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author | Aaron LI <aaronly.me@gmail.com> | 2016-06-07 16:06:46 +0800 |
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committer | Aaron LI <aaronly.me@gmail.com> | 2016-06-07 16:06:46 +0800 |
commit | f5aa194346fd59d8721d74b29b56ae6ceeabf9d0 (patch) | |
tree | 628a508cedf8749ec4e71167256e4b15182bcc65 | |
parent | a79be5a20705b8d751800ede1a8870cb982d9d31 (diff) | |
download | chandra-acis-analysis-f5aa194346fd59d8721d74b29b56ae6ceeabf9d0.tar.bz2 |
Add README.md for mass_profile tools
-rw-r--r-- | mass_profile/README.md | 32 | ||||
-rw-r--r-- | mass_profile/change.log | 25 |
2 files changed, 32 insertions, 25 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) + diff --git a/mass_profile/change.log b/mass_profile/change.log deleted file mode 100644 index c26f514..0000000 --- a/mass_profile/change.log +++ /dev/null @@ -1,25 +0,0 @@ -Changes: -v201208132246: - Change the fitting plot of surface brightness to log-log from the original linear one. - Add a constraint over the power law component and the Gaussian component of zyy model. - -v201208161900: - Utilize the mass calculation of -http://adsabs.harvard.edu/abs/2012MNRAS.422.3503W - -v201208172340: - Output the both components of the double beta model in rho_fit.qdp - added the cm per pixel parameter to fit_zyy_model -v201208180209: - add the cooling function calculation program -v201208181800: - add the 1-beta model fitting tools -v201208201200: - add the wang2012 model - make the temperature fitting programmes output fit_result.dat with a kpc x-axis -v201208261700: - use nfw to calcualte mass profile extrapolation -v201208281500: - change from calculate std error to 68% double-sided error - added output of ra and dec in query_source_info.sh - |