Far Wide Radio works from public astronomical data. This page carries the credits and the licence conditions that come with it, in full.
James Webb Space Telescope (MAST)
This work is based in part on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST.
Before Birth (Series 1) uses programs #1191, #1328, #1621, #2457, #2926, #4426, #4528 and #5086. First Eyes Were Ears (Series 2) uses programs #1191, #1328, #1621, #2457 and #2731.
We acknowledge the teams led by Lee Armus (#1328) and Roberto Maiolino (#4426) for developing their observing programs with a zero-exclusive-access period.
DESI — Dark Energy Spectroscopic Instrument
First Eyes Were Ears contains material derived from the DESI Early Data Release. DESI data is released under CC BY 4.0, and a sonification is a derived work, so the citation and acknowledgement below are licence conditions rather than courtesy.
Required citation
DESI Collaboration et al. (2024), “The Early Data Release of the Dark Energy Spectroscopic Instrument”
Required acknowledgement
This research used data obtained with the Dark Energy Spectroscopic Instrument (DESI). DESI construction and operations is managed by the Lawrence Berkeley National Laboratory. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of High-Energy Physics, under Contract No. DE–AC02–05CH11231, and by the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility under the same contract. Additional support for DESI was provided by the U.S. National Science Foundation (NSF), Division of Astronomical Sciences under Contract No. AST-0950945 to the NSF’s National Optical-Infrared Astronomy Research Laboratory; the Science and Technology Facilities Council of the United Kingdom; the Gordon and Betty Moore Foundation; the Heising-Simons Foundation; the French Alternative Energies and Atomic Energy Commission (CEA); the National Council of Humanities, Science and Technology of Mexico (CONAHCYT); the Ministry of Science and Innovation of Spain (MICINN), and by the DESI Member Institutions: www.desi.lbl.gov/collaborating-institutions.
The DESI collaboration is honored to be permitted to conduct scientific research on I’oligam Du’ag (Kitt Peak), a mountain with particular significance to the Tohono O’odham Nation. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the U.S. National Science Foundation, the U.S. Department of Energy, or any of the listed funding agencies.
The DESI collaboration is honored to be permitted to conduct scientific research on I’oligam Du’ag (Kitt Peak), a mountain with particular significance to the Tohono O’odham Nation. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the U.S. National Science Foundation, the U.S. Department of Energy, or any of the listed funding agencies.
The recordings
Far Wide Radio programmes are licensed CC BY-NC-SA 4.0.