{"action":"opened","issue":{"url":"https://api.github.com/repos/astropy/specutils/issues/175","repository_url":"https://api.github.com/repos/astropy/specutils","labels_url":"https://api.github.com/repos/astropy/specutils/issues/175/labels{/name}","comments_url":"https://api.github.com/repos/astropy/specutils/issues/175/comments","events_url":"https://api.github.com/repos/astropy/specutils/issues/175/events","html_url":"https://github.com/astropy/specutils/issues/175","id":318532676,"number":175,"title":"Feature request: Replacement for IRAF specshift","user":{"login":"pllim","id":2090236,"avatar_url":"https://avatars2.githubusercontent.com/u/2090236?v=4","gravatar_id":"","url":"https://api.github.com/users/pllim","html_url":"https://github.com/pllim","followers_url":"https://api.github.com/users/pllim/followers","following_url":"https://api.github.com/users/pllim/following{/other_user}","gists_url":"https://api.github.com/users/pllim/gists{/gist_id}","starred_url":"https://api.github.com/users/pllim/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/pllim/subscriptions","organizations_url":"https://api.github.com/users/pllim/orgs","repos_url":"https://api.github.com/users/pllim/repos","events_url":"https://api.github.com/users/pllim/events{/privacy}","received_events_url":"https://api.github.com/users/pllim/received_events","type":"User","site_admin":false},"labels":[],"state":"open","locked":false,"assignee":null,"assignees":[],"milestone":null,"comments":0,"created_at":"2018-04-27T20:01:12Z","updated_at":"2018-04-27T20:01:12Z","closed_at":null,"author_association":"MEMBER","body":"http://iraf.net/irafhelp.php?val=specshift&help=Help+Page\r\n\r\n*\"At the moment, I am using the task `iraf.specshift()` to shift spectra and slightly correct the wavelength calibration with narrow lines. I want to read and save the changed spectrum. Theoretically, it is not difficult to code it myself, but I run the script with \"normal\" and 1D spectra at the same time and I am afraid to manipulate directly the pixel values and to save the result in a corrupt format, especially for the 1D spectra. If you know any astro module in Python with this implemented IRAF task...\"*\r\n\r\nSubset of #165 (but not explicitly mentioned there)."}}
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