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- W2009694760 abstract "Observations using space telescopes should be optimized for conditions that prevail in space. Since the sky at 1 micron is very dark above the OH nightglow, and because distant galaxies are brightest at wavelength greater than 1 micron, the Hubble space telescope should be very good at detecting and measuring faint, distant galaxies in the R and I bands. For later-generation space telescopes the optimal wavelength for detecting high-redshift faint galaxies is the 3 micron window in the zodiacal light. Observations of faint galaxies in the 1-3 micron region will be less affected by evolution than optical observations, leading to a better determination of q0." @default.
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- W2009694760 date "1985-05-01" @default.
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- W2009694760 title "On using a space telescope to detect faint galaxies" @default.
- W2009694760 doi "https://doi.org/10.1086/131560" @default.
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