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<title>fg21sim.git/fg21sim/utils, branch v0.6.5</title>
<subtitle>Simulate foreground for 21cm EoR signal detection
</subtitle>
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<entry>
<title>Deprecate np.int, np.float</title>
<updated>2017-11-03T05:38:08+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-11-03T05:38:08+00:00</published>
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See: https://github.com/numpy/numpy/pull/6103
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See: https://github.com/numpy/numpy/pull/6103
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</entry>
<entry>
<title>utils/grid.py: Disable Numba JIT for make_ellipse() &amp; make_grid_ellipse()</title>
<updated>2017-10-26T01:37:58+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-10-26T01:37:58+00:00</published>
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</entry>
<entry>
<title>utils/transform/circle2ellipse: skip rotation if it's None</title>
<updated>2017-10-23T14:00:24+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-10-23T13:59:06+00:00</published>
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</entry>
<entry>
<title>clusters/halo: Add function "speed_sound()"</title>
<updated>2017-10-21T07:17:01+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-10-21T07:17:01+00:00</published>
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<content type='text'>
Also add "gamma" the adiabatic index of ideal gas to utils/units.py
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Also add "gamma" the adiabatic index of ideal gas to utils/units.py
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</entry>
<entry>
<title>utils/units.py: add "rad2arcmin" and some cleanup/simplifications</title>
<updated>2017-10-18T07:52:34+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-10-18T07:52:34+00:00</published>
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<entry>
<title>utils/analyze.py: countdist_integrated(): Add xmin and xmax param.</title>
<updated>2017-10-18T05:42:32+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-10-18T05:42:32+00:00</published>
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<entry>
<title>clusters: Use "hmf" to calculate halo mass functions/distributions</title>
<updated>2017-10-04T12:57:56+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-10-04T12:57:56+00:00</published>
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<content type='text'>
* New dependency "hmf" (halo mass functions) module
* Calculate halo mass distributions/functions (dndlnm) with respect to masses
  and redshifts, instead of use the previous data file ("ps_data")
* New section "[extragalactic][psformalism]" in configurations
* New functions to write and read the dndlnm data

TODO:
* update the method to sample (mass, redshift) for clusters from the dndlnm
  data
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* New dependency "hmf" (halo mass functions) module
* Calculate halo mass distributions/functions (dndlnm) with respect to masses
  and redshifts, instead of use the previous data file ("ps_data")
* New section "[extragalactic][psformalism]" in configurations
* New functions to write and read the dndlnm data

TODO:
* update the method to sample (mass, redshift) for clusters from the dndlnm
  data
</pre>
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</content>
</entry>
<entry>
<title>utils/cosmology.py: Add parameter Tcmb0 [K]</title>
<updated>2017-10-04T07:54:00+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-10-04T07:54:00+00:00</published>
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<entry>
<title>utils/units.py: Add "K2eV" and "K2keV"</title>
<updated>2017-10-04T05:37:23+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-10-04T05:37:23+00:00</published>
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<entry>
<title>utils/cosmology: Add scalar spectral index "ns"</title>
<updated>2017-10-04T04:07:15+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-10-04T04:07:15+00:00</published>
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