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Observations 2023-12-27 20:30-22:30 UTC
This time was chosen because of a good chance to see DAM signals from both hemispheres of Jupiter, so that that could be calibration relative to each other. We observed with NenuFAR, the LWA (LWA1, LWA-SV), KAIRA, GLOW, and other international LOFAR stations (). It is very sad that our Ukrainian friends cannot participate with UTR2 anymore.
All LOFAR(-like) stations observed in RCU mode 3 (band 10_90) with 8-bit recording of 244 subbands (40-283, 8-55 MHz). Beamforming was done in direction 0.5826639,0.2118205,J2000
or 0,0,JUPITER
.
Individual stations
KAIRA
Here are beamlet statistics (dynamic spectrum) just before the observations:
This plot was taken from the realtime display at https://www.sgo.fi/KAIRA/bst.php. It shows a nice Io-B arc (north).
People involved: Derek McKay
NenuFAR
Beamlet statistics (dynamic spectra for XX and YY) from NenuFAR show the great performance of this telescope:
20231227_202900_bst_sum_up_glisse_s_.pdf
These plots show the strong Io-B arc, but unfortunately not the Io-D counterpart from the southern hemisphere that we had hoped for. However, the signal is clearly strong enough for a VLBI analysis.
People involved: Laurent Lamy, Jean-Mathias Griessmeier, Philippe Zarka, Louis Bondonneau
LWA
The LWA participated with the stations LWA1 and LWA-SV with director's time in project DW005. The schedule file DW005_231227_2230_0001.idf was used. It defines two tunings with 19.6 MHz bandwidth each, one centred on 16.078125000 MHz, one on 31.390625000 MHz.
People involved: Greg Taylor, Jayce Dowell
GLOW
The German LOFAR stations DE601,602,603,604,605,609 observed using the standard scheduling system in mode UDP2lanesRCU3
. They all produced data, but DE601 had strong noise and dropped out too early. They all have their own RFI. I also recorded subband statistics (SST) and beamlet statistics (BST) with 1-sec time resolution for all stations, as well as 1-sec TBB dumps with DE604 and DE605 every about 8 minutes.
Plots of the BST files (dynamic spectra) can be found here.
People involved: Olaf Wucknitz, Francesco Angelo Iraci, Sai Chaitanya Susarla, Krishnakumar Moochickal Ambalappat
other stations