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

 

Handbook for the SX Spectrograph PRO with remote control 

 
 

 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
Introduction: 
 

Spectroscopy of astronomical objects is a relatively unexplored field for many amateur observers, as truly compact, inex-
pensive and effective spectrographs have been unavailable until recently. This situation is now changing and spectrometry is 
becoming popular as a way to extend the scientific value of amateur observations and to add a new dimension to the hobby. 
The first SX Spectrograph was introduced in 2016, but was intended for local operation, where the user could change slits, 
focus etc., by hand. The market has since evolved to include many remote observatories, well beyond the direct reach of the 
observer, so we have now 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 lamp, remotely. 
 

General description: 
 

The SX Spectrograph PRO is only 125 x 140 x 75 mm and weighs just over 1 Kg. It is solidly constructed in a machined 
aluminium enclosure and so will not flex during use. The optical design is based on a highly corrected, 550 groove concave 
reflecting grating, that provides a spectral length of 31 mm from 340 to 900 nM. The entire spectrum is accessible by adjust-
ing a sliding camera carrier, using a motor driven threaded drive screw, but most of the visible spectrum can be seen without 
adjustment, when using an SX694 imaging camera. A 6 position slit wheel, with various slit widths and lengths, is provided 
and will allow the sensitivity and resolution to be optimised for the user’s project. The best resolution R factor when using 

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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