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MAPS Oct. 2023B Night 3: 5 for 5

Tonight felt a lot like whiplash, from tired to energized to tired to energized, from starry to humidity to starry, and from failure to fix to failure to fix!

First of all the MAPS daytime/nighttime/whenevertime support crew (Oli, Grant, Dan) drove up this afternoon with the repaired (by Ken) bias board for the CCID-75 LittleJoe controller, as well as the IR dichroic for the Saphira. Unfortunately once we plugged in the board, we were still unable to communicate over serial. Manny’s next guess is we may also have a problem with the power supply. So ultimately that will require more lab testing and repair. Instead, we’ll use our other WFS for the rest of the run.

Anyway, so it was time to get on sky. Here are all the good AO setup stars, as defined by searching Simbad for zenith-y and bright:

dec  > 20 & dec <  50 & vmag <  2

Plus I added in Theta 1 Ori C for good measure(ments). (And actually Alpha Gem isn’t a good AO setup star, as it’s a binary with two very bright A stars only a few arcsec apart — but it’s zenith-y and bright.)

Airmass curves for the good (zenith-y and bright) AO setup stars, plus Theta 1 Ori C. [Image description: x-axis is time, y-axis is airmass and altitude. Stars are Alpha Lyr, Alpha Cyg, Alpha Per, Alpha Aur, Beta Aur, Beta Tau, Theta 1 Ori C, Alpha Gem, Beta Gem, and Eta UMa.]

Oli, Grant, and Dan then switched out dichroics and we moved to Deneb (aka Alpha Cyg) and they were about to complete the alignment when…

More humidity rolled in! Noooo! We were shut from about 9pm to 3:30am, and Oli and Grant became night crew too.

When it cleared up again, we got back on sky — this time on Beta Tau (real name: Elnath). We found it, aligned it, saved all the offsets — and tried to switch to a new star — and the offsets no longer worked! After some telescope dancing, we (Rory, Brian, me) realized we had the wrong units for our proper motion coordinates. Sigh. So I mostly* fixed that, and now we are off and running! [*I fixed the algebra but not the trig yet — just to do it as quickly as possible by hand — and the trig has only mattered once in my experience thus far, on Proxima Cen (which is apparently the highest-proper-motion star, with a large enough dec for the cosine to matter), that I’ve ever locked on.]

Here’s an IDL code snippet for future posterity:

;; Proper motions are given from Simbad in (Cartesian) mas/yr
ans = simbad_data(star)  ;; Calls the function simbad_data.pro

;; Returns ans.pm_ra which is RA proper motion in mas/yr
;; And ans.pm_dec which is Dec proper motion in mas/yr
;; And ans.icrs_dec which is sexagesimal Declination which you have
;; to convert to decimal-degrees which is the variable DEdeg

;; Magellan wants RA in sec of time per year and Dec in arcsec per year.
pmra_mag = (ans.pm_ra / 1e3) * (24/360.) / cos(DEdeg*!pi/180.)
pmde_mag = ans.pm_dec / 1e3

;; MMT wants RA in sec of time per century and Dec in arcsec per century.
pmra_mmt = ans.pm_ra * 24/3600. / cos(DEdeg*!pi/180.)
pmde_mmt = ans.pm_dec / 10. 

Right now Jared, Amali, and Lauren (and Andrew remotely) are taking AO calibrations with the Saphira IR WFS, and Rory is taking data with MIRAC. Oh BTW Lauren is our new team member as of this week, her first day was our first night on-sky, and she’s doing great!

Anyway, after our 0 for 5 first night, it’s great to be working with 5/5 — (1) stars are visible, (2) telescope is allowed to open, (3) conditions are safe enough for ASM, (4) AO hardware is working, and (5) science camera is ready!

And… the loop is closed just as we passed into civil twilight from nautical (having gone well past astronomical twilight)! (This is why we always get the full-moon bright time, our tiny pixels and kHz framerates don’t care about background light except for the actual Sun itself.)

And now for The Video Of The Night… I forgot to bring my Pilates travel equipment, but I can do a little bit of a workout just rotating my myofascia in spirals like in this video by my Pilates coach, “Spirals on the Cadillac for MyoFascia Release” by Arlene Corcoran:

Spirals on the Cadillac for MyoFascia Release by Arlene Corcoran

MAPS Oct. 2023B Night 2: Water falling from the sky!!!

As a current resident of Arizona and a former resident of New Mexico, part of me must celebrate when water falls from the sky in these drought-stricken drylands or deserts. As an astroengineer and astrophysicist, it does make observing …difficult. Either way, it’s still beautiful:

Afternoon at The Ridge. [Image description: A mountain scene straight outta the SouthWest. The valley floor is covered in brown rocky foothills that look like choppy waves in the ocean. The nearby mountainside is covered in dark green foliage with a scrubby texture. The sky is filled with thick heavy dark rain clouds. Yet a beauiful orange glow peaks through a gap below the clouds and above the distant valley where a sunbeam illuminates shafts of rain falling in the distance.]
A photo of the MMT today. [Image description: In the foreground are the crowns of some green and brown pine trees. In the middleground there is some sort of a brown ridgeline, kinda hazy. In the background there is white mist/fog (where the telescope dome is, but cannot be seen).]

You’ll recall yesterday we had trouble with our WFS controller. We reached out to our network of contacts for a spare part. We also began preparations to switch to our other WFS. And we even opened for around an hour tonight in a gap in the humidity and clouds! But we need more time… so we’re staying hopeful for tomorrow night.

The video of the night is “OUR LAND Episode 5: Dry Land”

OUR LAND Episode 5: Dry Land from The Greenhorns on Vimeo.

MAPS Oct. 2023B Night 1: 0 for 5

What’s this, another MAPS run? Yup, the moon is almost full, and here we are again!

Unfortunately tonight we are 0 for 5 on AO engineering/commissioning productivity. Here are the 5 things:

  1. Can we safely open the dome? No, the humidity is so high that condensation could ruin all the sensitive equipment.
  2. Can we safely expose the ASM to the elements? No, the wind is too high, it could damage/contaminate the shell.
  3. Can we see stars? No, there are clouds. Lots of very thick clouds.
  4. Can we close the AO loop? No, the controller of our wavefront sensor camera detector failed.
  5. Can we get PSFs with our science camera? No, it took longer to remove the previous instrument so longer to install ours.

Well the best night to have instrument failures is when the weather is bad anyway. We’re working on a solution. And now it’s time for bed.

No way we were opening tonight.
[Image description: Photo of the observatory status screen showing humidity at 99%, winds at 40.1 mph, and a completely socked-in all-sky cam.]
Part of trouble-shooting the Little Joe controller involved racking out the computer and directly connecting it to the controller, to make sure it wasn’t the extenders. Manny discovered the problem when he started examining individual boards. [Image description: Manny adjusts the cables and connectors of a computer placed below the Top Box, with cables directly connecting it to the instrument.]

Blog rules:

There must be a post every night.

There must be a “Video of the Night.” Something interesting to share. A song is allowed.

Video of the Night: “How this midcentury modern house harnesses the sun”

Annular eclipse of the heart: L&L adventures reprised

I suspect all of our readers will be aware that last Saturday there was an eclipse event over the US. At 9:30 am Tucson Time was the peak of the annular eclipse, an eclipse where the moon is at the furthest point on its orbit, called apogee, so the disk of the moon is a smaller angular size on the sky than the sun (where normally they are essentially the same size) so it doesn’t block the whole disk and you can’t see the corona. Instead you get a “ring of fire” caused by the moon’s antumbra on the Earth’s surface.

Source: https://www.eclipsewise.com/solar/SEhelp/SEbasics.html

Tucson was not in the area of max shadow, it only got about 80% coverage. So some XWCL members traveled to regions getting the full antumbra effect.

I met up with XWCL alum Lauren Schatz and UA OpSci grad Silvana Ovaitt. When Lauren was at XWCL she was my hiking and camping buddy, so we reunited for more L&L adventures by camping in Monument Valley Navajo Tribal Park!

We also went on a backcountry guided tour off the public access road and led by a local named Larry


Song of the day is Black Hole Sun by Soundgarden.

GMT: The 7th segment is in the oven!

This past weekend, the MagAO-X team got to take part in a historic event, the casting of the 7th and final GMT segment! The Giant Magellan Telescope is made up of 7th petal-like segments, and the Mirror Lab—a facility on the University of Arizona campus—is the only place in the world that can make them. These 8.4-meter segments have been in production for decades now, and this weekend the final one has started the 6 month journey of melting glass in the 5-rpm rotating furnace, until it cools to a room-temperature parabola. On Saturday the furnace reached its peak temperature, and from there it begins to cool. Interested parties, donors, and investors gathered to celebrate this milestone for the GMT.

On Friday and Saturday, some of the MagAO-X team helped the mirror lab staff give tours. Jialin and I have been training as tour guides for the last few months, Jared’s been doing it since his grad days, and Maggie was there as a GMagAO-X expert. First stop on the tour is the main attraction, the Furnace Room!

The GMT Segment melting in the spinning furnace.

The furnace is actually two levels, with the lower level focused on controls and system monitoring. You can see the large holder where the mirror segment will be hosed out.

Second view of the spinning furnace.
Ohara glass, what goes into the furnace.


The furnace room was hot! You could feel the difference in the oven heating just between Friday and its peak on Saturday. The next room over, where mirrors are ground and polished, is noticeably cooler than the first room. It’s kept at a constant temperature so that there’s no expansion of the glass as it’s brought to nanometers of the specified shape.

Polishing a 6.5m mirror.

Past the polishing room is the integration room, where GMT mirrors are stored in between their different stages of production. One of them, covered in blue, is actually on it’s way to being stored off site! Others are upside down, as they need their actuated backs attached, and so on. This set up is affectionately called the “CD Switcher”.

CD switcher with 3 different GMT segments.
A mirror almost ready to ship!

The three of us were stationed at the end of the tour in the integration room. This isn’t usually a stop on public tours, but it was opened up for the festivities. We got the honor of explaining how excited we are to do the science that the Giant Magellan telescope is built to do!

Prepping the talks and setting up the posters.

In the marching order, I was first! I introduced what MagAO-X is (an extreme AO instrument directly imaging exoplanets on the Magellan Clay telescope) and explained some of the basics of AO.

Me showing MagAO-X in action.

Next was Jialin, talking about the exciting science we get to do with MagAO-X, and the motivation for wanting to make our pretty pictures even prettier.

Jialin explaining what exactly is so cool about H-alpha acreating proto-planets.

Maggie then got to talk about the plans for GMagAO-X! Her work on HCAT, where we’ve done phasing development in lab, is a huge step forward in the feasibility of the project. She got to show the visitors what a GMT pupil would look like.

Maggie explaining the phasing problem in the next generation of ELTs

Finally, Jared got to talk about his favorite planet. Not caught in action, but by the end of his talk, everyone in the audience was thoroughly convinced of the impact that GMagAO-X will make on the exoplanets we love.

Jared prepping his slides, finding the best fake image of Prox-Cen B.

Hanging out with giant mirrors and speaking on the projects we work on was a huge honor! We hope to get to be back when they pull the mirror out of the furnace in March, and for plenty of tours in between.

The team after all the mirror lab tour madness.

Bonus Video:

The team talking about the GMT in an interview recently! This was shown to some of the guests this weekend, and will be around Steward for a while, I’m sure.