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Note in equations (7) that since theta is approximately 90o the terms involving p1 and p2 are small; neglecting them, as is usually done, gives us the equations for the ``SIN'' projection:
From equations (7), for an array which lies in the J2000.0 equatorial plane, we have
nu | = | 0 | (11) |
nv | = | cos![]() |
|
nw | = | sin![]() |
where
is the declination of the field centre, whence
p1 | = | 0 | (12) |
p2 | = | cot![]() |
and
These are the equations for the ``NCP'' projection. To first order the difference between equations (10b) and (13b) is
![]() ![]() |
(14) |
where r is the distance from the field centre in radians. This amounts to
nearly 1' for a position 1o from the field centre at
= 30o.