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The region of Re50 and Re50N observed in 2006 with SuprimeCam at the Subaru telescope, and in 2014 with the Gemini Multi-Object Spectrograph (GMOS) at the Gemini South telescope. A [SII] filter was used for both images. The seeing was in both cases 0.5 arcsec. Each image is about 3 arcmin wide. North is up and east is left.
Changes in the universe don’t often happen on human timescales.
The Users Committee for Gemini has reserved a 2-hour block for a hands-on, bring-your-own data workshop with Gemini staff and expert users. What topics would you like to see addressed in such a workshop? Examples might be mask-making with GMMPS or reducing GPI data; please tell us what YOU would like help with by submitting topics for discussion.
GN Summit Facility (summit)
As part of Gemini’s comprehensive energy savings initiative, Gemini North Telescope Facility (GN) seeks to provide a full range of improvements and services to reduce costs of energy and water use (referred to as Energy Savings Projects - ESP). Services may include a technical audit to assess energy, water, and operations and maintenance savings opportunities, design, acquisition, installation or modification of energy-using equipment, and maintenance and training in the operation of such equipment.
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