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uc:uc20230627_june_27_2023 [2023/06/27 18:28]
nchanove
uc:uc20230627_june_27_2023 [2023/06/27 18:43] (current)
nchanove
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 As for near term goals, we are currently in the conceptual design phase and hope to have a Conceptual Design Review by the end of CY23 or early 2024. We may also have a refined survey of the user community for people to weigh in on science needs. To reiterate, the instrument development team is really interested in getting feedback and engagement from the ARC community so that they can deliver an instrument that meets the needs of the community. As a more practical requirement, the funding environment for instrumentation is challenging and we will need to develop well thought out science cases to pursue funding opportunities. As for near term goals, we are currently in the conceptual design phase and hope to have a Conceptual Design Review by the end of CY23 or early 2024. We may also have a refined survey of the user community for people to weigh in on science needs. To reiterate, the instrument development team is really interested in getting feedback and engagement from the ARC community so that they can deliver an instrument that meets the needs of the community. As a more practical requirement, the funding environment for instrumentation is challenging and we will need to develop well thought out science cases to pursue funding opportunities.
  
-Chip indicated that having an R~60k mode would enable lots of science, for example stellar abundance work like Caty Pilachowsky at Indiana University is doing. Kevin countered that for solar or giant type stars there is no scientific advantage for R~30k or 60k.+Chip indicated that having an R~60k mode would enable lots of science, for example stellar abundance work like Caty Pilachowski at Indiana University is doing. Kevin countered that for solar or giant type stars there is no scientific advantage of R~60k over R~30k.
  
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 === Training update ===  === Training update === 
  
-book-keeping +Nancy mentioned three items: 
-surveys +  We are aware that the list of trained individuals on the APO web site is outdated. We have been maintaining a separate list and will be merging that with the online list to ensure that the information presented online is current. 
-heads-up for Q4+  For those who come to APO for training visits, please urge all training participants to complete the evaluation form provided by Nancy. We strive to continually improve our training offerings but we need to hear from recent trainees about what worked well and what can be improved. 
 +  - We are expecting at least three class visits during Q4, maybe more. **All institutions planning to bring classes to APO in Q4 should let us know ASAP so that we can prepare and begin to head off potential schedule conflicts.**
  
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 === June AAS meeting recap ===  === June AAS meeting recap === 
  
-New backdrops for booth, ppl liked swag - great contacts  +The June 2023 AAS meeting in Albuquerque was a success. We have new backdrops and banners for the booth, which looked really nice, and people liked the swag we gave out. The talk about APO that Nancy gave in the special session about astronomy in New Mexico was well received and generated interest, questions, and potential opportunities for new collaborations.
-good talks, interest, areas for new collab+
  
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 New action items from this meeting: New action items from this meeting:
 +  * UC reps: remind your users to let us know ASAP if they need any KOSMOS slit widths that are not listed in the planned set to be delivered in August. 
 +  * UC reps: ask your users to review the instrumentation notes above and provide Nancy with feedback if they have any. 
 +  * UC reps: ask your institutional colleagues to notify us ASAP if they are planning to bring a class to APO in Q4.
  
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uc/uc20230627_june_27_2023.1687890485.txt.gz · Last modified: 2023/06/27 18:28 by nchanove