diff options
Diffstat (limited to 'fg21sim/extragalactic')
| -rw-r--r-- | fg21sim/extragalactic/clusters/clusters.py | 35 |
1 files changed, 20 insertions, 15 deletions
diff --git a/fg21sim/extragalactic/clusters/clusters.py b/fg21sim/extragalactic/clusters/clusters.py index 68e1eb5..304603b 100644 --- a/fg21sim/extragalactic/clusters/clusters.py +++ b/fg21sim/extragalactic/clusters/clusters.py @@ -296,19 +296,22 @@ class GalaxyClusters: catalog["r_vir"] : 1D `~numpy.ndarray` The virial radii (unit: Mpc) calculated from the cluster masses catalog["size_major"], catalog["size_minor] : 1D `~numpy.ndarray` - The major and minor axes (unit: degree) of the clusters calculated + The major and minor axes (unit: arcmin) of the clusters calculated from the above virial radii and the random eccentricities. + NOTE: These major and minor axes are corresponding to the + diameter values; NOT semi-major/semi-minor axes! + Unit: arcmin NOTE ---- The elliptical major and minor axes are calculated by assuming the equal area between the ellipse and corresponding circle. - theta2 = r_vir / distance + theta2 = r_vir / distance # half angular size pi * a * b = pi * (theta2)^2 - e = sqrt((a^2 - b^2) / a^2) + e = sqrt((a^2 - b^2) / a^2) # eccentricity thus, - a = theta2 / (1-e^2)^(1/4) - b = theta2 * (1-e^2)^(1/4) + a = theta2 / (1-e^2)^(1/4) # semi-major axis + b = theta2 * (1-e^2)^(1/4) # semi-minor axis """ logger.info("Calculating the virial radii ...") overdensity = self.catalog_prop["overdensity"] @@ -321,12 +324,15 @@ class GalaxyClusters: # Calculate (elliptical) angular sizes, i.e., major and minor axes logger.info("Calculating the elliptical angular sizes ...") distance = self.catalog["distance"].data * self.units["distance"] - theta2 = (r_vir / distance).decompose().value # [ rad ] - size_major = theta2 / (1 - self.catalog["eccentricity"]**2) ** 0.25 - size_minor = theta2 * (1 - self.catalog["eccentricity"]**2) ** 0.25 - self.catalog["size_major"] = size_major * au.rad.to(au.deg) - self.catalog["size_minor"] = size_minor * au.rad.to(au.deg) - self.units["size"] = au.deg + # Half angular size + theta2 = (r_vir / distance).decompose().value # [rad] + theta = theta2 * 2 # angular size + # Major and minor axes (corresponding to diameter values) + size_major = theta / (1 - self.catalog["eccentricity"]**2) ** 0.25 + size_minor = theta * (1 - self.catalog["eccentricity"]**2) ** 0.25 + self.catalog["size_major"] = size_major * au.rad.to(au.arcmin) + self.catalog["size_minor"] = size_minor * au.rad.to(au.arcmin) + self.units["size"] = au.arcmin logger.info("Done calculate the elliptical angular sizes") def _calc_luminosity(self): @@ -506,7 +512,6 @@ class GalaxyClusters: """ logger.info("Simulating sky templates for each cluster/halo ...") templates = [] - pixelsize_deg = self.resolution.to(au.deg).value # Make sure the index is reset, therefore, the *row indexes* can be # simply used to identify the corresponding template image. self.catalog.reset_index(inplace=True) @@ -514,8 +519,8 @@ class GalaxyClusters: for row in self.catalog.itertuples(): # TODO: progress bar gcenter = (row.glon, row.glat) # [ deg ] - radii = (int(np.ceil(row.size_major * 0.5 / pixelsize_deg)), - int(np.ceil(row.size_minor * 0.5 / pixelsize_deg))) + radii = (int(np.ceil(row.size_major * 0.5 / self.resolution)), + int(np.ceil(row.size_minor * 0.5 / self.resolution))) rmax = max(radii) pcenter = (rmax, rmax) image = make_ellipse(pcenter, radii, row.rotation) @@ -559,7 +564,7 @@ class GalaxyClusters: luminosity = data.luminosity distance = data.distance specindex = data.specindex - size = (data.size_major, data.size_minor) # [ deg ] + size = (data.size_major/60.0, data.size_minor/60.0) # [deg] Tb = self._calc_Tb(luminosity, distance, specindex, frequency, size) val = val * Tb return (idx, val) |