MAPS Dec. 2024B Night 5: The big W problem

Usually you would think, the big W problem for an observing run would be Wind. And usually you would correct… but not this time. When we went to sleep today morning, we were prepared for facing clouds at night but not Water shortage. There was no water at the bowl…would be a statement a thirsty dog would say (maybe, idk I don’t speak dog yet). But thankfully, after a brief 4 hours, we got water running. So, we started our climb to the summit, in our cars. For Jorge, however, it was indeed a climb because he chose to walk to the summit.

When someone mentioned yesterday that we might want to increase the AO modes to 100 for this run, I personally thought it would take some time (to dot every t’s and cross every i’s). But Amali had it working in ~20 mins! So, just for fun, Jorge and I started looking at bright exoplanet hosts. The plan was to observe a planet hosting faint-ish star (Vmag>5). But we stumbled on something better. Not only was it a faint star (Vmag = 8.14), but also the only exoplanet system (WASP-33) to have its high-resolution observations taken with ARIES back in 2016 A.D. But wait, there is more, the planet (WASP-33 b) would soon be in an orbital phase where it would “emit” radiation before going behind WASP-33. So, we thought we would try to hit two stones with one bird — close the loop with 100 modes on a faint target, and capture WASP-33 b’s planetary emission.

The first task was a success! We were able to close loop with 100 modes on the faintest target so far! But regarding the second task, MIRAC grew impatient during the course of today’s adventure and began heating up so most of the images we took of WASP-33 were overwhelmed with noise 🙁

It might not be the best looking PSF there is, but it was still a great news!
Manny approves the closed loop

Manny quickly figured out what must be heating up (or not cooling down?) MIRAC — one of the cryo lines was not tight. After this fix, we decided to let MIRAC cool down for a while before we restart taking data. By that time, WASP-33 b had already been eclipsed behind the star so we switched to a slightly fainter target for the rest of the run. The rest of the night was just about maintaining the loop, observing the star at multiple altitudes in multiple bands. This night had all things W-centered — Water, WASP-33, Wemperature of the detector.

According to Jarron, only a 0.5K change would worsen MIRAC performance … and we were hitting a difference of 7K .

P.S. Shoutout to Jorge for helping me out with the text, both our brains were at 50% capacity by the end of the night so we needed to team up.

Song of the Day

Moon Over MMT

With all the bits and pieces working and at the end of last night. Tonight is geared toward the goal of the AO consistency, training, and reliability. As one can see from the picture from the start of the night it does not look promising.

Training Training Training

Amali had a classroom of future AO extraordinaire such as her. When you have to juggle CHAI, CACAO, MILK, INDI and every other software package. Being an AO operator is more of a lion tamer than anything else. In real time you have to be wrangling many different parts to make the AO system work. I am impressed and I think she is teaching a hopeful and bright future for AO and MAPS.

Thank you Amali for all your hard work and know how. Your expertise and know how is next to none.

And you know it is going to be good when you have laser dog poodle in the mix.

Hard work Pays off

This is starting to look like an AO system and we are starting to get to a point where we are no longer wondering how the parts work together, but rather how do we make them better. Congrats to all those that have worked on this system in the past, current, and for our future selves.

FK5-0074 star (-0.63 K mag), K-band image, closed loop with 50 modes, 73 degrees altitude (1.04 Airmass)

In the Spirt of Christmas I had Chatgpt put a poem together. Thank you AI

The 10 Days of AO Christmas

On the first day of Christmas, the AO team gave to me:
A single ASM guiding flawlessly.

On the second day of Christmas, the AO team gave to me:
Two WFS tracking,
And a single ASM guiding flawlessly.

On the third day of Christmas, the AO team gave to me:
Three MIRAC/BLINCs imaging,
Two WFS tracking,
And a single ASM guiding flawlessly.

On the fourth day of Christmas, the AO team gave to me:
Four CACAO scripts running,
Three MIRAC/BLINCs imaging,
Two WFS tracking,
And a single ASM guiding flawlessly.

On the fifth day of Christmas, the AO team gave to me:
FIVE TOP BOXES aligned!
Four CACAO scripts running,
Three MIRAC/BLINCs imaging,
Two WFS tracking,
And a single ASM guiding flawlessly.

On the sixth day of Christmas, the AO team gave to me:
Six RC3s pointing,
FIVE TOP BOXES aligned!
Four CACAO scripts running,
Three MIRAC/BLINCs imaging,
Two WFS tracking,
And a single ASM guiding flawlessly.

On the seventh day of Christmas, the AO team gave to me:
Seven Chai teas steeping,
Six RC3s pointing,
FIVE TOP BOXES aligned!
Four CACAO scripts running,
Three MIRAC/BLINCs imaging,
Two WFS tracking,
And a single ASM guiding flawlessly.

On the eighth day of Christmas, the AO team gave to me:
Eight milks for Chai tea,
Seven Chai teas steeping,
Six RC3s pointing,
FIVE TOP BOXES aligned!
Four CACAO scripts running,
Three MIRAC/BLINCs imaging,
Two WFS tracking,
And a single ASM guiding flawlessly.

On the ninth day of Christmas, the AO team gave to me:
Nine photons dancing,
Eight milks for Chai tea,
Seven Chai teas steeping,
Six RC3s pointing,
FIVE TOP BOXES aligned!
Four CACAO scripts running,
Three MIRAC/BLINCs imaging,
Two WFS tracking,
And a single ASM guiding flawlessly.

On the tenth day of Christmas, the AO team gave to me:
Ten lasers glowing,
Nine photons dancing,
Eight milks for Chai tea,
Seven Chai teas steeping,
Six RC3s pointing,
FIVE TOP BOXES aligned!
Four CACAO scripts running,
Three MIRAC/BLINCs imaging,
Two WFS tracking,
And a single ASM guiding flawlessly.

Song of the Day

In the spirit of the Holidays “Christmas Moon” · Emmy The Great · Tim Wheeler

MAPS Dec. 2024B Night 3: MAPS “Pop” Culture

‘Twas the night before running AO, when all through the telescope
The wind was violently stirring, we had lost all our hope;
The MAPS team decided that the night would finish
In hopes that tomorrow the gales would diminish;
There are 52 more lines in this old-time poem
So I will write the remainder of this blog in the way that we know ’em

༄ ⋆⁺₊❅.⁺˚⋆。°✩₊・:*༄:。

As soon as I stepped outside, I could tell tonight was the night we would be able to start running AO. The sky was clear, and the roaring winds of last night were gone.
It was silent… too silent. I couldn’t help but feel as if something else would soon stir up our night.

A nice, clear, calm sunset from the Bowl dorms
Another stunning, beautiful sunset. Photo credit: Bianca Payán

We all arrived at the telescope and set everything up just like any other night: Bianca and I filled BLINC and uncovered the science cameras, Amali booted up the ASM and prepared to start up CACAO/AO, Ben, our telescope operator, moved us to our first target, and Krishna and Jorge confirmed the absence of the target viewed from MIRAC.

Wait. What? Where’s the star!? Krishna and Jorge scramble around their work station trying to understand what is going on. Everything was fine yesterday! Why can’t we see our target tonight?? After two days of alignment, they are confused as to why this is happening.
Minutes pass by. *scramble scramble*
No star. *clickity clack*
Still no star. *brrrrrr… pop, pop!*
Popcorn is done!

In the heat of the moment, Krishna an ASU grad student (who is also looking to buy a car – check previous blog) fuels themselves with popcorn, hoping the sustenance will give them comfort in troubling times as well as the power to solve the issue. Everyone else joins in, munching on popcorn, as a call is made to MIRAC P.I. Jarron. The unnamed grad student’s popcorn munching intensifies. Right as Manny and the MIRAC team are about to head up to the chamber to delve into the instrument, a beautiful, amoeba-like blob appears on the MIRAC viewer. A star! During the stress-eating frenzy, we moved to a new target, made various telescope movements, fixed coma between the primary and secondary, and adjusted voltages on the MIRAC chopper. The combination of those actions allowed us to see our target on MIRAC as we desired.

The aftermath.

While we waited for Amali to get CACAO running, a few of us decided we wanted a break from staring at the sky on a screen so that we could instead stare at the sky with our own eyes. Conveniently, the Geminid meteor shower was happening tonight, and we were in the perfect place to view it. To my surprise, the meteors looked significantly brighter and closer to us than when viewing from Tucson. I stood out there for 20 minutes, attempting to get a picture of a shooting star for the blog (I am always thinking of you). I had hoped to capture a picture of a shooting star coming out from Orion and heading towards the telescope dome, as if Orion himself was shooting it. It got cold, and my arms were sore from holding my phone up in the sky, so I gave up and went inside. I shall leave you with a sky cam image instead.

Geminid meteor (circled in red) seen from the MMT sky cam.

We go back inside to continue working, still feeling the energizing effects of the popcorn that fueled us. Throughout the wee hours of the night, Amali works towards closing the loop on 50 modes. As expected, she is able to successfully do this, thus confirming we are back on track to continue where we left off in August! (For those of you who didn’t know, pushing the ASM to 100 modes during the August run resulted in the loss of 24 magnets. To keep things short, software issues lead to magnet detaching issues.) Four months of hard work pays off! Despite the seeing going between 1.5 and 2.2 arcsecs, Amali continues working. We even verified that CHAI responds appropriately to overheating actuators by going into ESTOP – we have learned this is a crucial part to not losing 24 magnets. Meanwhile, Krishna spends the entire last half of the night coding away, developing a script to find centroids of hot pixels. That popcorn really does work. Thank you, Manny!

MIRAC PSF of 50 modes.
Closed loop → open loop → closed loop
Krishna’s plot showing a MIRAC image and its corresponding PSF. The image is in L-band with the AO loop closed on 50 modes. The FWHM of the PSF is 0.13″ which is also the proposed slit width for the soon to be commissioned ARIES spectrograph!

The song of the night is “Popcorn” by The Muppets.

MAPS Dec. 2024B Night 2: Windy Boogaloo

We started the night with a group photo featuring the stars of the show: the 6.5-meter primary and our beloved ASM watching over us from directly above our heads. It’s a good thing Ruby, Dan and the MMT day-crew gang ensured its secure installation.

Courtesy of TO Ben Kunk. Peep Amali in her muppet coat! She’s just too cool for French fashion school.
(no muppets were harmed in the making of this fashion statement… that we know of)

Bonus photo! Obligatory mirror selfie with the ASM, courtesy of Krishna. In retrospect, we raised our hands in victory too early, we didn’t yet know how the night would go.

Amali and I are present as evidenced by the extra hands in the back, Krishna and Jorge are just really tall

We headed down to get work started and within the hour Grant, Oli and Maggie had aligned the dichroic. Amali’s judicious eye achieved us decent enough pupils that we could start looking for the culprit actuators keeping us from amazing pupils. Good progress so far!

But if there’s one thing I’ve learned on my handful of MAPS observing runs, it’s that the time equivalent of at least one night will be forced from our hands by adverse weather. This was to be our windy night, so around 7:30–a little over an hour after opening–we closed the telescope.

While we held out hope for the winds to wind down, Maggy, Oli and Grant kept us company. Manny found a floor heating pad to fight off the cold reaching up through the ground. Much to our dismay, however, a mouse had eaten through part of the power cable and after 7 glorious seconds of foot warming, the pad sparked and gave out. Thankfully, our boss was uninjured, our only misfortune being that our toes were none the warmer. Such is the price of commissioning magical mirrors.

Around 11 PM, Oli, Grant and Maggie called it a night and headed down the mountain. They made it back to Tucson safe, a testimony to our team’s spirit raging against the wind.

As we waged a war of attrition against the gusts, Amali trained Lauren and me to check how individual actuators respond to a “sweep” of current. 

Actuator 252 is not a problem child

Intermittently, Jorge kept our spirits up with Dad jokes, Manny made us popcorn, and Krishna read abstracts from the day’s arXiv feed aloud. (Yes, instead of doom-scrolling social media, Krishna scrolls through the latest astronomy and sometimes machine learning papers on the daily.)

Alas around 3 AM, the wind forecast pronounced we’d lost this battle and it was time to call it a night and head to bed.

WE INTERRUPT YOUR REGULARLY SCHEDULED PROGRAMMING TO BRING YOU THIS IMPORTANT MESSAGE: 

Krishna is looking to buy a car! If anyone is selling, any and all (legitimate and non-Craigslist-based) leads are greatly appreciated! He isn’t really picky so long as the vehicle is in good condition and runs nicely, but his top contenders are currently any model of the following makes:

  • Ducati
  • Kawasaki
  • Indian
  • Yamaha
Yes, this really exists! Totally unrelated: go watch The World’s Fastest Indian, you won’t regret it

Be present, enjoy nature

In keeping with Maggie’s blog rules, I give you a view of the MMT from the bowl dorms before heading up to the very same. Not only did this moment allow me to admire the mountain’s beauty, but it also made me wonder if the location of the bowl dorms along the winding road to the summit was determined by geography or by a thoughtful mountain road engineer who thought this vista would serve as the perfect inspiration for a night of hard work. Or, maybe some combination of the two.

It’s almost indiscernible, but the wind is starting to pick up

Song of the Day

Before Jefferson Starship (“We Built This City”, “Nothing’s Gonna Stop Us Now”), there was Jefferson Airplane. The song of the day is Planes, by Jefferson Airplane:

MAPS Aug. 2024B Night 6: On and Off

Welcome to the last blog for the MAPS August 2024 observing run!

The evening started off with Grant and Oli performing an LED strip test that would allow us to more clearly see out of focus images on our pupil lens and visible wavefront sensor. The LED light strip was placed in front of the ASM, along the radius of the shell. Our pupil image was clearly out of focus. Ideally, the circles of light (each individual LED bulb) should not be overlapping. They should look as they would if you were to look directly at the LED strip itself. The VIS WFS image looks better, as you can see more defined pixels of light.

Out of focus pupil image. If you own an LED light strip and ASM, you can replicate this at home!
LED strip test on the VIS WFS. WFS pupils should not normally look like this.
Spot the difference.

After waiting for a few storms to dissipate, we get straight to doing some AO. Amali closes the loop on 50 modes, then closes on a whopping 100 modes shortly after. The 50 mode loop had a 1.4 lambda/D full width half maximum, and the 100 mode loop had a 1.8 lambda/D FWHM. GO TEAM! Tonight’s honorable target was FK5 0672, theta Herculis.

Loop closed on 100 modes. Ooh… aah…
Open loop for comparison. Pupil and PSF quality courtesy of atmospheric turbulence.
50-mode loop on and off. Video taken by Amali Vaz.

Bonus Jared quote of the night: “We need more monitors.”

Now we hand things over to Grant and Oli. They battle the on and off cloudy weather as they work on VIS pyramid alignment.

Starlight, no starlight, starlight, no starlight, starlight, no sta-

After they scrambled the topbox (moved the vis CTL and CCID75), the VIS WFS pupils looked VISibly better.

After topbox alignment. The clouds took away some starlight on our pupil image.

With our new, beautiful WFS pupils, Amali, Bianca, and I take turns taking 50 and 100 mode response matrices. The image below is a 50-mode self RM, which confirms we are sensing the same modes that are being poked.

According to Jared, diagonal = good.

Unfortunately, AO had to come to a halt with about an hour left of observing time. While taking some RM’s, we noticed a giant red blob on our actuator position and current map. Red blobs are not good, as they indicate contamination in the ASM. What could this contaminant be? We are not sure yet, but it could be anything from a detached magnet to a bug seeking warmth.

That brings us to the end of the August 2024 MAPS run! I haven’t even hit the one year mark of working with the MAPS team, but I can still say that I am proud of how far we’ve come since my first run.

Goodnight MMT, goodnight air, goodnight stars, goodnight ladybugs and abnormally large daddy long leg spiders that are everywhere.

:・゚✧:・.☽˚。・゚✧:・.:

As we all make our way home, I would like us to keep the song of the night in mind: “On the Road Again”, but specifically Donkey’s version from Shrek.