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2025 ASTRON/JIVE Fantasy Formula 1

© Janssen, Bassa, McKenna

Last year around this time, while enjoying one of the regular Wednesday evening social dinners at the Bospub, some of us realised that there are many other Formula 1 enthousiasts among our colleagues. A slack channel #f1fanatics was created on the spot, and we assembled there to chat about the 2024 season that was just ending.

For 2025, we decided that a Fantasy Formula 1 game was the perfect way to share the fun. Based on the inspiring example of the Jodrell Bank version, it was set up by the time the 2025 season started.

How does it work? All F1 drivers have a unique value in virtual money, and are divided in three categories; top picks, mid-fielders and no-hopers. Each participant has to select six drivers in total: two drivers from each category, and has to stay within a given budget.

Then, for each race, based on the actual F1 results, all drivers that finished receive points. The participant's points for their selected drivers are added and the fantasy formula one competition emerges!

Given the cost cap, people had to be smart in their selections. It wasn't possible to choose only the best drivers per category, and sometimes there are surprises when drivers that were not expected to perform well, suddenly managed to get a podium position!

Watching Formula 1 suddenly got an extra dimension. You can support a real team, but maybe your selected driver is from the competition. Your most expensive driver may suddenly have bad luck and score less points than expected. You may be in a losing spot in FF1, but score most points in a single race. And our end-of-season was as exciting as the real Formula 1. Three people contended for the title, and it all came down to the very last race of the season.

We were kindly allowed to watch the race live together in the Oort room last Sunday. It was the perfect social ending of an amazingly entertaining F1 year.

And after we watched Lando Norris winning his first F1 championship, we crowned Aditya Parthasaraty as our first ever ASTRON-JIVE Fantasy Formula 1 champion.

A new Fantasy Formula 1 game will run next year. Are you interested? Or just up for some F1-related gossip? Join us in the slack channel: #f1fanatics.

Colloquia

May 1, 2022

The Commensal Radio Astronomy FAST Survey (CRAFTS)

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) has released its first call for proposal and will be open to the international community next year. Based on a novel technique of high-cadence CAL injection, we have realized the world's first calibrated commensal survey mode, simultaneously taking data for pulsar search, HI galaxies, HI imaging, and FRBs. I introduce here one of the major survey plans, namely, the Commensal Radio Astronomy FAST Survey (CRAFTS, Li et al. 2018), which has discovered more than 100 new pulsars, including a few dozen MSPs, 5 new FRBs, including one new repeater. I will also briefly describe recent FAST results from CRAFTS and other dedicated programs, including new insights into the characteristic energy of FRBs, the formation process of neutron stars, the evolution of interstellar medium, etc.
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May 14, 2022

Extreme UV Emission: Bridging Galaxy Evolution Across Cosmic Time

In the last few years, our first glimpse of the spectral properties of z∼5−7 galaxies has emerged. Deep UV spectra have revealed prominent high-ionization nebular emission lines (i.e., C IV, He II, C III]) indicating that extreme radiation fields may be characteristic of reionization-era systems. While such strong high-ionization emission lines are atypical of the well-studied z∼0−3 galaxy samples, our recent UV spectral campaigns have revealed several galaxies with analogous emission-line features to reionization-era systems. I will discuss the recent detection of extremely strong UV emission in nearby galaxies and the potential sources of their very hard ionizing radiation fields. Such strong detections of high-ionization emission lines have been linked to the leakage of Lyman continuum (LyC) photons (necessary for reionization) both theoretically and observationally. These extreme UV emission-line dwarf galaxies provide a template for the extreme conditions that are important for reionization, however their features are still poorly understood. In preparation for the coming UV window onto the early universe with the advent of ELTs and JWST, I will introduce the COS Legacy Archival Spectroscopic SurveY - an upcoming large HST program designed to disentangle the stellar and nebular spectral signatures of 45 star-forming galaxies. This program will calibrate new UV diagnostics that will allow us to trace galaxy evolution to the distant universe, unveiling the properties of reionization-era galaxies.
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