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Pixel Scale and Orientation

MIRAC has a continuous zoom mechanism that can create a range of image scales ranging from 0.054”/pixel (13.8” FOV) at the highest magnification ...

Refilling Cryogens

MIRAC is cooled via a closed cycle refrigerator and needs no daily maintenance. BLINC uses liquid nitrogen to keep its optics from contributing addit...

Observing Guidelines

Camera Operation The camera is operated via a Java-based GUI. Since the sky flux dominates the total photons r...

Beginning of Night Setup

MIRAC can be run remotely using any linux machine. To run MIRAC log into the mirac machine in the observing chmaber using ssh mirac@m...

Cornell Electronics Documentation

Preamp Characterization by Bill Hoffmann, Dec. 2008 [Download file "preamp performance_11.pdf"] Preamp offset measure emtns from Bil...

FORCAST Software Documentation

Documentation on FORCAST software that runs the Cornell electronics. FORCAST Technical Reference from Justin Schoenwald, September 2006. ...

MIRAC-BLINC User Manual

Introduction The Mid-Infrared Array Camera and Bracewell Infrared Nulling Cryostat (MIRAC-BLINC) is an instrument developed for use w...

Spring 2010 MIRAC detector characterization

Detector testing was carried out by Bill Hoffmann and Nathan Stock Nathan's spreadsheet of results: [Download file "Characterizations (1).xl...

LBTI engineering notes

Saturday, Oct. 9 The dark current appears to be: 440 dn/s in high well depth 7570 dn/s in low well depth

Filter Information

The filters in MIRAC4 are as follows. Some filters require additional blocking which may slightly affect their transmission profil...

BLINC

BLINC is a liquid nitrogen-cooled set of fore-optics for the MIRAC system. The entrance window provides the reflection surface for the v...

Spectrum Mode Information

A grism in the first filter wheel can be inserted to generate an R=50-100 spectrum. The grism is typically used with the lowest ma...

Detector Information

The Detector is a DRS MF/HF 256 pixel array. It has a measured well depth of 17 Me- and an RMS readout noise of 2024 e-. The detector can also be ...

Feature Request

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Known Bugs

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Removal From the Telescope

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Cool Down Instructions

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Installation and Setup

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Camera Optics

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