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INGRID basics:

Operation modes:
· With NAOMI
· At WHT Cassegrain
· Frame modes

Observing:

Documentation:

Future improvements:

Contact Person:
Johan Knapen
knapen [at] ing.iac.es

INGRID

NEWS (March 29, 2001, JK): Most filter curves are now on-line.

NEWS (March 27, 2001, JK): we have been able to commission the new aspheric foreoptics for INGRID, and from now on this will be used with INGRID. Subject to confirmation, throughput in all bands has been boosted by about 40%. SIGNAL still gives the old values for sensitivity, but is due to be updated soon. Also image quality is better than it was with the old foreoptics (doublet).

INGRID (Isaac Newton Group Red Imaging Device) is a near-IR camera for use at the 4.2m WHT, mostly built and developed at ING. At the heart of INGRID is a 1024x1024 Hawaii near-IR detector array for imaging from 0.8 to 2.5 microns. The pixel scale has been determined at 0.242 arcsec/pixel, see the Instrument overview.
This page is intended to give an overview of INGRID and contains information about the first results from INGRID, INGRID's capabilities and her characteristics. The information here is intended to serve as an overview of INGRID and will evolve - if you have any specific inquiries and for the most recent information please email the INGRID instrument specialist, Johan Knapen (email knapen [at] ing.iac.es).

For a basic introduction to INGRID, see the INGRID Press Release


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Last Updated: 26 February 2001
S. Prins stp@ing.iac.es