{"action":"created","issue":{"url":"https://api.github.com/repos/nrnapolita/KIWI_LSST/issues/20","repository_url":"https://api.github.com/repos/nrnapolita/KIWI_LSST","labels_url":"https://api.github.com/repos/nrnapolita/KIWI_LSST/issues/20/labels{/name}","comments_url":"https://api.github.com/repos/nrnapolita/KIWI_LSST/issues/20/comments","events_url":"https://api.github.com/repos/nrnapolita/KIWI_LSST/issues/20/events","html_url":"https://github.com/nrnapolita/KIWI_LSST/issues/20","id":328832464,"node_id":"MDU6SXNzdWUzMjg4MzI0NjQ=","number":20,"title":"UCMGs: future proposals","user":{"login":"ctortora","id":33893698,"node_id":"MDQ6VXNlcjMzODkzNjk4","avatar_url":"https://avatars2.githubusercontent.com/u/33893698?v=4","gravatar_id":"","url":"https://api.github.com/users/ctortora","html_url":"https://github.com/ctortora","followers_url":"https://api.github.com/users/ctortora/followers","following_url":"https://api.github.com/users/ctortora/following{/other_user}","gists_url":"https://api.github.com/users/ctortora/gists{/gist_id}","starred_url":"https://api.github.com/users/ctortora/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/ctortora/subscriptions","organizations_url":"https://api.github.com/users/ctortora/orgs","repos_url":"https://api.github.com/users/ctortora/repos","events_url":"https://api.github.com/users/ctortora/events{/privacy}","received_events_url":"https://api.github.com/users/ctortora/received_events","type":"User","site_admin":false},"labels":[],"state":"open","locked":false,"assignee":null,"assignees":[],"milestone":null,"comments":0,"created_at":"2018-06-03T14:16:41Z","updated_at":"2018-06-18T12:37:40Z","closed_at":null,"author_association":"COLLABORATOR","body":"I want to open this issue, since it is time to think about UCMGs in a wider perspective.\r\n\r\nIt is time to start thinking and planning new proposals, to complete the sample of UCMGs with other new spectroscopic redshifts and to do deeper analysis, e.g. by measuring for subsamples better quality spectra for stellar population analysis:\r\n\r\n1) TNG deadline is passed, let's discuss about future plans about the use of DOLORES@TNG\r\n2) To do plans for other telescopes. The deadline for INT and WHT is still far. To see other facilities.\r\n3) Since the paper is submitted, and it will be soon on ArXiv, it is also time to apply for something more ambitious. I will try with 8-10m facilities for fainter UCMG canidates: e.g. GRANTECAN (Trujillo can help, in time for semester 2019A) and VLT (for the next period 103). This should help to populate UCMG population around z = 0.5, but also to measure using less observing time brighter UCMG candidates.\r\n4) Since we have enough spectra to study systematics in number counts, it should be nice to start selecting some of the validated UCMGs, e.g. with particular characteristics (e.g. very small, with Re< 1 kpc) and plan higher-resolution observations with GTC or VLT, to study stellar populations: In particular ages which give the definitive word about the origin of our selected UCMGs. And, of course, we can try to understand more about othe properties, as e.g. IMF!\r\n5) For the same galaxies, we could also try for HST, to have better resolution for the fit of structural parameters, but this should be discussed accurately, since to have a proposal accepted from HST is very difficult. It is an ambitious project."},"comment":{"url":"https://api.github.com/repos/nrnapolita/KIWI_LSST/issues/comments/398039863","html_url":"https://github.com/nrnapolita/KIWI_LSST/issues/20#issuecomment-398039863","issue_url":"https://api.github.com/repos/nrnapolita/KIWI_LSST/issues/20","id":398039863,"node_id":"MDEyOklzc3VlQ29tbWVudDM5ODAzOTg2Mw==","user":{"login":"KiaraSpin","id":19711937,"node_id":"MDQ6VXNlcjE5NzExOTM3","avatar_url":"https://avatars3.githubusercontent.com/u/19711937?v=4","gravatar_id":"","url":"https://api.github.com/users/KiaraSpin","html_url":"https://github.com/KiaraSpin","followers_url":"https://api.github.com/users/KiaraSpin/followers","following_url":"https://api.github.com/users/KiaraSpin/following{/other_user}","gists_url":"https://api.github.com/users/KiaraSpin/gists{/gist_id}","starred_url":"https://api.github.com/users/KiaraSpin/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/KiaraSpin/subscriptions","organizations_url":"https://api.github.com/users/KiaraSpin/orgs","repos_url":"https://api.github.com/users/KiaraSpin/repos","events_url":"https://api.github.com/users/KiaraSpin/events{/privacy}","received_events_url":"https://api.github.com/users/KiaraSpin/received_events","type":"User","site_admin":false},"created_at":"2018-06-18T12:37:39Z","updated_at":"2018-06-18T12:37:39Z","author_association":"COLLABORATOR","body":"GM 18 June\r\nTogether with Lucia Marchetti, we can submit a proposal to SALT. \r\n@ctortora  will lead the proposal. A companion proposal on lenses will be lead by Lucia.\r\n"}}
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