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omid:br/06290177987 | 2023 | Standard cooling of rapidly rotating isolated neutron stars in 2D | 10.3847/1538-4357/ac9eb7 | https://arxiv.org/abs/2206.04539 | https://arxiv.org/pdf/2206.04539 | https://arxiv.org/e-print/2206.04539 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290142431 | 2023-03 | On the Calculation of the Variance of Algebraic Variables in Power System Dynamic Models with Stochastic Processes | 10.1109/TPWRS.2022.3226076 | https://arxiv.org/abs/2206.13839 | https://arxiv.org/pdf/2206.13839 | https://arxiv.org/e-print/2206.13839 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178627 | 2023-03-01 | The Physical Conditions of Emission-Line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations | 10.3847/1538-4357/acba8a | https://arxiv.org/abs/2207.12388 | https://arxiv.org/pdf/2207.12388 | https://arxiv.org/e-print/2207.12388 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178152 | 2023-02-01 | Probing the earliest phases in the formation of massive galaxies with simulated HST+JWST imaging data from Illustris | 10.3847/1538-4357/aca8ff | https://arxiv.org/abs/2207.14062 | https://arxiv.org/pdf/2207.14062 | https://arxiv.org/e-print/2207.14062 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178449 | 2023-02-01 | Synchrotron Polarization of Gamma-Ray Burst Afterglow Shocks with Hydrodynamic-scale Turbulent Magnetic Field | 10.3847/1538-4357/acac88 | https://arxiv.org/abs/2208.09242 | https://arxiv.org/pdf/2208.09242 | https://arxiv.org/e-print/2208.09242 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290177937 | 2023-04-01 | VapoRock: Thermodynamics of vaporized silicate melts for modeling volcanic outgassing and magma ocean atmospheres | 10.3847/1538-4357/acbcc7 | https://arxiv.org/abs/2208.09582 | https://arxiv.org/pdf/2208.09582 | https://arxiv.org/e-print/2208.09582 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629071994 | 2023-01 | SINDy for delay-differential equations: application to model bacterial zinc response | 10.1098/rspa.2022.0556 | https://arxiv.org/abs/2208.10826 | https://arxiv.org/pdf/2208.10826 | https://arxiv.org/e-print/2208.10826 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178536 | 2023-02-01 | Cosmicflows-4 | 10.3847/1538-4357/ac94d8 | https://arxiv.org/abs/2209.11238 | https://arxiv.org/pdf/2209.11238 | https://arxiv.org/e-print/2209.11238 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629092706 | 2023-06 | Regular covariant representations and their Wold-type decomposition | 10.1016/j.jmaa.2022.126997 | https://arxiv.org/abs/2209.13198 | https://arxiv.org/pdf/2209.13198 | https://arxiv.org/e-print/2209.13198 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178563 | 2022-12-01 | The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2 | 10.3847/1538-4357/ac99e0 | https://arxiv.org/abs/2210.05937 | https://arxiv.org/pdf/2210.05937 | https://arxiv.org/e-print/2210.05937 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178024 | 2023-05-01 | Effects of Emerging Bipolar Magnetic Regions in Mean-field Dynamo Model of Solar Cycles 23 and 24 | 10.3847/1538-4357/acaf69 | https://arxiv.org/abs/2210.08764 | https://arxiv.org/pdf/2210.08764 | https://arxiv.org/e-print/2210.08764 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290174482 | 2023-04-18 | Automated Coronary Arteries Labeling Via Geometric Deep Learning | null | https://arxiv.org/abs/2212.00386 | https://arxiv.org/pdf/2212.00386 | https://arxiv.org/e-print/2212.00386 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178197 | 2023-02-01 | Study of radio transients from the quiet Sun during an extremely quiet time | 10.3847/1538-4357/aca899 | https://arxiv.org/abs/2212.00503 | https://arxiv.org/pdf/2212.00503 | https://arxiv.org/e-print/2212.00503 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178016 | 2022-12-28 | Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence that Disks can be Optically Thick at 3 mm | 10.3847/1538-4357/aca52b | https://arxiv.org/abs/2212.00599 | https://arxiv.org/pdf/2212.00599 | https://arxiv.org/e-print/2212.00599 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178724 | 2023-03-01 | The First Flight of the Marshall Grazing Incidence X-ray Spectrometer (MaGIXS) | 10.3847/1538-4357/acbb58 | https://arxiv.org/abs/2212.00665 | https://arxiv.org/pdf/2212.00665 | https://arxiv.org/e-print/2212.00665 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178148 | 2023-02-01 | Timing the r-Process Enrichment of the Ultra-Faint Dwarf Galaxy Reticulum II | 10.3847/1538-4357/aca9d1 | https://arxiv.org/abs/2212.00810 | https://arxiv.org/pdf/2212.00810 | https://arxiv.org/e-print/2212.00810 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178198 | 2023-02-01 | Polarized Maser Emission with In-Source Faraday Rotation | 10.3847/1538-4357/aca595 | https://arxiv.org/abs/2212.01410 | https://arxiv.org/pdf/2212.01410 | https://arxiv.org/e-print/2212.01410 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178729 | 2023-02-01 | The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques | 10.3847/1538-4357/acacff | https://arxiv.org/abs/2212.01915 | https://arxiv.org/pdf/2212.01915 | https://arxiv.org/e-print/2212.01915 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178207 | 2023-01-31 | An analytical model of turbulence in Parker spiral geometry and associated magnetic field line lengths | 10.3847/1538-4357/aca892 | https://arxiv.org/abs/2212.02415 | https://arxiv.org/pdf/2212.02415 | https://arxiv.org/e-print/2212.02415 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290177989 | 2023 | On the origin of the North Celestial Pole Loop | 10.3847/1538-4357/aca4d2 | https://arxiv.org/abs/2212.02592 | https://arxiv.org/pdf/2212.02592 | https://arxiv.org/e-print/2212.02592 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178512 | 2023-07-21 | The prevalence and influence of circumstellar material around hydrogen-rich supernova progenitors | 10.3847/1538-4357/acd8be | https://arxiv.org/abs/2212.03313 | https://arxiv.org/pdf/2212.03313 | https://arxiv.org/e-print/2212.03313 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178740 | 2023-02-01 | The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions | 10.3847/1538-4357/acb43f | https://arxiv.org/abs/2212.03926 | https://arxiv.org/pdf/2212.03926 | https://arxiv.org/e-print/2212.03926 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290141769 | 2022 | Gradient-Type Methods for Optimization Problems with Polyak-Łojasiewicz Condition: Early Stopping and Adaptivity to Inexactness Parameter | null | https://arxiv.org/abs/2212.04226 | https://arxiv.org/pdf/2212.04226 | https://arxiv.org/e-print/2212.04226 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178020 | 2022-12-28 | On the presence of metallofullerenes in fullerene-rich circumstellar envelopes | 10.3847/1538-4357/aca529 | https://arxiv.org/abs/2212.05981 | https://arxiv.org/pdf/2212.05981 | https://arxiv.org/e-print/2212.05981 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178353 | 2023-03-01 | Terminator Habitability: the Case for Limited Water Availability on M-dwarf Planets | 10.3847/1538-4357/aca970 | https://arxiv.org/abs/2212.06185 | https://arxiv.org/pdf/2212.06185 | https://arxiv.org/e-print/2212.06185 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629072022 | 2023-07 | The density and pressure of helium nano-bubbles encapsulated in silicon | 10.1098/rspa.2023.0081 | https://arxiv.org/abs/2212.06474 | https://arxiv.org/pdf/2212.06474 | https://arxiv.org/e-print/2212.06474 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178084 | 2023-02-01 | Direct D-atom incorporation in radicals: An overlooked pathway for deuterium fractionation | 10.3847/1538-4357/acac1d | https://arxiv.org/abs/2212.08680 | https://arxiv.org/pdf/2212.08680 | https://arxiv.org/e-print/2212.08680 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178579 | 2023-02-01 | Constraints on Stellar Flare Energy Ratios in the NUV and Optical From a Multiwavelength Study of GALEX and Kepler Flare Stars | 10.3847/1538-4357/acab59 | https://arxiv.org/abs/2212.08696 | https://arxiv.org/pdf/2212.08696 | https://arxiv.org/e-print/2212.08696 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178175 | 2023-03-01 | Testing the Radio-Selection Method of Dual Active Galactic Nuclei in the Stripe 82 Field | 10.3847/1538-4357/acb646 | https://arxiv.org/abs/2212.08708 | https://arxiv.org/pdf/2212.08708 | https://arxiv.org/e-print/2212.08708 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290190821 | 2023 | Adaptive Uncertainty Distribution in Deep Learning for Unsupervised Underwater Image Enhancement | null | https://arxiv.org/abs/2212.08983 | https://arxiv.org/pdf/2212.08983 | https://arxiv.org/e-print/2212.08983 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290147591 | 2023 | Electronic and valleytronic properties of crystalline boron-arsenide tuned by strain and disorder | null | https://arxiv.org/abs/2212.09085 | https://arxiv.org/pdf/2212.09085 | https://arxiv.org/e-print/2212.09085 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629092519 | 2023-10 | Extendability of continuous quasiconvex functions from subspaces | null | https://arxiv.org/abs/2212.13789 | https://arxiv.org/pdf/2212.13789 | https://arxiv.org/e-print/2212.13789 | 0 | 0 | 0 | 0 | 0 |
omid:br/062302692938 | 2022-08 | Finding the dimension of a non-empty orthogonal array polytope | null | https://arxiv.org/abs/1909.02123 | https://arxiv.org/pdf/1909.02123 | https://arxiv.org/e-print/1909.02123 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290163638 | 2023-04-03 | Permutation-Based True Discovery Guarantee by Sum Tests | 10.1093/jrsssb/qkad019 | https://arxiv.org/abs/2102.11759 | https://arxiv.org/pdf/2102.11759 | https://arxiv.org/e-print/2102.11759 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290177904 | 2023-02-01 | The hydrodynamic evolution of binary black holes embedded within the vertically stratified disks of active galactic nuclei | 10.3847/1538-4357/aca967 | https://arxiv.org/abs/2103.12088 | https://arxiv.org/pdf/2103.12088 | https://arxiv.org/e-print/2103.12088 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290168129 | 2023-07 | An Annotation-based Approach for Finding Bugs in Neural Network Programs | 10.1016/j.jss.2023.111669 | https://arxiv.org/abs/2112.05567 | https://arxiv.org/pdf/2112.05567 | https://arxiv.org/e-print/2112.05567 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629072392 | 2023 | Stability of Image-Reconstruction Algorithms | null | https://arxiv.org/abs/2206.07128 | https://arxiv.org/pdf/2206.07128 | https://arxiv.org/e-print/2206.07128 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290141771 | 2022 | Decentralized Strongly-Convex Optimization with Affine Constraints: Primal and Dual Approaches | 10.1007/978-3-031-22990-9_7 | https://arxiv.org/abs/2207.04555 | https://arxiv.org/pdf/2207.04555 | https://arxiv.org/e-print/2207.04555 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178502 | 2023-02-01 | A new study on a type Iax stellar remnant and its probable association with SN 1181 | 10.3847/1538-4357/acb138 | https://arxiv.org/abs/2208.03946 | https://arxiv.org/pdf/2208.03946 | https://arxiv.org/e-print/2208.03946 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290177908 | 2023-02-01 | DESI Observations of the Andromeda Galaxy: Revealing the Immigration History of our Nearest Neighbor | 10.3847/1538-4357/aca5f8 | https://arxiv.org/abs/2208.11683 | https://arxiv.org/pdf/2208.11683 | https://arxiv.org/e-print/2208.11683 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290148639 | 2023-04-20 | Investigation of a Machine learning methodology for the SKA pulsar search pipeline | 10.1007/s12036-023-09920-4 | https://arxiv.org/abs/2209.04430 | https://arxiv.org/pdf/2209.04430 | https://arxiv.org/e-print/2209.04430 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178323 | 2023-03-01 | Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations | null | https://arxiv.org/abs/2210.04912 | https://arxiv.org/pdf/2210.04912 | https://arxiv.org/e-print/2210.04912 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178081 | 2023-02-01 | Constraining the cosmic merger history of intermediate-mass black holes with gravitational wave detectors | 10.3847/1538-4357/acb34e | https://arxiv.org/abs/2212.04056 | https://arxiv.org/pdf/2212.04056 | https://arxiv.org/e-print/2212.04056 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629092407 | 2023-12 | A lower bound on the quantitative version of the transversality theorem | null | https://arxiv.org/abs/2301.00432 | https://arxiv.org/pdf/2301.00432 | https://arxiv.org/e-print/2301.00432 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178040 | 2023-09-22 | Things that might go bump in the night: Assessing structure in the binary black hole mass spectrum | null | https://arxiv.org/abs/2301.00834 | https://arxiv.org/pdf/2301.00834 | https://arxiv.org/e-print/2301.00834 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178088 | 2023-02-01 | Proton and electron temperatures in the solar wind and their correlations with the solar wind speed | 10.3847/1538-4357/acb341 | https://arxiv.org/abs/2301.00852 | https://arxiv.org/pdf/2301.00852 | https://arxiv.org/e-print/2301.00852 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290168070 | 2023-04 | Characterizing Architecture Related Posts and Their Usefulness in Stack Overflow | null | https://arxiv.org/abs/2301.00943 | https://arxiv.org/pdf/2301.00943 | https://arxiv.org/e-print/2301.00943 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629092671 | 2023-11 | Dual of an extended locally convex space | null | https://arxiv.org/abs/2301.03243 | https://arxiv.org/pdf/2301.03243 | https://arxiv.org/e-print/2301.03243 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178830 | 2023-01-27 | The Low-Redshift Lyman Continuum Survey: Optically Thin and Thick Mg II Lines as Probes of Lyman Continuum Escape | 10.3847/1538-4357/aca89a | https://arxiv.org/abs/2301.04087 | https://arxiv.org/pdf/2301.04087 | https://arxiv.org/e-print/2301.04087 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178298 | 2023-02-01 | The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XXIV. Differences in internal kinematics of multiple stellar populations | 10.3847/1538-4357/acaec6 | https://arxiv.org/abs/2301.04148 | https://arxiv.org/pdf/2301.04148 | https://arxiv.org/e-print/2301.04148 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629099675 | 2023-03-26 | Energy-Efficient Physical Layer Security for Wearable IoT Devices | null | https://arxiv.org/abs/2301.06174 | https://arxiv.org/pdf/2301.06174 | https://arxiv.org/e-print/2301.06174 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290148647 | 2023-05-31 | Kronberger 55: A Candidate for End-dominated Collapse Scenario | 10.1007/s12036-023-09932-0 | https://arxiv.org/abs/2301.06310 | https://arxiv.org/pdf/2301.06310 | https://arxiv.org/e-print/2301.06310 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178629 | 2023-03-01 | Does the HCN/CO ratio trace the star-forming fraction of gas? I. A comparison with analytical models of star formation | 10.3847/1538-4357/acb352 | https://arxiv.org/abs/2301.06478 | https://arxiv.org/pdf/2301.06478 | https://arxiv.org/e-print/2301.06478 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178464 | 2023-02-01 | Probing Velocity Structures of Protostellar Envelopes: Infalling and Rotating Envelopes within Turbulent Dense Cores | null | https://arxiv.org/abs/2301.06969 | https://arxiv.org/pdf/2301.06969 | https://arxiv.org/e-print/2301.06969 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290148667 | 2023-04-25 | Real-time RFI Filtering for uGMRT: Overview of the Released System and Relevance to the SKA | 10.1007/s12036-023-09919-x | https://arxiv.org/abs/2301.07402 | https://arxiv.org/pdf/2301.07402 | https://arxiv.org/e-print/2301.07402 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178507 | 2023-02-01 | Photometric Calibrations of M-dwarf Metallicity with Markov Chain Monte Carlo and Bayesian Inference | 10.3847/1538-4357/acacf6 | https://arxiv.org/abs/2301.08036 | https://arxiv.org/pdf/2301.08036 | https://arxiv.org/e-print/2301.08036 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629092477 | 2023-10 | The double phase Dirichlet problem when the lowest exponent is equal to 1 | 10.1016/j.jmaa.2023.127270 | https://arxiv.org/abs/2301.08119 | https://arxiv.org/pdf/2301.08119 | https://arxiv.org/e-print/2301.08119 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178736 | 2023-02-01 | Effect of multiple scattering on the Transmission spectra and the Polarization phase curves for Earth-like Exoplanets | 10.3847/1538-4357/acb495 | https://arxiv.org/abs/2301.08487 | https://arxiv.org/pdf/2301.08487 | https://arxiv.org/e-print/2301.08487 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290162499 | 2023 | Existence result of the global attractor for a triply nonlinear thermistor problem | 10.2478/mjpaa-2023-0002 | https://arxiv.org/abs/2301.08561 | https://arxiv.org/pdf/2301.08561 | https://arxiv.org/e-print/2301.08561 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178078 | 2023-02-01 | Turbulence Driving by Interstellar Pickup Ions in the Outer Solar Wind | 10.3847/1538-4357/acb337 | https://arxiv.org/abs/2301.08710 | https://arxiv.org/pdf/2301.08710 | https://arxiv.org/e-print/2301.08710 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178011 | 2023-02-01 | Catalog of magnetic white dwarfs with hydrogen dominated atmospheres | 10.3847/1538-4357/acaf6e | https://arxiv.org/abs/2301.08862 | https://arxiv.org/pdf/2301.08862 | https://arxiv.org/e-print/2301.08862 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178336 | 2023-03-01 | A High-resolution Optical Survey of Upper Sco: Evidence for Coevolution of Accretion and Disk Winds | 10.3847/1538-4357/acb2c9 | https://arxiv.org/abs/2301.09240 | https://arxiv.org/pdf/2301.09240 | https://arxiv.org/e-print/2301.09240 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290174487 | 2023-04-18 | DELTA-MRI: Direct deformation Estimation from LongiTudinally Acquired k-space data | null | https://arxiv.org/abs/2301.09455 | https://arxiv.org/pdf/2301.09455 | https://arxiv.org/e-print/2301.09455 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290174877 | 2023-04-18 | Maximum Mean Discrepancy Kernels for Predictive and Prognostic Modeling of Whole Slide Images | null | https://arxiv.org/abs/2301.09624 | https://arxiv.org/pdf/2301.09624 | https://arxiv.org/e-print/2301.09624 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290173328 | 2022-09 | Thermal Neutrinos from the Explosion of a Minimum-Mass Neutron Star | 10.1134/S1063773722090067 | https://arxiv.org/abs/2301.10003 | https://arxiv.org/pdf/2301.10003 | https://arxiv.org/e-print/2301.10003 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629071866 | 2023-07 | Exact and rapid linear clustering of networks with dynamic programming | 10.1098/rspa.2023.0159 | https://arxiv.org/abs/2301.10403 | https://arxiv.org/pdf/2301.10403 | https://arxiv.org/e-print/2301.10403 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290173332 | 2022-09 | Interstellar Extinction in Galactic Cirri in SDSS Stripe 82 | 10.1134/S1063773722090031 | https://arxiv.org/abs/2301.10591 | https://arxiv.org/pdf/2301.10591 | https://arxiv.org/e-print/2301.10591 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290174619 | 2023-04-18 | Region-based motion-compensated iterative reconstruction technique for dynamic computed tomography | 10.1109/ISBI53787.2023.10230608 | https://arxiv.org/abs/2301.11029 | https://arxiv.org/pdf/2301.11029 | https://arxiv.org/e-print/2301.11029 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629092991 | 2024-02 | Matrix representations of multivalued projections and least squares problems | null | https://arxiv.org/abs/2301.12997 | https://arxiv.org/pdf/2301.12997 | https://arxiv.org/e-print/2301.12997 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290174952 | 2023-04-18 | Unpaired Image-to-Image Translation with Limited Data to Reveal Subtle Phenotypes | null | https://arxiv.org/abs/2302.08503 | https://arxiv.org/pdf/2302.08503 | https://arxiv.org/e-print/2302.08503 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290198083 | 2023-09-28 | LEAF: Navigating Concept Drift in Cellular Networks | 10.1145/3609422 | https://arxiv.org/abs/2109.03011 | https://arxiv.org/pdf/2109.03011 | https://arxiv.org/e-print/2109.03011 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629072341 | 2022 | An Educated Warm Start For Deep Image Prior-Based Micro CT Reconstruction | 10.1109/TCI.2022.3233188 | https://arxiv.org/abs/2111.11926 | https://arxiv.org/pdf/2111.11926 | https://arxiv.org/e-print/2111.11926 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178315 | 2023-09-01 | Hydrodynamics and survivability during post-main-sequence planetary engulfment | 10.3847/1538-4357/acbdfc | https://arxiv.org/abs/2203.11227 | https://arxiv.org/pdf/2203.11227 | https://arxiv.org/e-print/2203.11227 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290190857 | 2023-05-31 | Mobility Equity and Economic Sustainability Using Game Theory | null | https://arxiv.org/abs/2203.11421 | https://arxiv.org/pdf/2203.11421 | https://arxiv.org/e-print/2203.11421 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290168038 | 2023-06 | Runtime Software Patching: Taxonomy, Survey and Future Directions | null | https://arxiv.org/abs/2203.12132 | https://arxiv.org/pdf/2203.12132 | https://arxiv.org/e-print/2203.12132 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629072342 | 2023 | Memory-efficient model-based deep learning with convergence and robustness guarantees | null | https://arxiv.org/abs/2206.04797 | https://arxiv.org/pdf/2206.04797 | https://arxiv.org/e-print/2206.04797 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629092738 | 2023-09 | Non-degeneracy and uniqueness of solutions to general singular Toda systems on bounded domains | 10.1016/j.jmaa.2023.127132 | https://arxiv.org/abs/2207.11743 | https://arxiv.org/pdf/2207.11743 | https://arxiv.org/e-print/2207.11743 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629091641 | 2023-07 | Orthogonal Spin Current Injected Magnetic Tunnel Junction for Convolutional Neural Networks | 10.1109/TED.2023.3276850 | https://arxiv.org/abs/2207.14603 | https://arxiv.org/pdf/2207.14603 | https://arxiv.org/e-print/2207.14603 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178178 | 2023-03-01 | GRB 171205A: Hypernova and Newborn Neutron Star | 10.3847/1538-4357/acb771 | https://arxiv.org/abs/2208.02725 | https://arxiv.org/pdf/2208.02725 | https://arxiv.org/e-print/2208.02725 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290171907 | 2023-01 | The Effectiveness of Embedded Values Analysis Modules in Computer Science Education: An Empirical Study | null | https://arxiv.org/abs/2208.05453 | https://arxiv.org/pdf/2208.05453 | https://arxiv.org/e-print/2208.05453 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290177955 | 2023-04-01 | Overview of the DESI Milky Way Survey | 10.3847/1538-4357/acb3c0 | https://arxiv.org/abs/2208.08514 | https://arxiv.org/pdf/2208.08514 | https://arxiv.org/e-print/2208.08514 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178444 | 2023-05-01 | The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history | 10.3847/1538-4357/acbf51 | https://arxiv.org/abs/2209.03385 | https://arxiv.org/pdf/2209.03385 | https://arxiv.org/e-print/2209.03385 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629091919 | 2023-04 | Leveraging Voltage-Controlled Magnetic Anisotropy to Solve Sneak Path Issues in Crossbar Arrays | 10.1109/TED.2023.3246949 | https://arxiv.org/abs/2209.13677 | https://arxiv.org/pdf/2209.13677 | https://arxiv.org/e-print/2209.13677 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178496 | 2023-02-01 | High-redshift JWST Observations and Primordial Non-Gaussianity | 10.3847/1538-4357/acb5ea | https://arxiv.org/abs/2210.04812 | https://arxiv.org/pdf/2210.04812 | https://arxiv.org/e-print/2210.04812 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178302 | 2023-06-01 | The Type II-P Supernova 2019mhm and Constraints on Its Progenitor System | 10.3847/1538-4357/acbd32 | https://arxiv.org/abs/2210.05131 | https://arxiv.org/pdf/2210.05131 | https://arxiv.org/e-print/2210.05131 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178373 | 2023-03-01 | Role of magnetic fields in the formation of direct collapse black holes | 10.3847/1538-4357/acbcc2 | https://arxiv.org/abs/2210.05611 | https://arxiv.org/pdf/2210.05611 | https://arxiv.org/e-print/2210.05611 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178532 | 2023-02-01 | Inflationary and phase-transitional primordial magnetic fields in galaxy clusters | 10.3847/1538-4357/acb04d | https://arxiv.org/abs/2210.10183 | https://arxiv.org/pdf/2210.10183 | https://arxiv.org/e-print/2210.10183 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290174786 | 2023-04-18 | Normal reconstruction from specularity in the endoscopic setting | null | https://arxiv.org/abs/2211.05642 | https://arxiv.org/pdf/2211.05642 | https://arxiv.org/e-print/2211.05642 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178658 | 2023-01-31 | Breaking Degeneracies in Formation Histories by Measuring Refractory Content in Gas Giants | 10.3847/1538-4357/aca614 | https://arxiv.org/abs/2211.09080 | https://arxiv.org/pdf/2211.09080 | https://arxiv.org/e-print/2211.09080 | 0 | 0 | 0 | 0 | 0 |
omid:br/0629097020 | 2023-07-16 | Modeling 100% Electrified Transportation in NYC | null | https://arxiv.org/abs/2211.11581 | https://arxiv.org/pdf/2211.11581 | https://arxiv.org/e-print/2211.11581 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290193269 | 2022-12-29 | Dynamics and Equation of State Dependencies of Relevance for Nucleosynthesis in Supernovae and Neutron Star Mergers | null | https://arxiv.org/abs/2212.07498 | https://arxiv.org/pdf/2212.07498 | https://arxiv.org/e-print/2212.07498 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290177907 | 2023-02-01 | A Study of Primordial Very Massive Star Evolution | 10.3847/1538-4357/acac91 | https://arxiv.org/abs/2212.09629 | https://arxiv.org/pdf/2212.09629 | https://arxiv.org/e-print/2212.09629 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290171121 | 2023 | Nonminimal Higgs Inflation and Initial Conditions in Cosmology | null | https://arxiv.org/abs/2212.13077 | https://arxiv.org/pdf/2212.13077 | https://arxiv.org/e-print/2212.13077 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290174849 | 2023-04-18 | Addressing Deep Learning Model Calibration Using Evidential Neural Networks and Uncertainty-Aware Training | null | https://arxiv.org/abs/2301.13296 | https://arxiv.org/pdf/2301.13296 | https://arxiv.org/e-print/2301.13296 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290171132 | 2023 | Hořava models as palladium of unitarity and renormalizability in quantum gravity | null | https://arxiv.org/abs/2301.13580 | https://arxiv.org/pdf/2301.13580 | https://arxiv.org/e-print/2301.13580 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290177886 | 2023-03-01 | TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting An Extremely Eccentric Exoplanet | 10.3847/1538-4357/acb8ac | https://arxiv.org/abs/2302.01102 | https://arxiv.org/pdf/2302.01102 | https://arxiv.org/e-print/2302.01102 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178420 | 2023-03-01 | Crescent-Shaped Molecular Outflow from the Intermediate-mass Protostar DK Cha Revealed by ALMA | 10.3847/1538-4357/acb930 | https://arxiv.org/abs/2302.01612 | https://arxiv.org/pdf/2302.01612 | https://arxiv.org/e-print/2302.01612 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178427 | 2023-03-01 | A complex dust morphology in the high-luminosity AGN Mrk 876 | 10.3847/1538-4357/acb92d | https://arxiv.org/abs/2302.01678 | https://arxiv.org/pdf/2302.01678 | https://arxiv.org/e-print/2302.01678 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290149261 | 2023-04-03 | A Disparity Refinement Framework for Learning-based Stereo Matching Methods in Cross-domain Setting for Laparoscopic Images | null | https://arxiv.org/abs/2302.02294 | https://arxiv.org/pdf/2302.02294 | https://arxiv.org/e-print/2302.02294 | 0 | 0 | 0 | 0 | 0 |
omid:br/06290178023 | 2023-05-01 | 183 GHz water megamasers in active galactic nuclei: a new accretion disk tracer | 10.3847/1538-4357/acc57a | https://arxiv.org/abs/2302.02572 | https://arxiv.org/pdf/2302.02572 | https://arxiv.org/e-print/2302.02572 | 0 | 0 | 0 | 0 | 0 |
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