From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method | Paper Citation Record

Observation 817ad72e-ea36-43c0-b41d-b615c0802297 · outbound

This paper cites (4) with δ = 0 into Eq.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method (4) with δ = 0 into Eq

Reference 1

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Observation 95afb0af-e0b2-442d-9d17-5af01d29e8a1 · outbound

This paper cites (4) takes the form of a non-integer power series, as in the case of the general three-parameter model in Eq.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method (4) takes the form of a non-integer power series, as in the case of the general three-parameter model in Eq

Reference 2

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Observation 7220f18c-0e81-4be0-a550-e2f0787c763f · outbound

This paper cites For the potential Φ( r), we can simply substitute Eqs.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method For the potential Φ( r), we can simply substitute Eqs

Reference 3

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Observation a479b775-f5eb-4d75-a4b8-f72f7ce55a33 · outbound

This paper cites (11), along with the so- lution from Eq.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method (11), along with the so- lution from Eq

Reference 4

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Observation 01498ca1-19ef-4371-bd97-440c26ec32f1 · outbound

This paper cites It is worth noting that all the coefficients Pn,m in Eq.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method It is worth noting that all the coefficients Pn,m in Eq

Reference 5

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Observation 9961d02f-95a6-4731-a254-00d8b844c406 · outbound

This paper cites II A, if the logarithmic terms are absent, the results for the integrals in Eq.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method II A, if the logarithmic terms are absent, the results for the integrals in Eq

Reference 6

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Observation 99e17b57-5602-48c1-89c0-7ed2d5a9dd8a · outbound

This paper cites The coefficients yn,m can be determined by the metric functions A(r) and B(r), or by their ex- pansions in Eqs.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The coefficients yn,m can be determined by the metric functions A(r) and B(r), or by their ex- pansions in Eqs

Reference 7

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Observation aff698c8-1232-4f6c-8f4b-89dfb048d485 · outbound

This paper cites Due to the pres- ence of a nonzero ρ3, the metric functions for this model inherently contain logarithmic terms.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Due to the pres- ence of a nonzero ρ3, the metric functions for this model inherently contain logarithmic terms

Reference 8

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Observation 8ba5ccb0-070c-43d5-baa3-0a74ac6bc205 · outbound

This paper cites (62) and Eq.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method (62) and Eq

Reference 9

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Reference 10

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Observation ad35f17c-1124-4053-8709-32369d5531b8 · outbound

This paper cites (75) If γ ≤ 2, the mass function m(r) diverges as r → ∞, and the metric function B(r) and A(r) also blow up.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method (75) If γ ≤ 2, the mass function m(r) diverges as r → ∞, and the metric function B(r) and A(r) also blow up

Reference 11

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This paper cites Its density pro- file within the nonzero range takes the form of ρPIS(r) = ρcr2 m r2m + r2 , r ≤ R.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Its density pro- file within the nonzero range takes the form of ρPIS(r) = ρcr2 m r2m + r2 , r ≤ R

Reference 12

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This paper cites 1 rs,d + a1,0 + a1,1 ln rs,d 2v2r2 s,d + O ln2 rs,d r3 s,d !# =b±.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method 1 rs,d + a1,0 + a1,1 ln rs,d 2v2r2 s,d + O ln2 rs,d r3 s,d !# =b±

Reference 13

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Observation 53090f99-5857-4dc9-aff8-4de15d59bee7 · outbound

This paper cites Einstein, Science 84, 506 (1936).

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Einstein, Science 84, 506 (1936)

Reference 14

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Reference 15

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Observation 68365da5-2891-4600-a7a8-354aac4d2212 · outbound

This paper cites Bartelmann and P.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Bartelmann and P

Reference 16

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Observation be3fce7f-d219-4a1a-99ad-ab2bd8454b5f · outbound

This paper cites Collaboration et al., Astronomy and Astrophysics594, A15 (2016).

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Collaboration et al., Astronomy and Astrophysics594, A15 (2016)

Reference 17

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Observation 26b7b962-ca04-4905-8007-934b474d1913 · outbound

This paper cites Refregier, Annual Review of Astronomy and Astro- physics 41, 645 (2003).

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Refregier, Annual Review of Astronomy and Astro- physics 41, 645 (2003)

Reference 18

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Observation ad07c9d8-a5f8-443a-85cb-e22ce78f1bc8 · outbound

This paper cites Lewis and A.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Lewis and A

Reference 19

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Reference 20

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Observation 983f3b1d-0a9f-4c62-af9d-4d7d66312cb3 · outbound

This paper cites Refsdal, Monthly Notices of the Royal Astronomical Society 128, 307 (1964).

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Refsdal, Monthly Notices of the Royal Astronomical Society 128, 307 (1964)

Reference 21

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This paper cites Keeton and C.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Keeton and C

Reference 22

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Observation 35692e6a-c564-4996-8c4c-3b3fef2014c6 · outbound

This paper cites Falco, C.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Falco, C

Reference 23

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Observation 2347e289-d385-4abc-96e2-aba66a623ba0 · outbound

This paper cites Bartelmann and P.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Bartelmann and P

Reference 24

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Observation e843557c-7dff-4244-89a4-0764bb7b8632 · outbound

This paper cites Maoz and H.-W.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Maoz and H.-W

Reference 25

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Observation eff11de5-f77b-4b89-aee4-b1f311be39fa · outbound

This paper cites Kneib, R.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Kneib, R

Reference 26

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This paper cites Hoekstra, M.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Hoekstra, M

Reference 27

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Reference 28

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Reference 29

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Reference 30

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Observation 43a74779-9df5-4a79-813c-e36b5ab06aa2 · outbound

This paper cites Joyce, L.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Joyce, L

Reference 31

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This paper cites Perlick, Living reviews in relativity 7, 1 (2004).

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Perlick, Living reviews in relativity 7, 1 (2004)

Reference 32

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This paper cites Bozza, F.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Bozza, F

Reference 33

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This paper cites Pugliese, H.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Pugliese, H

Reference 34

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Reference 35

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From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Pugliese, H

Reference 36

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This paper cites Abdujabbarov and B.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Abdujabbarov and B

Reference 37

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This paper cites Al Zahrani, V.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Al Zahrani, V

Reference 38

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This paper cites Circular orbits and related quasi-harmonic oscillatory motion of charged particles around weakly magnetized rotating black holes.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Circular orbits and related quasi-harmonic oscillatory motion of charged particles around weakly magnetized rotating black holes

Reference 39

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This paper cites Deflection angle with electromagnetic interaction and gravitational-electromagnetic dual lensing.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Deflection angle with electromagnetic interaction and gravitational-electromagnetic dual lensing

Reference 40

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This paper cites Gravitational lensing in dispersive media and deflection angle of charged massive particles in terms of curvature scalars and energy-momentum tensor.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Gravitational lensing in dispersive media and deflection angle of charged massive particles in terms of curvature scalars and energy-momentum tensor

Reference 41

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This paper cites A Universal Density Profile from Hierarchical Clustering.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method A Universal Density Profile from Hierarchical Clustering

Reference 42

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From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Hernquist, Astrophys

Reference 43

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Reference 44

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Observation 5924a9d5-f8fd-4a2d-b893-e1aaeb09098d · outbound

This paper cites Perturbative deflection angle for signal with finite distance and general velocities.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Perturbative deflection angle for signal with finite distance and general velocities

Reference 45

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Observation ed60d050-2454-4aab-b569-bb243bef9440 · outbound

This paper cites The perturbative approach for the weak deflection angle.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The perturbative approach for the weak deflection angle

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-09T13:42:06.073121Z

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Observation 91099036-d46e-4473-a378-c8db146ca0e5 · outbound

This paper cites Gravitational lensing of massive particles in Schwarzschild gravity.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Gravitational lensing of massive particles in Schwarzschild gravity

Reference 47

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This paper cites Narayan and S.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Narayan and S

Reference 48

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T13:42:06.342463Z

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Reference 49

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Reference 50

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Reference 51

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This paper cites The Fundamental Plane of Gravitational Lens Galaxies and The Evolution of Early-Type Galaxies in Low Density Environments.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The Fundamental Plane of Gravitational Lens Galaxies and The Evolution of Early-Type Galaxies in Low Density Environments

Reference 52

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 3d093469-e4b4-45b4-8b9d-45dff9432600 · outbound

This paper cites The Evolution of a Mass-Selected Sample of Early-Type Field Galaxies.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The Evolution of a Mass-Selected Sample of Early-Type Field Galaxies

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-08-09T13:42:05.948143Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation b8cccc90-646b-40be-aecf-168fa5c5631a · outbound

This paper cites Analytical Models For Galactic Nuclei.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Analytical Models For Galactic Nuclei

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.440208Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d389f43e-b5d3-4a7f-abb1-9a2a7ea1c211 · outbound

This paper cites Determination of the Local Dark Matter Density in our Galaxy.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Determination of the Local Dark Matter Density in our Galaxy

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.445907Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e620fd62-c81e-4d47-9589-8add85a8c5fa · outbound

This paper cites an unresolved cited work.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Unresolved cited work

Reference 56

Resolution: verified exact; raw_fallback, observed 2026-08-09T13:42:05.914839Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 2f70068f-eaae-4560-859e-8fb402b3261b · outbound

This paper cites Zhao, Monthly Notices of the Royal Astronomical So- ciety 278, 488 (1996).

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Zhao, Monthly Notices of the Royal Astronomical So- ciety 278, 488 (1996)

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T13:42:06.311432Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 74612618-2c72-4f6c-917c-e7600c7412a6 · outbound

This paper cites Kazantzidis, J.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Kazantzidis, J

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T13:42:06.301683Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation c9ff1738-4cbd-4042-9e2e-7c6ebd7cf9f6 · outbound

This paper cites Investigation of Gravitational Lens Mass Models.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Investigation of Gravitational Lens Mass Models

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-08-09T13:42:05.778539Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 34c86dd6-fea6-4eee-bb45-57dfffeb11af · outbound

This paper cites The Optical Properties of Gravitational Lens Galaxies as a Probe of Galaxy Structure and Evolution.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The Optical Properties of Gravitational Lens Galaxies as a Probe of Galaxy Structure and Evolution

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.464423Z

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Unavailable: canonical work link unavailable.

Observation 7723a279-1ee6-40a0-9849-84b4851e7086 · outbound

This paper cites The statistics of wide-separation lensed quasars.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The statistics of wide-separation lensed quasars

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-08-09T13:42:05.754686Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation bb3231d8-adad-4467-b6d0-812a50c12fd7 · outbound

This paper cites Effects on the local dark matter distribution due to the Large Magellanic Cloud.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Effects on the local dark matter distribution due to the Large Magellanic Cloud

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.471742Z

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Unavailable: canonical work link unavailable.

Observation 68bdfbea-5709-4057-9098-52db3c95a1aa · outbound

This paper cites an unresolved cited work.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Unresolved cited work

Reference 63

Resolution: unresolved; raw_fallback, observed 2026-08-09T13:42:06.291942Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation bc530b12-e132-44cc-b1b4-40eca2b78e36 · outbound

This paper cites Modelling mass distribution in elliptical galaxies: mass profiles and their correlation with velocity dispersion profiles.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Modelling mass distribution in elliptical galaxies: mass profiles and their correlation with velocity dispersion profiles

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-08-09T13:42:05.729719Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 50999a0e-308c-4948-8124-c8c50d0eee04 · outbound

This paper cites The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.483124Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71a7c9e7-8b17-4957-a0ef-345aa5c26551 · outbound

This paper cites Galaxy Masses.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Galaxy Masses

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.486748Z

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Unavailable: canonical work link unavailable.

Observation 30d26fa0-8fe9-4dc6-aba1-ad1683b584b0 · outbound

This paper cites The Halo Boundary of Galaxy Clusters in the SDSS.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The Halo Boundary of Galaxy Clusters in the SDSS

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.490993Z

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Unavailable: canonical work link unavailable.

Observation 75e705f5-a7ae-4f1d-a7a0-27e26a5fb5c7 · outbound

This paper cites Improved Modeling of the Mass Distribution of Disk Galaxies by the Einasto Halo Model.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Improved Modeling of the Mass Distribution of Disk Galaxies by the Einasto Halo Model

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-08-09T13:42:05.688618Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 7a5af796-c7bc-4bfd-b557-3ae2da0bc060 · outbound

This paper cites Formation of Galaxy Clusters.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Formation of Galaxy Clusters

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.498160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7cc22d17-8f68-4dba-b215-46bc855e778c · outbound

This paper cites The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.501847Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 715e1f71-c230-4795-8412-6ba5d11344a3 · outbound

This paper cites CLASH: The Concentration-Mass Relation of Galaxy Clusters.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method CLASH: The Concentration-Mass Relation of Galaxy Clusters

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.505289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7b41babf-8546-4550-b8ab-496903e79360 · outbound

This paper cites The Structure of Cold Dark Matter Halos.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The Structure of Cold Dark Matter Halos

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.508994Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3fe70a9a-3391-49ad-8ada-ade860eef82a · outbound

This paper cites an unresolved cited work.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Unresolved cited work

Reference 73

Resolution: unresolved; raw_fallback, observed 2026-08-09T13:42:06.281422Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 56302109-3f74-43a1-b465-cff0c4c79a71 · outbound

This paper cites The effect of the deforming dark matter haloes of the Milky Way and the Large Magellanic Cloud on the Orphan-Chenab stream.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method The effect of the deforming dark matter haloes of the Milky Way and the Large Magellanic Cloud on the Orphan-Chenab stream

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.515728Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f0d1f07f-20aa-471c-8f12-c6ca3108d3a0 · outbound

This paper cites Exploration of a Singular Fluid Spacetime.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Exploration of a Singular Fluid Spacetime

Reference 75

Resolution: verified exact; local_arxiv, observed 2026-08-09T13:42:05.626676Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation e0209a98-2ea2-4ec4-abab-50c656d48f09 · outbound

This paper cites Bollati, A.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Bollati, A

Reference 76

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T13:42:06.269740Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 8b274746-5d09-4bf0-b606-906d2a54612a · outbound

This paper cites Begeman, A.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Begeman, A

Reference 77

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T13:42:06.258891Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation c8686e8a-2a7c-4604-ac98-3bba87db4307 · outbound

This paper cites an unresolved cited work.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Unresolved cited work

Reference 78

Resolution: unresolved; raw_fallback, observed 2026-08-09T13:42:06.247935Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation bc6d4c5d-9a25-4603-b3be-86af62c6d6bc · outbound

This paper cites Galaxy Mass Models: MOND versus Dark Matter Halos.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Galaxy Mass Models: MOND versus Dark Matter Halos

Reference 79

Resolution: metadata mismatch; local_arxiv, observed 2026-08-09T13:42:05.612728Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 9d59efab-e40d-4009-bb8c-0cfb4013cfe8 · outbound

This paper cites Burkert, The Astrophysical Journal 447, L25 (1995).

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Burkert, The Astrophysical Journal 447, L25 (1995)

Reference 80

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T13:42:06.236318Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation be291703-04f9-4034-896f-b4608443a7d9 · outbound

This paper cites VERITAS Search for VHE Gamma-ray Emission from Dwarf Spheroidal Galaxies.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method VERITAS Search for VHE Gamma-ray Emission from Dwarf Spheroidal Galaxies

Reference 81

Resolution: verified exact; local_arxiv, observed 2026-08-09T13:42:05.597995Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation c7dc2308-2c8a-4c26-afd8-93ff1cd8bd9c · outbound

This paper cites Bozza, Physical Review D 66, 103001 (2002).

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Bozza, Physical Review D 66, 103001 (2002)

Reference 82

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T13:42:06.226043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation d68febf3-849a-4150-839b-884b85afa746 · outbound

This paper cites Schwarzschild black hole lensing.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Schwarzschild black hole lensing

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.548412Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4657377a-aac3-4388-972e-661d2c2a71b9 · outbound

This paper cites an unresolved cited work.

From Matter Density to Deflection Angle and Gravitational Lensing Using a Perturbative Method Unresolved cited work

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-09T13:42:05.552141Z

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