Change page style:
The Gemini eNewscast is a monthly electronic distribution of information for users of Gemini Observatory.
|2015-06-26||Gemini e-Newscast #72|
|2015-05-22||Gemini e-Newscast #71|
|2015-04-15||Gemini e-Newscast #70|
|2015-03-19||Gemini e-Newscast #69|
|2015-02-24||Gemini e-Newscast #68|
|2015-01-21||Gemini e-Newscast #67|
|2014-12-30||Gemini e-Newscast #66|
|2014-11-18||Gemini e-Newscast #65|
|2014-10-23||Gemini e-Newscast #64|
|2014-09-26||Gemini e-Newscast #63|
|2014-08-22||Gemini e-Newscast #62|
|2014-07-21||Gemini e-Newscast #61|
|2014-06-19||Gemini e-Newscast #60|
|2014-05-21||Gemini e-Newscast #59|
|2014-04-24||Gemini e-Newscast #58|
|2014-03-21||Gemini e-Newscast #57|
|2014-02-14||Gemini e-Newscast #56|
|2014-01-17||Gemini e-Newscast #55|
Subscribe To The eNewscast
The 2014B Gemini Observing Tool is now available for download. This update is required to access the database. Installation instructions are linked off of the Observing Tool web page, and we recommend that everyone download their programs from scratch from the ODBs rather than import from saved XMLs.
Figure 1. Artist’s impression of a galaxy with a large-scale outflow. Credit: ESA/ATG medialab.
Figure 1. Artist's rendition of UY Aur's probable outflow system. Credit: National Astronomical Observatory of Japan, All Rights Reserved.
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.