Showing 1–17 of 17 results
/ Date/ Name
Jul 25, 2022Modeling HI at the field levelMay 2, 2018The HI content of dark matter halos at $z\approx 0$ from ALFALFAApr 14, 2021Anisotropic effective redshift and evolving clustering amplitudeJun 27, 2019Anisotropic halo assembly bias and redshift-space distortionsApr 15, 2020Detection of anisotropic galaxy assembly bias in BOSS DR12Oct 18, 2016Baryon Acoustic Oscillations reconstruction with pixelsSep 22, 2017High-redshift post-reionization cosmology with 21cm intensity mappingDec 2, 2024The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field levelJul 29, 2019Packed Ultra-wideband Mapping Array (PUMA): A Radio Telescope for Cosmology and TransientsFeb 12, 2020Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI ResponseFeb 20, 2024Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSSSep 11, 2019The Quijote simulationsJul 29, 2019Research and Development for HI Intensity MappingApr 24, 2018Ingredients for 21cm intensity mappingMay 28, 2024Improving cosmological analyses of HI clustering by reducing stochastic noiseSep 16, 2024Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomalyOct 22, 2018Inflation and Early Dark Energy with a Stage II Hydrogen Intensity Mapping Experiment