One of the questions children often ask is "How many stars are there in the sky?" Under ideal conditions, even with the naked eye, nearly eight thousands are observable in the northern hemisphere. With a decent telescope, you may find many more, but, as the sight field will be limited, you may find much less at a time.

Children may ask the same questions to their parents on a planet of some solar system billions of light-years away from the Earth. Their telescopes are similar to ours with circular sight fields, but alien kids have many eyes and can look into different directions at a time through many telescopes.

Given a set of positions of stars, a set of telescopes and the directions they are looking to, your task is to count up how many stars can be seen through these telescopes.

The input consists of one or more datasets. The number of datasets is less than 50. Each dataset describes stars and the parameters of the telescopes used.

The first line of a dataset contains a positive integer *n* not exceeding 500, meaning the number
of stars. Each of the *n* lines following it contains three decimal fractions, *s _{x}*,

Then comes a line containing a positive integer *m* not exceeding 50, meaning the number of
telescopes. Each of the following *m* lines contains four decimal fractions, *t _{x}*,

The first three numbers represent the direction of the telescope. All the telescopes are at the
origin of the coordinate system (0, 0, 0) (we ignore the size of the planet). The three numbers give
the point (*t _{x}*,

The fourth number *φ* (0 ≤ *φ* ≤ *π*/2) gives the angular radius, in radians, of the sight eld of
the telescope.

Let us defie that *θ _{i,j}* is the angle between the direction of the

Figure 1: Direction and angular radius of a telescope

The end of the input is indicated with a line containing a single zero.

For each dataset, one line containing an integer meaning the number of stars observable through the telescopes should be output. No other characters should be contained in the output. Note that stars that can be seen through more than one telescope should not be counted twice or more.

3 100 0 500 -500.243 -200.1 -300.5 0 300 200 2 1 1 1 0.65 -1 0 0 1.57 3 1 0 0 0 1 0 0 0 1 4 1 -1 -1 0.9553 -1 1 -1 0.9554 -1 -1 1 0.9553 -1 1 -1 0.9554 3 1 0 0 0 1 0 0 0 1 4 1 -1 -1 0.9553 -1 1 -1 0.9553 -1 -1 1 0.9553 -1 1 -1 0.9553 0

2 1 0

Source: ACM International Collegiate Programming Contest
, Asia Regional Yokohama, Yokohama, Japan, 2006-11-05

http://www.acm-japan.org/icpc2006/

http://www.acm-japan.org/icpc2006/