Today we moved our Adaptive Secondary Mirror (ASM), including our 1.6 mm thick 85 cm wide fragile thin shell, up to the aux building between the telescopes. Needless to say, it was an exciting time.
The ASM is stored on a handling cart specifically designed for this tripThe entire trip was under the watchful gaze of Armando the ASM guruEmilio is paying out the come-along, a device used to make sure the ASM is always under controlHere the ASM is leaving the cleanroomMiguel operating the come-along
Here’s a video of the cart being pushed and pulled onto the truck:
The ASM on the truckAdvisor and student share some shadeLaird and Katie are attaching a cover to prevent the sun from reflecting off our shell and melting something/someoneHere is the ASM all strapped down, and just beginning its journey to the topLaird held the ASM's hand all the way to the topThe MagAO ASM arriving at ClayThe come-along was used at the top too.The loading dock was specially adjusted to keep our shell safe
Other stuff got done today too.
Alan and Tyson finished installing our new cable management system today.
This guides the cable through the hole in the deck as our instrument rotates
Here it is in action, demonstrated by the lovely Tyson:
After dinner Marco and Armando went up to Clay to begin preparing to power up the ASM electronics tomorrow.
Armando and Marco opening the ASM electronics rack.
Derek Kopon (Arizona/Heidelberg) and Marco Xompero (Arcetri) arrived today. The dining hall is getting full!
quotes of the day:
Frank Perez: “Ok, who’s in charge”
Laird Close: “Well…I guess I am.”
“It can be disconcerting at first, but you’ll get used to it” (Povilas Palunas)
“Sometimes I wonder who’s the student and who’s the director here.” (Laird Close)
For today’s operation we broke out the steel toes. There was some question about style vs. function. In the end, style won. A skeptical Alan tests Katie's safety shoes, which are somewhat pinker than the norm around here
I managed to get close enough to this little guy today:
Armando Riccardi is here. That means it is all going to be fine. Seriously – stop worrying.
O.k. Maybe worry a little. We had a 6.2 magnitude earthquake today, almost right under us. That’s telescope shaking, rock slide causing, all work stopping strong. Strong enough that Armando abandoned the ASM in the cleanroom. Here’s a map:
Coordinates and strength of the quake from Universidad de Chile . It was only 34 miles away.
The valley between us and the epicenter had clouds of dust rising, presumably from rock slides. [check back, I’ll post some pics when I get them]
In the end everything is fine. Nothing broke and we just kept working.
Alan and Tyson tweak our guider.Tyson working on wrapping the 'Anaconda', which regular blog readers will remember from our last adventure. Katie and Alan are safety watches in case it turns on Tyson.
Progress was made on site cleanliness as well.
Alan gets it done again. Our various mothers will be grateful for once-more poop-free pictures of their children.
And we discovered what “the problem has been dealt with” actually meant. The Viscacha den in the attic of the ASB was screened over.
The screens put in place to stop the banana raids. The white streaks are evidence of the former occupants. Vizzy looks on with seeming distinterest.
The MagAO project put together an instrument on a shoestring budget from borrowed parts, to observe one of Nature’s most beautiful spectacles:
Approaching sunset at LCO
The solar eclipse!
We built a pinhole camera using an obsolete cable bulkhead, an authentic piece of MagAO hardware. We call it the MagAO Solar Eclipse Viewer. You can see the cable bulkhead below, in this photo of the PI and Instrument Scientist who did all the planning, design, and prep work with the hardware.
Dr. Katie Morzinski, PI and Jared Males, Instrument Scientist
The instrument passed internal Feasibility (FDR)/Conceptual (CoDR), Preliminary (PDR), and Critical Design Reviews (CDR) this afternoon. There was no Pre-Ship Review (PSR) because we hand-carried the instrument from the Aux building to the dining hall. Integration and Testing (I&T) was completed in the afternoon at the Aux building by the PI and Instrument Scientist.
The commissioning and observing run began immediately after everyone finished eating a delicious dinner together in the LCO dining room.
Software and operations were provided by Tyson Hare. He first upgraded the detector from a wall to a sheet of paper, and then commissioned the instrument outside…
Commissioning the MagAO Solar Eclipse Viewer
…then took it inside to the LCO dining room, where the curtains could be drawn to reduce the ambient “dome” light.
Optimization of the MagAO Solar Eclpse Viewer
Here is Tyson operating the MagAO Solar Eclipse Viewer detector:
Tyson Hare operating the detector
Laird Close operated the pinhole camera:
Dr. Laird Close, camera operator
We simulated the eclipse with a 100-peso coin, to test our optical design and alignment:
Simulation of the solar eclipse, on a shoestring budget
A lot of the LCO staff and other LCO observers joined in on the fun!
LCO enjoying the solar eclipse
Here we show the entire instrument and overlay the light path:
Light path of the MagAO Solar Eclipse Viewer
It was only a grazing or nibbler eclipse at LCO, and here are some of the best images we got:
Solar eclipse images
Eclipse through welding glasses
It was a lot of fun, and we hope you enjoyed the first on-sky results by the MagAO project!
We had an exciting day on the MagAO project here at Las Campanas Observatory. There were bugs, birds, left-handed translations, a handoff, some solidified N2, and the sun got a little fainter too.
Today was the crew changeover. See Katies’s post about how the next Turno was shown the workings of Clio’s dewar and LN2 refilling procedure.
The big excitement for the day was the solar eclipse. See this post for more on MagAO’s first on-sky results.
We got a little done on the NAS today too. Alan did a bunch of guider testing, and has declared victory. Jared and Katie tested the bayside stage motors, our very powerful X-Y-Z translation motors which move the entire W-Unit to align and focus. These weren’t tested last night since we like to be careful and make sure we don’t destroy the project (as a general rule). We tested their movement in 3 axes to verify that everything works smoothly and that no hoses or cables are pinched. Now, in optics the Z-axis is traditionally along the optical axis, and positive in the direction of motion of photons. Katie noticed that our X and Y axes then follow the “left-hand rule” for their coordinates, and was inspired to pose for a picture. This is Katie’s way of saying, politely, that we do things a little backwards at Arizona.
Katie demonstrates the "left-hand rule" for the coordinate system of the X, Y, Z Bayside stages.
After getting the stages up and running, we could then align the system. This means using the stages to get our artificial star on the optical axis of the W-unit. With a pyramid AO system, we always feel good when we get a nice set of 4 round pupil images.
Our pyramid wavefront sensor pupils at left, and the VisAO spot on the left.Here Jared is showing some relief that everything turned back on.
There have been a few animal sightings. She’s the only one on the project to date, but Katie has seen a bunch of bugs. It is spring, so maybe they are coming out. We also saw a turkey vulture circling the summit. Nobody got a good pic, but there was unambiguous evidence of its passage.
Our various mothers are going to be disappointed.
Quotes of the Day:
While discussing VisAO’s tiny field of view:
Matt Walker: “it would take a long time to do a sky survey with an 8 arcsecond field of view”
Alan Uomoto: “well, that depends, do you want to do it at 20 milliarcseconds?”
(good comeback Alan)
Tyson Hare: “Look how easy it is to entertain a room full of nerds.” (during the eclipse)
After the eclipse, we were treated to yet one more amazing LCO sunset.
The Magellan 6.5m telescopes at sunset. Clay at left, Baade on the right.
Tuesdays are when LCO staff swap shifts. A meeting is held with all technical staff, who share information in order for the handover to go smoothly. This afternoon, the instrument staff who are keeping Clio cool met to show each other how it works.
Clio handover 1 - Victor Meriño, Mauricio Navarrete, Alan Uomoto, and Gabriel MartinClio handover 2 - Mauricio Navarrete, Jorge Bravo, Gabriel Martin, and Alan UomotoClio handover 3 - Victor Meriño, Jorge Bravo, Gabriel Martin, Emilio Cerda, and Mauricio Navarrete
Clio handover 4 - Gabriel Martin, Jorge Bravo, Mauricio Navarrete, and Alan Uomoto
