A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf | Paper Citation Record

Observation 5144e888-8eca-46d0-bd54-ce7124736e3e · outbound

This paper cites , keywords =.

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

Reference 1

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Observation ff9cc5c1-d667-418a-aa91-c179f2ac02b2 · outbound

This paper cites an unresolved cited work.

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

Reference 2

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Observation f4a3f943-f848-4639-8f49-410ff8ecae58 · outbound

This paper cites CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results

Reference 3

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Observation e24780a9-0ffa-4ed2-8fdf-30605df7d330 · outbound

This paper cites The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey

Reference 4

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Observation eb7dea14-4b5d-4c36-8eb4-9a4549efd8e1 · outbound

This paper cites Bright z~9 Galaxies in Parallel: The Bright End of the Rest-UV Luminosity Function from HST Parallel Programs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Bright z~9 Galaxies in Parallel: The Bright End of the Rest-UV Luminosity Function from HST Parallel Programs

Reference 5

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Observation 4ec7db51-367c-4ec8-a1ec-4512806d77b1 · outbound

This paper cites , keywords =.

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

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.134565Z

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Observation 8ee8b16a-8652-40ec-a863-ee2ab3e19788 · outbound

This paper cites Two Exciting High-redshift Galaxy Candidates Turn Out to Be Two Exciting Ultra-cool Brown Dwarfs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Two Exciting High-redshift Galaxy Candidates Turn Out to Be Two Exciting Ultra-cool Brown Dwarfs

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.139618Z

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Observation 43395e25-4c95-490d-85c3-a8383aabf397 · outbound

This paper cites The evolution of [OIII]$+\rm{H}\beta$ equivalent width from $\mathbf{z\simeq3-8}$: implications for the production and escape of ionizing photons during reionization.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The evolution of [OIII]$+\rm{H}\beta$ equivalent width from $\mathbf{z\simeq3-8}$: implications for the production and escape of ionizing photons during reionization

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.146470Z

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Observation 2a6ff666-1ebc-4764-a119-43e08d1a152b · outbound

This paper cites The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.154655Z

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Observation 105ad807-b32a-448d-8909-6ad162ea52ef · outbound

This paper cites The galaxy luminosity function at z ~ 6 and evidence for rapid evolution in the bright end from z ~ 7 to 5.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The galaxy luminosity function at z ~ 6 and evidence for rapid evolution in the bright end from z ~ 7 to 5

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.161279Z

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Observation 25baee46-e2b4-4f63-8e70-49dd811accf4 · outbound

This paper cites A lack of evolution in the very bright-end of the galaxy luminosity function from z = 8-10.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf A lack of evolution in the very bright-end of the galaxy luminosity function from z = 8-10

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.166828Z

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Observation a6ce54df-2486-4b3a-8fb0-7ce59d11649b · outbound

This paper cites Spectroscopic confirmation of two luminous galaxies at $z\sim14$.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Spectroscopic confirmation of two luminous galaxies at $z\sim14$

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.173174Z

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Observation 77e05c43-b459-422e-8fca-f74d77e3797a · outbound

This paper cites , keywords =.

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

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.179551Z

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Observation aeef09d1-dbc9-4b11-a1e4-255a4ed6b834 · outbound

This paper cites The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.184841Z

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Observation 650ac4a3-74b8-40a4-9ea7-116b443a9f6b · outbound

This paper cites JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\mathbf{z \simeq 9-15}$.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\mathbf{z \simeq 9-15}$

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.191106Z

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Observation 435ebec4-1148-4e85-9356-b403ff661271 · outbound

This paper cites , keywords =.

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

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.197182Z

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Observation ddda7a84-efee-4945-8637-679cf8016e55 · outbound

This paper cites an unresolved cited work.

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

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.202497Z

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Observation b6f9065a-d076-4d75-ab59-f9f5ea0bc7e5 · outbound

This paper cites Overview of the JWST Advanced Deep Extragalactic Survey (JADES).

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Overview of the JWST Advanced Deep Extragalactic Survey (JADES)

Reference 18

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Observation 41e801e8-7e9d-4b66-b7a0-f57bd359e7fe · outbound

This paper cites A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.213392Z

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Observation af3f4c6d-1b40-4b5d-b373-04416262a267 · outbound

This paper cites CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.219570Z

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Observation 3cbf5152-ab4a-49a0-b88b-cb399a77c71e · outbound

This paper cites The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.225190Z

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Observation c887a646-0d09-4a6c-b68c-e8e4b680b230 · outbound

This paper cites Physical properties of galaxies and the UV Luminosity Function from $z\sim6$ to $z\sim14$ in COSMOS-Web.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Physical properties of galaxies and the UV Luminosity Function from $z\sim6$ to $z\sim14$ in COSMOS-Web

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.230026Z

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Observation cc46524e-88e1-49bc-8d7b-2d35db143817 · outbound

This paper cites , keywords =.

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

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.236305Z

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Observation e99e0ac8-ec5f-4f31-bbc2-f3cd0b468d50 · outbound

This paper cites JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.241249Z

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Observation 66ca2166-c535-4a24-b07a-91dbe334b379 · outbound

This paper cites JADES: An Abundance of Ultra-Distant T- and Y-Dwarfs in Deep Extragalactic Data.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf JADES: An Abundance of Ultra-Distant T- and Y-Dwarfs in Deep Extragalactic Data

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.246251Z

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Observation 120fb685-cf89-41e4-987c-0dbb22ebdf85 · outbound

This paper cites A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.252784Z

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Observation 5317d584-f7d3-4d73-8448-f74dc5ff44c6 · outbound

This paper cites , keywords =.

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

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.258288Z

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Observation 724901f7-2e08-4702-aac9-92d07952af2f · outbound

This paper cites New redshift z ~ 9 galaxies in the Hubble Frontier Fields: Implications for early evolution of the UV luminosity density.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf New redshift z ~ 9 galaxies in the Hubble Frontier Fields: Implications for early evolution of the UV luminosity density

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.263130Z

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Observation 6e281d1c-7c90-434c-93f0-4415b02072c7 · outbound

This paper cites The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: The z=9 LF and further evidence for a smooth decline in UV luminosity at z >= 8.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: The z=9 LF and further evidence for a smooth decline in UV luminosity at z >= 8

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.269537Z

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Observation 5c524a1c-c11a-48a9-86a4-7e1dd5498df9 · outbound

This paper cites The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.275333Z

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Observation b25e0651-08af-4930-9ecc-349df6c59504 · outbound

This paper cites arXiv e-prints , keywords =.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf arXiv e-prints , keywords =

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.281613Z

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Observation 76459e39-be6e-4247-9525-2ae46d407a8f · outbound

This paper cites The Sonora Substellar Atmosphere Models. IV. Elf Owl: Atmospheric Mixing and Chemical Disequilibrium with Varying Metallicity and C/O Ratios.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Sonora Substellar Atmosphere Models. IV. Elf Owl: Atmospheric Mixing and Chemical Disequilibrium with Varying Metallicity and C/O Ratios

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.286834Z

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Observation 6e406349-5943-41e7-be9b-0f4327042bb4 · outbound

This paper cites doi:10.5281/zenodo.15150865 , url =.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf doi:10.5281/zenodo.15150865 , url =

Reference 33

Resolution: verified exact; doi, observed 2026-08-10T04:20:28.794655Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation e0fff534-e78b-4b2c-bbf3-88d61b4902a2 · outbound

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

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant Universe

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.298053Z

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Observation b274fb03-06a5-473b-a756-90d1e87fe880 · outbound

This paper cites The Open Journal of Astrophysics , keywords =.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Open Journal of Astrophysics , keywords =

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.304348Z

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Observation c42f5cda-1e92-476f-8e0d-928789b9f74b · outbound

This paper cites The Dearth of z~10 Galaxies in all HST Legacy Fields -- The Rapid Evolution of the Galaxy Population in the First 500 Myr.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Dearth of z~10 Galaxies in all HST Legacy Fields -- The Rapid Evolution of the Galaxy Population in the First 500 Myr

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.309819Z

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Observation f9c9b41e-cab1-436e-8150-997110a50d10 · outbound

This paper cites , year = 1974, month = feb, volume =.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf , year = 1974, month = feb, volume =

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.317107Z

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Observation cc523aba-2c40-4c3a-8fd2-37dfe99c0e1d · outbound

This paper cites , keywords =.

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

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.323643Z

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Observation 3cdfa893-9bcc-40f8-94ed-93aab02fa3b1 · outbound

This paper cites , keywords =.

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

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.330695Z

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Observation 7ba76536-1c2a-4485-a957-fd3012f2f878 · outbound

This paper cites , keywords =.

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

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.336810Z

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Observation 767e0fd9-5cb4-4cf7-9d7d-6079fdd54058 · outbound

This paper cites Mapping dark matter in the Bullet Cluster using JWST imaging and spectroscopy.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Mapping dark matter in the Bullet Cluster using JWST imaging and spectroscopy

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.342412Z

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Observation 7f97377d-ab20-44eb-b091-937b498ea600 · outbound

This paper cites doi:10.5479/ADS/bib/2012ivoa.rept.1015R , adsurl =.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf doi:10.5479/ADS/bib/2012ivoa.rept.1015R , adsurl =

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.348667Z

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Observation 9f7f1eb2-23fa-42ee-bab5-14249dcfacf0 · outbound

This paper cites XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society , year = 2020, month = jul, eid =.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society , year = 2020, month = jul, eid =

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.355457Z

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Observation 3e3b9914-82f5-459c-a54d-47eac51e9247 · outbound

This paper cites Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.361420Z

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Observation 3d3f7fe0-05e2-4f59-a896-6c4faa54c82f · outbound

This paper cites JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.366190Z

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Observation 4b60eff3-b482-4893-ba94-2f3393725501 · outbound

This paper cites Constraining the Distribution of L- & T-Dwarfs in the Galaxy.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Constraining the Distribution of L- & T-Dwarfs in the Galaxy

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.370865Z

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Observation 4cb4c7c2-b218-46af-b0ca-1bcc5a4faba4 · outbound

This paper cites Brown dwarf census with the Dark Energy Survey year 3 data and the thin disk scale height of early L types.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Brown dwarf census with the Dark Energy Survey year 3 data and the thin disk scale height of early L types

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.375848Z

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Observation 10482913-40df-4588-aa54-a740642361be · outbound

This paper cites Evaluation of the Vertical Scale Height of L dwarfs in the Galactic Thin Disk.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Evaluation of the Vertical Scale Height of L dwarfs in the Galactic Thin Disk

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.381322Z

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Observation 4e7046bf-3c80-45ee-9b81-2c62708b5bca · outbound

This paper cites The Brown Dwarf Kinematics Project (BDKP) I. Proper Motions and Tangential Velocities for a Large Sample of Late-type M, L and T Dwarfs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Brown Dwarf Kinematics Project (BDKP) I. Proper Motions and Tangential Velocities for a Large Sample of Late-type M, L and T Dwarfs

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.386182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cfa4a2f8-bf98-45c3-ab2d-5cadb35ae22d · outbound

This paper cites Space Velocities of L- and T-type Dwarfs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Space Velocities of L- and T-type Dwarfs

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.392793Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 16ebab8f-9de1-495a-8b61-383ac41c04a1 · outbound

This paper cites Activity and Kinematics of Ultracool Dwarfs Including An Amazing Flare Observation.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Activity and Kinematics of Ultracool Dwarfs Including An Amazing Flare Observation

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.399652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5595ff2a-2455-41ff-a6fc-a358784b6bf9 · outbound

This paper cites Astronomical Data Analysis Software and Systems XII , year = 2003, editor =.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Astronomical Data Analysis Software and Systems XII , year = 2003, editor =

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.407009Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d4645263-eee9-4f70-932e-fd3b85f6ec0c · outbound

This paper cites Possible evidence for a pair-instability supernova nature of ultra-early JWST sources.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Possible evidence for a pair-instability supernova nature of ultra-early JWST sources

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.413716Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 483c0fb2-8bb5-4d32-aca9-95e91336e895 · outbound

This paper cites Spectroscopic confirmation of a large and luminous galaxy with weak emission lines at $\mathbf{z = 13.53}$.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Spectroscopic confirmation of a large and luminous galaxy with weak emission lines at $\mathbf{z = 13.53}$

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.419106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 31ee53de-51a8-4eaa-a417-4ae7dc00d3e4 · outbound

This paper cites BEACON: JWST NIRCam Pure-parallel Imaging Survey. III. Constraints on the UV LF and the Clustering of z~7-14 Galaxies.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf BEACON: JWST NIRCam Pure-parallel Imaging Survey. III. Constraints on the UV LF and the Clustering of z~7-14 Galaxies

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.424973Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95358567-c7f4-490e-85ad-0e1f23c8214e · outbound

This paper cites an unresolved cited work.

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

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.431556Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 36c1f884-71d2-495b-9b5e-809274d8f674 · outbound

This paper cites A Type Ia Supernova Candidate at $z\sim4.3$: A Transient Interloper in the Search for $z\sim14$ Galaxies.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf A Type Ia Supernova Candidate at $z\sim4.3$: A Transient Interloper in the Search for $z\sim14$ Galaxies

Reference 57

Resolution: metadata mismatch; local_arxiv, observed 2026-08-10T04:20:28.546574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation efa4b010-a40b-4718-a34c-7a5605903ec8 · outbound

This paper cites Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.444008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 24d0979d-8bcd-4724-9676-1c06b8b935b1 · outbound

This paper cites Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.451010Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5e083814-8373-46b4-adb7-d41018c32172 · outbound

This paper cites The Discovery of Y Dwarfs Using Data from the Wide-field Infrared Survey Explorer (WISE).

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Discovery of Y Dwarfs Using Data from the Wide-field Infrared Survey Explorer (WISE)

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.456841Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c43517e-be04-406c-b5f7-2130261cb2a9 · outbound

This paper cites Measuring and Replicating the 1-20 um Energy Distributions of the Coldest Brown Dwarfs: Rotating, Turbulent and Non-Adiabatic Atmospheres.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Measuring and Replicating the 1-20 um Energy Distributions of the Coldest Brown Dwarfs: Rotating, Turbulent and Non-Adiabatic Atmospheres

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.462196Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3c6098aa-e6ba-499e-81f3-860dd21383c5 · outbound

This paper cites Near-infrared photometry.

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

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.467326Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ade7485-fd49-4cd9-b157-93d2014d2119 · outbound

This paper cites The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.472204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb763d36-a899-4a0b-8a51-2322e1ec40ab · outbound

This paper cites The Y Dwarf Population with HST: unlocking the secrets of our coolest neighbours -- II. Parallaxes and Proper Motions.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Y Dwarf Population with HST: unlocking the secrets of our coolest neighbours -- II. Parallaxes and Proper Motions

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.477691Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d54258aa-099d-4ca1-ac5e-2cdbef412d79 · outbound

This paper cites A temperate super-Jupiter imaged with JWST in the mid-infrared.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf A temperate super-Jupiter imaged with JWST in the mid-infrared

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.482895Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1638d887-49d8-4e3f-89f0-68f16a65a86e · outbound

This paper cites Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.490123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2e2ff747-c2d2-4f06-8401-bf1fd31b4ecf · outbound

This paper cites Evidence for a sub-jovian planet in the young TWA7 disk.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Evidence for a sub-jovian planet in the young TWA7 disk

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.496739Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cb852e23-a6b4-466a-83bc-b9c995d5e1a7 · outbound

This paper cites Follow-Up Exploration of the TWA 7 Planet-Disk System with JWST NIRCam.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Follow-Up Exploration of the TWA 7 Planet-Disk System with JWST NIRCam

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.501703Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation baec30cf-e788-41a5-aeef-66bb9b8fa6e4 · outbound

This paper cites JWST Coronagraphic Images of 14 Her c: a Cold Giant Planet in a Dynamically Hot, Multi-planet System.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf JWST Coronagraphic Images of 14 Her c: a Cold Giant Planet in a Dynamically Hot, Multi-planet System

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.506670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a81d5270-4207-4dc2-8819-f437c2255974 · outbound

This paper cites Discovery of an Exterior Third Planet Orbiting $\beta$ Pictoris.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Discovery of an Exterior Third Planet Orbiting $\beta$ Pictoris

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.511566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7739a5f1-53f6-4806-88ea-9f6568d3fbfd · outbound

This paper cites Direct Imaging Discovery of Giant Exoplanet $\beta$ Pictoris d: A Decade-Long Game of Hide-and-Seek.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Direct Imaging Discovery of Giant Exoplanet $\beta$ Pictoris d: A Decade-Long Game of Hide-and-Seek

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.517673Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb310e19-2d3a-4007-a767-5478a8e9feb4 · outbound

This paper cites Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.523449Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 76880ef9-d7b2-4924-8688-14599b459d51 · outbound

This paper cites The First Spectrum of the Coldest Brown Dwarf.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The First Spectrum of the Coldest Brown Dwarf

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.529319Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e8b98413-ae7d-4037-bdca-859b52affa7c · outbound

This paper cites Discovery of Cold Brown Dwarfs or Free-Floating Giant Planets Close to the Sun.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Discovery of Cold Brown Dwarfs or Free-Floating Giant Planets Close to the Sun

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.535226Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 46054c44-ca48-425f-a1e3-db3e76cab0db · outbound

This paper cites Indications of Water Clouds in the Coldest Known Brown Dwarf.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Indications of Water Clouds in the Coldest Known Brown Dwarf

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.541058Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a97dccd4-f9c3-4faf-a8f0-dac157596db3 · outbound

This paper cites Distances, Luminosities, and Temperatures of the Coldest Known Substellar Objects.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Distances, Luminosities, and Temperatures of the Coldest Known Substellar Objects

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.546593Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 29752af6-ba17-495b-873a-7cc6d8cfb5d8 · outbound

This paper cites WISE Y Dwarfs As Probes of the Brown Dwarf-Exoplanet Connection.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf WISE Y Dwarfs As Probes of the Brown Dwarf-Exoplanet Connection

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.552111Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d11c4826-5108-4bdf-93c6-163a45e67d57 · outbound

This paper cites Self-consistent Models of Y Dwarf Atmospheres with Water Clouds and Disequilibrium Chemistry.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Self-consistent Models of Y Dwarf Atmospheres with Water Clouds and Disequilibrium Chemistry

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.557799Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f1995a8-04d2-4e01-a549-a4c34bfafb58 · outbound

This paper cites Microphysics of Water Clouds in the Atmospheres of Y Dwarfs and Temperate Giant Planets.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Microphysics of Water Clouds in the Atmospheres of Y Dwarfs and Temperate Giant Planets

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.563461Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aa216b95-6f9f-43cb-a5f2-c5844d0e093c · outbound

This paper cites Three-dimensional dynamical evolution of cloud particle microphysics in sub-stellar atmospheres I. Description and exploring Y-dwarf atmospheric variability.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Three-dimensional dynamical evolution of cloud particle microphysics in sub-stellar atmospheres I. Description and exploring Y-dwarf atmospheric variability

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.568862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2856dbb9-d5d1-4d1c-8cbf-6baa18f8cf1e · outbound

This paper cites Spectral Variability from the Patchy Atmospheres of T and Y Dwarfs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Spectral Variability from the Patchy Atmospheres of T and Y Dwarfs

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.574850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9bfb8ff3-674d-4475-a6a0-57de2ed5f05a · outbound

This paper cites Science Advances , keywords =.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Science Advances , keywords =

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.581199Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f5121ee-8ee2-46b5-9fc5-ad5eaf09877c · outbound

This paper cites A new set of atmosphere and evolution models for cool T-Y brown dwarfs and giant exoplanets.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf A new set of atmosphere and evolution models for cool T-Y brown dwarfs and giant exoplanets

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.588772Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50e88a74-c588-4570-9059-55dd20dec37e · outbound

This paper cites Observations of Disequilibrium CO Chemistry in the Coldest Brown Dwarfs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Observations of Disequilibrium CO Chemistry in the Coldest Brown Dwarfs

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.595388Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a77c58aa-391e-43b1-9b79-5088e213fe7e · outbound

This paper cites The Y dwarf population with HST: unlocking the secrets of our coolest neighbours -- I. Overview & First astrometric results.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Y dwarf population with HST: unlocking the secrets of our coolest neighbours -- I. Overview & First astrometric results

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.600695Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 55ea4776-db26-4779-94bd-bef4429b80d4 · outbound

This paper cites Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the "Planetary" Mass Regime.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the "Planetary" Mass Regime

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.605993Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 719151ae-67d7-4e4a-8d76-45a8ab6422de · outbound

This paper cites , keywords =.

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

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.611351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bb5963ac-a134-4f0d-83bc-041e1f712bad · outbound

This paper cites , keywords =.

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

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.616019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 35eba4fe-3d93-461e-ba78-519098d029e4 · outbound

This paper cites UNCOVER: JWST Spectroscopy of Three Cold Brown Dwarfs at Kiloparsec-scale Distances.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf UNCOVER: JWST Spectroscopy of Three Cold Brown Dwarfs at Kiloparsec-scale Distances

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.621544Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fc402fa8-3fb4-4fd4-b61c-f9ba3f252bd3 · outbound

This paper cites Little Red Dots or Brown Dwarfs? NIRSpec Discovery of Three Distant Brown Dwarfs Masquerading as NIRCam-Selected Highly-Reddened AGNs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Little Red Dots or Brown Dwarfs? NIRSpec Discovery of Three Distant Brown Dwarfs Masquerading as NIRCam-Selected Highly-Reddened AGNs

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.627571Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4c550b3-0b56-4885-9722-b6a74ab414b3 · outbound

This paper cites JADES: Spectroscopic Confirmation and Proper Motion for a T-Dwarf at 2 Kiloparsecs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf JADES: Spectroscopic Confirmation and Proper Motion for a T-Dwarf at 2 Kiloparsecs

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.633119Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2622b58a-d03a-43d4-9039-ac80d418867d · outbound

This paper cites an unresolved cited work.

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

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.638297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 76c9d03d-bce9-4308-a1c7-48546221eb3b · outbound

This paper cites and others , title =.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf and others , title =

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.643352Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc73acb8-3909-4d7e-94bd-0db6d4f9cd08 · outbound

This paper cites The Gaia mission.

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

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.648064Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aae7e137-568f-43a6-a543-720b8f27429c · outbound

This paper cites Gaia Data Release 3: Summary of the content and survey properties.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Gaia Data Release 3: Summary of the content and survey properties

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.653366Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7a9cbc0a-9699-409e-b408-4d53fcb85294 · outbound

This paper cites Weather on Other Worlds. II. Survey Results: Spots Are Ubiquitous on L and T Dwarfs.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Weather on Other Worlds. II. Survey Results: Spots Are Ubiquitous on L and T Dwarfs

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.659262Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7a404b7-b56a-45f4-92a8-c6c8a626c573 · outbound

This paper cites Let the Great World Spin: Revealing the Stormy, Turbulent Nature of Young Giant Exoplanet Analogs with the Spitzer Space Telescope.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Let the Great World Spin: Revealing the Stormy, Turbulent Nature of Young Giant Exoplanet Analogs with the Spitzer Space Telescope

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.665507Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 72fa8779-dfca-4390-a9c4-7b4af4610923 · outbound

This paper cites A Near-infrared Variability Survey of Young Planetary-mass Objects.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf A Near-infrared Variability Survey of Young Planetary-mass Objects

Reference 98

Resolution: verified exact; local_arxiv, observed 2026-08-10T04:20:30.518652Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 78ddb666-d526-4a6f-bdab-427f81030ca7 · outbound

This paper cites A Spitzer Space Telescope Exploration Science Program to Search for Y Dwarf Variability.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf A Spitzer Space Telescope Exploration Science Program to Search for Y Dwarf Variability

Reference 99

Resolution: metadata mismatch; local_arxiv, observed 2026-08-10T04:20:28.497644Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation daf9bf90-8e29-4bad-9d34-7c12b020cc26 · outbound

This paper cites Roaring Storms in the Planetary-Mass Companion VHS 1256-1257 b: Hubble Space Telescope Multi-epoch Monitoring Reveals Vigorous Evolution in an Ultra-cool Atmosphere.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Roaring Storms in the Planetary-Mass Companion VHS 1256-1257 b: Hubble Space Telescope Multi-epoch Monitoring Reveals Vigorous Evolution in an Ultra-cool Atmosphere

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-08-10T04:20:30.492480Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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