Change page style:
Figure 1. Image of HD 100546 obtained with the Gemini Planet Imager at near-infrared wavelengths (1.6 microns). The cross shows the position of the star, the green hatched lines show the region interior to which GPI's coronagraph blocks our view of the system. HD 100546 b appears as a bright point source sitting on a finger of disk emission.
Observations using the Gemini Planet Imager are featured prominently at the Extreme Solar Systems III meeting ongoing this week (Nov. 29 - December 4) in Waikoloa Hawai‘i. Below are two results from a press conference on December 1, 2015.
The GeMS / GSAOI laser run that was planned to take place this week had to be canceled. Unfortunately the laser and the Canopus Real Time Control system were not operational and in spite of intense efforts to resolve these problems in time for the laser window there was just not sufficient time to get the system in an operational state. We will continue to work towards ensuring that the upcoming January GeMS / GSAOI run will be a success.
Figure 1. Image of Cheshire Cat gravitationally lensed galaxies produced by combining Chandra X-ray data with Hubble Space Telescope optical data. Gemini spectroscopy provided critical spectroscopic data for characterizing the foreground lensing cluster and understanding its history and likely fate as a "fossil group." Image Credit: Hubble Space Telescope and Chandra X-ray Observatory
Gemini Observatory is pleased to announce the release of the public GIFS reports.
- General Inquiries
- Operations general (science and engineering)
- Science Operations South
- Science Operations North
- Science user support inquiries including HelpDesk and Archive
- Engineering & Mountain Operations South
- Engineering & Mountain Operations North
- Telescope Performance
- Adaptive Optics Performance
- Research Activity at Gemini
- Public Information and Outreach
Polycom Videoconference Directory
National Gemini Offices
Gemini is operated by a partnership including the United States, Canada, Chile, Brazil, Argentina and the University of Hawaii. Each partner maintains a “National Gemini Office”.
Contact information for each of the partners:
Dr. Lydia S. Cidale
Facultad de Ciencias Astronómicas y Geofisicas
Universidad Nacional de La Plata
Instituto de Astrofísica La Plata (CONICET-UNLP)
Paseo del Bosque - B1900FWA - La Plata - Buenos Aires Argentina
Tel: +54-221-4236593 (ext: 153)
The Brazilian Gemini Office
Dr. Eder Martioli
Laboratório Nacional de Astrofísica
Rua Estados Unidos, 154
37504-364 Itajubá - MG
Phone: (+55)-35-3629-8220 (direct)
Phone: (+55)-35-3629-8110 (LNA general)
The Chilean Gemini Office
Prof. Edgardo Costa
The Chilean National Gemini Office
Programa de Astronomía
Comisión Nacional de Investigación Científica y Tecnológica de Chile
Bernarda Morin 551, Providencia, Santiago
Additionally, Gemini may have “limited-term partners” - countries or institutions who have acquired temporary access to a subset of the telescope’s operating modes. These may or may not maintain an NGO.
Contact information for the current limited-term partners (if none, contact the observatory directly):
K-GMT Science Program Office
Dr. Narae Hwang
Center for Large Telescopes
Korea Astronomy and Space Science Institute
776 Daedeokdae-Ro Yuseong-Gu
Daejeon 34055 Rep. of KOREA
The OCTOCAM study was led by Antonio de Ugarte Postigo and managed by Pete Roming and Christina Thöne. The project was coordinated from the Instituto de Astrofisica de Andalucia (IAA-CSIC), with main collaborators at the Southwest Research Institute, Fractal SLNE, and George Washington University. The study began in April 2015 and concluded in October 2015.
This page describes the steps to properly configure the instrument using the OT. Generally the user should use the skeleton templates that are created in Phase II and apply them to obtain the proper sequences. Instructions on for the general use of the OT can be found on the OT page and related links, as this page describes particular details for using OT with GPI.
The GPI in the OT can be broken down into the following components: