The Occultation of a w=12.2 Star by (30500) 2000QC193

Dec 23, 2023 at 9:11:00pm

 

This event is a narrow path centered on Karl's place, and not far from the Bonny Doon Church where I'll try it. 0.7s duration, full drop. Az=59 Az=109. Bright moon only 22 deg away, keep integrations short, even if hard to see.

     

 

Results

Richard Nolthenius

Odds of a hit were only 40%, but the result was a solid positive within 1 second of the predicted time, satisfied the FP test just fine. 4x setting, The rest of the settings were standard; sharpness=4, gain=41, gamma=1.

Below is the first reduction and not the final better reduction to follow. I used 5 px radius static apertures, no reference star calibration.

magDrop report: percentDrop: 78.3 magDrop: 1.658 +/- 0.483 (0.95 ci)

DNR: 2.89

D time: [05:10:58.1288]
D: 0.6800 containment intervals: {+/- 0.0216} seconds
D: 0.9500 containment intervals: {+/- 0.0624} seconds
D: 0.9973 containment intervals: {+/- 0.1454} seconds

R time: [05:10:58.6341]
R: 0.6800 containment intervals: {+/- 0.0216} seconds
R: 0.9500 containment intervals: {+/- 0.0624} seconds
R: 0.9973 containment intervals: {+/- 0.1454} seconds

Duration (R - D): 0.5054 seconds
Duration: 0.6800 containment intervals: {+/- 0.0326} seconds
Duration: 0.9500 containment intervals: {+/- 0.0768} seconds
Duration: 0.9973 containment intervals: {+/- 0.1600} seconds

       

 

2nd Analysis
I then tried a second analysis; using TME and a ref star using metric interval minimization too. I also employed the vertical median noise filter. The FP test improved, the light curve looked a cleaner. The mag drop was deeper, as appropriate as well. DNR was stronger at 4.41 vs. 2.89. Timing accuracies were much improved, by a factor of 3.

MagDrop report: percentDrop: 85.3 magDrop: 2.085 +/- 0.283 (0.95 ci)

DNR: 4.41

D time: [05:10:58.1243]
D: 0.6800 containment intervals: {+/- 0.0113} seconds
D: 0.9500 containment intervals: {+/- 0.0280} seconds
D: 0.9973 containment intervals: {+/- 0.0530} seconds

R time: [05:10:58.5874]
R: 0.6800 containment intervals: {+/- 0.0113} seconds
R: 0.9500 containment intervals: {+/- 0.0280} seconds
R: 0.9973 containment intervals: {+/- 0.0530} seconds

Duration (R - D): 0.4631 seconds
Duration: 0.6800 containment intervals: {+/- 0.0164} seconds
Duration: 0.9500 containment intervals: {+/- 0.0364} seconds
Duration: 0.9973 containment intervals: {+/- 0.0653} seconds

Composite light curves, occultation target is in gold.

The occultation looks clearer and cleaner in this second analysis inside PyMovie

The false positive test passed, and with an improved score. This is the first time I've used the latest PyOTE which eliminates the red bar and instead as 1-, 3-, and 5-sigma green bars.

Zoomed in on the event. I'm quite pleased that the event was so solid and clear given it was only a 12.2 mag star and only 22 degrees from a near full moon.

I used the smoothing interval which gave the best (lowest) scatter within the metric interval I chose, which was to the right of the event for most of the remained of the taped interval.

 

Karl von Ahnen

Clear skies and initially found target, but telescope drift and lack of time combined to fail target star ID and getting/staying on target. No data. Karl's track was close to mine and he very likely would have had a positive.

Kirk Bender

Out of town on Christmas weekend. Did not attempt.