... Magnitudes, the prerequisite for later applications, are obtained in a lengthy process: each measured isophotal magnitude or aperture magnitude is subjected to transformations, corrections and calibrations, amounting to 8 steps for galaxies and 6 steps ...
... The accuracy strongly depends on the number of bright 2MASS stars within the filed of view, but ranges from a few 1/100th of a magnitude to 0.1 magnitudes if only faint stars are contained in the field. ...
... Note that for the M11 (absolute magnitude) plot as a function of perihelion distance q, the red lines indicate opposition magnitudes of R=20, 22, 24. ...
... Minor Bodies in the Outer Solar System: . Magnitudes and Colours . ... Absolute magnitude and Colour Histograms and Cummulative Distributions. ... The absolute R magnitude M11 and colour distributions are represented as histograms ...
... Target Name . Target Magnitude . Magnitude in band of observation . ... Target Magnitude . Magnitude in band of observation . Magnitude in H band . ... Magnitude in band of observation . Magnitude in H band . Magnitude in V band . ...
... Minor Bodies in the Outer Solar System: . Magnitudes and Colours . Database Tables. ... colour database : colour, absolute magnitude, spectral gradient, dynamical class for ...