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The following table shows a summary of GCAL emission line plots for two lamps (Ar and Xe) at near IR wavelengths. The spectra all have the same integration time. Wavelengths are in vacuum. See also the general wavelength calibration page for more line lists etc.
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 is offered to investigators of regular semester Band 1 queue programs and is the default observing mode for Large and Long Programs (LLPs) . Investigators wishing to have their program considered for PV observing should indicate their desire to participate in the Technical Design portion of their queue proposal.
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.