activity
20182020
most citedPrimordial Non-Gaussianity

54 citations · 150 across the 6 of their papers we have counts for

collaborators

13 papers

astro-ph.IM202015 cited

Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI Response

Emanuele Castorina, Simon Foreman, Dionysios Karagiannis +13

The Packed Ultra-wideband Mapping Array (PUMA) is a proposed low-resolution transit interferometric radio telescope operating over the frequency range 200 - 1100MHz. Its rich scien…

astro-ph.HE2020

Wave effects in the microlensing of pulsars and FRBs by point masses

Dylan L. Jow, Simon Foreman, Ue-Li Pen +1

Wave effects are often neglected in microlensing studies; however, for coherent point-like sources, such as pulsars and fast radio bursts (FRBs), wave effects will become important…

astro-ph.CO2019

Low-redshift 21cm Cosmology in Canada

Adrian Liu, Simon Foreman, Hamsa Padmanabhan +6

Line-intensity mapping of the 21cm line is a powerful probe of large scale structure at z<6, tracing large-scale structure via neutral hydrogen content that is found within galaxie…

astro-ph.CO2019

Baryonic effects on the matter bispectrum

Simon Foreman, William Coulton, Francisco Villaescusa-Navarro +1

The large-scale clustering of matter is impacted by baryonic physics, particularly AGN feedback. Modelling or mitigating this impact will be essential for making full use of upcomi…

astro-ph.IM2019

The CCAT-Prime Submillimeter Observatory

Manuel Aravena, Jason Austermann, Kaustuv Basu +53

The Cerro Chajnantor Atacama Telescope-prime (CCAT-prime) is a new 6-m, off-axis, low-emissivity, large field-of-view submillimeter telescope scheduled for first light in the last…

astro-ph.IM2019

Research and Development for HI Intensity Mapping

Zeeshan Ahmed, David Alonso, Mustafa A. Amin +51

Development of the hardware, data analysis, and simulation techniques for large compact radio arrays dedicated to mapping the 21 cm line of neutral hydrogen gas has proven to be mo…