31 citations · 55 across the 7 of their papers we have counts for
7 papers
Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr
Roberta Tripodi, Nicholas Martis, Vladan Markov +29
The James Webb Space Telescope (JWST) has recently discovered a new population of objects at high redshift referred to as `Little Red Dots' (LRDs). Their nature currently remains e…
CANUCS: UV and Ionising Properties of Dwarf Star Forming Galaxies at z = 5 to 7
Anishya Harshan, Maruša Bradač, Roberto Abraham +14
The epoch of reionisation progressed through the emission of ionising photons from galaxies to their local intergalactic medium. In this work, we characterise the dwarf star-formin…
Modelling and Subtracting Diffuse Cluster Light in JWST Images: A Relation between the Spatial Distribution of Globular Clusters, Dwarf Galaxies, and Intracluster Light in the Lensing Cluster SMACS 0723
Nicholas S. Martis, Ghassan T. E. Sarrouh, Chris J. Willott +9
We present a methodology for modeling and removing light from cluster galaxies and intracluster light (ICL) from () images of gravitational le…
MOSEL survey: JWST reveals major mergers/strong interactions drive the extreme emission lines in the early universe
Anshu Gupta, Ravi Jaiswar, Vicente Rodriguez-Gomez +7
Extreme emission line galaxies (EELGs), where nebular emissions contribute 30-40% of the flux in certain photometric bands, are ubiquitous in the early universe (z>6). We utilise d…
Star Formation at the Epoch of Reionization with CANUCS: The ages of stellar populations in MACS1149-JD1
Maruša Bradač, Victoria Strait, Lamiya Mowla +15
We present measurements of stellar populations properties of a z = 9.1 gravitationally lensed galaxy MACS1149-JD1 using deep JWST NIRISS slitless spectroscopy as well as NIRISS and…
A First Look at Spatially Resolved Balmer Decrements at from JWST NIRISS Slitless Spectroscopy
Jasleen Matharu, Adam Muzzin, Ghassan Sarrouh +14
We present the first results on the spatial distribution of dust attenuation at traced by the Balmer Decrement, H/H, in emission-line galaxies using deep JWST NIR…