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Once the metallicity, age, extinction and distance modulus for a given cluster have been found, plot the ZAMS corresponding to that metallicity value shifted by that extinction and distance modulus, a…
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Are all QHE-binary BPASS evolution models in the subdirectories of NEWSINMODS that are named in the format of hmg?
Also, to be extra sure, should I look at the Age=0.0 years value of the M2 value of …
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As brought to my attention by @Reagen, `ratios.flux_ratios` adopts the same naming convention for flux ratios, `logR23`, `logO32`, `two_beta`, and `three_beta`. When implementing this between individ…
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DOD 1 - We need at least 1 more feature to separate the classes. Find it, through whatever means necessary.
Explanation: Many of the overlapping 4 galaxies are actually 3.
Solution: Search KDEPLOT…
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Hello,
I need to work with output data from isochrones function in FSPS library. I tried to find any kind of documentation about units and names of output data which are presented as a huge Numpy arr…
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Download, install, and run ESPRESSO pipeline (https://www.eso.org/sci/software/pipelines/espresso/espresso-pipe-recipes.html). We will want to refer and compare our performance to the ESPRESSO pipelin…
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Hi all,
I am working on a project in which I want to solve the following equation: R*X=Y where R is the response matrix, X is the intrinsic spectrum (i.e. model spectrum), and Y is the observed spec…
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**Describe the bug**
On some specific initial conditions, COMPAS will completely hang. Cause is unknown, but it seems to occur for massive binaries with short separations, so I would guess that these…
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Currently, during BH formation we lose 10% of mass in neutrinos (following Fryer+2012). This is an excesive amount that should be reduced for high mass stars.
We should add an user specified maximu…
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**Description**
Allow a portion or all of the dust in each location (i.e. in each spatial cell) to be destroyed based on the local radiation field (or its effect on the dust, e.g. the dust temperatur…