Showing 1–20 of 54 results
/ Date/ Name
Jan 16, 2023Evidence of 3D Dirac conical bands in TlBiSSe by optical and magneto-optical spectroscopyMay 3, 2020GeantV: Results from the prototype of concurrent vector particle transport simulation in HEPSep 28, 2020An Ultra-deep Multi-band VLA Survey of the Faint Radio Sky (COSMOS-XS): Source Catalog and Number CountsMar 18, 2016Star-forming galaxies versus low- and high-excitation radio AGN in the VLA-COSMOS 3GHz Large ProjectApr 27, 2018VLBA+GBT observations of the COSMOS field and radio source counts at 1.4 GHzMar 28, 2017The VLA-COSMOS 3~GHz Large Project: AGN and host-galaxy properties out to z$\lesssim$6Mar 28, 2017VLA-COSMOS 3GHz Large Project: The infrared-radio correlation of star-forming galaxies and AGN to $z\lesssim6$Sep 27, 2024Magneto-optical response of magnetic semiconductors EuCd2X2 (X= P, As, Sb)Jul 12, 2018"Super-deblended" Dust Emission in Galaxies: II. Far-IR to (sub)millimeter photometry and high redshift galaxy candidates in the full COSMOS fieldJul 28, 2020The Ionised- and Cool-Gas Content of The BR1202-0725 System as seen by MUSE and ALMADec 10, 2013Two types of Dirac-cone surface states on (111) surface of topological crystalline insulator SnTeDec 14, 2015The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programmeMar 12, 2018HEP Software Foundation Community White Paper Working Group - Detector SimulationJul 7, 2016The XXL Survey: IX. Optical overdensity and radio continuum analysis of a supercluster at $z=0.43$Sep 28, 2020A Multi-wavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio PopulationSep 17, 2018SMBH accretion properties of radio-selected AGN out to z~4Jan 29, 2019A closer look at the deep radio sky: Multi-component radio sources at 3-GHz VLA-COSMOSSep 30, 2022Offloading electromagnetic shower transport to GPUsDec 8, 2018The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of highly star-forming galaxiesDec 11, 2014Physical properties of z>4 submillimeter galaxies in the COSMOS field