Employment at Keck – Engineering Project Manager

W. M. Keck Observatory position announcement

Project Manager/Engineer

The W.M. Keck Observatory seeks a Project Manager/Engineer to work under the general supervision of the Deputy Director and in close collaboration with the Principal Engineer to manage activities for a major optics renewal program. Be part of a challenging, fast-paced, technical environment where ability, leadership, teamwork, communication and interpersonal skills are highly prized. This is a regular position with future assignments to other exciting optics development programs.

Segment
A Keck mirror segment after stripping and cleaning, ready to place in the chamber to receive a new reflective coating
The Observatory operates two of the largest, most scientifically productive optical/infrared telescopes in the world. The twin 10-meter telescopes are located at one of the premier sites for astronomy, set amidst several other world class observatories at the 14,000 foot summit of Mauna Kea, on the spectacular Big Island of Hawaii. The successful candidate will have the opportunity to join a highly skilled, innovative and deeply committed team of professionals who excel at enabling the most exciting and important astronomical discoveries in the world.

The successful candidate will need to exhibit leadership ability, very strong communication and inter-personal skills and a strong personal commitment to the success of the program.

The principal activities of this position will be:

  1. Project planning, tracking, reporting and proactive management of schedule, budget, risk and contingency
  2. Responsibility for requests for proposal, vendor selection, contract negotiation and contract management
  3. Obtaining staff resources for project
  4. Managing the overall logistics to ensure smooth and effective workflow
  5. Development of quality assurance plans
  6. During the production phase: management and technical responsibility for the renewal program

Subsequent assignments may involve significant technical leadership along with project management activities.

Minimum qualifications for this position include:

  1. Bachelor’s degree in Optics Engineering, or other engineering or physical sciences degree with experience of optics, materials science, physics, or mechanical engineering, and at least 5 years of optical systems design and implementation experience
  2. At least 5 years of significant project management experience in managing projects of $5M or greater. Experience must include devising budgets, schedules and contingency, critical path analysis, risk identification and mitigation, and project tracking and reporting
  3. 5 years of experience in managing contracts, including generating and managing requests for proposal and statements of work, vendor selection, contract negotiation and contract management
  4. Staff supervisory experience

Highly desirable qualifications include

  1. An advanced degree: a master’s or doctorate in a relevant discipline
  2. Experience dealing with optical component vendors
  3. Experience in devising and running quality assurance programs
  4. Familiarity with general mechanical engineering analysis techniques, ideally including experience in finite element analysis and fracture mechanics
  5. Experience with Zemax
  6. Experience in handling large optics (~2m diameter)
  7. Experience in specifying, measuring and aligning optics
  8. Experience in devising efficient information management systems for bulk technical data

This position requires you to submit your resume on-line at: http://keckobservatory.iapplicants.com with your cover letter that states why you are uniquely qualified for the position.

Additional information about WMKO and this position may be found on our website at www.keckobservatory.org EEO Employer

Life of a Photo

It took ninety minutes of sitting in the cold to get the shot. Every minute the camera took another exposure. Sitting on the summit ridge overlooking Keck, it was a very dark night with three lasers working the sky, Keck 1, Keck 2 and Subaru. The tripod was set up as close to the vehicle as I could get it to shelter the camera from the wind. Ninety minutes of shivering in the front seat of the truck, playing cribbage on my phone, and fervently hoping that the gusting wind was not shaking the camera enough to destroy the images.

The result was ninety frames on the memory card. When downloading the material I knew that my time spent in the cold at fourteen thousand feet had been worth it.

Material like this can be used a couple different ways. You can stack the images together to create a single shot equivalent to one exposure 90 minutes long. Taking single long exposures is problematic on a digital camera, a leakage signal called dark current will swamp the image. Better to take many short exposures and add them together in processing.

You can also play the images sequentially, creating a few seconds of video. In this case I assembled all ninety images as nine seconds of video when played at ten frames per second.

I found that the best single frame was assembled from only 23 of the original images. Keck 2 changed targets during the session, creating a confusion of beams over the telescopes when I added all ninety images. The 23 frame version is the definitive version that has been widely distributed. During this slice of time the Keck 2 laser was aimed at the galactic center in Sagittarius, the beam aimed right over me and the camera.

I released the photo as a PR photo for Keck, only fair as I had been on the mountain to work that night, taking the photo before driving down from the summit in a Keck vehicle. The PR folks have used the photo for a number of press releases and observatory literature including the 2011 annual report. You can even download it from the Keck website photo collection.

This particular photo can now be found on websites across the net, has been featured in the Honolulu Daily Star, West Hawai’i Today and other local papers. It has also been used for numerous professional presentations by Keck affiliated astronomers and staff.

I understand that this month it is in Hana Hou! the inflight magazine for Hawaiian Airlines. (Somebody get me a copy. Please! I am not flying anywhere in the next month.) Not the first magazine appearance, you can also find the shot in an issue of Astronomy magazine.

It can be a lot of fun seeing an image I created become something of an iconic image of the observatory.

Three Lasers
Three lasers in operation, Subaru, Keck 1 and Keck 2, 23 x 4min with a Canon 60D

Meeting Sean Faircloth and Richard Dawkins

There is one thing about working at Keck, everyone seems to come here.

I have met a few interesting folks working on the mountain… Famous astronomers like Alex Filippenko and Andrea Ghez, one of my favorite SciFi authors David Brin. Politicians of all levels, county through federal, routinely visit the facility. Just wait a bit, they will come.

Richard Dawkins
Richard Dawkins nice enough to pose with me for a quick photo despite the effects of jetlag and altitude.
This proved true again this week with visits from a pair of famous, infamous to some, visitors. Richard Dawkins is a British author and campaigner for science and reason in the public sphere. Sean Faircloth is an ex-politician, lawyer and eloquent speaker who has likewise taken up that torch. Knowing who was coming I had overstayed my usual shift on the summit to be around for an evening tour.

Unfortunately Richard was not in best form, his legendary wit and charm in short supply. I suspect a little too much travel combined with 13,600ft altitude was taking its toll, he was tired, but seemed to make the best of the tour. Sean on the other hand, was in fine form. The party was rounded out by Christopher Amos, Robin Cornwell, executive director for RDF and IfA astronomer Roy Gal. Our guests were full of questions about the facility and the work we were doing.

We toured the telescopes while the operators and astronomers were preparing for the night. It should have been no surprise that there were quite a few fans in this science centered place, even the visiting astronomers were fans, happy to pause and answer a few questions.

Dawkins Tour
Posing in front of Keck 2 are (right to left) Christopher Amos, Robin Cornwell, Roy Gal, Richard Dawkins and Sean Faircloth
Observing this night included the use of the Keck 1 AO laser and everyone was able to see the beam against a beautiful starry sky. I introduced Sniffen, one of our night attendants and laser spotters. Not that they could see his face, Sniffen was bundled to the eyes, comfortable in the spotter’s chair outside in the cold. The fact that we are mandated to use people to watch the sky for aircraft around the laser was an interesting subject of conversation.

It is always a bit odd meeting someone in person that you have known for years through electronic media. Having read their writings, seen the videos, you form a mental image of a person that may, or may not match who you meet. Personal interaction offers a chance to reconcile that mental image.

It was a pleasure to host a tour of Keck for guests such as these. People who tirelessly push back against the efforts of religious demagogues and extremists to control the path of our society.

Walk through the Solar System

A scale model of the solar system, laid out along Mamalahoa Highway through the center of Waimea. That is what we create every year for the Waimea Solar System Walk.

Starting on the lawn of Keck Observatory headquarters you can walk from the Sun to the outer solar system at the Canada France Hawai’i Telescope headquarters. Four and a half billion kilometers reduced to one kilometer (2.8 billion miles to about 1/2 mile). At this scale the Earth becomes a the size of a small bead and Jupiter a marble. Walking a model like this give a whole new appreciation for the scale of our solar system, driving home the idea that space is really, really big.

Dozens of kids and parents took advantage of the event to learn a bit about space and astronomy. Starting at the Sun they could wander from the inner solar system to the outer solar system. Passports handed out at Keck HQ were stamped at each planet along the way as the tour and each planet was manned by volunteers to answer questions.

Against the odds, it was a pretty nice day in Waimea. The characteristic strong winds and blowing drizzle was absent. We had sunny skies and when the wind died away in the afternoon, it became somewhat hot. This allowed for great views through the solar telescopes and nice conditions to stroll the length of the main street.

The experience was aided by volunteers who came in from organizations across the island, each bringing some educational fun to the planet walk. Nancy Tashima from the Onizuka Center covered Mercury, using some great material from the MESSENGER mission including 3D photos and glasses.

Gary Fujihara brought a splendid collection of meteorites. Using the asteroid belt as his home base to educate folks about the many minor bodies in the solar system and the material that falls to Earth.

Keck and CFHT staff put everything together and manned most of the booths. Members of the West Hawai’i Astronomy club helped out at registration and brought solar telescopes to view our Sun. Given clear skies in Waimea the view was fantastic. There were several good sunspots and wonderful prominences to be seen. It was great to see all those who volunteered their Saturday to help out.

A lot of smiling faces to be seen as kids and parents explored our solar system and learned. Always nice when you can slip a little knowledge in with the fun.

Dusty Road

Rush hour for Mauna Kea is just before sunset. This is when the day crews are coming down, while the summit tours and telescope operators are heading up.

The timing of this rush can be variable depending on time of year and what time sunset occurs. Twice a year this rush is at its worst, when everyone heads up and down at the same time. This can lead to some difficult driving conditions… A lot of vehicles on a road that can be challenging. A cloud of fine cinder dust and a setting Sun just adding to the confusion…

Dust Out
Fine cinder dust creating a hazardous “dust out” condition on the Mauna Kea summit access road

Atop Mt. Hamilton

The visitor directions on the website had specifically cautioned that the summit road was curvy, something I found to be a drastic understatement. From the very bottom it is curve after curve all the way up, with almost no straight sections. S-curves followed sharp bends leading to hairpins. Nearer the observatory the curve intensity only increases as the road narrows. Local history indicates that the horse-drawn wagons that transported heavy equipment up this road could not negotiate steep grades, the only solution was to follow the contour of the mountain, resulting in an incredibly curvy road.

On a sunny Saturday afternoon there were other users, the road is apparently popular with local cyclists. With the density of the sharp curves there was often little choice but to follow at bicycle speeds at times. I would much rather drive up Mauna Kea than this road again. Next time up Saddle to the summit I will recall Mt. Hamilton road and consider myself lucky.

The reason I was climbing this winding road was simply to be a tourist. Unlike the previous seven days, this day was to be fun. For much of the previous week there had been full day sessions of lectures and labs covering the intricacies of adaptive optics systems. Spending a full week in Santa Cruz might be considered a vacation, aside from the fact there had been very little open time to explore the surrounding area. There was only one open day in my travel plans, and I had specific plans for that day, a visit to an observatory.

The 36" refractor at Lick Observatory
The 36″ refractor at Lick Observatory
I arrived well ahead of my late afternoon tour appointment, no problem, just play tourist for a while. At the gift shop / information desk I met Lotus Baker, a longtime Mt. Hamilton resident. She was full of stories and information. We chatted for a while, until her turn to lead a tour of the classic 36″ Lick refractor. Lotus proved to be an excellent tour guide, providing an enjoyable tour of this beautiful telescope.

Continue reading “Atop Mt. Hamilton”

The Last Interferometer Run

Tomorrow morning I will begin to power down the systems. One by one I will open the switches on gear that has rarely been powered off in years. In a matter of minutes it will be off. Dozens of computers, servo drives, camera controllers, racks of gear, silent and dark. I will also shut off the liquid nitrogen to each camera in turn. This will take a bit longer, a couple weeks will be needed to properly warm and back-fill each camera with dry nitrogen for storage. Meanwhile, Brett will carefully cover each optical surface in optical cloth and plastic. A few bits of gear installed in the telescope will be removed to be stored in the basement. By the end of August the Keck Interferometer will be mothballed.

This is the last run, three nights of observations. Two of those are behind us, the third beginning, the end is rapidly approaching.

FATCAT Dichroics
The FATCAT dichroic beamsplitters in the Keck interferometer beam lab
I look about at all of the gear and consider the thousands upon thousands of hours it took to assemble, test and troubleshoot this complex scientific instrument. Years of work by so many people. I look about the control room at the racks of equipment, the masses of cabling, the physical results of so much effort. The non-physical likewise represents a staggering amount of work, the software that allows the entire system to operate. My own contribution seems insignificant. Here and there I note pieces of gear I installed, cables run, cards I have modified, and some many parts of the system that I have had to repair across the years. The sense of loss at shutting this system down is overwhelming.

The plan is to carefully mothball the interferometer in place, in such a way as it could be reactivated with a few weeks of work. Maybe, some source of funding might allow the instrument to be used again, that is the hope. But we know how difficult the current budget environment has become.

Fast Delay Lines
The Keck Interferometer beam expanders and fast delay lines
Still, we are going out in style. This last run has attempted what has never been tried before… We are using AO lasers on both telescopes to reach targets never reachable before. The newly commissioned Keck 1 laser capability making this possible. We have successfully gathered data using the dual laser AO mode, a real first.

Oddly, one of our laser spotters did not make it to the summit and I was obliged to fill in. Fortunately it was a lovely night on the summit, not very cold and with no wind to make it miserable. For a couple hours I relaxed in the Laser Suzan chair, watching the sky. Above me arched the Milky Way, somewhat dimmed by a bright Moon, but still beautiful. A few bright meteors punctuated the night. The scene was a made a bit surreal by three lasers, all targeting the galactic core, the very center of our galaxy. Beside me the camera regularly issued the soft sound of the shutter, taking images of the night.

The second night was a series of galactic targets and a couple AGN’s. The final analysis will take time, but initial indications are that we have good data on at least some of the targets. A couple targets proved too faint for the system to track on. No surprise, we planned to reach a little with this last run.

Thus we begin this last night, the practiced evening routine is complete, final checks done. The last targets a list of selected YSO’s (young stellar objects) to be observed in L-Band. We settle in for the night, hopefully a quiet night. As usual, if I am busy, things are not good. All is going well, a fitting end to the instrument and a testament to all those who have put so much into the system. Something to remember.