Originally posted by cheekygeek Sorry for the question dump! Thanks for any replies. I hope to take another run at it tonight.
Some very good questions cheekygeek - and actually a good script for you to make your own tests and experiences, because hardly any astrophotographers - including astrotracer users - do things exactly in the same way and sequence. But here are some answers from my point of view, actually very much in line with gleeman's above:
1. How do you determine the proper exposure for your sub-exposures? Do you want the histogram spike to be just off the left edge?
Using histograms doen't make much sense to me. I shoot under skies where light pollution plays it's heavy hand. But I do use the LCD viewer a lot. If I can see my subject, if only just and barely, on top of the light pollution I know that I have captured some excess photons to work with.
Unprocessed image, DA* 200mm lens at f/3.5, 20 seconds and ISO 1600. Shot in late July under a very bright summer night sky.
Click on images to see larger versions.
2. Do you find that the menu is wildly over-optimistic in what it says your maximum time of exposure is possible?
That depends. There is obviously a significant difference in shooting a 5000 px wide image for un-cropped and downsized viewing on the web and then for shooting with tight, 100% "pixel-to-pixel" presentation in mind:
Uncropped stack of Hercules-M13 images. Same exposure details as above.
Non-resized 100% crop of the above. I.e.: Each pixel that you see matches one pixel on the sensor.
Obviously, you will have to establish your own limit as to acceptable drifts. My limit is usually around 4 pixel widths and in that case, I should say that stated maximum exposure times are overly optimistic. But I think the times shown assume "uncropped images for web-viewing".
3. I shoot in RAW+, is that OK?
That is perfectly OK. I do the same. raw-files have the obvious benefit that there are 12 or 14 bit levels for the stacking software to work with and thus, you should be able to get a better dynamic range in the final picure when that is needed.
4. Are you going to see results in the JPEGs or only after you have stretched the histogram in post-processing?
See also answer to Q1. above. You will never get near to an acceptable result without some serious post-processing but here's a small dirty trich, reference the image for Q1: Autostretch your levels. That will (normally) give you a clear indication of whether you have captured enough excess light to work with:
Same Image as 1 above. Levels stretched.
And then, finally:
Stacked, Post-Processed and Cropped final result.
5. Do you turn Auto-ISO off?
Yes, by all means! Your camera doesn't have a chance to guess, what scene you are shooting.
6. What about noise reduction?
You should turn all type of noise recuction off. BUT DON'T "CHEAT" and leave flat-frames and dark-frames out of your work-flow. You can stack without such frames, but results will usually be MUCH better if you do that extra effort.
7. Any other camera menu settings that I should change?
If you use JPEG-files, you should set white balance to Daylight and not Auto. I may also immodestly refer to my tutorial on camera settings for astrphotography here:
Camera Settings for Astrophotography 8. Any tricks for "locking down" your lens focus once you have it? (I'm using manual lenses... trying the K 135mm f2.5 (at f4)
That's a VERY fine lens to start with. I would avoid using lenses with any tendency to focus creep (or zoom-creep, but I prefer not to use zoom lenses). However, my Tamron Adaptall-2 350mm mirror lens is exceedingly sensitive to proper focus, and here, I often use a small piece of tape to fix focus once I am confident, that my system is in thermal equilibrium. I establish focus and check it regularly using live view on a brigt star at maximum (8X or 10X) magnification.
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Whising you a lot of pleasure and fun under the stars!