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The GPI Pipeline
The Gemini Planet Imager Data Pipeline allows transformation of raw data from GPI into calibrated spectral and polarimetric data cubes. It also provides some basic capabilities for PSF suppression through differential imaging, and for astrometry and spectrophotometry of detected sources.
Priority Visitor observing will be available (and the default) for Large and Long Programs in 2014B; it may also be granted to experienced observers for 2014B Band 1 programs.The following notes apply to 2014B, and will be updated for 2015A when more extensive use of PV observing is anticipated.
GPI programs selected for Early Science Observations
The table below summarizes the programs that have been approved for GPI Early Science observations.
Gemini's near-infrared instruments are capable of imaging and spectroscopy from 1 to 5 microns (see the Instrument Overview for a brief description of each). This page provides information common to all NIR instruments, specifically targeting calibrations and data reduction resources. Detailed, instrument-specific information is available on each instrument's own web pages.
Observatorios Gemini y Keck Confirman Existencia de un Planeta Potencialmente Habitable del Tamaño de la Tierra
- Have you selected appropriate templates from the GMOS OT library? Have you gone through the checklist in the Top-level Program Overview note and included relevant standardized notes? Add notes with information about the program and acquisition that will make it easier for the observer. Try to use the standardized notes provided in the OT Library.