E. Buckley‐Geer
40 ta ish
Fermi National Accelerator Laboratory
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
T. M. C. Abbott, M. Aguena, A. Alarcon +96
MaqolaOchiq kirish202221 iqtibosABIThe Robotic Multiobject Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI)
J. Silber, Parker Fagrelius, Kevin Fanning +97
MaqolaOchiq kirish202219 iqtibosABIValidation of the Scientific Program for the Dark Energy Spectroscopic Instrument
A. G. Adame, J. Aguilar, S. Ahlen +96
MaqolaOchiq kirish202419 iqtibosABIThe DESI Experiment Part I: Science,Targeting, and Survey Design
DESI Collaboration, Amir Aghamousa, Aguilar, Jessica +97
PreprintOchiq kirish201615 iqtibosABIThe Dark Energy Survey: more than dark energy – an overview
Dark Energy Survey Collaboration, T. Abbott, F. B. Abdalla +48
MaqolaOchiq kirish201613 iqtibosABIDark Energy Survey Year 1 results: measurement of the baryon acoustic oscillation scale in the distribution of galaxies to redshift 1
T. M. C. Abbott, F. B. Abdalla, A. Alarcon +97
MaqolaOchiq kirish201811 iqtibosABIThe DESI Experiment Part II: Instrument Design
DESI Collaboration, Amir Aghamousa, Aguilar, Jessica +97
PreprintOchiq kirish20169 iqtibosABIDark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing
T. M. C. Abbott, M. Aguena, A. Alarcon +97
MaqolaOchiq kirish20208 iqtibosABIDark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration
A. Amon, D. Gruen, M. A. Troxel +96
MaqolaOchiq kirish20227 iqtibosABIDESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints
M. Abdul Karim, J. Aguilar, S. Ahlen +97
MaqolaOchiq kirish20257 iqtibosABIValidating the galaxy and quasar catalog-level blinding scheme for the DESI 2024 analysis
U. Andrade, J. Mena-Fernández, Humna Awan +62
MaqolaOchiq kirish20255 iqtibosABIDark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
T. M. C. Abbott, F. B. Abdalla, A. Alarcon +96
MaqolaOchiq kirish20185 iqtibosABIDark Energy Survey Year 1 results: Cosmological constraints from cosmic shear
M. A. Troxel, N. MacCrann, J. Zuntz +96
Maqola20185 iqtibosABIDESI 2024 V: Full-Shape galaxy clustering from galaxies and quasars
A. G. Adame, J. Aguilar, S. Ahlen +96
MaqolaOchiq kirish20254 iqtibosABIObservation of Top Quark Production in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mrow><mml:mover><mml:mrow><mml:mi mathvariant="italic">p</mml:mi></mml:mrow><mml:mrow><mml:mi>¯</mml:mi></mml:mrow></mml:mover></mml:mrow></mml:mrow><mml:mi mathvariant="italic">p</mml:mi></mml:math>Collisions with the Collider Detector at Fermilab
F. Abe, H. Akimoto, A. Akopian +97
MaqolaOchiq kirish19954 iqtibosABIJ/ψ and ψ(2s) Production pp collisions at √ s = 1.8TeV
F. Abe, H. Akimoto, A. Akopian +97
Maqola19974 iqtibosABI<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">J</mml:mi><mml:mi>/</mml:mi><mml:mi mathvariant="italic">ψ</mml:mi></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">ψ</mml:mi><mml:mo>(</mml:mo><mml:mn>2</mml:mn><mml:mi mathvariant="italic">S</mml:mi><mml:mo>)</mml:mo></mml:math>Production in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">p</mml:mi><mml:mrow><mml:mrow><mml:mover><mml:mrow><mml:mi mathvariant="italic">p</mml:mi></mml:mrow><mml:mrow><mml:mi>¯</mml:mi></mml:mrow></mml:mover></mml:mrow></mml:mrow></mml:math>Collisions at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>√</mml:mi><mml:mi mathvariant="italic">s</mml:mi><mml:mspace/><mml:mo>=</mml:mo><mml:mspace/><mml:mn>1.8</mml:mn><mml:mn/><mml:mi/><mml:mi>TeV</mml:mi></mml:math>
F. Abe, H. Akimoto, A. Akopian +97
Maqola19974 iqtibosABI