The next Samsung Unpacked is expected to showcase plenty of new devices on Wednesday morning — and if the leaks prove accurate, the South Korean tech giant’s anticipated Galaxy Fold 5 and Flip 5 foldable smartphones will be front and center.The next Samsung Unpacked is expected to showcase plenty of new devices on Wednesday morning — and if the leaks prove accurate, the South Korean tech giant’s anticipated Galaxy Fold 5 and Flip 5 foldable smartphones will be front and center.
Sanyam Chaurasia, an analyst at Canalys India, writes that “an aggressive 2023 foldable series remains critical” for Samsung as it competes against Apple. Where can you watch Samsung Unpacked? Samsung will be streaming its product launch event live on its YouTube channel and on its website.
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JADES: deep spectroscopy of a low-mass galaxy at redshift 2.3 quenched by environmentWe report the discovery of a quiescent galaxy at $z=2.34$ with a stellar mass of only $M_\star=9.5^{+1.8}_{-1.2} \times 10^{8} \mathrm{M}_\odot$, based on deep JWST/NIRSpec spectroscopy. This is the least massive quiescent galaxy found so far at high redshift. We use a Bayesian approach to model the spectrum and photometry, and find the target to have been quiescent for 0.6 Gyr with a mass-weighted average stellar age of 0.8-1.7 Gyr (dominated by systematics). The galaxy displays an inverse colour gradient with radius, consistent with environment-driven quenching. Based on a combination of spectroscopic and robust (medium- and broad-band) photometric redshifts, we identify a galaxy overdensity near the location of the target (5-$σ$ above the background level at this redshift). We stress that had we been specifically targetting galaxies within overdensities, the main target would not have been selected on photometry alone; therefore, environment studies based on photometric redshifts are biased against low-mass quiescent galaxies. The overdensity contains three spectroscopically confirmed, massive, old galaxies ($M_\star=8-17 \times 10^{10} \mathrm{M}_\odot$). The presence of these evolved systems points to accelerated galaxy evolution in overdensities at redshifts z | 2, in agreement with previous works. In projection, our target lies only 35 pkpc away from the most massive galaxy in this overdensity (spectroscopic redshift z=2.349) which is located close to overdensity's centre. This suggests the low-mass galaxy was quenched by environment, making it possibly the earliest evidence for environment-driven quenching to date.
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