Published September 15, 2021 | Version v1
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Resimulation of Multispectral Kinematics of the Multi-mission Space Telescopes

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Description

The set of data resimulated the multi-mission space telescopes' orbits in relation to the NGC 3034 local black hole and white hole. Astrochemical analysis cross-processed with Harvard-Smithsonian MicroObservatory observation data was performed. Thermonuclear explosive astrochemical recombination and analysis were performed on the multi-mission space telescope spectra.

Notes

This research is based on observations made with the NASA/ESA Hubble Space Telescope obtained from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. This research is based on observations made with the Galaxy Evolution Explorer (GALEX) satellite, a NASA mission led by the California Institute of Technology, obtained from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. The scientific results reported in this article are based [in part] on observations made by the Chandra X-ray Observatory. This work is based [in part] on observations made with the Spitzer Space Telescope, which was operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. The observations are performed on Harvard-Smithsonian Micro-observatory, and the data are processed by JS9-4L online and SAOImage DS9 MacOS.

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Cites
Software: 10.5281/zenodo.2530958 (DOI)
Journal article: 10.1093/mnras/sty2448 (DOI)
Is published in
Book: 978-99949-82-66-0 (ISBN)
Journal article: 10.5281/zenodo.6044904 (DOI)
Journal article: 10.5281/zenodo.6796083 (DOI)