Showing 1–20 of 59 results
/ Date/ Name
Jul 22, 2022H$α$ and Continuum Sizes with the HST/WFC3 G141 Grism: Outside-In Quenching for $z=1.0-1.4$ Fast Quenchers?Mar 11, 2022Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$Sep 14, 2016HST Grism Confirmation of Two $z \sim 2$ Structures from the Clusters Around Radio-Loud AGN (CARLA) SurveyJul 14, 2025Global sky background images for JWST/NIRISS Wide-Field Slitless SpectroscopyApr 4, 2018$HST$ Grism Confirmation of $16$ Structures at $1.4 < z < 2.8$ from the Clusters Around Radio-Loud AGN (CARLA) SurveyOct 31, 2022The Near Infrared Imager and Slitless Spectrograph for JWST -- V. Kernel Phase Imaging and Data AnalysisJul 28, 2025A deep dive down the broad-line region: permitted OI, CaII and FeII emission in an AGN Little Red Dot at z=5.3Dec 14, 2022The first large catalogue of spectroscopic redshifts in Webb's First Deep Field, SMACS J0723.3$-$7327Jan 7, 2026A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13Feb 19, 2026UV slopes of Starforming Galaxies in Strong Lensing fields at the Epoch of Reionization with JWSTSep 26, 20233D tomography of the giant Ly$α$ nebulae of $z$$\approx$3--5 radio-loud AGNNov 20, 2023A Steep Decline in the Galaxy Space Density Beyond Redshift 9 in the CANUCS UV Luminosity FunctionNov 30, 2022The galaxy mass-size relation in CARLA clusters and proto-clusters at 1.4 < z < 2.8: larger cluster galaxy sizesDec 14, 2022JWST catches the assembly of a $z\sim5$ ultra-low-mass galaxyApr 21, 2023Spectroscopy from Photometry: A Population of Extreme Emission Line Galaxies at $1.7 \lesssim z \lesssim 6.7$ Selected with JWST Medium Band FiltersOct 27, 2024A Jet-Induced Shock in a Young, Powerful Radio Galaxy at z=3.00Jun 26, 2025CANUCS/Technicolor Data Release 1: Imaging, Photometry, Slit Spectroscopy, and Stellar Population ParametersSep 24, 2025Star Formation under a Cosmic Microscope: Highly magnified z = 11 galaxy behind the Bullet ClusterOct 7, 2025The rise and fall of Little Red Dots could be driven by the environmentDec 8, 2022The Pan-STARRS1 z>5.6 quasar survey II: Discovery of 55 Quasars at 5.6<z<6.5