... Among these are images of GRB 990123, a burst which reached an apparent visual magnitude of V=9 (bright enough to be observed with a pair of binoculars), yet was at a distance of some 10 billion light years. ...
... The catalogue lists F, B J and V magnitudes, and includes some sources as faint as 19th magnitude in R, although it is not complete at those magnitudes. ...
... Fig. 1a shows the amount of correction in magnitudes owing to the PMT deadtime which needs to be applied to the instrumental magnitudes as derived from the measured counts as a function of visual Johnson magnitude. ...
... 7.8 . IR Sensitivity . 7.8.1 Limiting Magnitudes . 7.8.1 Limiting Magnitudes . ... Table 7.10 presents the predicted limiting-magnitude performance of the WFC3 IR channel and compares it with that of the NIC3 ...
... The positions, magnitudes, and colors of all stars to approximately visual magnitude 15 will be measured. ... proper motions and parallaxes of all stars to 15 magnitude, with magnitude dependent accuracy of positions, proper motions and ...
... 6.8 . UVIS Sensitivity . 6.8.1 Limiting Magnitudes . 6.8.1 Limiting Magnitudes . ... Table 6.10 presents the predicted limiting-magnitude performance of WFC3 and compares it with that of the ACS camera. ...
... The integrated magnitude limit gives the total magnitude from all stars (or galaxies, or diffuse objects) of spectral type O which can appear in the MAMA field of view. ...
... magnitude of that component indicates that a numeric overflow would occur when it is squared, or if it indicates that an underflow would occur when squared (falsely giving a magnitude of zero) then the following expression is used: vnormg_c = v1max ...
... The quantity AB is a color-dependent correction from V magnitude to AB magnitude at frequency . ... AB is defined as a color-dependent correction from V magnitude to AB magnitude at frequency . ...