LWIR Stellar Calibration: Infrared Spectral Curves for 30 Standard Stars
Abstract
Best estimate spectral energy distributions are created for approximately 30 stars by fitting theoretically expected spectral curves to the available empirical flux data on the stars at a variety of wavelengths. The curves can be integrated over the band response functions for a given sensor in order to produce broadband power predictions against which to calibrate.
Document Details
- Document Type
- Technical Report
- Publication Date
- Apr 10, 1991
- Accession Number
- ADA236766
Entities
People
- Charles W. Engelke
Organizations
- Massachusetts Institute of Technology