From the 1 of 32 papers with an AI index.
68 citations
- D. Brooks3 profiles19 · h 28
- E. Sanchez6 profiles19 · h 82
- R. Miquel19 · h 42
- B. Weaver17 · h 32
- D. Sprayberry17 · h 41
- F. Prada2 profiles17 · h 27
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- G. Tarlé4 profiles17 · h 92
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- NSF NOIRLabUS24 papers
- Centre National de la Recherche ScientifiqueFR23 papers
- Fermi National Accelerator LaboratoryUS22 papers
- University of MichiganUS22 papers
- University College LondonGB21 papers
- Centro de Investigaciones Energéticas, Medioambientales y TecnológicasES20 papers
- Institute for High Energy PhysicsES20 papers
- Instituto de Astrofísica de AndalucíaES20 papers
- Institució Catalana de Recerca i Estudis AvançatsES19 papers
- Sorbonne UniversitéFR19 papers
- University of PortsmouthGB19 papers
- Boston UniversityUS18 papers
11 papers · 1 filter
The Dark Energy Camera All Data Everywhere cosmic shear project V: Constraints on cosmology and astrophysics from 270 million galaxies across 13,000 deg of the sky
D. Anbajagane, C. Chang, A. Drlica-Wagner +78
The paper presents cosmological and astrophysical constraints derived from cosmic shear measurements of 270 million galaxies covering 13,000 deg², combining data from the DECADE pr…
Fiducial-Cosmology-dependent systematics for the DESI 2024 Full-Shape Analysis
R. Gsponer, S. Ramirez-Solano, F. RodrÃguez-MartÃnez +65
We assess the impact of the fiducial cosmology choice on cosmological inference from full-shape (FS) fits of the galaxy power spectrum in the DESI 2024 Data Release 1 (DR1). Using…
Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1
E. A. Zaborowski, P. Taylor, K. Honscheid +58
The sound horizon scale is a key source of information for early-time measurements, and is therefore a common target of new physics proposed to solve the Hubble tension…
DESI Strong Lens Foundry III: Keck Spectroscopy for Strong Lenses Discovered Using Residual Neural Networks
Shrihan Agarwal, Xiaosheng Huang, William Sheu +49
We present spectroscopic data of strong lenses and their source galaxies using the Keck Near-Infrared Echellette Spectrometer (NIRES) and the Dark Energy Spectroscopic Instrument (…
Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI
J. Choppin de Janvry, S. Gontcho A Gontcho, U. Seljak +56
The calibration of tomographic redshift distributions is essential for cosmological analysis of weak lensing data. In this work, we calibrate all four tomographic bins of the Hyper…
Clustering analysis of medium-band selected high-redshift galaxies
H. Ebina, M. White, A. Raichoor +57
Next-generation large-scale structure spectroscopic surveys will probe cosmology at high redshifts , relying on abundant galaxy tracers such as Ly emitters (LA…