Journal Article GSI-2022-00747

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From atomic physics, to upper‐atmospheric chemistry, to cosmology: A “laser photometric ratio star” to calibrate telescopes at major observatories

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2022
Wiley Weinheim, Germany

Natural sciences 2(2), e20220003 () [10.1002/ntls.20220003]

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Note: J.E.A. gratefully acknowledges support from Canadian Space Agency grants 19FAVICA28 and 17CCPVIC19. D.B. gratefully acknowledges support from the PRISMA+ Cluster of Excellence funded by the German Research Foundation (DFG); from the European Research Council (project Dark-OST); and from the DFG Reinhart Koselleck project. H.R.S. gratefully acknowledges support from the National Science Foundation grant for the Institute for Theoretical Atomic, Molecular, and Optical Physics (ITAMP) at Harvard University and the Smithsonian Astrophysical Observatory. This is an open access article under the terms of the Creative Commons Attribution License

Contributing Institute(s):
  1. HIM / MAM (MAS)
Research Program(s):
  1. 612 - Cosmic Matter in the Laboratory (POF4-612) (POF4-612)
  2. Dark-OsT - Experimental Searches for Oscillating and Transient effects from the Dark Sector (695405) (695405)
Experiment(s):
  1. External experiment at external facility/ no experiment at GSI (POF3; other)

Appears in the scientific report 2022
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Creative Commons Attribution CC BY 4.0 ; DOAJ ; OpenAccess ; Article Processing Charges ; DOAJ Seal ; Fees ; NCBI Molecular Biology Database
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HI Mainz

 Record created 2022-11-14, last modified 2023-10-15