Thomas Pasini (@thomaspasini94) 's Twitter Profile
Thomas Pasini

@thomaspasini94

Postdoctoral researcher in Astrophysics at Hamburg University

ID: 1246739202164895744

linkhttps://it.linkedin.com/in/thomas-pasini-389b05181 calendar_today05-04-2020 09:59:33

61 Tweet

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129 Takip Edilen

Low Frequency Array (@lofar) 's Twitter Profile Photo

Amazing new results for #LOFAR, an international team of astronomers has published the most detailed images yet seen of galaxies beyond our own. A special issue of A&A journal has come out today dedicated to 11 papers describing the results. bit.ly/2W0QjbH

Amazing new results for #LOFAR, an international team of astronomers has published the most detailed images yet seen of galaxies beyond our own. A special issue of <a href="/AandA_journal/">A&A journal</a> has come out today dedicated to 11 papers describing the results. bit.ly/2W0QjbH
Nature Astronomy (@natureastronomy) 's Twitter Profile Photo

Multiple generations of cosmic-ray bubbles in a galaxy group indicate that magnetic fields prevent their mixing with the external medium. Brienza et al.: nature.com/articles/s4155…

Multiple generations of cosmic-ray bubbles in a galaxy group indicate that magnetic fields prevent their mixing with the external medium. Brienza et al.: nature.com/articles/s4155…
Thomas Pasini (@thomaspasini94) 's Twitter Profile Photo

The eFEDS data release by eROSITA keeps on giving! Check out this beautiful work led by @dresrabulbul , in which we managed to find hundreds of galaxy clusters and groups that were simply...in disguise. ui.adsabs.harvard.edu/abs/2021arXiv2…

@HambObs@mastodon.social (@hambobs) 's Twitter Profile Photo

We published more beautiful MeerKAT results today. arxiv.org/abs/2111.06940 showing that relics are filled with network of filaments w different spectral & polarisation properties led by Francesco Dega with HirokiAkamatsu Shane O'Sullivan Paola Domínguez et al. SARAO - South African Radio Astronomy Observatory

We published more beautiful MeerKAT results today. arxiv.org/abs/2111.06940 showing that relics are filled with network of filaments w different spectral &amp; polarisation properties led by <a href="/fradega/">Francesco Dega</a> with <a href="/HirokiAkamatsu/">HirokiAkamatsu</a> <a href="/aghatubrid/">Shane O'Sullivan</a> <a href="/PaolaDom1/">Paola Domínguez</a> et al. <a href="/SKA_Africa/">SARAO - South African Radio Astronomy Observatory</a>
Thomas Pasini (@thomaspasini94) 's Twitter Profile Photo

Check out this beautiful work led by Marisa Brienza! A combination of radio and X-ray observations of NGC 507 revealed the interaction between gas sloshing and remnant plasma

@HambObs@mastodon.social (@hambobs) 's Twitter Profile Photo

An international team of astronomers led by Francesco Dega made the most detailed images of the largest cosmic shock waves ever observed. The observations are based on data from the MeerKAT telescope in South Africa UHH - MIN-Fakultät Francesco Dega Quantum Universe SARAO - South African Radio Astronomy Observatory qu.uni-hamburg.de/activities/new…

Andrea Botteon (@and_botteon) 's Twitter Profile Photo

Check out the detailed analysis of the merging cluster Abell 1550 led by Thomas Pasini+ This cluster is rich of diffuse sources in radio: a halo, a relic, and revived plasma..it is a nice environment to study re-accelration processes in the ICM! arxiv.org/abs/2205.12281

Check out the detailed analysis of the merging cluster Abell 1550 led by <a href="/ThomasPasini94/">Thomas Pasini</a>+
This cluster is rich of diffuse sources in radio: a halo, a relic, and revived plasma..it is a nice environment to study re-accelration processes in the ICM! 
arxiv.org/abs/2205.12281
Thomas Pasini (@thomaspasini94) 's Twitter Profile Photo

#paperday An ultra-steep halo, a relic, a phoenix and gentle re-acceleration in A1550: just a "small" preview of what LOFAR LBA+HBA can do. Much more to be coming soon ;) With @[email protected] Henrik Edler Andrea Botteon Fabio Gastaldello Max Gaspari Francesco Dega and many more ui.adsabs.harvard.edu/abs/2022arXiv2…

#paperday An ultra-steep halo, a relic, a phoenix and gentle re-acceleration in A1550: just a "small" preview of what LOFAR LBA+HBA can do. Much more to be coming soon ;)

With <a href="/HambObs/">@HambObs@mastodon.social</a> <a href="/hen_edler/">Henrik Edler</a> <a href="/and_botteon/">Andrea Botteon</a> <a href="/fabiogasta/">Fabio Gastaldello</a> <a href="/max_gasp/">Max Gaspari</a> <a href="/fradega/">Francesco Dega</a> and many more

ui.adsabs.harvard.edu/abs/2022arXiv2…
ESA Webb Telescope (@esa_webb) 's Twitter Profile Photo

📢 The moment we have been waiting for is here. #Webb delivers deepest infrared image of Universe yet in special briefing. Known as Webb’s First Deep Field, this image features the galaxy cluster SMACS 0723, which is overflowing with detail esawebb.org/announcements/… 👇

📢  The moment we have been waiting for is here. #Webb delivers deepest infrared image of Universe yet in special briefing. Known as Webb’s First Deep Field, this image features the galaxy cluster SMACS 0723, which is overflowing with detail esawebb.org/announcements/… 👇
Thomas Pasini (@thomaspasini94) 's Twitter Profile Photo

PhD thesis and postdoc applications submitted, three in-person conferences, two talks. Definitely a busy month! Here an highlight of the talk I got to present at #agnfeeds2 (a bit late though!)

PhD thesis and postdoc applications submitted, three in-person conferences, two talks. Definitely a busy month! Here an highlight of the talk I got to present at #agnfeeds2 (a bit late though!)
Thomas Pasini (@thomaspasini94) 's Twitter Profile Photo

Check out this beautiful thread by franco_vazza on our latest paper (out today!) How does the injection of electrons by radio galaxy jets promote (future) radio emission?

@HambObs@mastodon.social (@hambobs) 's Twitter Profile Photo

Out today: Ultra-low frequency Low Frequency Array spectral indices of cluster radio halos led by Thomas Pasini w Rossella Cassano Andrea Botteon Henrik Edler et al. Main result: more massive clusters host flatter-spectrum halos arxiv.org/abs/2406.12005