Friday 21 March 2025, by Corentin Louis
This collection is composed of pre-processed data from the NenuFAR Key Project 07 observations of Jupiter used and described in Louis et al. (2025)
This data collection contains pre-processed data from the NenuFAR Key Project 07 observations of Jupiter used in Louis et al. (2025).
The data files are provided in hdf5 format. Each file contains:
Time
array (format: unix
, units: s
) that contains the Epoch information (see below for the coverage). The data have been rebinned to a time resolution of 600 seconds.Frequency_Obs
array (units: MHz
that contains the Frequency of the observation. The data have been rebinned to a frequency resolution of either 1 or 5 MHz.Dataset
2D array containing the data for each Epoch and frequency step.Stokes
variable that indicates the Stokes parameters in Dataset
.key_project
variable that indicates this data were acquired for the Key Project 07 (Jupiter).Target
variable that indicates the target of the observation (Jupiter).T_star
indicates here the periodicity of Jupiter (units: hours
).T_exoplanet
indicates here the periodicity of the Galilean Moon Io (units: hours
).Coverage
How to use
The data files can be read using the Louis et al. (2025b) pipeline:
from lomb_scargle_calculation import read_hdf5_file
filename = <filename.hdf5>
(time_datetime_beam_ON_VI,
frequencies_beam_ON_VI,
data_final_beam_ON_VI,
stokes_beam_ON_VI,
key_project_beam_ON_VI,
target_beam_ON_VI,
T_exoplanet_beam_ON_VI,
T_star_beam_ON_VI
) = read_hdf5_file(filename, dataset=True, LS_dataset = False)
Acknowledgments
The authors acknowledge funding from the ERC under the European Union’s Horizon 2020 research and innovation program (grant agreement no 101020459 - Exoradio)