We kept at it on our 2nd day (our 1st full day). Today we unpacked the NAS, installed the guider in the NAS (for the first time), unpacked and tested our computers, and after dinner we unpacked and inspected the WFS. Some pix:
Author: Jared Males
MagAO Arrives at Las Campanas: Unpacking Day 1
Today, for the first time, all of the MagAO system was on the same continent, and even in the same building. On top of that, after a 50 hour odyssey Laird, Victor, and Jared arrived at LCO to begin unpacking. MagAO is officially at Magellan! Here are some pictures from today.
Meanwhile, somewhere between Tucson and La Serena:
And finally at the top of the mountain:
At the end of our first day the inner box was safely stowed in the clean room, and we have started unpacking our electronics. A big first day.
Shipping Update: NAS on the Ground!
The NAS and all the W-unit and VisAO electronics landed in Chile early on Tuesday morning. The first part of MagAO has now arrived in Chile!
Our other big news is that the ASM – meaning the thin shell itself and the ‘unit’, which means the reference body and attached electronics – has left Arcetri and is on the way to the airport in Firenze. This process will take a few days for customs etc. The pictures below, courtesy of Armando Riccardi, show the final stages of packing the ASM and loading it on a truck.
Cleared To Ship!
After our pre-ship review, we had a few things to fix – the only difficult one was a misbehaving actuator in the ASM. These have all been dealt with, and after a final review by the director we today received permission to ship the Magellan AO system to Chile.
LCO here we come!
Some packing pictures courtesy of Carmelo Arcidiacono:
The Shutter in Closed Loop Action
The Magellan AO VisAO camera includes a novel system for performing “frame selection”, which is the technique of using only periods of good seeing and/or AO correction in the final science image. Traditional “lucky imaging” does this by reading short exposures and selecting in post processing. In our system, we use measurements of Strehl ratio in real time and open and close the shutter based on those measurements. This video shows our shutter working with the AO loop closed in the Solar tower in Arcetri, Italy. It was taken during the week after our pre-ship review.
The Strehl time series is derived from our custom wavefront reconstructor (calculations are done on a GPU). During this testing the shutter decisions were based only on the most recent Strehl measurement, meaning that we did not use any predictive algorithms. Note the fleeting moments of a clear Airy pattern as the shutter finds the highest peaks in the Strehl ratio time series.
The real question is: does it do any good? We’re still analyzing all the data we took, but for now this demonstration is an important step showing that our telemetry and hardware systems can do real-time frame selection.