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About FraserClarke

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  1. Nice. In the interests of minimising weight -- what purpose does the top-ring serve in the design?? Seems like you could lose those grams without affecting anything??
  2. Wikipedia gives a formula here; https://en.wikipedia.org/wiki/Heliocentric_Julian_Day It depends on the distance to the sun. Depending on the accuracy you need, you either use the mean value, or calculate it for the specific time (few % difference only) What language are you using? There may well be a library which does all this for you already of course...
  3. Have you got an OAG in the train? Looks a bit like something like that just creeping into the beam...
  4. Some of my favourites from the past 20 years; 1) On an old (late 1980s) computer with just enough disc space for one night's worth of data, zipping up the previous night's data to transfer, and then doing; rm *,fts (rather than: rm *.fts) before I'd done the transfer.... Deleted the entire night's data... 2) Taking a 20 minute exposure of a flat field lamp because I forgot to move a mirror (on the Palomar 200-inch) 3) Leaving the flat field lamp on in the observatory overnight and wondering why the background was so high... (last night) Nothing to do with being a newbie -- being more exp
  5. In principle yes. Not sure about the specific optics combinations. We use this kind of set-up to demonstrate spectroscopy indoors. We set a small telescope up looking at a pair of pinholes ~20m away (with an eyepiece). They look just like a pair of identical stars. Then we flip in an SA-100 grating; and hey-presto -- you clearly see that one of the pinholes is illuminated by an incandescent bulb (continuum spectra), and the other by energy-saving/CFD bulb (whole bunch of emission spectra). They're not identical at all, despite what they 'look' like!
  6. Well I have a lakeside controller driving a moonlite stepper -- so you can combine both if you want! The moonlite stepper itself has not had a single problem in the past 4--5 years for fairly intensive operation (50-100 nights/year). The moonlite stepper controller however developed an increasingly frequent problem with communincation dropping out and needing to be reset manually (pull out the USB lead and plug it in again -- pretty inconvenient for a basically robotic observatory). I think this was down to a dodgy joint somewhere in the power connector electronics, but I could never track
  7. X axis of the chart is the Abbe number, which as Nigel says is a measure of dispersion. Low Abbe number corresponds to higher dispersion. Combining glasses with high and low dispersion is how you achieve chromatic correction in lenses. Unfortunately glass isn't evenly distributed across this diagram, so you don't have infinite choice in the combinations... There is a general (negative) correlation between Abbe number and refractive index.
  8. Have you spoken to diffraction limited? If you have the licencing information, they might well be able to get you a copy of MaximDL5. I think they have a good list of all the licences/customers, and they've been pretty helpful sorting out issues with multiple licences I've had with them...
  9. That looks like a pretty classic polar alignment error. The field appears to rotate around the guide star (presumably you're using an off-axis guider, which is located just "above" this image?) because the guider forces the telescope to stay pointing exactly on the guide star, and therefore forces the scope to wander around to keep it in the right place. How "pretty much bang on" are you with the polar alignment? The fact the trails are not the same all across the image is probably telling you how far off, and in which direction, the polar alignment is -- but I'm afraid I'm not quite clever
  10. Yes, this also happens on our (old) ST8 camera. The cooling system pulls the CCD chip down fastest, so any moisture condenses there first. As the rest of the system gets colder, the ice sublimates off the chip and ends up on whatever is the coldest bit. It's a good sign the desiccant needs replaced/regenerated. I do the same as Zakalwe -- cooling in steps to try and make the chip not the coldest bit. I also leave the camera cooling running all the time (permanent observatory), only letting it warm up to -5C between observing sessions. In professional instruments we spend a fair bit of effort
  11. ACP also uses astrometry.net as a back up when the local solve fails. I'd still rather download the catalogs once and during a daytime than waste time/bandwidth repeatedly uploading images during nighttime though...
  12. A google search returns; http://deepskypedia.com/wiki/List:Terzan All near the centre of the MW, so late summer/early autumn objects...
  13. The cameras on professional telescopes are effectively very fancy focal reducers (combined with filter wheels, gratings, focusing mechanisms, etc), and they tend to work around F/2. Going faster is possible (I've seen designs for F/0.9 cameras), but is expensive, complex, and usually only works in very specialized cases. A hyperstar is probably the closest you'll get in the amateur world I guess...
  14. Yeah, Rubbish data is worse than useless, because it costs you time afterwards trying to salvage something... Best just to chuck it. Even with professional telescopes, it takes a few attempts to realise it's pointless trying to take data if the conditions aren't up to it -- it's a better use of time just to sit idle...
  15. I've done a bit of stuff with Maxim scripts (usually scripting maxim from an external programme). I don't have any examples to hand, but I always trip myself up by thinking it's more complex than it is! The interface and calling structure is very simple -- so much so it usually seems to me that it shouldn't work :-\
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