コード例 #1
0
ファイル: plot.py プロジェクト: lkreidberg/SPIDERMAN
def plot_system(spider_params,t,ax=False,min_temp=False,max_temp=False,temp_map=False,min_bright=0.2,use_phase=False,show_cax=True,mycmap=plt.cm.inferno,theme='white',show_axes=True):

	if theme == 'black':
		bg = 'black'
		tc = ("#04d9ff")
	else:
		bg = 'white'
		tc = 'black'

	if use_phase == True:
		t = spider_params.t0 + spider_params.per*t

	if ax == False:
		f, ax = plt.subplots(facecolor=bg)
	image = sp.get_star_png()
	star_r_pix = 180
	star_offset_pix = 200

	p_imrat = star_r_pix*spider_params.rp

	coords = sp.separation_of_centers(t,spider_params)

	planet_pix = [star_offset_pix - coords[0]*p_imrat,star_offset_pix - coords[1]*p_imrat]

	ax = sp.plot_planet(spider_params,t,ax=ax,min_temp=min_temp,max_temp=max_temp,temp_map=temp_map,min_bright=min_bright,scale_planet=p_imrat,planet_cen=planet_pix,mycmap=mycmap,show_cax=show_cax,theme=theme,show_axes=show_axes)

	if(abs(abs(spider_params.phase)-0.5) > 0.25):
		#in front 
		s_zorder = 1
	else:
		s_zorder = 3

	im = ax.imshow(image,zorder=s_zorder)
	patch = patches.Circle((200, 200), radius=200, transform=ax.transData)
	im.set_clip_path(patch)

	ax.set_xlim(star_offset_pix+40*p_imrat,star_offset_pix+-40*p_imrat)
	ax.set_ylim(star_offset_pix+-10*p_imrat,star_offset_pix+10*p_imrat)

	ax.set(aspect=1)

	arrr = np.array([-1000,-500,0,500,1000])
	arrr2 = np.array([-200,0,200])

	ax.set_xticks(arrr+star_offset_pix)
	ax.set_xticklabels([round(x,3) for x in -1*arrr/(star_r_pix*spider_params.a/spider_params.a_abs)])

	ax.set_yticks(arrr2+star_offset_pix)
	ax.set_yticklabels([round(x,3) for x in 1*arrr2/(star_r_pix*spider_params.a/spider_params.a_abs)])

	ax.set_xlabel('Projected separation (AU)')

	return ax
コード例 #2
0
ファイル: plot.py プロジェクト: tomlouden/SPIDERMAN
def plot_system(spider_params,t,ax=False,min_temp=False,max_temp=False,temp_map=False,min_bright=0.2,use_phase=False,show_cax=True,mycmap=plt.cm.inferno,theme='white',show_axes=True):

	if theme == 'black':
		bg = 'black'
		tc = ("#04d9ff")
	else:
		bg = 'white'
		tc = 'black'

	if use_phase == True:
		t = spider_params.t0 + spider_params.per*t

	if ax == False:
		f, ax = plt.subplots(facecolor=bg)
	image = sp.get_star_png()
	star_r_pix = 180
	star_offset_pix = 200

	p_imrat = star_r_pix*spider_params.rp

	coords = sp.separation_of_centers(t,spider_params)

	planet_pix = [star_offset_pix - coords[0]*p_imrat,star_offset_pix - coords[1]*p_imrat]

	ax = sp.plot_planet(spider_params,t,ax=ax,min_temp=min_temp,max_temp=max_temp,temp_map=temp_map,min_bright=min_bright,scale_planet=p_imrat,planet_cen=planet_pix,mycmap=mycmap,show_cax=show_cax,theme=theme,show_axes=show_axes)

	if(abs(abs(spider_params.phase)-0.5) > 0.25):
		#in front 
		s_zorder = 1
	else:
		s_zorder = 3

	im = ax.imshow(image,zorder=s_zorder)
	patch = patches.Circle((200, 200), radius=200, transform=ax.transData)
	im.set_clip_path(patch)

	ax.set_xlim(star_offset_pix+40*p_imrat,star_offset_pix+-40*p_imrat)
	ax.set_ylim(star_offset_pix+-10*p_imrat,star_offset_pix+10*p_imrat)

	ax.set(aspect=1)

	arrr = np.array([-1000,-500,0,500,1000])
	arrr2 = np.array([-200,0,200])

	ax.set_xticks(arrr+star_offset_pix)
	ax.set_xticklabels([round(x,3) for x in -1*arrr/(star_r_pix*spider_params.a/spider_params.a_abs)])

	ax.set_yticks(arrr2+star_offset_pix)
	ax.set_yticklabels([round(x,3) for x in 1*arrr2/(star_r_pix*spider_params.a/spider_params.a_abs)])

	ax.set_xlabel('Projected separation (AU)')

	return ax
コード例 #3
0
 def calc_substellar(self, t):
     self.calc_phase(t)
     coords = sp.separation_of_centers(t, self)
     substellar = _web.calc_substellar(self.phase, np.array(coords))
     self.lambda0 = substellar[0]
     self.phi0 = substellar[1]
コード例 #4
0
ファイル: params.py プロジェクト: lkreidberg/SPIDERMAN
 def calc_substellar(self,t):
     self.calc_phase(t)
     coords = sp.separation_of_centers(t,self)
     substellar = _web.calc_substellar(self.phase,np.array(coords))
     self.lambda0 = substellar[0]
     self.phi0 = substellar[1]