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Semester 14B Call for Proposals

Gemini Observatory invites its community to propose scientific investigations for the 2014B semester, 1 August 2014 - 31 January 2015.

GMOS-N Array (EEV)

The original GMOS-N detector array consisted of three 2048x4608 EEV chips arranged in a row. This array was replaced by e2v deep depletion devices in October 2011.

The table below gives a summary of the original EEV detector/controller characteristics.

Detector Array

Detector characteristics are given in this section. Note that the GMOS-South detectors will be upgraded for 14B. Note also that the telescope optics are now silver-coated, reducing the system throughput in the blue.

Public Data Readme

GPI Public Data Early Release Readme

AstroDay Chile 2014