Category Archives: WFU

Wide Field Upgrade is the commissioning effort to prepare for the new improved HET with the new secondary and instrument suite.

The week of June 30th

In the past week we have had a number of very strong thunder storms one of which blew out one of our 480 V contactors in the new tracker electronics. We found we don’t have a spare for this relatively inexpensive components so we are ordering a replacement and several spares. We hope to have this in place in the next day or so. Once back up we will continue to work on the TCS trajectory generation.

Next week we have some of the engineers and most of the software team coming out from Austin for a first attempt at running trajectories with metrology. The DMI is back from France and ready to be installed on the test mass along with the tip-tilt camera and the Video Alignment Telescope (VAT). This week we are just making sure all of the communications and power connections are in place for this set of tests.

We have four different contractors on site this week working on the Remote Thermal Area project. One is building the forms for the remote concrete pads, another is digging a trench between those pads and the vault which was completed last week, another is putting in ducting in the vault and the last is installing ducting inside the spectrograph room, lower and upper electrical rooms. The afternoon storms are slowing the work slightly.

The week of June 23

The rainy season has begun in West Texas. In the last week we only opened once at night; during that night we were able to capture the mirrors taken out for the 21 point test. Mirror alignment is now routine.

The rain is also having a small impact on the contractors working in W. Texas on the remote thermal area. The large pipe vault has become a nice reflecting pool and it is clear that we will need a french drain at the low end of this vault even though the expectation is that the vault with be mostly sealed to the runoff. The concrete vault has been completed and this week the electrical and mechanical contractors are placing conduit in the vault.

This week the Distance Measuring Interferometer (DMI) arrived from France and the engineering team in Austin made sure that it will fit into the test mass mounts which will come out in the 2nd week in July. The DMI will arrive in W. Texas on Thursday so that we can get it setup in the coming week both for the test mass and for the CCAS tower.

Work on the TCS (telescope control software) continues this week. The team hopes to be generating trajectories using RA/DEC or Alt/Az by the end of the week.

The week of June 16

This last week the two engineering teams from Austin worked both days and nights to get their work done. The day time team was able to get the mounts for the Tip-Tilt camera, VAT and DMI on the telescope. They were able to get the VAT installed and found that the center mirror is just 30 mm off from the center of the X and Y tracker encoder ranges. We still need to determine where the encoder ranges are with respect to the upper hex which brings us to the work of the other engineering team. This team worked most of the nights this past week including weekends to get the 97 point test started. They determined that to take a set of 18 laser tracker data points at each tracker position takes far longer than anticipated and so descoped to a 21 point test instead of a 91 point test. Even with this descope the 21 point test took 15 hours of work.

This week the Austin engineering teams have departed and are working on new mounts for the test mass based on lessons learned from this past week. The data from the 21 point test needs to be analyzed and we will followup any questions that analysis may bring up with further laser tracker measurements.

The mirror teams are swapping two mirrors into the array this week and later this week the cabling teams will be putting on the clamps in the Azimuth cable wrap and fixing any cabling problems that might have developed with the full range to tracker motion that we can now make.

The contractors from Veliz Construction made substantial progress this past week. They completed the first concrete pour for the pipe and electrical vault and this week they will be setting up the forms for the second pour (which will be the walls of the vault. We will also have the electrical contractor on site to complete some Phase I punch list items and review the site for the Phase II electrical work. We will also have Gaffey Crane on site to work on the dome crane box which must have a new form factor to avoid collisions with the stinger from the Y-drive.

The week of June 9

A great deal of effort was put into fixing small problems with the tracker software and hardware last week. By the end of the week we were able to run a mock 97 point test and even a mock trajectory. There are still some small problems using the GPS timing signal which is needed for running a true trajectory but this is a significant step forward. This week we will have two sets of engineers from Austin. One group will work on the 97 point test which will map out the tracker sphere in space and tie that sphere to the mirror truss through the use of the laser tracker. This will be done at night so that significant temperature changes do not alter the results. The corrections to tie the tracker and mirror truss spheres together will be the first components of our mount model.

The second team will be installing the mounts for the Video Alignment Telescope and the DMI on the corrector. Once these items are in place and we can run trajectories we will will begin to tie the tracker sphere to the central mirror and then refine the mount model further.

The contractors did not begin the “vault” cement pour as expected this last Friday. Delays caused by the significant heat and a small delay in the rebar arrival have put that off until this coming Wednesday.

The night operations team has been able to get all of the mirror with current electronics installed into the stack. As soon as more SAMS (Segment Alignment and Maintenance System) electronics cards come in from the contractor the remaining segments will be brought into the array.

The week of June 2

We are experiencing exceptionally hot temperatures over the weekend and these are expected to continue through the week. These high temperatures seem to be impacting some of the electronics that allow us to align and maintain alignment of the primary mirror. The mirror team will continue to improve the actuator zero points, clocking of the segments and gaps between the sensors.

We did not complete the 97 point test last week. This was largely due to teething problems with the new tracker control software. We will continue to work these out this week in preparation for another attempt at this milestone next week. Next week we will also be installing the Video Alignment Telescope and DMI mounts on the corrector test mass to prepare for the alignment of the tracker with the primary mirror. We hope to be able to do both sets of tests next week.

The contractors working on our remote thermal area are making good progress and will continue their preparation for the “vault” cement pour which should take place this Friday. The vault will protect the power and glycol lines as they pass under the service road behind the HET.

The week of May 26

Slightly shorter week since Monday is a holiday. The main goal for the week is the 97 point test. This is a mapping of the tracker surface such that we hope to generate a series of trajectories that map out a sphere above the primary. This sphere should be centered on the geometric center of the upper hex and have the same shape as the primary mirror. This will require that our Telescope Control System (TCS) is up and running. This will be the first test of the TCS systems and we should expect the normal number of communication protocol problems and software glitches. This 97 point test will be a significant milestone for the WFU project.

The duty Telescope Operator and the mirror team will continue to get the primary mirror in shape by aligning the mirrors every night and adjusting actuators and sensors every morning.

The week of May 19

In the past week we began several new projects at the HET. One is the Remote Thermal Area. This week that project continues with the contractors from Veliz Construction and BP locating all of our buried water, glycol and lightening protection lines around the back of the facility and starting the trench work for the new lines. This work should continue all week.

The other project is the sealing of the dome louvers. Over the years the brass seals on these louvers have blown off and we have had significant ingress of dust and rain under high winds. We have identified a new adhesive that should keeps those seals on over a much longer time scale. One of our TOs is working on the installation of these seals and based on last weeks work she finds that it takes a full day to install a seal all the way around each louver and there are 4 louvers in each bank. She hopes to be finished by the end of July.

Mirror alignment was begun last week. This is a fairly slow process and we have captured about 70 mirrors into our array and the rest require some by hand alignment, which will be done this week. This is moving along steadily and should be ready by the deadline to stay to schedule… the 2nd week of June.

Last week we made considerable progress in getting the track to run consistently. The source of the metal shavings was located: with the additional weight of the tracker the encoder track deflected and the encoder trolley had to be realigned. We will continue to fine tune the encoder head position as we add more weight to the tracker.

The Constant Force Drive is now operational and can move the track at will in the Y direction. We have repaired the burned out cards but we have not identified the source of that damage. This week we have a few odds and ends to prepare for next week’s 97 point tracking test.

The week of May 12

In the past week we made some progress with the Constant Force Drive (CFD). We found that one of the units of the Current to Voltage board had burned out. We also found that all of our spares have had a similar problem. We ordered an industrial drop-in part which does not quite fit the form factor for the electronics rack but did allow us to continue commissioning. We still have not determined why the boards were burned out but we will try to refurbish the parts and replace them as time allows. We also have one of our Telescope Operators now running the tracker. On a less positive note we found some metal fillings in the lower X encoder. This may simply be the race finding a new home under the weight of the tracker but we need some additional testing to determine if further damage may be occurring.

The mirror team was able to get all of the edge sensors back on the mirrors but we have run into significant communication problems with the CCAS alignment tower that did not allow us to fine align any of the mirrors in the array.

This week will be taken up with getting the communication problems with the CCAS alignment tower sorted out, investigating the problems with the lower X encoder, and trouble shooting the Current to Voltage boards.

We will also have contractors from Veliz Construction on site to start our big Remote Thermal Area project which actually includes a number of small projects including: Ducting heat from the Krabbenhut away from the telescope, ducting away and diluting acid vapor from the strip and wash room, installing the remote air conditioning and glycol chilling units, and installing the huge liquid nitrogen tank for the VIRUS instrument.

The week of May 5

It has been a few weeks since the last blog post. The blogger was out of town…

In the past few weeks there has been considerable progress. The hexapod assembly and PFIP have been mounted on the tracker. Many of the tests have pointed to significant communications troubles with different circuit boards, broken wires etc.. Many of these have been resolved and we have fairly stable X motion of the tracker but the Constant Force Drive (CFD) has been not been behaving well so that has limited the use of the tracker in Y. Since most of tracker cabling work and repainting of the upper hex are complete we have been able to remove the safety net above the primary mirror and begin installing the mirrors. In the past week the mirror team removed the net and installed 40 recoated mirrors.

In the rest of this week the mirror team will be installing the last mirrors (leaving a few holes in the array so that we can install test spots for the laser tracker). Once the mirrors sensors are in place we will begin aligning (stacking) all of the mirrors with night operations. This will be the first night time operations for the Telescope Operators since August 2013. Once the mirrors are aligned the mirror team will piston the array. This work will likely take the rest of the week.

In parallel, we hope to have some new circuits in place later this week which will allow the tracker team to test the CFD and Y motions again. Once those are working then they can test the hexapod motion.

Other work that will be done this week in parallel are the work on the purge air lines, installing mounting plates for future testing equipment and a punch-list of software and hardware work.

The Week of April 7

In the last week we saw some further new use of the Strip And Wash (SAW) Room. The mirror team was able to install the wash pan into the mirror bracket allowing them to install a mirror either face up or face down. This allows them to use a hot brine bath for the mirrors to further clean the mirror. The current procedures now involve installing a mirror face down; a soak in the brine bath; remove the mirror and bath; install the mirror face up; a rinse; a ZrO scrub; a final rinse; sheet dry; hot air drying of all other parts. We are well on our way to doing acid stripping of the coating once we have the acid vapor removal in place.

At the end of the last week the tracker team was able to get the system to track and slew upon request. The problem seems to have been an intermittently bad connection to the encoder.

With the encoder problem solved the team will now use the laser tracker to map out the position of the tracker through all positions, X and Y. Once that is done they will install the hexapod assembly and begin testing those, first independently and then as part of a trajectories.