activity
20082024
most citedDusty Star-Forming Galaxies at High Redshift

803 citations · 10.9k across the 152 of their papers we have counts for

collaborators
Showing 2017Show all

11 papers · 1 filter

astro-ph.GA2017★ 2 cited

AMI-LA Observations of the SuperCLASS Super-cluster

C. J. Riseley, K. J. B. Grainge, Y. C. Perrott +21

We present a deep survey of the SuperCLASS super-cluster - a region of sky known to contain five Abell clusters at redshift - performed using the Arcminute Microkelvin I…

astro-ph.IM2017★ 7 cited

Key Science Goals for the Next Generation Very Large Array (ngVLA): Report from the ngVLA Science Advisory Council

Alberto D. Bolatto, Shami Chatterjee, Caitlin M. Casey +20

This document describes some of the fundamental astrophysical problems that require observing capabilities at millimeter- and centimeter wavelengths well beyond those of existing,…

astro-ph.GA2017★ 181 cited

The Constant Average Relationship between Dust-obscured Star Formation and Stellar Mass from to

Katherine E. Whitaker, Alexandra Pope, Ryan Cybulski +3

The total star formation budget of galaxies consists of the sum of the unobscured star formation, as observed in the rest-frame ultraviolet (UV), together with the obscured compone…

astro-ph.GA2017★ 26 cited

The Fine Line Between Normal and Starburst Galaxies

Nicholas Lee, Kartik Sheth, Kimberly S. Scott +10

Recent literature suggests that there are two modes through which galaxies grow their stellar mass - a normal mode characterized by quasi-steady star formation, and a highly effici…

astro-ph.GA2017★ 86 cited

An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution

Drew Brisbin, Oskari Miettinen, Manuel Aravena +28

We carried out targeted ALMA observations of 129 fields in the COSMOS region at 1.25 mm, detecting 152 galaxies at S/N5 with an average continuum RMS of 150 Jy. These fiel…

astro-ph.GA2017★ 74 cited

An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling

Oskari Miettinen, Ivan Delvecchio, Vernesa Smolčić +25

We determine the physical properties of a sample of SMGs in the COSMOS field that were pre-selected at the observed wavelength of mm, and followed up at $λ_{\rm o…