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Imprints of Explosion Conditions on Late-Time Spectra of Type Ia Supernovae
Imprints of Explosion Conditions on Late-Time Spectra of Type Ia Supernovae
On-Shell Methods Applied to Exotic Higgs Production at Hadronic Colliders
On-Shell Methods Applied to Exotic Higgs Production at Hadronic Colliders
Search for the Dark Matter Signature in the Lepton Jet Final State √(S) = 7 TeV
Search for the Dark Matter Signature in the Lepton Jet Final State √(S) = 7 TeV
Nuclear Structure of Neutron Rich ²⁶Na and the Lifetimes and Electromagnetic Transitions in Neutron Rich ²²F
Nuclear Structure of Neutron Rich ²⁶Na and the Lifetimes and Electromagnetic Transitions in Neutron Rich ²²F
Measurement of Polarization Observables in Vector Meson Photoproduction Using a Transversely-Polarized Frozen-Spin Target and                 Polarized Photons at CLAS, Jefferson Lab
Measurement of Polarization Observables in Vector Meson Photoproduction Using a Transversely-Polarized Frozen-Spin Target and Polarized Photons at CLAS, Jefferson Lab
Higgs Boson Production with Heavy Quarks at Hadron Colliders
Higgs Boson Production with Heavy Quarks at Hadron Colliders
Constraining the Evolution of Massive Stars
Constraining the Evolution of Massive Stars
Search for New Physics with a Three Photon Final State Using the CMS Detector
Search for New Physics with a Three Photon Final State Using the CMS Detector
Nuclear Structure Studies of ¹⁹O, ²⁷Mg, and ²⁹Al Using in-Beam γ-Ray Spectroscopy
Nuclear Structure Studies of ¹⁹O, ²⁷Mg, and ²⁹Al Using in-Beam γ-Ray Spectroscopy
Measurement of the Top Mass in the All-Jets Channel with the DØ Detector at the Fermilab Tevatron Collider
Measurement of the Top Mass in the All-Jets Channel with the DØ Detector at the Fermilab Tevatron Collider
Study of Nuclear Structure and Neutron Stars with a Bayesian Neural Network Approach
Study of Nuclear Structure and Neutron Stars with a Bayesian Neural Network Approach
Search for Heavy Stable Charged Particles √s = 13 TeV Utilizing a Multivariate Approach
Search for Heavy Stable Charged Particles √s = 13 TeV Utilizing a Multivariate Approach
Sunyaev-Zel'Dovich Effect in Galaxy Clusters
Sunyaev-Zel'Dovich Effect in Galaxy Clusters