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181
LoTSS/HETDEX: Disentangling star formation and AGN activity in gravitationally lensed radio-quiet quasars
Published 2019“…We present the detection of the gravitationally lensed radio-quiet quasars SDSS J1055+4628, SDSS J1313+5151, and SBS 1520+530 at 144 MHz, which fall in the HETDEX Spring Field targeted in the LOFAR Two-metre Sky Survey (LoTSS) first full data release. …”
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182
The Atacama Cosmology Telescope: temperature and gravitational lensing power spectrum measurements from three seasons of data
Published 2014“…We also present a measurement of the CMB gravitational lensing convergence power spectrum at 4.6σ detection significance. © 2014 IOP Publishing Ltd and Sissa Medialab srl.…”
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183
Resolving star formation on subkiloparsec scales in the high-redshift galaxy SDP.11 using gravitational lensing
Published 2018“…This is consistent with the high intrinsic FIR luminosity (~3 × 1012 L ⊙), ~16 Myr gas depletion timescale, and lesssim8 Myr timescale since the last starburst episode, estimated from the hardness of the UV radiation field. By applying gravitational lensing models to the visibilities in the uv-plane, we find that the lensing magnification factor varies by a factor of two across SDP.11, affecting the observed line profiles. …”
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184
KiDS-i-800: Comparing weak gravitational lensing measurements from same-sky surveys
Published 2018“…We present a weak gravitational lensing analysis of 815 deg2of i-band imaging from the Kilo-Degree Survey (KiDS-i-800). …”
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185
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186
Weak-lensing Analysis of the Complex Cluster Merger A746 with Subaru/Hyper Suprime-Cam
Published 2024-01-01Subjects: Get full text
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187
Two Lensed Star Candidates at z ≃ 4.8 behind the Galaxy Cluster MACS J0647.7+7015
Published 2023-01-01Subjects: “…Strong gravitational lensing…”
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188
The GLASS-JWST Early Release Science Program. III. Strong-lensing Model of Abell 2744 and Its Infalling Regions
Published 2023-01-01Subjects: Get full text
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189
Probing the Solar Interior with Lensed Gravitational Waves from Known Pulsars
Published 2023-01-01Subjects: “…Gravitational lensing…”
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190
Magnification Cross Sections for the Elliptic Umbilic Caustic Surface
Published 2019-07-01Subjects: “…strong gravitational lensing…”
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191
RELICS: Small-scale Star Formation in Lensed Galaxies at z = 6–10
Published 2023-01-01Subjects: “…Gravitational lensing…”
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192
PASSAGES: The Wide-ranging, Extreme Intrinsic Properties of Planck-selected, Lensed Dusty Star-forming Galaxies
Published 2024-01-01Subjects: “…Gravitational lensing…”
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193
Optical and Near-infrared Continuum Emission Region Size Measurements in the Lensed Quasar FBQ J0951+2635
Published 2023-01-01Subjects: Get full text
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194
Accretion Disk Size and Updated Time-delay Measurements in the Gravitationally Lensed Quasar SDSS J165043.44+425149.3
Published 2024-01-01Subjects: Get full text
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195
HybPSF: Hybrid Point-spread Function Reconstruction for the Observed JWST NIRCam Image
Published 2024-01-01Subjects: “…Gravitational lensing…”
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196
Lensing Magnification Seen by Gravitational Wave Detectors
Published 2021-12-01Subjects: Get full text
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197
Etherington’s Distance Duality with Birefringence
Published 2017-07-01Subjects: Get full text
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198
Generalized Extended Uncertainty Principle Black Holes: Shadow and Lensing in the Macro- and Microscopic Realms
Published 2022-10-01Subjects: Get full text
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199
Motion of particles and gravitational lensing around the (2+1)-dimensional BTZ black hole in Gauss–Bonnet gravity
Published 2021-09-01“…Further, we consider the gravitational lensing, to test the GB gravity in (2+1) dimensions and show that the presence of the GB parameter causes the bending angle to first increase with the increase in the inverse of the closest approach distance, $$u_0$$ u 0 , reaching a peak value for a specific $$u_0^*$$ u 0 ∗ , and then decreasing to zero. …”
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200
Pixelated Reconstruction of Foreground Density and Background Surface Brightness in Gravitational Lensing Systems Using Recurrent Inference Machines
Published 2023-01-01“…Modeling strong gravitational lenses in order to quantify distortions in the images of background sources and to reconstruct the mass density in foreground lenses has been a difficult computational challenge. …”
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