| _version_ |
1826202909171253248
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| collection |
MIT
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| first_indexed |
2024-09-23T12:25:57Z
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| format |
Article
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| id |
mit-1721.1/134575
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| institution |
Massachusetts Institute of Technology
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| language |
English
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| last_indexed |
2024-09-23T12:25:57Z
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| publishDate |
2021
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| publisher |
American Astronomical Society
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| record_format |
dspace
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| spelling |
mit-1721.1/1345752022-09-28T08:00:24Z TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up 2021-10-27T20:05:38Z 2021-10-27T20:05:38Z 2021-08-01 2021-09-28T17:54:25Z Article http://purl.org/eprint/type/JournalArticle https://hdl.handle.net/1721.1/134575 en 10.3847/1538-3881/ac06cd The Astronomical Journal Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Astronomical Society The American Astronomical Society
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| spellingShingle |
TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
|
| title |
TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
|
| title_full |
TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
|
| title_fullStr |
TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
|
| title_full_unstemmed |
TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
|
| title_short |
TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
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| title_sort |
toi 2076 and toi 1807 two young comoving planetary systems within 50 pc identified by tess that are ideal candidates for further follow up
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| url |
https://hdl.handle.net/1721.1/134575
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