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Draft version September 4, 2015, Preprint typeset using LATEX style emulate v. 5/2/11ASSESSING GALAXY LIMITING MAGNITUDES IN LARGE OPTICAL SURVEYS E. S. Rykoff1,2, E. Rozo3, R. Keisler1arXiv:1509.00870v1
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What is assessing galaxy limiting magnitudes?
Assessing galaxy limiting magnitudes is the process of determining the faintest visible magnitude of galaxies that can be observed with a telescope or other optical instrument.
Who is required to file assessing galaxy limiting magnitudes?
Researchers, astronomers, and observatories are usually required to file assessing galaxy limiting magnitudes.
How to fill out assessing galaxy limiting magnitudes?
Assessing galaxy limiting magnitudes can be filled out by recording observations of galaxies and noting the faintest magnitude visible.
What is the purpose of assessing galaxy limiting magnitudes?
The purpose of assessing galaxy limiting magnitudes is to understand the sensitivity and capabilities of optical instruments for observing galaxies.
What information must be reported on assessing galaxy limiting magnitudes?
Information such as the type of telescope used, observation location, date and time of observation, and the limiting magnitude of observed galaxies must be reported on assessing galaxy limiting magnitudes.
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