Science Operations


Observing With Gemini

Call for Proposals
Most recent calls for proposals 2011A | 2010B
Observing Modes
Links to information regarding queue, target of opportunity, classical, director's discretionary, and poor weather observing time.
Phase I
Overview of the proposal process and links to the Gemini Phase I Tool (PIT)
Phase II
For principal investigators with accepted programs. Instructions and tutorials for defining observations with the Observing Tool (OT)
Target of Opportunity
North and South ToO configuration pages.

Visiting Gemini

Visitor's Guides
Instructions for visitors to Gemini North and Gemini South
Feedback Forms
For classical and queue observers

Instruments

Current Gemini Instruments
Gemini North: Altair | GMOS-North | GNIRS | Michelle | NIFS | NIRI
Gemini South: FLAMINGOS-2 | GMOS-South | NICI | Phoenix | T-ReCS
Integration Time Calculators
Calculate exposure times for Gemini instruments
Future Instrumentation at Gemini
Description of current instrument development and processes used to plan new instruments

Telescopes and Sites

Weather
Weather conditions at Gemini North and South
Observing Condition Constraints
Guidelines on Image Quality (IQ), Cloud Cover (CC), Water Vapor (WV), and Sky Background (SB)

Schedules

Semester Schedules
Current semester schedules for GN and GS
Queue Summary
Status of the queue for the current semester
Classical Schedules
Current semester schedules for classical observers and programs
NGO Schedules
Current semester scheduled for NGO visitors

Data and Results

Gemini Science Archive
Hosted by the Canadian Astronomy Data Centre
Gemini IRAF Packages
Updates on current IRAF packages, important announcements, and downloads
Gemini Publications
Science publications written by Gemini users and staff.
Science Operations Statistics
Completion rates for queue programs, open shutter efficiency, weather losses and other statistics related to operations at both telescopes

Helpdesk

Gemini Helpdesk

The Gemini Observatory is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the National Science Foundation on behalf of the Gemini partnership. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.