Pith. sign in

Paper Citation Record · LEDGER

MEGA Mass Assembly with JWST: The MIRI EGS Galaxy and AGN Survey

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2503.19078.

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

pith.paper-citation-record.v1
2503.19078 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:20:27.827625Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation abe954a3-4fe0-4258-a04a-8cbdd7000963 · inbound

The Identification of Two JWST/NIRCam-Dark Starburst Galaxies at $z=6.6$ with ALMA cites this paper.

The Identification of Two JWST/NIRCam-Dark Starburst Galaxies at $z=6.6$ with ALMA MEGA Mass Assembly with JWST: The MIRI EGS Galaxy and AGN Survey

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-07T06:00:04.378840Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T06:00:04.378840Z digest=sha256:dc8a193aef2a6b2824d3154e1d7b56bf8cbf1d1dbdb6cae5f8c5a64f06312beb

Observation d6c6399e-7b42-4d57-9f1d-6a84e76b0fc6 · inbound

MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant Universe cites this paper.

MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant Universe MEGA Mass Assembly with JWST: The MIRI EGS Galaxy and AGN Survey

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-06T14:12:18.002881Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T14:12:18.002881Z digest=sha256:add1562580bffc5a62ada0f43507bb81b5596e45082cfcfc6f5bd28fb278b2f2

Observation b9cef6a2-a53f-45a7-b4ae-8d4cc17958e3 · inbound

NOEMA$^\rm{3D}$: A deep view of cold gas flows in a barred spiral galaxy at $z\sim1$ cites this paper.

NOEMA$^\rm{3D}$: A deep view of cold gas flows in a barred spiral galaxy at $z\sim1$ MEGA Mass Assembly with JWST: The MIRI EGS Galaxy and AGN Survey

Reference 239

Resolution
verified exact
arxiv_id, observed 2026-06-28T13:42:15.512867Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-06-28T13:41:32.806663Z digest=sha256:9875d3fffbc3578a2958406d961de6731c9f14b408662d5f3592b0e5571555c5

Observation 2ddbbeb0-0930-4e5c-9d26-2bde70a99e86 · inbound

MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon cites this paper.

MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon MEGA Mass Assembly with JWST: The MIRI EGS Galaxy and AGN Survey

Reference 17

Resolution
verified exact
arxiv_id, observed 2026-06-27T03:40:28.348085Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-06-27T03:22:47.800684Z digest=sha256:af930ba9a95cb3b9ffd5a3c68342dd604eefe3ef24f607f3e053a52fd54d8353

Observation c0018d40-3188-41a1-a86c-da6af15cd157 · inbound

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf cites this paper.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf MEGA Mass Assembly with JWST: The MIRI EGS Galaxy and AGN Survey

Reference 121

Resolution
unresolved
no resolver link, observed 2026-08-10T04:20:27.827625Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T04:20:27.827625Z digest=sha256:b41a0f1ab05ffe3636a5f54769972af24aa2e019848215cea5bea718ad398c32