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Notes (S611.2) |
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Notes (S612.2) |
Main Aims
This was a night-time session was to continue formal commissioning of the new Dome Observatory including :
Equipment & Software
Highlights
Notes
Jupiter and 4 main moons |
Jupiter - B Filter | |
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Annotated CCD Image (cropped) 0.12s sec exposure (single frame), 3x3 binning, C Filter 2018-06-06 23:58 h UT (#612002) 12" LX200R (at f/5.7) + ST-10XME (more pictures) |
CCD Image (cropped, unsharp masked) 0.5s sec exposure (single frame, half-frame), 2x2 binning, B Filter 2018-06-07 01:03 h UT (#612013) 12" LX200R (at f/5.7) + ST-10XME |
Summary Plots & Logs
Observing Plan Created for Session, 2018-06-06 (more information) |
Night Sky Summary Plot -
2018-06-06 Top axis: Sky Brightness at Zenith (in ADU/s) Lefthand axis: Local Time (hh LT). Righthand axis: Sun Altitude (degs) |
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Whilst trying to find, centre and align the scope on the star Arcturus an unusual linear light artifact was imaged in a 5s snap shot. The artifact was unlike anything seen before. A second frame was taken and confirmed the artifact as something 'real'. (Light Artifact 1 below)
Moving the scope a very short distance revealed a light artifact much more typical of the 'glare' associated with a very bright star just outside the field of view. Indeed a short jog revealed the mag 0 star Arcturus that is the 'source' of the light artefacts.
Light Artifact 1 |
Raw CCD Image (50% size, North - Down) 5s sec exposure (snap shot), 3x3 binning, C Filter 2018-06-06 23:20 h UT (Snap.2320.22) 12" LX200R (at f/5.7) + ST-10XME [ full size image ] |
Light Artifact 2 Shadow indicates that the light artefact is due to the light from star just outside CCD FOV being reflected within the camera or optical train |
Raw CCD Image (50% size, North - Down) 5s sec exposure (snap shot), 3x3 binning, C Filter 2018-06-06 23:20 h UT (Snap.2321.39) 12" LX200R (at f/5.7) + ST-10XME |
Arcturus, Mag 0 star |
Raw CCD Image (50% size, North - Down) 0.12s sec exposure (snap shot), 3x3 binning, C Filter 2018-06-06 23:24 h UT (Snap.2324.22) 12" LX200R (at f/5.7) + ST-10XME |
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One of aims of this session was to test automated acquisition of a sequence of targets (Observing Plan) that have been scheduled by a newly developed genetic algorithum optimisation program working with target data held in SQLite. In the event it was not possible to execute the Plan / Job Queue due to instability of POTH Hub, Scope and CCDSoft5. Pictures of the Observing Plan and its generation are included here for information
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This Web Page: | Notes - Session 612 (2018-06-06) |
Last Updated : | 2023-11-29 |
Site Owner : | David Richards |
Home Page : | David's Astronomy Web Site |