APO 3.5-m Users Committee Phonecon, 4/04/11 Attending: Suzanne Hawley, Mark Klaene, Michael Strauss, Bill Ketzeback, Scott Anderson, Remy Indebetouw, Sean Moran, Jon Holtzman, John Bally, Al Harper, and Bruce Gillespie ********************************** User feedback, comments from institutional representatives: o New Mexico State (Jon Holtzman) - Jon had nothing to report. o Washington (Scott Anderson) - Scott said that one of the UW users could not display DIS slit-viewer images. This was within TUI, and seemed to be a permissions issue. Nobody else on the phonecon reported similar problems, so the problem may rest at UW. Mark said that there is a problem report that seeks to get rid of permissions for slit-viewer and guide camera images, which may be related to this problem. This also could be because of the known "two IP addresses needed" feature, one for login and the other for HTML. Bill Ketzeback agreed to look further into this. ACTION: Bill Ketzeback to look into and suggest fix to permissions and/or IP issues in TUI related to slit-viewer and guide camera images. o Colorado (John Bally) - John had nothing new to report o Princeton (Michael Strauss) - Michael said everything is fine. o Johns Hopkins (Sean Moran) - Sean had nothing new to report. o Virginia (Remy Indebetouw) - Remy said that he couldn't get to the APO weather pages or users manuals from a hotel. He could run TUI fine, which is weird. Mark said that he will verify that all the APO pages are "open". o Chicago (Al Harper) - no report. ********************************** Discussion of telescope/instruments report - Klaene: Mark mentioned the highlights from the past few weeks. It was a hectic month, and quarter, at APO. There was the GFP upgrade effort with the NASA/Goddard folks at the site, a Colorado student group, closely followed by the 2nd annual open house, and then the BOSS team meeting in Cloudcroft. It has been dry and windy, more dry than usual and that could lead to forest restrictions being put in place within weeks. Nonetheless, with the generally clear skies a lot of observing has gotten accomplished. The DIS slit-view camera will be removed soon so that measurements can be taken; a rebuild is being planned. The spontaneous Agile aborts seem to be much improved, and as far as we are concerned, fixed as well as can be without undertaking a complete replacement of the Agile computer and controller. The other instruments are working well, and for NIC-FPS, the read noise is much better, but the upside-down readout problem is still with us. Although the controller often fails when the instrument is inverted while tracking and observing, the recovery is quick. The GFP upgrade will continue in June. Mark's detailed report for the reporting period follows: ************************* 3.5-m Telescope, Instruments, and CIF Projects Highlights 2/24//10 through 3/30/11 0) Overview Weather has been generally good with occasional spring winds and elevated dust levels. The site was busy much of March with the NASA Goddard folks on site in early March working on GFP-IFS followed immediately by a large group of students from Colorado, then the APO Open House which brought about 88 members of the public, and ending with nearly 100 SDSS-III astronomers in town for a BOSS collaboration meeting. In preparing for the open house the APO display at the Sunspot Astronomy Visitor Center was completely remodeled and updated. Gretchen Van Doren was a key organizer for many of these events and did a magnificent job. The forest remains dry and extreme forest fire danger is expected with access restrictions starting soon. 1) Telescope Virtually no telescope problems were reported during this period. The spare direct-drive motor is now complete. 2) Instruments DIS performed well this period. Work is planned for April to remove the slit-viewer assembly to investigate new mounting options and replacing the camera and optics. SPICam operated with no new issues. Agile spontaneous aborts work is complete for now. There may still be a rare failure at the start of an exposure sequence, but changes to software have all but eliminated the problems of the past. Also work has begun to install a brake on the rotator. Previous work has eliminated the rotator failures and the brake will eliminate the need for the pin and will hold the rotator in place when the power is off. TripleSpec is not reporting slit position in the headers. This is on the list of things to fix. The echelle has been running slightly warmer than normal so time has been set aside in April to vacuum pump the Schmidt camera. NIC-FPS was returned to the observatory after a very successful trip to CU. Upon return, the read noise is now better than the 2 channel configuration. However the problem of spontaneous reset of the Leach controller when rotated upside still exists. Users are advised to start their observations at specific recommended rotation angles, depending on sky position, to avoid tracking upside down. There is also a software alert in place that should trigger if an image is bad. See more below. GFP upgrade started on the mountain in February. After a return trip by the Goddard folks in March the direct imaging and IFS modes are working. The FPS and photon-counting modes are still under development as is TUI integration. We are hopeful that in the scheduled June engineering run they will make further significant progress. The instrument is currently not available for use. ********************************** current NIC-FPS readnoise, gain, linearity information (recommended observing is with NFS=8) NFS readnoise 1 30.0 2 20.9 3 18.3 4 15.3 5 14.4 6 13.5 7 12.6 8 12.4 Gain = 2.94e/DN linear to within 3% up to 54,400 raw counts and at 5% up to 56,800 counts. ------------------ NIC-FPS rotation recommendations depending on sky position of object: Basically, the northeast is the problem quadrant; that's where the instrument will be upside-down at default 0 object rotation. Sky quadrant recommended object rotation northeast +-180 (positive better if observer plans to track for awhile) southeast to south -90 southwest 0 northwest +90 Note: the rotation needs to be changed for every target. For example, when leaving program star and moving to standard star, users must put in new rotation appropriate for standard star's position in the sky. Best way to see where the next target will be is from the TUI window showing the telescope position on the sky (window is labeled "SKY"). If in doubt, ask the Observing Specialist! The current plan is to take the instrument back to CU during the summer shutdown and replace all of the detector cabling inside the dewar with the hope that this will fix the rotation problem. ********************************** NIC-FPS status - Hawley: Suzanne had three things to mention: o NIC-FPS characterization - see the report, and we're pleased with the reduced noise performance. NIC-FPS is back in service. o the rotation issue - should we set rotation limits in software? It is hard to imagine simple tools for the users to avoid the inverted rotation angles (50 to 60 degrees range around -180), although Sky View will show you this information for the next target on your list. Observers need to watch their images closely to see if the controller is hung up; a warning message is now displayed. NIC-FPS users need to be especially vigilant while observing. ACTION: Users committee members to advise NIC-FPS users about instrument rotation angle issue and need for vigilance. o Stephane Beland will work on the rotation problem this summer. After 19 June, NIC-FPS will return to CU and will have all its internal cabling replaced during July. A message to this effect will go out to the schedulers next month. ********************************** GFP upgrade - Klaene: Mark reported that the GFP upgrade is in the early stages of commissioning. The Goddard team is working to get the new features functioning through the instrument control computer, after which some of the new capabilities will be implemented in a TUI interface. A concentrated effort to work on commissioning is planned for June. The new capabilities include an integral field unit, a new detector with 3 electrons read noise, and a lenslet array. The GFP throughput is now estimated to be 20%. There is still a fair amount of work left to do. Suzanne added that the Users Committee members should share this information with prospective users, and collect feedback. The slides that were included with the agenda give more details on FOV, etc. and can be shared by committee members with interested users. Michael suggested that the new GFP detector could be used for direct imaging; even though the field is relatively small, the lower read noise might make it advantageous for some projects. Suzanne said if anyone has interest in using the upgraded GFP for early science in Q3, they should let her know and she will make sure contact is made with the Goddard group. The earliest return of GFP for regular science use will likely be in Q4. ********************************** Summer shutdown schedule - Klaene, Hawley: Mark said that planning for the summer shutdown is progressing, and will include a realumization of the primary mirror at Kitt Peak. The shutdown will begin on 5 July and nominally end on 28 July. The last five days of the shutdown involve on-sky testing before returning to routine science observing. Given the typical weather vagaries in late July, the actual return-to-science date could slip. ********************************** Update on logging scripts - Ketzeback: Mark noted that the logging scripts for DIS are in good shape, and are being considered for some of the other instruments. Bill said that the DIS scripts match science images with the corresponding guider images. Adam Kowalski (grad student at UW) wrote most of the core code for the DIS script, and Bill did some additional work on it. Bill provided a description of the DIS script [see note below]. John Bally, who was instrumental in requesting this capability, said that he's looking forward to using it. Suzanne mentioned that we still need to understand what is required to implement the logging script working for TripleSpec. The echelle would be another possible instrument to consider. Suzanne added that we would like to get user feedback on the logging scripts. ACTION: Remy Indebetouw to get the logging script specifications for TripleSpec. [note added, from Bill Ketzeback]: Adam Kowalski and Bill Ketzeback have a program running on newton.apo.nmsu.edu for matching up DIS exposures with corresponding slit viewer images. To run the program, log into your institutional account on newton and in the home directory (or subdirectory) type: "dcam_match". The program will prompt for the program id (example: Q1PU04) and the ut date of the observations (in the form YYMMDD, example 110327). The program will output a unique log file with information in the title (example: dcam_match_110327_Q1PU04.out). The contents of the file contains a header explaining each of the columns. The following is an example output for a recent program. # UT110327, number of science files = 11 # Column 1: Science file (only IMAGETYP=object are included) # Column 2: Nearest slitviewer image # Column 3: MJD (hours) for the midtime of the science file # Column 4: Midtime of science image - midtime of nearest slitviewer image (seconds) # Column 5: Range of slitviewer images that have mid-times within the exposure of the science image dvb.0001r.fits d0058.fits 7.8607 15.22 d0042.fits - d0075.fits dvb.0002r.fits d0094.fits 8.2656 9.94 d0086.fits - d0102.fits dvb.0003r.fits d0121.fits 8.4737 -0.56 d0120.fits - d0122.fits dvb.0004r.fits d0146.fits 8.7376 -14.58 d0129.fits - d0162.fits dvb.0005r.fits d0186.fits 9.2046 -0.71 d0170.fits - d0202.fits dvb.0006r.fits d0215.fits 9.5523 14.51 d0207.fits - d0223.fits dvb.0007r.fits d0247.fits 10.0089 9.18 d0230.fits - d0264.fits dvb.0008r.fits d0302.fits 10.5684 -17.61 d0293.fits - d0310.fits dvb.0009r.fits d0322.fits 10.8101 13.25 d0314.fits - d0330.fits dvb.0010r.fits d0340.fits 11.1214 -36.44 None dvb.0011r.fits d0341.fits 11.1598 54.43 None For more experienced users, the user id and ut date can be entered on the command line, for example: dcam_match Q1PU04 110327 Plans for similar scripts for the other instrument-guider pairs are in the works. ********************************** Echelle upgrade - Holtzman: With help from the instrument development group at JHU, Jon hopes to identify, acquire, and install a more efficient grating for the echelle this summer. Other upgrade options including a new detector are on hold at the moment, pending additional effort to determine if the payback will be worth the cost/risk. ********************************** Miscellaneous - Hawley: Suzanne gave her appreciation to the site staff, Gretchen Van Doren in particular, for all the support provided for recent site activities. ********************************** ACTION ITEMS: [open from previous meeting]: ===> ACTION: User committee members to poll their users to determine if astronomers and/or students are willing to help with the ARCSAT upgrade proposal and/or its implementation if funded, and for what scientific objectives? There was no feedback from Princeton, Colorado or Virginia. NMSU is interested, as are several people from UW. There is some interest at Chicago, and Sean will check again at JHU. Suzanne said that we need "interest" that includes a strong motivation to get involved; we'll keep this action open for another month. [new actions from this meeting]: ===> ACTION: Bill Ketzeback to look into and suggest fix to permissions and/or IP issues in TUI related to slit-viewer and guide camera images. ===> ACTION: Users committee members to advise NIC-FPS users about instrument rotation angle issue and need for vigilance. ===> ACTION: Remy Indebetouw to get the logging script specifications for TripleSpec. ********************************** Next meeting: The next Users Committee phonecon will be on Monday 9 May at 8:30 AM Pacific Time. The agenda and other materials will be sent to the committee members during the preceding week. APO APO APO APO APO Apache Point Observatory 3.5m APO APO APO APO APO This is message 1223 in the apo35-general archive. 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