#paperday Aligned radio galaxies in the ELAIS-N1 field? Apparently no! Why is that important? Have a look at my new paper ( 🧵

@franco_vazza I assume professors are too lazy/busy to read the email till the end (let alone the email contact). That's why I usually introduce myself

Pretty spiral galaxies that keep fooling a poor student looking for radio galaxies. I will present the catalogue of 1600+ radio galaxies I compiled in the @LOFAR Deep Fields at the next LOFAR Family Meeting #LFM23

The cosmology is safe (for now)! We can go back to the black holes as source of dark energy.

RT @pratikd13: Delighted to share my first review paper on our understanding of #giant radio sources (#GRSs). It also highlights the impor…

RT @hen_edler: Paper day! We studied the cluster Abell 1033 featuring the GReET, one of the steepest spectrum radio sources known. What hap…

Cluster community: we study the largest structures in the universe. GRG people: hold my beer. 70+ new very large radio galaxies in the Boötes field. Check them out! In collaboration with @HambObs et al. #paperday

RT @HambObs: 1st and 2nd go to the University of Hamburg.

Just gave my first live talk on giant radio galaxies in the Boötes deep field at the LFM in Cologne. Such an amazing experience! #LFM22

RT @VolkerHeesen: German taster evening with fish 🐠 Brötchen, 🍺 and Aquavit ⁦@HambObs⁩

Some of the giant radio galaxies we found in the Boötes field. Soon.. 👀

RT @FUbertosi: Here is the press release on our recent paper " The Deepest Chandra View of RBS 797: Evidence for Two Pairs of Equidistant X…

The turbulent anisotropy parameter, β, shows the effects of radial accretion, which appears to be the dominant driver for the gas fluctuations in our simulations. As a consequence, the Richardson number does not act as a good proxy of the dynamics and gas fluctuations of the ICM.