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| author | Aaron LI <aly@aaronly.me> | 2017-07-19 16:34:40 +0800 |
|---|---|---|
| committer | Aaron LI <aly@aaronly.me> | 2017-07-19 16:34:40 +0800 |
| commit | 9b7f99bbd0eca0e611601dd936c1f7948f8cd58a (patch) | |
| tree | cde8dd145d1a560213fa1f4eacefe9ad80b7e40b /fg21sim/extragalactic/clusters/emission.py | |
| parent | bfc2b52d6c12553290742fcf793e48b1133e7dad (diff) | |
| download | fg21sim-9b7f99bbd0eca0e611601dd936c1f7948f8cd58a.tar.bz2 | |
Use [arcsec] as the unit for pixel size and resolution
Signed-off-by: Aaron LI <aly@aaronly.me>
Diffstat (limited to 'fg21sim/extragalactic/clusters/emission.py')
| -rw-r--r-- | fg21sim/extragalactic/clusters/emission.py | 4 |
1 files changed, 2 insertions, 2 deletions
diff --git a/fg21sim/extragalactic/clusters/emission.py b/fg21sim/extragalactic/clusters/emission.py index 345e3db..93e04ff 100644 --- a/fg21sim/extragalactic/clusters/emission.py +++ b/fg21sim/extragalactic/clusters/emission.py @@ -184,7 +184,7 @@ class SynchrotronEmission: ---------- pixelsize : float The pixel size of the output simulated sky image - Unit: [arcmin] + Unit: [arcsec] Returns ------- @@ -195,7 +195,7 @@ class SynchrotronEmission: DA = self.cosmo.DL(self.z) * AUC.Mpc2cm # [cm] radius = self.radius * AUC.kpc2cm # [cm] omega = (np.pi * radius**2 / DA**2) * AUC.rad2deg**2 # [deg^2] - pixelarea = (pixelsize/60.0) ** 2 # [deg^2] + pixelarea = (pixelsize * AUC.arcsec2deg) ** 2 # [deg^2] if omega < pixelarea: omega = pixelarea F_nu = self.flux(nu) |