taldcroft

#   ~/.ipython/profile_default/startup/10-mystartup.py

import numpy as np

ip = get_ipython()

def import_astropy(self, arg):
    ip.ex('import astropy')
    ip.ex('print(astropy.__version__)')
    ip.ex('from astropy.io import ascii')

ycopin

#!/usr/bin/env python
# Copyright: This document has been placed in the public domain.

"""
Taylor diagram (Taylor, 2001) implementation.

Note: If you have found these software useful for your research, I would
appreciate an acknowledgment.
"""

piscisaureus

Locate the section for your github remote in the .git/config file. It looks like this:

[remote "origin"]
	fetch = +refs/heads/*:refs/remotes/origin/*
	url = git@github.com:joyent/node.git

Now add the line fetch = +refs/pull/*/head:refs/remotes/origin/pr/* to this section. Obviously, change the github url to match your project's URL. It ends up looking like this:

phn

PyFITS: FITS files in Python

In this article, we provide examples of using the python module PyFITS for working with FITS data. We first go through a brief

astrofrog

import numpy as np

def distance(ra1, dec1, ra2, dec2):
    return np.degrees(np.arccos(np.sin(np.radians(dec1))
                              * np.sin(np.radians(dec2))
                              + np.cos(np.radians(dec1))
                              * np.cos(np.radians(dec2))
                              * np.cos(np.radians(ra1) - np.radians(ra2))))
          
def distance_approx(ra1, dec1, ra2, dec2):

astrofrog

from sampy import *
import time

import urllib

myhub = SAMPHubProxy()
myhub.connect()

client = SAMPClient(myhub)