Showing 1–20 of 55 results
/ Date/ Name
Apr 17, 2023JWST CEERS probes the role of stellar mass and morphology in obscuring galaxiesApr 15, 2016Properties of galaxies at the faint end of the H$α$ luminosity function at $z\sim0.62$May 1, 2017A comparison between the soft X-ray and [O III] morphologies of active galactic nucleiMar 22, 2021Sub-millimetre compactness as a critical dimension to understand the Main Sequence of star-forming galaxiesJul 25, 2022A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS ImagingSep 23, 2019Quiescent galaxies 1.5 billion years after the Big Bang and their progenitorsDec 19, 2022Massive galaxy formation caught in action at z~5 with JWSTJan 10, 2023$JWST$ Insight Into a Lensed $HST$-dark Galaxy and its Quiescent Companion at $z=2.58$Apr 24, 2023Two massive, compact, and dust-obscured candidate $z\sim 8$ galaxies discovered by JWSTOct 6, 2022The hidden side of cosmic star formation at z > 3: Bridging optically-dark and Lyman break galaxies with GOODS-ALMAFeb 6, 2018ALMA 26 Arcmin$^{2}$ Survey of GOODS-S at One-millimeter (ASAGAO): Average Morphology of High-$z$ Dusty Star-Forming Galaxies is an Exponential-Disk ($n \simeq 1$)Nov 27, 2023Measuring the gas reservoirs in $10^{8}<$ M$_\star<10^{11}$ M$_\odot$ galaxies at $1\leq z\leq3$Jun 17, 2024PRIMER: JWST/MIRI reveals the evolution of star-forming structures in galaxies at z<2.5May 28, 2024A$^3$COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4 < z < 5$Jan 7, 2025The Cosmic Evolution Early Release Science Survey (CEERS)Jan 9, 2025Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxiesMay 21, 2019Confirming Herschel candidate protoclusters from ALMA/VLA CO observationsJun 24, 2021GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxiesJul 13, 2023Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at $z\geq3$ in Public $JWST$ FieldsDec 9, 2023Fitting pseudo-S${\rm \acute{e}}$rsic(Spergel) light profiles to galaxies in interferometric data: the excellence of the $uv$-plane