diff options
author | Aaron LI <aaronly.me@gmail.com> | 2016-06-07 16:06:46 +0800 |
---|---|---|
committer | Aaron LI <aaronly.me@gmail.com> | 2016-06-07 16:06:46 +0800 |
commit | f5aa194346fd59d8721d74b29b56ae6ceeabf9d0 (patch) | |
tree | 628a508cedf8749ec4e71167256e4b15182bcc65 /mass_profile/README.md | |
parent | a79be5a20705b8d751800ede1a8870cb982d9d31 (diff) | |
download | chandra-acis-analysis-f5aa194346fd59d8721d74b29b56ae6ceeabf9d0.tar.bz2 |
Add README.md for mass_profile tools
Diffstat (limited to 'mass_profile/README.md')
-rw-r--r-- | mass_profile/README.md | 32 |
1 files changed, 32 insertions, 0 deletions
diff --git a/mass_profile/README.md b/mass_profile/README.md new file mode 100644 index 0000000..5ebb421 --- /dev/null +++ b/mass_profile/README.md @@ -0,0 +1,32 @@ +Mass Profile Calculation Tools +============================== + +Junhua GU, Weitian LI, Zhenghao ZHU + + +Introduction +------------ +This directory contains the tools/scripts used to calculate the mass profile +for our big Chandra ACIS sample of galaxy groups and clusters. + + +NOTE +---- +* mass calculation references: + + Walker et al. 2012, MNRAS, 422, 3503-3515 + [ADS:2012MNRAS.422.3503W](http://adsabs.harvard.edu/abs/2012MNRAS.422.3503W) + + Ettori et al. 2013, Space Science Reviews, 177, 119-154 + [ADS:2013SSRv..177..119E](http://adsabs.harvard.edu/abs/2013SSRv..177..119E) +* Errors are calculated at 68% confident level. +* NFW profile is employed to extrapolate the mass profile. +* We use a self-proposed model (i.e., *wang2012* model) to describe/fit the gas + temperature profile. +* The single-beta and double-beta models (with a constant background) are used + to describe the gas density profile. + + +TODO +---- +* to merge the scripts/tools for single-beta and double-beta SBP models + (to reduce code duplications) + |