Identikit is a numerical method, combining test-particle and self-consistent techniques, which allows a rapid exploration of the parameter space of galactic encounters. It can be used to find the parameters required to reproduce the observed morphology and kinematics of interacting disk galaxies.
— Paper describing the Identikit 1 system and a blind test of its abilities. Published in The Astronomical Journal, 137, 3071—3090, February 2009.
— Paper describing the Identikit 2 algorithm. Published in the Monthly Notices of the Royal Astronomical Society, 413, 2860—2872, June 2011.
— Web interface to Identikit 1 allows the user to select encounter and viewing parameters, and see the results instantaneously.
— Random merger simulations from the Identikit 1 paper; click on individual systems to see matches.
— Summary of the parameters needed to define an encounter between disk galaxies.
— Source code and key makefiles for Identikit 1.7. Requires the Zeno software environment.
— Source code and key makefiles for Identikit 2.1. Requires the Zeno software environment.
— A small set of data files for experimenting with the Identikit
software. The file jhat12X.dat records initial spin directions
of test particles, while the r124_*.dat files are individual
frames from an encounter between equal-mass galaxies. After downloading
these files, do
./idkit jhat12X.dat
r124_%04x.dat incr=0x100
to try the program.
— Talk given at Academia Sinica Institute of Astronomy and Astrophysics, June 4, 2008.
— John Hibbard's page describing an earlier version.
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Joshua E. Barnes
(barnes at ifa.hawaii.edu)
Updated:
16 May 2012
http://www.ifa.hawaii.edu/~barnes/research/identikit/index.html |
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