Showing posts with label Patriot Astrophotography. Show all posts
Showing posts with label Patriot Astrophotography. Show all posts

Sunday, August 21, 2022

Backfocus & Hocus Focus (a NINA plugin) and a New Image

Backfocus

When I first heard about the focusing plugin Hocus Focus (HF) I was unsure if it was something I wanted. NINA's built-in autofocus seemed to work perfectly. Then I watched one of the Patriot Astronomy videos that demonstrated what else HF can do and I realized I not only wanted it, but I needed it!

HF (created by George Hilios) features what he calls Aberration Inspector. Much of what it does is beyond my ability to intepret meaningfully, much less act on. But it has one key ability: to measure error in backfocus. Having proper backfocus is a problem when using focal reducers.

If the backfocus isn't right, you won't be in focus across the field; if you focus on stars at the field's center, stars in the corners will be out of focus. This is why an old fix for this problem is to focus on stars some distance out from the center. Like most compromises it's hardly a perfect solution: stars in the center and corners will be slightly out of focus.

The better remedy is to get the backfocus as close to correct as possible. Usually this means taking images, examining them closely, guessing the distance of the correction to make, making the correction, then shooting more images, etc. It's time consuming and inexact. Fortunately there's a better way--use Hocus Focus.

HF can quickly estimate the magnitude and direction of your backfocus error during a special autofocus session. Then you can make the correction if you have the proper spacers on hand. And you're done.

I have a Takahashi CR 0.73X reducer That I want to use with my FSQ-106. The CR wants a backfocus of 72.2mm. My camera and filter wheel add to 32.5mm, so I need my adapters to provide 39.7mm.

For my first run of the Aberration Inspector I had this:

  • M56 to M48 adapter, 12.1mm
  • M48 to M42 adapter, 16.5mm
  • M42 spacer ring, 10mm

These add to 38.6mm. Close, but 1.1mm too small. The Inspector told me I needed to add 3 focuser steps to the backfocus, which is the right sense of change, but the magnitude seems off. 

One of my focuser's steps is about 0.004mm (30mm/8000steps), so 3 steps is a mere 0.012mm. My assumption is that somewhere in how I set up NINA or HF a factor of 100 error sneaked in. If that's correct, then the correction it's suggesting is to add 1.2mm.

So I added two thin spacers totaling 1.2mm and ran the inspector again. Here is the result 


As you can see (if you click the image to enlarge it), the Inspector now says the error is zero steps and the difference in star quality between center and corners is almost imperceptible. I think it's safe to say that I'm now within 0.1mm of having correct backfocus!

This means the next clear night I'm going for a larger target, maybe the Elephant's Trunk, M31, or the entire Veil!

Some incidentals for those of you who like miscellaneous information...

  • All of the goodness of fit (R squared) values were 1.00
  • This was performed without polar alignment or guiding, the exposure time was 2s through my luminance filter
  • I had to increase the autofocus backlash from 450 to 600 steps. I should probably redo all my filter offsets, too, if only to see if they have changed. The autofocus step size was unchanged.

New Image

I've imaged the two nebulae (IC 59 and IC 63) near gamma Cas before, and it was time to revisit that to see how I have progressed. 

Here is my 2009 attempt


This poor image was tortured with wild stretching and clipping, then oversaturated to show some color. 

In 2022 things are looking better: better mount, better camera, better telescope, better processing. Here is the full frame


And here is the nebular part of the image at full scale


Acquisition details are at AstroBin

What really surprised me about this image was that it looks so good for having so little data. It's based on about 82 minutes total exposure spread across the LRGB channels. And short exposures, too: only 90s each! 

The optical performance of the FSQ is--at least to me--breathtaking.

 

Thursday, June 23, 2022

First Image using NINA, PixInsight

I'm going to start this post with the credits. Usually these are left for the end but the amount of help they've given me earns them top billing.

For using NINA and associated plugins, you could not do better than to watch closely the many tutorials created by Patriot Astrophotography . Chad's presentations are concise and clear; even when he suggests some of the technical portions might be a little on the dull side, they're anything but.

Also well worth viewing are tutorials by the Cuiv, The Lazy Geek . His tutorials are often in demonstration form and tend to be more informal than Patriot's.

You probably already know this great reference for PixInsight, Inside PixInsight by Warren A. Keller. It's been my main resource for starting LRGB processing.

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Although I hated to do it, my first clear night in quite a while was dedicated to playing with NINA's autofocusing (AF). 

AF starts at a good (but not necessarily great focus position). From there it racks your focuser out by several "step sizes," takes an image and analyzes it, then racks in a step size and reimages, continuing until it has taken however many steps you specified. Because every geared focuser has some backlash (which has a first guess value of zero distance), that first inward rack will be soaking up that backlash. If your step size is smaller than the backlash no change in focus will result. Through iteration you work you way to producing a nice bowl-shaped hyperbolic curve with the minimum at the point of best focus.

In doing this you will determine two values: step size and backlash. Patriot Astro has a great video showing you how to do this. I was able to determine the values for my FSQ-106-mounted Pegasus FocusCube and was able to get hyperbolic fits with R^2 values uniformly 1.0. 

A second convenience that NINA provides is the use of filter offsets; these are basically the distance by which your filters are not parfocal with a reference filter (usually taken as the luminance filter). Using filter offsets allows you to move from filter to filter without having to go through an AF sequence. This saves you time that you can use for collecting light frames.The process of measuring offsets is automated by a plugin called Darks Customs, and this video explains how to use it. So how parfocal are Astrodon LRGB filters? Very! 

[Here are the numbers for my FocusCube: step size = 35 and backlash = 450. Filter offsets are luminance = 0 by definition, red = +7 focuser steps, green = -6, blue = -1; The narrowband Baader filter offsets are Ha = -52, O3 = -20, and S2 = -48. For perspective, the FSQ focuser has a travel of about 30mm; this corresponds to about 8000 FocusCube steps. The distance in mm for an offset is therefore equal to 

offset in mm = offset in steps * 30mm / 8000 steps = offset in steps * 0.00375

The largest RGB offset is therefore 7 * 0.00375mm or 0.02525mm. That's 1/38th of a millimeter!

Another way to think about the offsets is to compare them to the step size, which can be thought of as the travel needed to change star diameter by 25 to 50 %. An offset of 7 is just 1/5 of the step size, so using the offset in this case may lead to some improvement over assuming parfocal,  but it probably won't be much.]

Getting AF ready was one night's chore. The second night was doing a trial image using the Advanced Sequencer. Using filter offsets made for a very simple sequence: Cool the camera, unpark the mount, run AF on the luminance, slew and center on NGC 188, start guiding and shoot 20 frames of each filter in the order of offsets from negative to positive: green, blue, luminance, and red. (This ordering means the focuser  only moves in one direction, eliminating the need to deal with backlash.) The triggers for this were AF after a significant change in star width and to dither every third light frame. 

Almost everything worked perfectly. But--it was crazy windy and that gave PHD2 fits while trying to recover from dithers. This resulted in a number of frames that had terrible stars, and those triggered AF runs that wasted time. I need to apply a better settling time the next gusty night. 

AF worked to perfection. Stars for each filter were near perfect. My target was NGC 188, an open cluster near Polaris. Processing in PI resulted in this image.

I had trouble dealing with the light pollution and the end result is a rather blotchy image. I'm sure flats would have helped a lot. 

New moon is coming up, so weather  permitting there will be more imaging!