Pith. sign in

Paper Citation Record · LEDGER

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics

As of 19 August 2026, this Paper Citation Record lists 40 of 40 outbound references and 2 inbound Pith citation observations for arXiv:2502.02246.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2502.02246 v3

Coverage vector

measured 40 of 40 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-09T12:55:47.940004Z

measured 42 of 42 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T12:04:06.876717Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-23T04:32:31.999451Z

Reference resolution

40 of 40 outbound references displayed

  • verified exact0
  • verified fuzzy8
  • unresolved32
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 5f748d72-543a-475f-bbb6-70977938b8f2 · outbound

This paper cites an unresolved cited work.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

Reference 1

Resolution
unresolved
raw_fallback, observed 2026-08-09T12:55:48.825675Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.802291Z digest=sha256:b4731187c1d3b8e5c8d026d4b0c9b8c75f4672edddf3847dad409294ed9f0ec5

Observation 736eb0ed-c002-47e2-8ef1-33c5ddd778f5 · outbound

This paper cites One simple solution for low redshift galaxy distributions is to use the same specification as for sources.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics One simple solution for low redshift galaxy distributions is to use the same specification as for sources

Reference 2

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T12:55:48.815287Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.806404Z digest=sha256:8e8e39b54dedc027e55cffc2afcd7acb709ac7e940b066590ae959c3b0be285e

Observation 51a426c2-6e29-4145-b565-b2f41036c281 · outbound

This paper cites The binning is opti- mized for different values of the photometric redshift uncer- taintyσz.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics The binning is opti- mized for different values of the photometric redshift uncer- taintyσz

Reference 3

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T12:55:48.728413Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.836373Z digest=sha256:3ed773f84b4290a4f831606d775a5f4212e0de3c5096d7320d8d832d7d5bfb35

Observation fc4ad3cd-67c4-4c90-81b0-7c2537f49cac · outbound

This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.851494Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.851494Z digest=sha256:c5898d5d1d811ea3482c4a250acc5fbb1e3afbfd6a6f411fb50cbefee5ca9786

Observation 22079c61-7a87-4638-94f0-34ca92f242ed · outbound

This paper cites (A2) For simplicity, we will drop the tilde in the main text.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics (A2) For simplicity, we will drop the tilde in the main text

Reference 5

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T12:55:48.793796Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.814762Z digest=sha256:682ab7501209266540e6182ff87594d07a5c7e6cacb56aa5ce724d01af93be7b

Observation bb8bee30-7790-44d7-975b-d1277c9c0902 · outbound

This paper cites an unresolved cited work.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

Reference 6

Resolution
unresolved
raw_fallback, observed 2026-08-09T12:55:48.783610Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.818348Z digest=sha256:a0851d10779ee34b0bcbd7defa68a4b0229b41602884a01a5061e964dd9348c8

Observation 5ef80445-5521-4f1a-9f98-f539014ed232 · outbound

This paper cites an unresolved cited work.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

Reference 7

Resolution
unresolved
raw_fallback, observed 2026-08-09T12:55:48.772334Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.821976Z digest=sha256:5b2974896e3f14da9786a0b0234d018e3f2ca57e0e8d2aaeb19ef1ab6109adda

Observation d0f574d5-0961-492b-a37a-a3c4b09e930d · outbound

This paper cites This procedure is purely geometri- cal and thus scale-independent and independent of the power spectrum or matter density contrast.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics This procedure is purely geometri- cal and thus scale-independent and independent of the power spectrum or matter density contrast

Reference 8

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T12:55:48.836405Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.797715Z digest=sha256:d9378fbeae18a4bb6f369422b3c7f4f92e0510721f0b94fa13661b52352a2aee

Observation 095d31b6-622b-47bf-b6b5-b96ae5dc478c · outbound

This paper cites Specifically, we require ˆwa(z) ⩽ 0.1× max( ˆwa(z))≈ 0.02 for z ⩽ z ˆw(a), where we take 0.2 as an approximated common maximum value across all nulled lensing kernels.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Specifically, we require ˆwa(z) ⩽ 0.1× max( ˆwa(z))≈ 0.02 for z ⩽ z ˆw(a), where we take 0.2 as an approximated common maximum value across all nulled lensing kernels

Reference 9

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T12:55:48.761220Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.825747Z digest=sha256:c7dfedb9288e1f2230c0d791717f84e755a43d7377b7556ec52e0024e9f1babf

Observation dbbe45c6-20af-412d-ae70-9a1e69d32e9a · outbound

This paper cites Specifically, we require na−3(z ˆw(a)) ⩽ 0.1× n(z), to ensure that the overlap between na−3(z) and ˆwa(z) con- tributes negligibly to the signal.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Specifically, we require na−3(z ˆw(a)) ⩽ 0.1× n(z), to ensure that the overlap between na−3(z) and ˆwa(z) con- tributes negligibly to the signal

Reference 10

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T12:55:48.750403Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.829314Z digest=sha256:a1efca9458ff6f3d62d3c9e7fcc45cefd02702a3bf22b0ce6a720dc628e972b1

Observation e3b43209-601e-4022-b917-22e613f5592e · outbound

This paper cites an unresolved cited work.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

Reference 11

Resolution
unresolved
raw_fallback, observed 2026-08-09T12:55:48.738928Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.832679Z digest=sha256:03dfb529c3db1984e894a92fb0bd2e64914ff1b210887f7ec01c0c8b024c018d

Observation c191010f-4f88-419f-acea-40ce699ffd17 · outbound

This paper cites The Kilo-Degree Survey.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics The Kilo-Degree Survey

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.839871Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.839871Z digest=sha256:eda35d0ff050f61ce6ee17faaa0612ee3b1cf6959255750334b9e931f238c1ae

Observation 6d1d3d24-b511-4a33-959b-e3c9b3de9a31 · outbound

This paper cites KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.843497Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.843497Z digest=sha256:c8e21a86b63634832747e6cf7e161e47c18f36980515388950f3c24e93e633cb

Observation 6b8c9672-1dfd-4f42-b467-29726471ba10 · outbound

This paper cites The Dark Energy Survey.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics The Dark Energy Survey

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.847749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.847749Z digest=sha256:0c2f9c3dbf1513577ea585b6f3fdf6f4383bf4b958676fec1d426949dfc03fa5

Observation 6a229f70-d015-429e-a763-af8426b16ac4 · outbound

This paper cites pre-factor unity approximation.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics pre-factor unity approximation

Reference 15

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T12:55:48.804641Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.810205Z digest=sha256:765b8f7c8510c1a28acdc1b644f2ff2c50e00c05ee62c7a52c08b29f5fdd2f96

Observation 7ca583ec-7712-40cc-90f3-5f690008a7d5 · outbound

This paper cites Large Synoptic Survey Telescope: Dark Energy Science Collaboration.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Large Synoptic Survey Telescope: Dark Energy Science Collaboration

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.855301Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.855301Z digest=sha256:0e9267ca0823ab5017bfb25e4639bd6957c5e716491bc3c9ea663832973c085a

Observation 1eb9323a-8061-424f-9689-01e807cbea46 · outbound

This paper cites Mellier et al.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Mellier et al

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.859297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.859297Z digest=sha256:66d0d13f0d9b02959a4bcc365cc8927903089d9cad432d45681a7b3829384dec

Observation d69a906f-7290-4e3c-b844-13e332b3d289 · outbound

This paper cites Power Spectrum Tomography with Weak Lensing.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Power Spectrum Tomography with Weak Lensing

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.862610Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.862610Z digest=sha256:2da33d7310e3c5b5508a7ef8bde041fb8d4a4971b3bb9ef8bf7ec8c48ae39fb8

Observation c0b6aa2f-1bc0-4071-a21e-ac232c5b6203 · outbound

This paper cites Cosmic shear full nulling: sorting out dynamics, geometry and systematics.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Cosmic shear full nulling: sorting out dynamics, geometry and systematics

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.866420Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.866420Z digest=sha256:910b090074b74dd4e1dd8af23507b1348e382381872a5cd62c994064d491353d

Observation 13831607-3175-44b3-a60c-361ac0da02a7 · outbound

This paper cites x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.870316Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.870316Z digest=sha256:2a2284d2ce0cb6e0e2b3e9f7e2079e2315eac880ecd5f811448366acaa7acec3

Observation b9ef5b4a-1b26-498c-8fd9-ba2674a1a447 · outbound

This paper cites Observing Baryonic Acoustic Oscillations in tomographic cosmic shear surveys.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Observing Baryonic Acoustic Oscillations in tomographic cosmic shear surveys

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.873808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.873808Z digest=sha256:6544b2adaf4159c1f710489d1ba905cc3687f10045b1b11c8a46cbd43e5bf013

Observation a6fb5e18-fc5d-4968-b905-a1eecd3df173 · outbound

This paper cites Constraining Cosmology With the CMB $\times$ LIM-Nulling Convergence.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Constraining Cosmology With the CMB $\times$ LIM-Nulling Convergence

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.877313Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.877313Z digest=sha256:2c772ac69ffd6717b1e5acb4ac77cb0cc88018cf04c328a0cc6f9b1216801e25

Observation 33137865-d991-4e6d-8d2a-c79d191b2942 · outbound

This paper cites A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.880956Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.880956Z digest=sha256:a5db91a35d18248fef8a5776b510bd690e2c443b7fb14a1cd35c5b420e8aacc4

Observation f24286d2-475b-4db8-afb1-b45581c7ef88 · outbound

This paper cites Controlling intrinsic alignments in weak lensing statistics: The nulling and boosting techniques.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Controlling intrinsic alignments in weak lensing statistics: The nulling and boosting techniques

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.884407Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.884407Z digest=sha256:78e38fdb79ec168b1205e307c68d1467f2d534b6c8e731d694d24d6a445abf0e

Observation 2e24f19d-4c44-45dd-9da3-e58aed7c2b31 · outbound

This paper cites Cosmological lensing ratios with DES Y1, SPT and Planck.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Cosmological lensing ratios with DES Y1, SPT and Planck

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.888160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.888160Z digest=sha256:f9b5f9605f26e8b8ec707c9ad9993e46bfa4fae9033607fe714006aa3b85c7c4

Observation 64776b1c-9e37-4583-915a-6233e4539f93 · outbound

This paper cites Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.891675Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.891675Z digest=sha256:1809d0a81b67037e40b999c31aa95a5a0bd28bac0136ea493d6696c5c7cc67b1

Observation 7c5f45b2-0164-4370-8c5b-387b07ce6097 · outbound

This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.895384Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.895384Z digest=sha256:aa9c9928cc4e576be8727f3c5d413ed0bd8bdc2f654b65e5915bb68bd08045f3

Observation 59334726-e935-46f5-a885-152fb3a75a78 · outbound

This paper cites Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.898728Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.898728Z digest=sha256:c8b556ced137683c501d98ea46a8b3f780cc4a9d790391868376bbc80ab6f43d

Observation ebafa744-030d-45f0-8eba-0470bca164c8 · outbound

This paper cites Kaiser, Weak gravitational lensing of distant galaxies, As- trophys.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Kaiser, Weak gravitational lensing of distant galaxies, As- trophys

Reference 29

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T12:55:48.716439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-09T12:55:47.902304Z digest=sha256:a2c5134d5aa9c23e420804c2529acbf05a02db97bf378757b2f6514528fb553f

Observation 6e7f3c71-62fd-4550-828f-f3e2a57ad477 · outbound

This paper cites Revising the Halofit Model for the Nonlinear Matter Power Spectrum.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Revising the Halofit Model for the Nonlinear Matter Power Spectrum

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.905601Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.905601Z digest=sha256:a672b73ed34dd6f67c40807b6331007ed5300f534556e122499c72e5f3a99451

Observation ac1348f0-bd31-462d-a10b-9c7cd61f4803 · outbound

This paper cites Stable clustering, the halo model and nonlinear cosmological power spectra.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Stable clustering, the halo model and nonlinear cosmological power spectra

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.908917Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.908917Z digest=sha256:e1056ecb3b68e8e3dd8eaa30f8a4c674e0ce8f23b4ac76270cec770c8bf6dd80

Observation 0d67cf4c-4bcc-49e5-b133-fe7d26ca7f83 · outbound

This paper cites Planck 2018 results. I. Overview and the cosmological legacy of Planck.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Planck 2018 results. I. Overview and the cosmological legacy of Planck

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.912330Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.912330Z digest=sha256:9d28d533d9f6f9f03e8a06bcb94a4cba66341f0e5da8acd14ece1a3641a74f3a

Observation 9094f4f3-7674-4ed3-b9f3-d09ad57f05d1 · outbound

This paper cites Euclid preparation: VII. Forecast validation for Euclid cosmological probes.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Euclid preparation: VII. Forecast validation for Euclid cosmological probes

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.915891Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.915891Z digest=sha256:3d539737209e92aef1cc60b38daa06361e7a32f4b7382d102053a51575c56145

Observation dc450b70-7630-4c89-9955-282a076b5052 · outbound

This paper cites Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.919318Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.919318Z digest=sha256:4b772056c5dcd264bc274bae4920e7e790b378ac1b3dea0c48f842ede342b446

Observation 7c6d36b5-a57c-4d1a-86bd-8fbd4ef52a42 · outbound

This paper cites Determination of Inflationary Observables by Cosmic Microwave Background Anisotropy Experiments.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Determination of Inflationary Observables by Cosmic Microwave Background Anisotropy Experiments

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.923053Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.923053Z digest=sha256:d7984286e5742c4cbf3e43552644c785e05ab73fd319ca266b508b9ffe673676

Observation 889d050d-4645-4d70-bdfe-cd5c8a9e2673 · outbound

This paper cites The Limits of Cosmic Shear.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics The Limits of Cosmic Shear

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.926373Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.926373Z digest=sha256:d0f176666fb24b2a3448d081f091feeac5a0d38aac6e20d6b36ba9c67b09ed98

Observation 15716fa1-c7bc-4552-8ac8-c7d0a231e5c0 · outbound

This paper cites Precision calculations of the cosmic shear power spectrum projection.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Precision calculations of the cosmic shear power spectrum projection

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.929842Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.929842Z digest=sha256:62b759a14335b0f00d110a871c00d4ee83ce9fa72154980ee0b83155376bc31e

Observation 043877b2-57be-434d-95ee-8e886f77dcc1 · outbound

This paper cites an unresolved cited work.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.933304Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.933304Z digest=sha256:0dcb45bcde5bc5dbd95add7760ed1bea5330b59dd33af9f5a05e374c431a5f50

Observation a9c9d668-0c94-4ffc-b684-a3276fbe080d · outbound

This paper cites A Fitting Formula for the Non-Linear Evolution of the Bispectrum.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics A Fitting Formula for the Non-Linear Evolution of the Bispectrum

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.936428Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.936428Z digest=sha256:98c38d47914513d75a4afadaf888b2d5d4282bf4584a28f89850db630df7b778

Observation 8ef0b689-b5fe-4478-804a-da40676710d1 · outbound

This paper cites Cobaya: Code for Bayesian Analysis of hierarchical physical models.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Cobaya: Code for Bayesian Analysis of hierarchical physical models

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-09T12:55:47.940004Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:55:47.940004Z digest=sha256:f5ff664a3c8adebe3dd98caa74f7c3a26c62cc3c326a14802e3cb87851d30d9e

Pith citing papers

Observation e14bc32a-5c18-4498-9c4c-186245e6d632 · inbound

Mitigating Nonlinear Systematics in Weak Lensing Surveys: The Bernardeau-Nishimichi-Taruya Approach cites this paper.

Mitigating Nonlinear Systematics in Weak Lensing Surveys: The Bernardeau-Nishimichi-Taruya Approach Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-11T12:04:06.876717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T12:04:06.876717Z digest=sha256:f8f284b360812e3a3059b7ed5929567119e0f13f13c6b9963a119d3dba4e130c

Observation c04b687f-8582-4c03-a915-647dca75840d · inbound

Novel geometrical test of cosmological expansion from photometric data cites this paper.

Novel geometrical test of cosmological expansion from photometric data Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics

Reference 2

Resolution
verified exact
arxiv_id, observed 2026-06-12T02:09:04.973400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-05-23T04:32:26.187684Z digest=sha256:6803669bd5279cb1da39ccbd6a64065a9a8b99567993b0659043616b2537756b