Tootfinder

Hallo Apple-Benutzende! Was nutzt man bei iOS, um MIDIs abzuspielen ? Frage für eine Freundin, die mit meinen MIDIs üben will.

🔊 #NowPlaying on BBCRadio1's #Radio1sClassicEssentialMix
Apollo:
🎵 Way Out West
#BBCR1 #Apollo
https://open.spotify.com/track/0GV8A360LgMx002TZbevo9
https://generalmidiuk.bandcamp.com/track/apollo-general-midis-apollo-8-mix

This https://arxiv.org/abs/2308.16895 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_…

MIDIS: JWST/MIRI reveals the Stellar Structure of ALMA-selected Galaxies in the Hubble-UDF at Cosmic Noon
We present deep James Webb Space Telescope (JWST)/MIRI F560W observations of a flux-limited, ALMA-selected sample of 28 galaxies at z=0.5-3.6 in the Hubble Ultra Deep Field (HUDF). The data from the MIRI Deep Imaging Survey (MIDIS) reveal the stellar structure of the HUDF galaxies at rest-wavelengths of >1 micron for the first time. We revise the stellar mass estimates using new JWST photometry and find good agreement with pre-JWST analysis; the few discrepancies can be explained by blending is…

This https://arxiv.org/abs/2309.15671 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_…

MIDIS: Unveiling the Role of Strong Ha-emitters during the Epoch of Reionization with JWST
By using the ultra-deep \textit{JWST}/MIRI image at 5.6 $μm$ in the Hubble eXtreme Deep Field, we constrain the role of strong H$α$-emitters (HAEs) during Cosmic Reionization at $z\simeq7-8$. Our sample of HAEs is comprised of young ($<35\;\rm Myr$) galaxies, except for one single galaxy ($\approx 300\;\rm Myr$), with low stellar masses ($\lesssim 10^{9}\;\rm M_{\odot}$). These HAEs show a wide range of UV-$β$ slopes, with a median value of $β= -2.15\pm0.21$ which broadly correlates with st…

This https://arxiv.org/abs/2309.15671 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_…

MIDIS: Unveiling the Role of Strong Ha-emitters during the Epoch of Reionization with JWST
By using the ultra-deep \textit{JWST}/MIRI image at 5.6 $μm$ in the Hubble eXtreme Deep Field, we constrain the role of strong H$α$-emitters (HAEs) during Cosmic Reionization at $z\simeq7-8$. Our sample of HAEs is comprised of young ($<35\;\rm Myr$) galaxies, except for one single galaxy ($\approx 300\;\rm Myr$), with low stellar masses ($\lesssim 10^{9}\;\rm M_{\odot}$). These HAEs show a wide range of UV-$β$ slopes, with a median value of $β= -2.07\pm0.20$ which broadly correlates with st…