Pith. sign in

Paper Citation Record · LEDGER

The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars

As of 25 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1612.03728.

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

pith.paper-citation-record.v1
1612.03728 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-07-24T06:31:00.690269+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T03:29:42.101488Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T00:46:40.230706Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 6632b1ba-18d3-4fb7-917d-47a4c8f42a42 · inbound

Nested Fermi and eROSITA bubbles require very similar $\sim10^{56}$ erg collimated Galactic-center outbursts; their asymmetry indicates an eastern density gradient cites this paper.

Nested Fermi and eROSITA bubbles require very similar $\sim10^{56}$ erg collimated Galactic-center outbursts; their asymmetry indicates an eastern density gradient The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars

Reference 7

Resolution
verified exact
local_arxiv, observed 2026-05-16T09:10:47.194628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.

source=pdf_text observed=2026-05-16T09:10:43.109855Z digest=sha256:493cfeb21d9e15892008a2e9163cf3bd5ecba544493cc4cfbcffc235dc59696c

Observation b0f3509f-710f-4865-b9d9-4c0b88e532d3 · inbound

The X-ray-to-UV relation does not evolve in homogeneous quasar samples cites this paper.

The X-ray-to-UV relation does not evolve in homogeneous quasar samples The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars

Reference 201

Resolution
verified exact
local_arxiv, observed 2026-06-27T21:01:15.766660Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c65a5b0f07b1c9255391bccaf6d1e981cb31aa447aaa5b5d110cbe9d7de2e372

Observation bae1c83b-1d20-4b2f-9ee2-106f001f7ec1 · inbound

SUNRISE-3D: Sharp UNveiling of AGN feedback Regulation and its Impact on Star-formation at the cosmic noon Epoch cites this paper.

SUNRISE-3D: Sharp UNveiling of AGN feedback Regulation and its Impact on Star-formation at the cosmic noon Epoch The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars

Reference 1

Resolution
verified exact
local_arxiv, observed 2026-07-01T01:35:13.170456Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:58eeb27abf8baab1edc098451dfe05d781d94bea3491a041cde28a0d34ce2d2c

Observation 8cf30a58-3590-4991-b5ce-a1a707502a1e · inbound

Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference cites this paper.

Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars

Reference 73

Resolution
unresolved
no resolver link, observed 2026-07-12T03:29:42.101488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T03:29:42.101488Z digest=sha256:6e2ccaaf93fc91e99426be885bd49a63640ea194a040c72cee5921f027dbc797

Observation 158c5772-bec2-4254-8815-d2aa4b2ab918 · inbound

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ cites this paper.

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars

Reference 119

Resolution
unresolved
no resolver link, observed 2026-07-11T06:23:06.110361Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:23:06.110361Z digest=sha256:72ffa4acea6d4fe3fcf9ab3c3e4882b3f9ef85d9415720231315ec2c662d08ae

Observation 05e4c51b-9724-43bd-abf2-efc046787795 · inbound

First detection of ultra-fast outflows in a quiescent galaxy cites this paper.

First detection of ultra-fast outflows in a quiescent galaxy The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars

Reference 300

Resolution
verified exact
local_arxiv, observed 2026-07-10T00:46:40.232099Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:75fb5099c5ef6be95ecb40ec4eba5b7b2074ad30e3b277f1d19863718a99b9c5