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Notes (S609) |
Main Aims
This was an early morning session with main aims :
Equipment & Software
Highlights
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An image problem affected nearly all of the images acquired during session using LX200 + ST-10XME imaging train. Images show vignetting pattern and raw photometry showed significant reduction below normal transparency levels. Reason for the problem isn't entirely clear. There was some dew formation during the session but it wasn't obviously enough to cause the problem. Clearing the dew with hairdryer didn't eliminate the problem, neither did bringing the CCD Temperature back to 5 degC (ie above freezing point). No condensation was seen on A07 tilt glass or C Filter when the imaging train was partially broken apart the following day.
NGC 2301 - Raw Frame with Problem |
Raw CCD Image (50% size) 90s exposure (single frame), 3x3 binning, C Filter 2017-12-22 03:42h UT (#608090) 12" LX200R (at f/10.4) + ST-10XME (Autoguided using TS 80mm APO + ZWO ASI178MC) |
NGC 2242 - Stacked Image with Problem (after conventional dark/flat frame reduction and stacking) |
CCD Image (50% size) 5 x 60s exposure (average combine), 3x3 binning, C Filter 2017-12-22 04:04h UT (#608097-101) 12" LX200R (at f/10.4) + ST-10XME (Autoguided using TS 80mm APO + ZWO ASI178MC) |
A reduction process to correct the problem and make the images semi-usable is described in a following section
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Poor visual transparency (probably either dew and/or other condensation in the LX200 + ST-10XME imaging train, resulted in the recording of images that would normally be considered too poor to use for public viewing. A reduction process was used to make the images partially useable.
NGC 2242 - Original Image (after conventional dark/flat frame reduction and stacking) |
CCD Image (50% size) 5 x 60s exposure (average combine), 3x3 binning, C Filter 2017-12-22 04:04h UT (#608097-101) 12" LX200R (at f/10.4) + ST-10XME (Autoguided using TS 80mm APO + ZWO ASI178MC) |
NGC 2242 - Computed Flat Frame 1 (Flat computed from background values in orginal image) |
(Computed using own software - AstroImageTool) |
NGC 2242 - Intermediate Image (Original with flat reduction using Computed Flat Frame 1 |
Image details as above |
NGC 2242 - Computed Flat Frame 1 (Flat computed from background values in intermediate image) |
(Computed using own software - AstroImageTool) |
NGC 2242 - Final Image (Intermediate Image with flat reduction using Computed Flat Frame 2) |
Image details as above |
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The right hand region of images taken with TS 80mm APO + ASI178MC camera during this session shows obvious coma. Coma is a known potential issue for my TS 80mm APO scope which doesn't currently have a field flattener. Whilst the ASI178MC chip is smaller enough not to show coma when precisely on-axis, the image very probably lies off-axis due to the current setting of Orion X/Y guidestar finder which hasn't been recently recentered & checked.
Image Coma on right hand side of image |
CMOS Image (16% size) 69 x 10s exposure (Live Stack), 1x1 binning 2017-12-22 04:37h UT (#04_37_15Z) TS 80mm APO + ZWO ASI178MC [ Larger Image, 32% size ] |
Image Detail from different parts of above image |
CMOS Image (16% size) with 100% sized inserts Image details as above |
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This Web Page: | Notes - Session 608 (2017-12-22 |
Last Updated : | 2023-11-29 |
Site Owner : | David Richards |
Home Page : | David's Astronomy Web Site |