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

 
 

 

 

 
 
You can now see if the spectrograph will give a spectrum from an object within the slit cursor of PHD. To test this, switch 
off guiding in PHD2, set PHD2 to looping images, and then slew a bright star into the spectrograph slit cursor box. The 
slewing can be done by using the ‘Manual guide’ option in PHD2, or by operating your telescope controls. Centre the star in 
the slit cursor and then select it as the guide star, so that PHD2 keeps it in position. 
 
Imaging a test spectrum: 
 
1) Centring the slit: 
 
I will assume that you already have a camera attached to your spectrograph and that the imaging software is connected to 
this camera. Almost any software can be used - the SX software, Maxim DL, Sky X, AstroArt, Nebulosity etc., just set an 
exposure of about 5 seconds and see if a spectrum can be seen on your computer monitor. There is a good chance that some-
thing will be visible, but you can try a longer exposure, if necessary. Note the brightness of the spectrum and then try 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 slit cursor is correctly positioned, otherwise adjust the 
cursor co-ordinates to optimise its location. Note that the optimum position is likely to be slightly different for each slit 
width, so you may want to keep a note of the co-ordinates for each slit for future reference. 
 
2) Focusing the spectrum: 
 
Having centred your test star in the slit, take an exposure of a few tens of seconds to examine the quality of the spectrum. If 
the star is yellow or red (e.g. Arcturus), you should see plenty of dark absorption lines - white or blue stars, such as Vega, 
will have only a few hydrogen lines on a uniform continuum. If the dark lines are clearly defined, then the camera is in fo-
cus, otherwise try pressing the ‘Focus’ buttons to see if you can improve it. Seriously out of focus spectra may need the lid 
to be removed and the coarse focus lock screw loosened to allow the T2 adaptor to get closer to the correct focus position. I 
also recommend that you rotate the camera so that the spectrum is close to parallel to the long axis of the CCD. 
 
 

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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