Contact Scientist Support for ALMA project 2019.1.00219.S
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00541230" target="_blank" >RIV/67985815:_____/20:00541230 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Contact Scientist Support for ALMA project 2019.1.00219.S
Original language description
Phase 2 Contact Scientist Support for the ALMA Project 2019.1.00219.S (What is the Heating Source of the Dusty Streamers in the High Redshift Obscured Quasar W2246-0526?), PI Jorge Gonzalez Lopez.
Czech name
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Czech description
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Classification
Type
O - Miscellaneous
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/LM2018106" target="_blank" >LM2018106: Atacama Large Millimeter/ Submillimeter Array – participation of the Czech Republic</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů