Showing 1–20 of 31 results
/ Date/ Name
Jan 17, 2013Impact of substrate on magnetic phase coexistence in bicritical $Sm_{0.53} Sr_{0.47} Mn O_3$ thin filmsJan 17, 2013Carrier localization and out of plane anisotropic magnetoresistance in $Nd_{0.55-x} Sm_x Sr_{0.45} Mn O_3$ thin filmsNov 11, 2016New High-z Fermi BL Lacs with the Photometric Dropout TechniqueApr 24, 2024Broadband Multi-wavelength Properties of M87 during the 2018 EHT Campaign including a Very High Energy Flaring EpisodeApr 14, 2021Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope CampaignDec 5, 2022Identifying the 3FHL Catalog. VI. Swift Observations of 3FHL Unassociated Objects with Source Classification via Machine LearningSep 20, 2020Interstrip Capacitances of the Readout Board used in Large Triple-GEM Detectors for the CMS Muon UpgradeJul 20, 2021Performance of a Triple-GEM Demonstrator in $pp$ Collisions at the CMS DetectorJan 12, 2016Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report, Volume 4 The DUNE Detectors at LBNFMar 30, 2017High-redshift blazars through nustar eyesJan 17, 2013Impact of strain on metamagnetic transitions in $Sm_{0.5} Sr_{0.5} Mn O_3$ thin filmsSep 20, 2022Revealing high-z Fermi-LAT BL Lacs using Swift and SARA data with photometric analysisJul 8, 2021Modeling the triple-GEM detector response to background particles for the CMS ExperimentJul 27, 2016M31N 2008-12a - the remarkable recurrent nova in M31: Pan-chromatic observations of the 2015 eruptionNov 11, 2013A genome wide dosage suppressor network reveals genetic robustness and a novel mechanism for Huntington's diseaseMay 30, 2017CXO J004318.8+412016, a steady supersoft X-ray source in M 31Feb 18, 2020Hunting distant BL Lacs with the photometric technique using Swift and SARAJan 7, 2020NuSTAR perspective on high-redshift MeV blazarsMay 28, 2020Investigation of particle production in $h{\text -}A$ collisions using statistical distributionsApr 27, 2021Identifying the 3FHL catalog: V. Results of the CTIO-COSMOS optical spectroscopy campaign 2019