Howlett, Cullan

The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z=0.15

Ross, A. J., Samushia, L., Howlett, C., Percival, W. J., Burden, A., & Manera, M. (2015) · Monthly Notices of the Royal Astronomical Society

Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, Phenomena

Cited by 1,745

DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints

Abdul Karim, M., Aguilar, J., Ahlen, S., Alam, S., Allen, L., Prieto, C. A., Alves, O., Anand, A., Andrade, U., Armengaud, E., et al. (2025) · Physical Review D

Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, Phenomena

Cited by 856

Full-shape galaxy power spectra and the curvature tension

Glanville, A., Howlett, C., & Davis, T. (2022) · Monthly Notices of the Royal Astronomical Society

Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, Phenomena

Cited by 69

Measuring the Growth Rate of Structure with Type IA Supernovae from LSST

Howlett, C., Robotham, A. S. G., Lagos, C. D. P., & Kim, A. G. (2017) · The Astrophysical Journal

Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, Phenomena

Cited by 59