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| [[ http://www.stsci.edu/jwst/software/point-spread-function-modeling.pdf | Point spread function modeling software paper ]] | |
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| [[ http://www.stsci.edu/jwst/software/webbpsf | Point spread modeling software ]] | [[ http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-001157.pdf | Point spread function paper ]] |
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| [[ http://www.stsci.edu/jwst/software/point-spread-function-modeling.pdf ]] [[ [[ http://www.stsci.edu/jwst/doc-archive/technical.../JWST-STScI-001157.pdf | Point Spread paper ]] |
[[ http://www.stsci.edu/hst/wfc3/tools/etcs/ | Hubble Exposure Time Calculators ]] |
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| ==== What can JWST resolve? ==== A [[ https://en.wikipedia.org/wiki/Jansky | Jansky ]] is 1e-26 W / m^2^-Hz. The Hz bandwidth can be estimated from the wavelength and wavelength window: Hz = c Δλ / λ^2^ . Two pixels needed for Nyquist deconvolution of point spread function. 0.11 arcsecond (as) pixels means 0.22 as minimum for estimating size (more is better) A 100 AU round shell is 0.22 as across at 450 pc. The galactic disk is 300 pc thick, G stars ------ == SOFIA airborne observatory, DLR/NASA == https://www.sofia.usra.edu/Science/ObserversHandbook/FORCAST.html [[ attachment:FORCAST_Sensitivity_v3.jpg | {{ attachment:FORCAST_Sensitivity_v3.jpg | width=300 }} ]] ==== What SOFIA can resolve? ==== ------ == Spitzer Infrared Satellite, NASA == ==== What can Spitzer resolve? ==== ------ == Herschel Infrared Satellite, ESA == ==== What can Herschel resolve? ==== ------ |
James Webb Space Telescope
http://ircamera.as.arizona.edu/MIRI/performance.htm
Frontier Science with the James Webb Space Telescope - great slides!
search http://www.stsci.edu for point spread function:
Point spread function modeling software paper
Hubble Exposure Time Calculators
GSMT AND JWST: Looking Back to the Future of the Universe
A GIANT SEGMENTED MIRROR TELESCOPE: SYNERGY WITH JWST
What can JWST resolve?
A Jansky is 1e-26 W / m2-Hz. The Hz bandwidth can be estimated from the wavelength and wavelength window: Hz = c Δλ / λ2 .
Two pixels needed for Nyquist deconvolution of point spread function. 0.11 arcsecond (as) pixels means 0.22 as minimum for estimating size (more is better) A 100 AU round shell is 0.22 as across at 450 pc. The galactic disk is 300 pc thick, G stars
SOFIA airborne observatory, DLR/NASA
https://www.sofia.usra.edu/Science/ObserversHandbook/FORCAST.html
What SOFIA can resolve?
Spitzer Infrared Satellite, NASA
What can Spitzer resolve?
Herschel Infrared Satellite, ESA
What can Herschel resolve?
balloon
PIROG 4 (Pointing InfraRed Observing Gondola)
THE BALLOON-BORNE LARGE APERTURE SUBMILLIMETER TELESCOPE: BLAST