Blog

MagAO-X 2024B Day 10: Telescope Limbo

With us finally getting used to working on the night shift, it sure feels like we have been racking up the overtime hours. However, we still find time to get our daily Vizzy content. I have decided to start this blog post by giving the people what they want…Viscacha’s and behind the scenes footage.

After capturing the cutest photos of those little guys, we continued our content creation with some beautiful photos of Clay. Thank you Jialin for taking this timelapse!

Prior to making our way up the mountain we spent some time pondering the great science advancements we are all going to make.

Alright, now onto the actual science. Tonight was dedicated to Laird and Jialin. The setup went smoothly, and we were quickly ready to start collecting data. The primary science goal for the first half of the night was to search for binary stars and planets in the i and z bands. We began with a target that has been indirectly observed to host a ~5 Jupiter-mass planet. With this data set, we hope Jialin will be able to confirm its existence.

The second half of the night transitioned into H-alpha science targets. This allows us to observe specific emission of ionized hydrogen (around 656nm). This is particularly interesting as it provides valuable insight into accretion activity in binaries or planetary systems.

While we captured some excellent observations, the highlight of the night was pushing the telescope’s limits. As morning approached, we continued observing a target star as it reached an altitude below 23 degrees—remarkably low, considering our telescope operator had previously noted that the scope is not designed to operate below 21 degrees.

Song of the Day

MagAO-X 2024B Day 9: In the groove

We had an all-Laird, all- night. With everything working so well, the most exciting thing going on instrument-wise was the initial setup, which I was able to get in on.

From our control workstation, I dutifully applied the “F-test” (which displays the letter “R”, for reasons lost to history), applied the “J-test” (works as advertised), performed the 253-click process to satisfy the prerequisites for the automated alignment loop, and then performed the other remaining steps when the automated alignment loop ran away. (“Apparently it’s shy and only works when it’s just me and the instrument” — Jared)

Then, we went to look at a star, and instead found two!

Visible near α Eri at almost 12 o’clock, the companion (star, not planet) lies at about 0.25″ separation. Without an adaptive optics system and a decent-sized telescope, you’d have a hard time seeing it at all. With the AO correction, we get diffraction rings around the stars in the scene. That means we can’t get any sharper—or resolve any more details—without a bigger telescope.

Speaking of binaries, we also imaged Mira (ο Ceti), a red giant star with a companion star.

Hmm, one star has a nice core and diffraction ring, but Mira (in the center) does not look as sharp. Why does the scene look so different from the first binary? Baby, don’t you go over-analyze. No need to theorize; I can put your doubts to rest.

Mira is 400x size of the sun but approximately the same mass. So, a big puffball. But the reason for the fuzzy image is not (just) that the star is a puffball. It has to be a nearby puffball for our system to resolve it. We can actually measure half a dozen pixels across the star, though our choice of filter and telescope means that’s only two “resolution elements”. (That’s just physics saying you can use as many pixels as you like but you ain’t getting any more information.)

I regret to inform you that on this night, there were no viscacha observations recorded. But worry not, gentle reader: many graduate students have gone on to have perfectly good careers using only archival viscacha data.

So, instead, I’ll share some computer stuff.

(Yeah, I know, I know. Just shut your eyes and scroll really fast to get to the song.)

It’s not entirely new this run, but I’ve been doing some shaking-out of the data pipeline feeding our dashboards (among other things). This is what a “normal” night looks like: most of the time we’re open, we’re saving data (that’s the “observing” row on the Observations chart). Since it’s a Laird night, it’s all Hα imaging, and everything’s colored red for our filters and beamsplitters.

Before an astronomer takes exception to me calling this a “normal” night when the seeing was hovering around 0.75 arcseconds, I should clarify that ≤0.5″ nights are the only ones worth seeing, the only place worth being.

Song of the Day

“Cold Cold Man” by Saint Motel

Bonus Literary Interlude

—No multipliques los misterios —le dijo—. Estos deben ser simples.
Recuerda la carta robada de Poe, recuerda el cuarto cerrado de Zangwill.

—O complejos —replicó Dunraven—.
Recuerda el universo.

“Abenjacán el Bojarí, muerto en su laberinto” by Jorge Luis Borges (1949)

In English:

“Don’t go on multiplying the mysteries,” he said. “They
should be kept simple. Bear in mind Poe’s purloined letter,
bear in mind Zangwill’s locked room.”

“Or made complex,” replied Dunraven. “Bear in mind
the universe.”

“Ibn Hakkan al-Bokhari, Dead in His Labyrinth” by Jorge Luis Borges (1949)

MagAO-X 2024B Day 8: International Geographic

Empanada Sunday is always hard to follow, but today started off on a really strong note: an adult and a baby vizzy graced us with their presence just before sunset. Viscachas are notoriously jumpy creatures (in both senses of the word), so there was a National Geographic-esque effort to get some decent shots. Fortunately, our efforts paid off. I now present to you some full-resolution images of the cutest little guys known to mankind:

you should see these lil guys bounce
a very tired looking parent
the feets! the nose! the EARS!

And some slightly-less-cute behind-the-scenes footage:

After the sun went down and vizzy-viewing was over, we got straight to work. Jay and I first fiddled with some cables on the platform to diagnose a shutter issue, and before we knew it, we were on-sky. The seeing started off a little rough at >1 arcsecond, but after a little patience and a little tweaking the AO system, we started to produce some good images for our collaborators at Michigan/MIT.

(quick aside: if you don’t know what we mean by “seeing,” this blog post by Logan offers a quick and easy explanation).

The last few hours of the night were for engineering. We started off with a game of telephone: Laird went onto the telescope platform to do some alignment with Jialin acting as chief flashlight-holder and walkie-talkie user. I sat in the driver’s seat in the telescope control room with the other walkie-talkie and Jared on Zoom. To get our mirror aligned, I relayed communication from Jared over the walkie-talkie to Jialin, who then relayed the message to Laird. Then Laird would tweak the alignment and tell Jialin, who radioed the message to me where it was finally heard by Jared. Thankfully it only took us a couple of iterations, and nothing got too garbled as the message made its way from Point A to Point B.

After alignment we continued with more engineering tasks, mostly trying to use our low-order wavefront sensor to get vibrations under control. I also got some time to experiment with the ADCs (atmospheric dispersion controllers). Unbeknownst to me, as I tinkered with speckle fitting and prism angles, the other two first-year grad students on the mountain (with the help of the talented Jialin Li) were taking portraits that would make any astronomy aficionado burn with envy:

Thanks for inviting me, guys

Oh well. There are many nights yet to come. In honor of finally (sort of) getting into the rhythm of a night schedule, the song of the day:

Daysleeper – R.E.M.

Don’t wake me with so much
. . .
My bed is pulling me, gravity

Michael Stipe (and also me)

MagAO-X 2024B Day 7: It’s Empanada Sunday!

With our third car stolen by an unknown observer/animal on the mountain/crew a few days ago, the uber arrangement for our 9 people crew has been a bit tricky. Two brave and kind souls volunteered themselves for a hike up to the telescope, Eden and Katie. They were soon rewarded with spotting of the cutest clean room vizzy on this run (thus far).

What a good clean room vizzy! Look at those bunny like ears!(pc: Katie)

Before the dome opening, the crew added the 24B sticker onto the instrument. (Yeah, we are a lil’ late this run).

The sunset viewing session proceeded after the “ensticken” ceremony. Parker’s head acted as the coronagraph for the group photo. Please try to call him by his new middle name, “The Vortex”, from now on. The long anticipated green flash was finally captured by human eyes. On video, which was taken by our one and only Professor Close, the flash doesn’t seem to be so green.

For the “best part of this video”, watch till the end!

Along with our T.O.’s arrival, a basket full of empanadas entered the kitchen. Whether if the cheese empanadas were deep fried this time around remains a mystery, but they were a lot less greasy, which made it a lot more enjoyable for the meat and non-meat eaters.

Another Sunday and another basket full of empanadas (pc Jaylycious)

On the science end, the first half of the night was VIS-X time, and Sebastiaan observed quite a few targets in high resolution mode during this time. These data will probably be reduced by one of his current or future grad students, so look out for more MagAO-X papers? The good seeing persisted through the second half of the night, which was an joint collaboration between Jensen (graduate student from MIT) , Gabrielle, and us. We spent the rest of the night observing a protoplantary disk in Halpha.

Do you know what LMC stands for? Laird Miller Close.
Beautiful picture of the MW and Baade along with the LMC.

Song of the Day

Since we are now in South America, I have been trying to listen to more music from this continent, particularly pieces by Astor Piazzolla. Per the 24B blog rules, I must include two sentences from the song in the blog post. So here are the lyrics that I like the most:

“Y canto un tango que nadie jamás cantó
y sueño un sueño que nadie jamás soñó,
porque el mañana es hoy con el ayer después, che!”

As a non-Spanish speaker, I won’t attempt to translate for you. I would suggest a google search instead.

MagAO-X 2024B Day 6: Making Rainbows

Last night, after such quality science, and the night before with rapid fire engineering accomplished, tonight was set to be a good mix of the both. Jared engineering in the early eve and Sebastiaan reanimating the Vis-X visible spectrograph for the rest of the night.

Alas, the mountain had other ideas for how we should be entertained. But what’s a crisis to this elite team? What’s two? What’s three? We are robust, especially with a remote PI directing us like agents on chessboard. Today we survived a glycol booger, a power outage, and mysteriously missing vis-x camera software. Ultimately, it’s not a novel crisis that dampened the night, but our old enemy atmospheric seeing.

The strong, independent, folks keeping MagAO-X running. They don’t even have their PI on site.
The strong, independent telescope that keeps MagAO-X running. It doesn’t even have it’s TO on site.

Wakey, wakey, rise and shine, the computers are at 99 (deg C). Do not fear, the timely work of Parker and Jay before dinner, in which they had to squeeze the tubes and flush the filters and whatnot, halved the temperatures our control computers. Computers which we would prefer to not live at boiling temps.

Fig. 1. One should observe a sharp spike to 100 degrees, a gap as the computers went down for tube repairs, and then a much cooler system post fix.

The glycol team triumphantly entered the dining hall before service stopped, a real win considering how often we miss dinner for these kinds of things. The night was off to a good start with clear skies and decent seeing for the first few hours of engineering. By the time engineering wrapped up, things were looking very un-twinkly.

This DIMM number, for those who don’t live their life by them, is very, very good.

Next up, Sebastiaan. Which required half a postdoc professor in the instrument to shift the optics into a Vis-X configuration. Fingers in the blackbird pie, if you would. His spectrograph disperses visible light from 400-900nm in both low and high resolutions modes.

And then things got dark. Literally, the power went out for a good minute. It’s on again, off again, on again. But MagAO-X? It stayed on. A testament to ol’ reliable, the UPS’s. Almost simultaneously, Joseph sprinted to get camera software back where it should have been on ICC. No really, we should all be impressed and very grateful the whole thing didn’t fall apart. Take a bow, take a bow, take a bow.

Back in action, we were pumped to start seeing the spectra roll in:

Locking in on the first spectrograph target of the run.
The binary loud and clear on the spectrograph

But then we started to look more like this:

The face you don’t want to see sebastiaan make when the data comes in.

For no good reason, the seeing spiked. And when we say spike, we mean a dramatic 0.6″ to 1.7″ swing. And then we were looking at the DM struggling. The seeing was so unfriendly that even our backup backup engineering targets weren’t interested in the 6.5m telescope.

When the seeing gets above 1.5, MagAO-X starts to mock us.

This didn’t stop our tenacious dutchman from exposing till civil twilight.

See: The pink of pre-sunrise in the open door.

All things considered, it was a night. We’re still adjusting to the sleep schedule, and the people are sleepy. Enjoy some photos, and we’ll see you tomorrow. Hopefully we’ll get more of the 0.4″ nights and no more of this 1.2″ nonsense.

Bonus: inaccurate quoting

Thanks to Elena’s camera enthusiasm, we now have a little piece of midnight whimsy captured. For better or for worse. Hover for some choice quote picks that have been randomly assigned.

Thanks Elena! Thanks everyone for having no filter at 3am! or 3pm!

Song of the Day

As per the rules, lyrics from the song of the day can be found sprinkled throughout the blog.

Faust Arp by Radiohead