def plotPerfVSpectralType():
teff = np.linspace(3000, 7000, 9)
prad_earth = 4
prad = prad_earth * const.earthRadius/const.solarRadius
srad = sp.getParam(teff)
mp.clf()
apj.pre()
for m in [9,12,15]:
signal_ppm = 1e6*(prad/srad)**2
noise_ppm = noiseModel_ppm(m, expTime_sec=1800, teff_K=teff)
snr = signal_ppm/noise_ppm
mp.plot(teff, snr, '-', lw=4, label="V=%i" %(m))
apj.post()
mp.xlim([7000, 3000])
# mp.ylim(0, 50)
mp.legend(loc=2)
mp.xlabel("Stellar Temperature (K)")
mp.ylabel("Expected Signal-to-Noise")
mp.gca().set_yscale('log')
mp.grid(True, which='both')
mp.title("Estimated SNR For %.1f Re radius planet" %(prad_earth))
apj.pgid()
def main():
sk = schmidtKaler()
hh = habetsHeinze()
hb = huber()
mp.clf()
apj.pre()
col = 'radius'
mp.plot(sk[:,'teff'], sk[:, col], 'o-', label="SK")
mp.plot(hh[:,'teff'], hh[:, col], 'o-', label="HH")
mp.plot(hb[:,'teff'], hb[:, col], 'o', label="Huber")
mp.legend(loc=2)
mp.xlabel("Teff")
mp.ylabel(col)
mp.axvline(5770, color='grey', lw=.5)
mp.axhline(1, color='grey', lw=.5)
def main():
hdCatFile = "/home/fergal/all/kepler/twowheel/hdcat.txt"
nCompanions = 10
print "Loading ..."
hdCat = scenery.loadHdCatalogue(hdCatFile, maxMag=12)
fn = "distMat.npz"
if os.path.exists(fn):
print "Using cached values..."
npzFile = np.load(fn)
distMat = npzFile['distMat']
mags = npzFile['mags']
npzFile.close()
pass
else:
print "Computing ..."
distMat, mags = computeDistMatrix(hdCat, magCol=3, maxMag=8)
np.savez(fn, distMat=distMat, mags=mags)
mp.clf()
apj.pre()
# mp.imshow(distMat, interpolation="nearest")
print "Computing focal plane radius..."
for nCompanions in [30, 10,3]:
radius = computeDistToNNearestStars(distMat, nCompanions)
mp.plot(mags, radius, '-', label="%i stars" %(nCompanions))
mp.xlabel("Magnitude")
mp.ylabel("Distance (degrees)")
mp.legend(loc=1)
mp.title("Distance to nearest bright stars")
mp.ylim(0,40)
apj.post()
return distMat, mags