activity
20192026
most citedJADES NIRSpec Spectroscopy of GN-z11: Lyman- emission and possible enhanced nitrogen abundance in a luminous galaxy

396 citations · 2.1k across the 60 of their papers we have counts for

collaborators
Showing 2022Show all

6 papers · 1 filter

astro-ph.GA2022

Spectroscopic confirmation of four metal-poor galaxies at z=10.3-13.2

Emma Curtis-Lake, Stefano Carniani, Alex Cameron +56

Finding and characterising the first galaxies that illuminated the early Universe at cosmic dawn is pivotal to understand the physical conditions and the processes that led to the…

astro-ph.GA2022★ 274 cited

Identification and properties of intense star-forming galaxies at redshifts z>10

B. E. Robertson, S. Tacchella, B. D. Johnson +53

Surveys with James Webb Space Telescope (JWST) have discovered candidate galaxies in the first 400 Myr of cosmic time. Preliminary indications have suggested these candidate galaxi…

astro-ph.GA2022★ 80 cited

Morpheus Reveals Distant Disk Galaxy Morphologies with JWST: The First AI/ML Analysis of JWST Images

Brant E. Robertson, Sandro Tacchella, Benjamin D. Johnson +21

The dramatic first images with James Webb Space Telescope (JWST) demonstrated its power to provide unprecedented spatial detail for galaxies in the high-redshift universe. Here, we…

astro-ph.GA2022★ 10 cited

Revealing the Galaxy-Halo Connection Through Machine Learning

Ryan Hausen, Brant E. Robertson, Hanjue Zhu +5

Understanding the connections between galaxy stellar mass, star formation rate, and dark matter halo mass represents a key goal of the theory of galaxy formation. Cosmological simu…

astro-ph.IM2022

FitsMap: A Simple, Lightweight Tool For Displaying Interactive Astronomical Image and Catalog Data

Ryan Hausen, Brant Robertson

The visual inspection of image and catalog data continues to be a valuable aspect of astronomical data analysis. As the scale of astronomical image and catalog data continues to gr…

astro-ph.IM2022

Partial-Attribution Instance Segmentation for Astronomical Source Detection and Deblending

Ryan Hausen, Brant Robertson

Astronomical source deblending is the process of separating the contribution of individual stars or galaxies (sources) to an image comprised of multiple, possibly overlapping sourc…