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2014B Day 16: What Color Is Your Pyramid?

We had an action packed night, with many more targets than we’ve been observing so far on this run. The AO system wasn’t on its best behaviour, but we have learned to recognize most of its bad moods quickly and we can usually slap it back into shape right away.

A door opens to a busy night

Kate Follette is here, ready to help take up some of the operations load. Our visiting observers tonight were Hector Canovas and Adam Hardy from Universidad de Valparaiso. Here’s a shot of the bleary eyed “aoistas” this morning right before we quit, minus Katie who’s behind the camera, and minus Kate who went to bed too early to get her picture took.

Left to right (in 2D): Jared, Adam, Hector, and Jorge. Katie is behind you. Kate == false.

In Kate’s defense, she made it to the half-way point after 24 hours of travel from Tucson.

Most of the targets we looked at for our new friends Hector and Adam were faint and red. When we set up the system for such targets we need to have a good guess how many photons per second the pyramid wavefront sensor (PyWFS – following the obviously correct conventions of Guyon 2006) will get. This can be tricky because our PyWFS has a very wide and very red pass band, something like R+I. So if you use the R magnitude on an M5 star, you’ll set up to run slower and with fewer modes than you need too. It’s worse if you give us the V magnitude. So tonight I whipped up a set of synthetic color corrections, and compared them to our PyWFS’s own estimates.

UPDATE: A day later, we have investigated why the R band colors were weird in the first version of these plots. We are now using a self-consistent set of VRI magnitudes, from the USNO UCAC4 catalog, transformed from APASS gri (AB). I think we can now declare the MagAO WFS pass band done. I’ve updated the next two plots to the latest, most correct version.

Our PyWFS filter, calculated from manufacturer curves for everything I can think of. The VRI curves are from Bessel (nineteen I forget the year).
MagAO WFS color corrections from standard “Bessel” VRI filters, using the Pickles spectral atlas. The data points are from the PyWFS estimated magnitude which is an independent calculation of Alfio’s, and the UCAC4 magnitudes.

Here’s a fun set of bookends on the night. We took flats at evening and at morning twilight. During this, you can see a really cool pattern on the PyWFS. You can also see the secondary mounting structure lit up by the sun. See the difference?

ThePWFS during night time flats
The PWFS during morning flats.

Here’s a just-after-dawn shot to the west, towards the Pacific Ocean.

The marine layer intrudes through the coastal passes below us every morning. It tries, but almost never makes it here.

Though you might think this was about the ASM supports being too reflective, the song of the day is for Veteran’s Day.

2014B Day 15: The Aoista Operation

Our T.O. for the last week, Jorge, has dubbed us “the aoista operation”. Tonight was pretty calm – no major technical problems, a few scientific discoveries, and a pretty relaxed night. The clouds rolled in a couple of hours before dawn, so we closed out with some minor engineering tasks.

Tonight was TJ’s last night. So long. Kate is (possibly) arriving today, and tonight is the first night for our Chilean observers. We’ll have some new faces on the blog this week.

Here’s what the control room looks like from the middle of a calm night
Katie worked on Clio’s FITS headers. If you look closely she’s editing the c code that runs Clio.
A lone burro was seen after dinner
No burrows at the top today. But they were there earlier.

This is not the greatest blog post in the world.

Nay. We are but men.

2014B Day 14: Remote

Baade (left) and Clay (right) at sunset.

Things went pretty well tonight. Alfio called us to check in and we could proudly show him that his software is keeping MagAO running smoothly:

Alfio calls in from Firenze to check on our progress.

In fact, we are mostly keeping his chair empty for him:

Also, Alfio is here in spirit, running the AO system — his software has been working so well, we just leave this chair empty and let Alfio’s code run the show.

Except for when things need attention:

Jared, T.J., and Jorge running AO, Clio, and the telescope

Our friends over at Cerro Pachon are observing with GPI on the Gemini South telescope for the Gemini Planet Imager Exoplanet Survey (GPIES):

Chilean telescopes tonight: MagAO and GPI

I was Skype-chatting with them a bit tonight:

Here I am chatting with GPIES

We talked about astrometric calibrator fields, such as the Trapezium:

Jared shows us how it’s done

At the end of the night, seeing spiked up to 2” and we couldn’t keep a lock on our faint science target — it was the equivalent of clouds rolling in, we lost so much light.

At the end of the night, the seeing spiked up to 2”, making the WFS think clouds had rolled in.

So we tried an experimental target instead. Here is a quick snapshot of HD 269433 (all we could get before the loop opened again, as the Sun was rising too). It looks like this one, which is in the LMC and our WFS read as R=12.1 mag, will not work as a good astrometric calibrator for GPI.

Attempting an astrometric field – a quick snap-shot of HD 269433 in Ks-band Narrow camera. The circle is the GPI field of view.

Jason Wang is blogging about GPI this week and we tried to keep up with him:

Trying to keep up with Jason

Over at GPI, the GPIES team saw a vizcacha tonight by Gemini. I wonder if they stole ours, we have had so few sightings this run! But tonight, Jared did see one or two vizzies by Magellan at sunset:

Vizcachas at sunset

Also, we also saw a herd of burros on our way up to the top tonight:

Donkeys on our way up to the top

And we took a picture for our loved ones back home:

Hello everybodeeee!

Finally, today is Jared’s mom’s birthday, so here are some pictures of her favorite oldest son for her to enjoy:

Happy birthday to Jared’s mom!

And finally, here is a beautiful song from South Africa:

2014B Day 13: Settling In

It’s day 13 – we’ve been here almost 2 weeks out of 6 now – so we’re almost a third of the way through. I think of it like running a 5k (3.1 miles) where the first mile is the phase where you try to get out ahead of the pack, and the second mile is where you settle in to your pace. That’s where we are now, we’re settling in. Here’s a little bit about what that looks like.

Jared is starting up at the beginning of the night.

I’ve been monitoring the temperatures on Clio. Last week we hooked up the new pump, which is stronger than the old pump, and I was worried that the temperature wasn’t settling quickly enough.

Clio temperature monitor, plotted as a function of # of hours since we started cool-down this run. Top: The temperature of the Clio optics in Kelvin (77 K). Center: The temperature of the Clio detector in K. Bottom: The percent the heater is turned on. Each spike in temperature of the detector is when the Clio dewars are filled with 77-K liquid nitrogen, which melts the solid nitrogen and warms it up. Then the pump starts pumping away and lowers the pressure so that the nitrogen freezes and solidifies. The temperature keeps dropping, but we want to keep it stable, so when the temperature drops below the set point (53.3 K), the heater engages and tries to keep it at a stable temperature.

But take a closer look at just the detector temperature. I don’t think it’s quite as stable as it could be. I will think about this some more and possibly throttle the pump, crank up the heater, or go back to the old pump.

Take a closer look at just the detector temperature (bottom plot here). It isn’t quite stabilizing at the tenth-of-a-Kelvin level. I have to examine the darks to see how much it affects us. Also, the new set-point means I had to adjust the bias voltage, which means there is going to be a new linearity correction this run. Stay tuned.

Finally, some LCO lifestyle pix as we are settling in:

Sunrise from the summit

Dos huevos fritos por favor con aguacate, oatmeal, and fresh-squeezed orange juice
Life at LCO – breakfast then bed (please do not disturb)

A great song:

2014B Day 12: Who’s Driving This Thing?

Now that we have 3.3V where we’re supposed to have 3.3V, and we’re using good fiber cables, everything is easy. It was also a nice night, with stable (if not always good) seeing. This is much more relaxing than some earlier nights. It also means there isn’t much to write about.

I pretended to be Yuri tonight.
T. J. closed the loop for himself.

These next two pictures were taken about 10 minutes apart.

Moonrise over the Andes
Sunset in the valley