 16: ...1 The equipment shall only be used for normal purposes described in the standard operating instructions and within the relevant safety standards of the country where the equipment is used 2 Repairs u...

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