After the completion of the GHOST commissioning, the GHOST Cassegrain Unit was removed from the telescope and IGRINS was installed back on the same port last Monday. Back on sky checks were performed successfully on Tuesday night and the instrument was used immediately for science operations.
The GeMS Real Time Computer is currently experiencing technical difficulties preventing the use of the instrument for the rest of the June 2022 Run. Sincere apologies to our user's community!
The Gemini North Adaptive Optics system, Altair, is currently offline due to a recurrent and intermittent issue with its deformable mirror (DM). Please email your contact scientist if you have any questions or concerns about the potential impact on your program.
On April 28th, 2022 GNIRS is planned to be removed from the telescope and warmed up in order to perform the GNIRS IFU installation and various refurbishment work, which includes replacement of ball bearings for both filter wheels. It is foreseen to have GNIRS back on sky for the IFU commissioning on July 6th, 2022. During this period, NIRI will replace GNIRS on the telescope.
In January 2022, itermittent problems began to occur with GNIRS' filter wheel two (FW2). This was found to be due to a faulty ball bearing, which increased drag and friction on the wheel assembly. In order to prevent damage to FW2 or other components internal to GNIRS, a decision was made to avoid FW2 movements entirely. As a result, as of March 15th, 2022, observations were limited to cross dispersed mode only. The faulty ball bearing is to be substituted when GNIRS is warmed up to install the IFU at the end of April 2022.
The GHOST project commissioning has begun, with the Canadian and Australian teams able to travel to the summit following the easing of COVID-19 related restrictions. Optical bench assembly has begun, with alignment tests scheduled for late April. Twilight tests are to take place in mid-May. On-sky science commissioning is planned to take place in mid-late June, 2022.
A new webpage with information on the current status of the GMOS-N detector array is now available here. The webpage provides details on the recent hot column features (see March 10 announcement) and updated recommendations for dither strategies to minimize the impact of the hot columns on science data. Any future updates from the ongoing characterization of the hot columns will be posted on this webpage.
As of July 2022 the noise problem on CCD2 and CCD1 persists.
The GMOS-N detector issue reported on March 2 has largely been resolved by the full thermal cycle performed between March 2 and 3. The extended bright columns on amplifiers 7 and 12 are no longer present. The narrow bad column of hot pixels on amplifier 5 persists and saturates in longer science exposures. The following figure shows the hot column in an overscan-subtracted bias image (as marked by the blue arrow).
Multi object spectroscopy with Flamingos-2 is now offered via the latest Fast Turnaround Call for proposals and also for regular queue in 2022B. Details on this capability can be seen here.