galaxies_disperse_test_f335m.list

#
# 
#
#Columns 1 and 2 can be either x,y positions on the detector aperture (e.g.
#0,0 is lower left corner of the full frame of the subarray used for the 
#output) or RA,Dec location of the center of the source. If they are x,y
#positions, make the top line of the file '# position_pixels'
#
#radius is the half-light radius in pixels or arcseconds. If in pixels
#make the second line of the file '# radius_pixels
#
#pos_angle is the position angle of the semimajor axis, in degrees.
#0 causes the semi-major axis to be horizontal.
x_or_RA    y_or_Dec  radius  ellipticity  pos_angle  sersic_index  magnitude
23:59:59.9986 +00:00:00.0047  1.0      0.25        20           2.0  19.300
00:00:00.0003 +00:00:00.0216  1.5      0.5         79           1.2  19.200
23:59:58.6185 +00:00:32.1260  1.5      0.25        0            2.0  20.500
00:00:02.1327 +00:00:20.7322  1.5      0.25        70           2.0  20.000
00:00:01.3983 -00:00:32.3796  1.0      0.3         0            2.0  19.100
23:59:57.8535 -00:00:20.5960  1.0      0.3         0            2.0  19.200
00:00:00.3940 +00:00:03.6792  3.0      0.3         45           2.0  18.300
00:00:00.6557 +00:00:06.2135  1.0      0.3         0            2.0  17.600