Unpacking Day 10: Aligned W

The PI got hit with a rock this morning. That’s how hard the wind was blowing. He’s o.k., and the wind has died down tonight.

I’ll let Marco update us on progress with fixing the TSS. For now here are a couple of pictures of the work being done there:

The ASM was flipped all the way upside down to work on the TSS.
The fix required going deep into the electronics of the unit.

Laird and I finalized the alignment of the W unit tonight. It looks like none of the components shifted during shipping so we don’t have to re-align anything on the board – a big relief. We also took a set of readout noise measurements, with decent results. Things are as good or better than they were at Arcetri. For the AO-nerds out there, the CCD 39 (our WFS camera) is turning in around 9 electrons RON at 1 kHz frame rate, and roughly 4.2 to 4.4 electrons on our slow (~100 fps) mode. We had both cameras running and were modulating during these measurements, so we fell pretty good about them.

A few pictures of the WFS in the NAS:

The W-Unit, our WFS, mounted in the NAS. When it's mounted on the telescope you would have to be standing on the primary mirror to get this view.
This is the VisAO side of the W.
Here we're checking the aligment of VisAO's new gimbal mirror. We're going to attach the motors to it tomorrow.
We left the lab about 10 minutes too late to catch what must have been a gorgeous sunset. Crappy observing weather.

Some good quotes from the last 2 days:

“It’s pretty hard to keep VisAO down for more than an afternoon.” (Jared Males, spectacularly wrong)

“No! I want this to be a bonding ritual between us – and you know we’re going to do this every time we come up here.” (Laird Close, after Jared whinged about taking the same measurement for the 427th time in the last year).

“My attiude is when something is unknown, take the conservative choice, so fix it.” (Armando Riccardi, the ASM man)

For my mom again. This seemed like an awesome idea . . . I didn't notice the bird poop until later. Baade is behind me, Clay further back.

Unpacking Day 11: The Clouds Break

The storm is finally gone, and the beautiful clear sky is back. The TSS is fixed too, and after we installed our gimbal mirror motors the W-unit is complete.

It's nice to see the sun again, and to not feel like you're going to blow away.
The white light calibration source, in focus in the SDSS i' filter. Note the 3.2 pixel FWHM.

This (kind of lame) video shows our little W-Unit robot responding to a Board Setup command. This tells it to go to a set of pre-determined positions which makes it ready to operate.

The Burros came back after the storm. We hadn't seen them for a few days. A Guanaco walked by at lunch, so they're around somewhere.
Saturday was GTL night.

At this point most of our urgent critical path stuff is done, and we are starting to relax a little. We have a few more days of ASM testing to do, and some mundane odds and ends in the W-unit to take care of, like cable management. We also plan to do some testing of our software interfaces with the telescope control system.

Unpacking Day 12: Starting to Blend

An argument broke out at lunch today over how many days we’ve actually been here. Luckily we have a blog, so we just looked it up.

As the Guanaco noticed, Mario and Frederico have left us after more than pulling their weight. They took the early bus to La Serena.

Frederico, Laird, and Mario just before the boys from Microgate left for their long journey back to Bolzano. Thanks guys.

Now that the TSS is fixed, we moved on to mounting our windscreen. This is just a metal ring that encircles the bottom of the ASM to protect the shell from high wind. We also removed a set of shims from the mounting system.

The windscreen about to be lifted into place. This requires some fine alignment since our calibration system hangs from it.
If you're going to have someone climb on top of your ASM, it should be Armando.
The ASM with the windscreen.

In the afternoon Laird spent some time perfecting the routing of cables to the W-Unit. This is a hard problem – the whole thing translates in 3 dimensions, and has to be able to turn upside down, and cables tugging on optics generally ruins nights.

We had to make a few adjustments to the cable housing to get enough flexibility.
The final product.
This is for Enrico. After dinner we cleaned some dust off our WFS side fold mirror, and recorded these white light images. Pupils look great, and the SDSS i' is in focus. Click to enlarge.

Today’s quote: “You know Laird, you need to seriously think about hiring an exorcist.” (Armando Riccardi, commenting on Jared’s project long bad luck with electronics).

The remaining 4. Click for a rotated image - we leave it as an exercise for the reader to determine the correct orientation of this image.
A nice shot by Laird of newly snow-capped peaks. The big storm improved the view a bit, once we could see it.

Unpacking Day 13: Modulating Away An Afternoon

Tip for users of pyramid wavefront sensors: you are not very sensitive to focus with a large modulation amplitude. For MagAO in particular, you have to get amplitude down to ~.1 milliradians before you really have any z-stage resolution.

Tip for users of the VisAO camera: there is a huge factor (it appears to be about eight) between z-stage motion and VisAO focus stage motion. So failure to heed the above PWFS tip will cause you to tear your camera apart several times in one day trying to find why your focus position shifted. You will feel very dumb later.

So that’s the story of Laird and Jared’s day. Because we forgot these two things, we were completely and totally baffled by the results we were getting when running focus tests on our camera. Since we replaced our gimbal mirror (the motorized mirror that lets us steer stars around our detector) we naturally assumed that was the problem. We even made up a bunch of reasons why it could be and proceeded to apply made up solutions. But in the end, we just hadn’t been careful enough with focusing on the pyramid, and so our numbers were meaningless and our time wasted. The good news, I guess, is that we earned a bunch of intuition for how our stuff works. When life gives you lemons . . .

We pulled the Gimbal back out of the system (I won't admit how many times) to try to adjust its position.
Tightening down the bolts on the Gimbal mount.

This story started last night, when we figured out how to tighten the beam splitter wheel – making it much more repeatable. This changed the angle of our beam slightly, causing us to adjust our gimbal angle a little.

It's a bit terrifying, given the tight space and delicate optics nearby.

See Katie’s post here for a demo on why we’re so obsessed with our gimbal and beamsplitter. Those two devices need to be reliable and repeatable for us to efficiently acquire the stars we use to measure turbulence. They also need to be as free of vibrations as possible for VisAO science operations.

All this visible light focusing meant working with the lights off in the lab. That didn’t stop the ASM testing.

Armando and Marco are verifying that various mirror calibrations are still good.
I came across this spider on my way to work this morning. Nobody panic, I gingerly poked it with a long stick and it didn't move.

Unpacking Day 14: Plumbing and Noise

Things are winding down here.

Today we did a big set of readout noise measurements on both of our cameras. We did a preliminary set a few days ago to make sure shipping went okay, but now that we are pretty much fully integrated we did it again. We’re really happy with the results – it looks like both cameras are performing as well as they ever have. Maybe the most important result is that there is no sign of any coupling between the cameras or any interaction with other components of the system. That means that no matter what I turn on or off while taking data the noise doesn’t change. Great news!

We routed our cooling hoses around the NAS, making sure they all fit. We won’t actually run glycol through them until our next trip.

Laird about to put a cover on the NAS while working on the plumbing. You can see two newly installed (in Chile) hoses running away from our motor driver electronics box.

Marco already told us about the final steps in ASM testing, and lots of other odds and ends were taken care of in WFS land too. But that’s enough work for today.

Today’s quote: “I can’t tell if you’re here to do zoology or adaptive optics.” (Glenn Eychaner)

This morning Amanda Zangari, who is using the Clay telescope, was walking down after sunrise and spotted a Vizcacha outside the Astronomer Support Building. In exchange for a tour of the AO system today, she sent me these pictures to post.

A Vizcacha outside the ASB. Thanks to Amanda Zangari for the great pics.
Camera shy?
There it goes.

Now that we know they’re around, I think it’s official: VisAO has a mascot.

The noble ex-vizcacha.lco.cl, the savior of VisAO.

And I managed to catch the Magellan telescopes right at sunset tonight.

Baade and Clay opening for the night.
Magellan casts a long shadow.