activity
20132026
most citedThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples

1.9k citations · 7.8k across the 73 of their papers we have counts for

collaborators
Showing 2019Show all

12 papers · 1 filter

astro-ph.CO2019★ 22 cited

Barry and the BAO Model Comparison

Samuel R. Hinton, Cullan Howlett, Tamara M. Davis

We compare the performance of four state-of-the-art models for extracting isotropic measurements of the Baryon Acoustic Oscillation (BAO) scale. To do this, we created a new, publi…

astro-ph.CO2019★ 7 cited

Multi-wavelength consensus of large-scale linear bias

Hengxing Pan, Danail Obreschkow, Cullan Howlett +4

We model the large-scale linear galaxy bias as a function of redshift and observed absolute magnitude threshold for broadband continuum emission from the far inf…

astro-ph.CO2019★ 64 cited

Standard Siren Speeds: Improving velocities in gravitational-wave measurements of

Cullan Howlett, Tamara M. Davis

We re-analyze data from the gravitational-wave event GW170817 and its host galaxy NGC4993 to demonstrate the importance of accurate total and peculiar velocities when measuring the…

astro-ph.CO2019★ 67 cited

Can redshift errors bias measurements of the Hubble Constant?

Tamara M. Davis, Samuel R. Hinton, Cullan Howlett +1

Redshifts have been so easy to measure for so long that we tend to neglect the fact that they too have uncertainties and are susceptible to systematic error. As we strive to measur…

astro-ph.CO2019★ 39 cited

The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys

Cullan Howlett

Low redshift surveys of galaxy peculiar velocities provide a wealth of cosmological information. We revisit the idea of extracting this information by directly measuring the redshi…

astro-ph.CO2019★ 70 cited

The Redshift Space Momentum Power Spectrum II: measuring the growth rate from the combined 2MTF and 6dFGSv surveys

Fei Qin, Cullan Howlett, Lister Staveley-Smith

Measurements of the growth rate of structure, in the low-redshift Universe allow stringent tests of the cosmological model. In this work, we provide new constraints on $fσ_{…

astro-ph.CO2019★ 33 cited

2MTF - VII. 2MASS Tully-Fisher survey final data release: distances for 2,062 nearby spiral galaxies

Tao Hong, Lister Staveley-Smith, Karen L. Masters +8

We present the final distance measurements for the 2MASS Tully-Fisher (2MTF) survey. The final 2MTF catalogue contains 2,062 nearby spiral galaxies in the CMB frame velocity range…

astro-ph.IM2019★ 37 cited

The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

The MSE Science Team, Carine Babusiaux, Maria Bergemann +258

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unvei…

astro-ph.CO2019

4MOST Consortium Survey 8: Cosmology Redshift Survey (CRS)

J. Richard, J. -P. Kneib, C. Blake +14

The 4MOST Cosmology Redshift Survey (CRS) will perform stringent cosmological tests via spectroscopic clustering measurements that will complement the best lensing, cosmic microwav…

astro-ph.IM2019★ 311 cited

4MOST: Project overview and information for the First Call for Proposals

R. S. de Jong, O. Agertz, A. Agudo Berbel +335

We introduce the 4-metre Multi-Object Spectroscopic Telescope (4MOST), a new high-multiplex, wide-field spectroscopic survey facility under development for the four-metre-class Vis…

astro-ph.CO2019★ 8 cited

Cosmology with the MaunaKea Spectroscopic Explorer

Will J. Percival, Christophe Yèche, Maciej Bilicki +11

This document summarizes the science cases related to cosmology studies with the MaunaKea Spectroscopic Explorer (MSE), a highly-multiplexed (4332 fibers), wide FOV (1.5 sq deg), l…

astro-ph.CO2019★ 17 cited

Testing Gravity Using Type Ia Supernovae Discovered by Next-Generation Wide-Field Imaging Surveys

A. G. Kim, G. Aldering, P. Antilogus +29

In the upcoming decade cadenced wide-field imaging surveys will increase the number of identified Type~Ia supernovae (SNe~Ia) from the hundreds to the hundreds of thousands…