{
"status": "new",
"changetime": "2019-02-04T12:10:21Z",
"_ts": "1549282221449479",
"description": "McLaughlin et al post on astro ph\narXiv:1102.5127v1 [astro-ph.EP] 24 Feb 2011 \n\ngives cs for optical / IR lines - systematically smaller than what we have now ",
"reporter": "gary",
"cc": "",
"resolution": "",
"time": "2011-03-01T13:46:42Z",
"component": "atomic/molecular data base",
"summary": "Ne III collision strength update",
"priority": "good to do",
"keywords": "",
"version": "trunk",
"milestone": "c19 branch",
"owner": "nobody",
"type": "enhancement"
}
reported by: @CloudyLex
McLaughlin et al post on astro ph arXiv:1102.5127v1 [astro-ph.EP] 24 Feb 2011
gives cs for optical / IR lines - systematically smaller than what we have now
Migrated from https://www.nublado.org/ticket/198