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Line 3: Unlike the [[stellar parallax]] method, photometric parallax can be used to estimate the distances of stars over 10 kpc away, at the expense of much more limited accuracy for individual measurements. Strictly speaking, it does not actually employ any measurements of parallax and can be considered a misnomer. == References ==▼ * {{cite journal \|author=Mario Juric ''et al.'' \|title=The Milky Way Tomography with SDSS \|year=2005 \|doi=10.1086/523619 \|journal=The Astrophysical Journal \|volume=673 \|issue=2 \|pages=864–914 \|arxiv=astro-ph/0510520}}▼ ==See also== [[Spectroscopic parallax]] [[Dynamical parallax]] ▲== References == ▲* {{cite journal \|author=Mario Juric ''\|author2=et al.'' \|title=The Milky Way Tomography with SDSS \|~~year~~date=2005 \|doi=10.1086/523619 \|journal=The Astrophysical Journal \|volume=673 \|issue=2 \|pages=864–914 \|arxiv=astro-ph/0510520}} [[Category:Astrometry]]

Photometric parallax: Difference between revisions