{"action":"created","issue":{"url":"https://api.github.com/repos/lsstdarkmatter/dark-matter-paper/issues/10","repository_url":"https://api.github.com/repos/lsstdarkmatter/dark-matter-paper","labels_url":"https://api.github.com/repos/lsstdarkmatter/dark-matter-paper/issues/10/labels{/name}","comments_url":"https://api.github.com/repos/lsstdarkmatter/dark-matter-paper/issues/10/comments","events_url":"https://api.github.com/repos/lsstdarkmatter/dark-matter-paper/issues/10/events","html_url":"https://github.com/lsstdarkmatter/dark-matter-paper/issues/10","id":302493734,"number":10,"title":"Galaxy cluster constraints of dark matter","user":{"login":"wadawson","id":3067471,"avatar_url":"https://avatars2.githubusercontent.com/u/3067471?v=4","gravatar_id":"","url":"https://api.github.com/users/wadawson","html_url":"https://github.com/wadawson","followers_url":"https://api.github.com/users/wadawson/followers","following_url":"https://api.github.com/users/wadawson/following{/other_user}","gists_url":"https://api.github.com/users/wadawson/gists{/gist_id}","starred_url":"https://api.github.com/users/wadawson/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/wadawson/subscriptions","organizations_url":"https://api.github.com/users/wadawson/orgs","repos_url":"https://api.github.com/users/wadawson/repos","events_url":"https://api.github.com/users/wadawson/events{/privacy}","received_events_url":"https://api.github.com/users/wadawson/received_events","type":"User","site_admin":false},"labels":[{"id":857142981,"url":"https://api.github.com/repos/lsstdarkmatter/dark-matter-paper/labels/hack","name":"hack","color":"6cd879","default":false}],"state":"open","locked":false,"assignee":null,"assignees":[],"milestone":null,"comments":2,"created_at":"2018-03-05T22:42:58Z","updated_at":"2018-03-07T05:56:30Z","closed_at":null,"author_association":"NONE","body":"The basic idea is to write up some material on the galaxy cluster constraints of dark matter. In particular what LSST can do in conjunction with other facilities (e.g. X-ray telescopes, and spectroscopic facilities). The could include probes such as: wobbling BCG’s, merging galaxy clusters, and halo density profiles."},"comment":{"url":"https://api.github.com/repos/lsstdarkmatter/dark-matter-paper/issues/comments/371031675","html_url":"https://github.com/lsstdarkmatter/dark-matter-paper/issues/10#issuecomment-371031675","issue_url":"https://api.github.com/repos/lsstdarkmatter/dark-matter-paper/issues/10","id":371031675,"user":{"login":"sazabi4","id":7751063,"avatar_url":"https://avatars1.githubusercontent.com/u/7751063?v=4","gravatar_id":"","url":"https://api.github.com/users/sazabi4","html_url":"https://github.com/sazabi4","followers_url":"https://api.github.com/users/sazabi4/followers","following_url":"https://api.github.com/users/sazabi4/following{/other_user}","gists_url":"https://api.github.com/users/sazabi4/gists{/gist_id}","starred_url":"https://api.github.com/users/sazabi4/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/sazabi4/subscriptions","organizations_url":"https://api.github.com/users/sazabi4/orgs","repos_url":"https://api.github.com/users/sazabi4/repos","events_url":"https://api.github.com/users/sazabi4/events{/privacy}","received_events_url":"https://api.github.com/users/sazabi4/received_events","type":"User","site_admin":false},"created_at":"2018-03-07T05:56:30Z","updated_at":"2018-03-07T05:56:30Z","author_association":"NONE","body":"I would also be interested in knowing how spectroscopy can help on merging cluster and halo density profile, and,  whether a signal of wobbling BCG is detectable in velocity with a large sample..."}}
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