Calnic C

From Wikipedia, the free encyclopedia

This article does not cite any references or sources. (May 2007) Please help improve this article by adding citations to reliable sources. Unverifiable material may be challenged and removed.

Calnic C is a programme to analyze spectral data obtained with the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) on board the Hubble Space Telescope (HST). The program was designed at the Space Telescope European Coordinating Facility (ST-ECF) and is programmed in IDL. Maintenance of Calnic C has stopped in 2000 and the program is now considered to be obsolete. An interactive version of the programme called NICMOSlook is available and is still actively maintained.

v • d • e Hubble Space Telescope Associated Shuttle missions Launch STS-31 Servicing STS-61 · STS-82 · STS-103 · STS-109 Planned STS-125 Onboard instruments Current Advanced Camera for Surveys (ACS) · Corrective Optics Space Telescope Axial Replacement (COSTAR) · Fine Guidance Sensor (FGS) · Near Infrared Camera and Multi-Object Spectrometer (NICMOS) · Space Telescope Imaging Spectrograph (STIS) · Wide Field and Planetary Camera 2 (WFPC2) Planned Cosmic Origins Spectrograph (COS) · Wide Field Camera 3 (WFC3) Previous Faint Object Camera (FOC) · Faint Object Spectrograph (FOS) · Goddard High Resolution Spectrograph (GHRS/HRS) · High Speed Photometer (HSP) · Wide Field and Planetary Camera (WFPC) Italics indicate instruments that are currently failed and/or shut-down