Sep 16, 2019
April 2, 2019
NIFS has been available since semester 2006B for classical and queue scheduled observing at Gemini-North.
January 2013: On Instrument Wave Front Sensor (OIWFS) is unavailable due to a faulty sensor.
October 2012: New 'LGS+P1' guide mode is now operational, allowing 'seeing improver' AO correction with essentially 100% sky coverage.
2018 Nov 26 - Dec 14
GNIRS was removed from the telescope to work on filter wheel #2 which had been showing increasing instances of not going into position reliably. The filter wheel datum switches were replaced on both filter mechanisms, a temporary light baffle was removed from wheel #1, and dust was removed from the filters using CO2 snow.
2018 Jun 20-25
Re-seated the detector controller boards, replaced the sequencer board, and replaced a voltage regulator. The read noise levels are now back to normal.
2018 Jun 5
2018 Oct 17
2019 Dec 31 - Zorro runs in 2020A have been scheduled between March 10 and 18, and June 29 and July 5. Phase II deadline has been set for February 17th.
2019 Oct 05 - 'Alopeke spent the weekend in the Hilo lab where Nic installed a new pickoff arm position sensor and realigned the optics in preparation for using the new mounting spacer ring.
To highlight relevant issues that are still relevant I have moved old/historical information to the end.
Update June 26th, 2019
As a friendly reminder proposers should be aware that:
August 26, 2019
Update November 6th, 2019
F2 is back on sky, fully operational for imaging and long-slit spectroscopy with the OIWFS.
Update September 26th, 2019
Recovery of the cooling was unsuccessful and the cold-heads in F2 must be replaced. This means that the instrument will be unavailable for approximately 4 weeks.
Update September 12th, 2019
The F2 detector has been warming up and has reached the limit for operation. We are working to recover the cooling, but until this is fixed F2 is not available for observations.
New GMOS-N B600 Grating Available
A new B600 grating has been commissioned and is available for science use in GMOS-N. This grating replaces the original B600 grating which was damaged in December 2008. Active programs that are configured to use the original B600 grating will automatically use this new grating for any new observations executed.