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Paper Citation Record · LEDGER

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy

As of 10 August 2026, this Paper Citation Record lists 100 of 135 outbound references and 0 inbound Pith citation observations for arXiv:2607.15340.

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pith.paper-citation-record.v1
2607.15340 v1

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measured 100 of 135 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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100 of 135 outbound references displayed

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External citation measurements

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Outbound references

Observation 1db388f3-ad9f-4ab8-903f-cd5573635747 · outbound

This paper cites , keywords =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

Reference 1

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Observation 20a5189d-d914-4e55-af56-deb33b9ee910 · outbound

This paper cites , keywords =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

Reference 2

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Observation 64dd0d4b-eb8f-4623-8c23-656b26a1f0ab · outbound

This paper cites , keywords =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

Reference 4

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Observation b2e399e7-6808-442b-94e2-7e9b0a42f148 · outbound

This paper cites The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations

Reference 5

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Observation 19b48ef1-644e-4ee4-8125-68843ccb6d1c · outbound

This paper cites On the baryonic, stellar, and luminous scaling relations of disk galaxies.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy On the baryonic, stellar, and luminous scaling relations of disk galaxies

Reference 6

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Observation a860d1db-a164-4c35-9612-8669dca4d70b · outbound

This paper cites Size evolution of star-forming galaxies with $2<z<4.5$ in the VIMOS Ultra-Deep Survey.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Size evolution of star-forming galaxies with $2<z<4.5$ in the VIMOS Ultra-Deep Survey

Reference 7

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Observation e76085f6-e7fe-4bcf-946f-36d8f9280e6d · outbound

This paper cites Annales d'Astrophysique , year = 1948, month = jan, volume =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Annales d'Astrophysique , year = 1948, month = jan, volume =

Reference 8

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Observation cf22a473-d277-4c44-9d74-b5aa8e4a1e34 · outbound

This paper cites Total Galaxy Magnitudes and Effective Radii from Petrosian Magnitudes and Radii.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Total Galaxy Magnitudes and Effective Radii from Petrosian Magnitudes and Radii

Reference 9

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Observation 15096953-0957-4447-97f2-542c942dcd89 · outbound

This paper cites NASIM: Revealing the low surface brightness Universe from legacy VISTA data.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy NASIM: Revealing the low surface brightness Universe from legacy VISTA data

Reference 10

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Observation 877c0201-5912-4abd-a5a4-0774c4b7d1d8 · outbound

This paper cites Fossil groups origins II. Unveiling the formation of the brightest group galaxies through their scaling relations.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Fossil groups origins II. Unveiling the formation of the brightest group galaxies through their scaling relations

Reference 11

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Observation e86edd56-9fe9-4096-9517-65772b334c51 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Unresolved cited work

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Observation ee950db3-db40-4211-aacc-2870561477f0 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

Reference 13

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Observation b76a0a4b-346f-4038-b3d2-1626c4661d96 · outbound

This paper cites Minor mergers and the size evolution of elliptical galaxies.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Minor mergers and the size evolution of elliptical galaxies

Reference 14

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Observation 53837d92-7474-402f-ab26-dd3e2b4a027b · outbound

This paper cites 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since $z=3$.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since $z=3$

Reference 15

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Unresolved cited work

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Observation 04582c00-2158-4b75-b593-563d61cc36db · outbound

This paper cites The luminosities, sizes and velocity dispersions of Brightest Cluster Galaxies: Implications for formation history.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The luminosities, sizes and velocity dispersions of Brightest Cluster Galaxies: Implications for formation history

Reference 17

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Observation a3d4ce8f-9728-4a0e-a9d4-b47ac476e90a · outbound

This paper cites The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars

Reference 18

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Observation 282cb10f-fee4-4ca9-a0ee-ec76c12c6443 · outbound

This paper cites Dissipation and Extra Light in Galactic Nuclei: III. 'Core' Ellipticals and 'Missing' Light.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Dissipation and Extra Light in Galactic Nuclei: III. 'Core' Ellipticals and 'Missing' Light

Reference 19

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

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Observation fd6223b1-8a13-49a8-86ee-071c8cfb425c · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Theoretical Challenges in Galaxy Formation

Reference 21

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This paper cites The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes

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Observation 324d4e42-4fd4-45c6-8879-8a3223b9c99c · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The structure of galactic disks: Studying late-type spiral galaxies using SDSS

Reference 23

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Monthly Notices of the Royal Astronomical Society , volume =

Reference 25

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy and d’Eugenio, Francesco and Sharp, Rob and Cortese, Luca and Scott, Nicholas and Croom, Scott M

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Observation 494636ba-abb3-4d50-89a5-dad9992557e0 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The splashback radius as a physical halo boundary and the growth of halo mass

Reference 27

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Observation 02d06a34-498f-45b1-ac96-d145668a5634 · outbound

This paper cites Dependence of the outer density profiles of halos on their mass accretion rate.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Dependence of the outer density profiles of halos on their mass accretion rate

Reference 28

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This paper cites The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology

Reference 29

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Detection of the Splashback Radius and Halo Assembly bias of Massive Galaxy Clusters

Reference 30

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Splashback in accreting dark matter halos

Reference 31

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Beyond 31 mag/arcsec^2: the low surface brightness frontier with the largest optical telescopes

Reference 32

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Unresolved cited work

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Observation 4da30feb-7e35-4b02-aa28-8ceb1c2e6a4e · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The splashback boundary of haloes in hydrodynamic simulations

Reference 34

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Observation ef6b1321-210b-4da7-94cf-50dbf47556a0 · outbound

This paper cites The Growth in Size and Mass of Cluster Galaxies since z=2.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Growth in Size and Mass of Cluster Galaxies since z=2

Reference 35

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy VEGAS: A VST Early-type GAlaxy Survey. II. Photometric study of giant ellipticals and their stellar halos

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Sloan Digital Sky Survey: Technical Summary

Reference 37

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Observation 02d65990-8e5a-4a21-aaa6-991e601efd90 · outbound

This paper cites The Sloan Digital Sky Survey extended point spread functions.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Sloan Digital Sky Survey extended point spread functions

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Observation a5f955f9-02e8-4fa7-ad63-8b4c2c10c8a6 · outbound

This paper cites LIGHTS. The extended point spread functions of the LIGHTS survey at the LBT.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy LIGHTS. The extended point spread functions of the LIGHTS survey at the LBT

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Observation d09b0313-33a1-40ff-aa69-3b394e006c4e · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Unresolved cited work

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Observation bf991fb2-fb48-4397-995c-518747ac6def · outbound

This paper cites The Fornax Deep Survey with VST. VIII. Connecting the accretion history with the cluster density.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Fornax Deep Survey with VST. VIII. Connecting the accretion history with the cluster density

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Observation 18090484-8b72-4924-a02e-aa24f79f35cb · outbound

This paper cites Removing Internal Reflections from Deep Imaging Datasets.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Removing Internal Reflections from Deep Imaging Datasets

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Observation ac0c2eb1-86b0-4bc8-8306-57b92bb62bf9 · outbound

This paper cites The Luminosity Profiles of Brightest Cluster Galaxies.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Luminosity Profiles of Brightest Cluster Galaxies

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Observation 837ca704-28fd-4859-975b-19cfa5d4d79e · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

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Observation 984cb299-0fc7-41f9-9836-6e25c4dfbf0e · outbound

This paper cites Galactic cirri in deep optical imaging.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Galactic cirri in deep optical imaging

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no resolver link, observed 2026-08-01T23:42:36.170327Z

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Observation cdabb244-d3a1-4f65-9a86-05defb62f51a · outbound

This paper cites Structure of Brightest Cluster Galaxies and Intracluster Light.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Structure of Brightest Cluster Galaxies and Intracluster Light

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Observation 90783cf0-f2a8-4a90-b5e0-fef5f7f0cb7e · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

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verified exact
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Observation 421fd245-d98c-4a30-b9cd-7c0c2714c329 · outbound

This paper cites The buildup of the intracluster light of Abell 85 as seen by Subaru's Hyper Suprime-Cam.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The buildup of the intracluster light of Abell 85 as seen by Subaru's Hyper Suprime-Cam

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Observation b545c77c-e4e3-4054-abac-297c7be83397 · outbound

This paper cites Noise Based Detection and Segmentation of Nebulous Objects.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Noise Based Detection and Segmentation of Nebulous Objects

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no resolver link, observed 2026-08-01T23:42:36.943056Z

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Observation a2bdec9e-939e-43b8-a4a2-44bd35b3aea3 · outbound

This paper cites Carving out the low surface brightness universe with NoiseChisel.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Carving out the low surface brightness universe with NoiseChisel

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Observation e1e6697f-09f2-4805-88fe-92273c093957 · outbound

This paper cites Trager and Michael H.F.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Trager and Michael H.F

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Observation 8ebd7def-9ea3-4eca-b187-550aa4970801 · outbound

This paper cites The Gaia mission.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Gaia mission

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Observation 037e3b15-f191-42e7-a181-ec94ce14336c · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Gaia Data Release 3: Summary of the content and survey properties

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Observation ec3f321b-bb20-4c15-a22c-e338f52da9db · outbound

This paper cites The influence of diffuse scattered light I. The PSF and its role to observations of the edge-on galaxy NGC 5907.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The influence of diffuse scattered light I. The PSF and its role to observations of the edge-on galaxy NGC 5907

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source=arxiv_source observed=2026-08-01T23:42:37.538619Z digest=sha256:595b9ea790b40e6ae0e1bf4af9bd0979ca48d8dea46eb7a07b88fd99a9e800b2

Observation e023f523-9b0a-447f-8fa9-53eae0ddc6f6 · outbound

This paper cites The influence of diffuse scattered light II. Observations of galaxy haloes and thick discs and hosts of BCGs.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The influence of diffuse scattered light II. Observations of galaxy haloes and thick discs and hosts of BCGs

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Observation 5f151349-5bde-473c-873e-6be8569bd269 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Gnuastro: measuring radial profiles from images

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Observation bf974a6c-04e5-4854-b68a-45fa2b8509ec · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Sparse Image and Signal Processing : Wavelets, Curvelets, Morphological Diversity , isbn =

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source=arxiv_source observed=2026-08-01T23:42:37.782464Z digest=sha256:45b340b2a03e2a9d33033ce5d520001e0cda69d6cad86ef9555097cae06f6086

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy A robust technique to identify galaxy edges

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source=arxiv_source observed=2026-08-01T23:42:37.832270Z digest=sha256:19cbbd7799f96afe7115da355f2ec6f60e66525d555b6b66ea2e70db0a5167c5

Observation 5b11abac-4487-4770-bb86-804689caaa67 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy and Wilkinson, Michael H

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source=arxiv_source observed=2026-08-01T23:42:37.836910Z digest=sha256:0c456d993f44c334a094920d57fd6091a8ac4e5750ed57bfc910b69ae0c669f6

Observation f46771e2-a47e-43ac-806f-e8a941ab0100 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Strong size evolution of disc galaxies since z = 1: Readdressing galaxy growth using a physically motivated size indicator

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source=arxiv_source observed=2026-08-01T23:42:37.841324Z digest=sha256:eac5680c447675d2b45efcc97494aa2ce4adc7e864023372c42ceed4c58a2ff0

Observation 7a005135-79fc-4ce0-a057-3a3726352d6c · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Color Profiles of Spiral Galaxies: Clues on Outer-Disk Formation Scenarios

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source=arxiv_source observed=2026-08-01T23:42:37.846423Z digest=sha256:caf2c6ee131e2dcbf487e92ab3af74cc8bc3d36a98eabfa2155d337980a35c0d

Observation 6df927f9-c6ea-4752-a88e-cf27246ba8a8 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Unresolved cited work

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source=arxiv_source observed=2026-08-01T23:42:37.851949Z digest=sha256:0eb8a9b1788dcfc700e425d0bf7e1890f380135b840671688f31b37abb8456ea

Observation bb3788ce-f095-4ba3-a195-bc6a9cda9319 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Intra-Cluster Light at the Frontier: Abell 2744

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Observation 36c9eecc-7dfe-464c-8275-012f164e6a93 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Properties of extragalactic thick discs recovered from ultra-deep Stripe82 imaging

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Observation 4f0f5305-eb44-411a-83ca-8978f64710b0 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

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source=arxiv_source observed=2026-08-01T23:42:37.866318Z digest=sha256:9767f1ec20d4691e5ab5da4b4012c0d20e6b0d701382bccda2f22bd24a7b485a

Observation 9265e060-133b-4f83-b401-94780a7250c1 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

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source=arxiv_source observed=2026-08-01T23:42:37.870670Z digest=sha256:399c779d1671049946caa2e8809e6cda7aad840dc51b82fab7ca6fc9a7305849

Observation 94cd771b-6dde-4685-a2f2-f13ed27d362d · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy A physically motivated definition for the size of galaxies in an era of ultra-deep imaging

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Observations, reduction and results

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Observation 94de1aef-ee79-4ef4-b8f0-3c386f131ea7 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy doi:10.5281/zenodo.3478575 , version =

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy On the Uncertainties of Stellar Mass Estimates via Colour Measurements

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Observation 74b84a9d-f816-4006-9598-61613b7d04b1 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The edges of galaxies: Tracing the limits of star formation

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Absolute Magnitude of the Sun in Several Filters

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source=arxiv_source observed=2026-08-01T23:42:37.899209Z digest=sha256:596329bedb9f7889b507da6c08b4e9d879f8c2f624ce1a2b313df5e754b60e34

Observation 4adee474-28d4-4e0a-9491-82caacf5b61f · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Gnuastro: visualizing the full dynamic range in color images

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source=arxiv_source observed=2026-08-01T23:42:37.904458Z digest=sha256:c8869133e823c19c5153c4d7e11239292b9d2036db9f25811c4a14bda51e62a8

Observation eec06abb-6f6f-4571-906d-32e5c63e9685 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy On the formation and physical properties of the Intra-Cluster Light in hierarchical galaxy formation models

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source=arxiv_source observed=2026-08-01T23:42:37.909270Z digest=sha256:94b441aabfaf2f24061b900501f2343701dbec03d33c6a3962ae269b4e6a6a00

Observation d3325576-9a67-439e-b5d1-9983bdbf7e66 · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Deep Chandra Observations of the Extended Gas Sloshing Spiral in A2029

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source=arxiv_source observed=2026-08-01T23:42:37.914345Z digest=sha256:c18562de9ad27a6ba09be597753eace9d6d865202d5609bb3d3801b50b70c007

Observation ed0a1e4e-b6de-4825-8606-2142baf76f0c · outbound

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How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Planck 2015 results. XIII. Cosmological parameters

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Observation d48162c6-d0b6-46be-898c-5dc87ebe1e89 · outbound

This paper cites Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD

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Observation 4aabe61f-74e8-4313-87cd-56fe970bcb3a · outbound

This paper cites The Massively Accreting Cluster A2029.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Massively Accreting Cluster A2029

Reference 79

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source=arxiv_source observed=2026-08-01T23:42:37.927954Z digest=sha256:3fd5454f24051009da126da47bac62b0d22ad4dd8aeab1626640a50e43a32d67

Observation bded9184-fea4-4e81-a687-c92e4c92d7ec · outbound

This paper cites Zahra and Infante-Sainz, Raúl and Martin, Garreth and Montes, Mireia and Román, Javier and Sedighi, Nafise and Sharbaf, Zahra , title =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Zahra and Infante-Sainz, Raúl and Martin, Garreth and Montes, Mireia and Román, Javier and Sedighi, Nafise and Sharbaf, Zahra , title =

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source=arxiv_source observed=2026-08-01T23:42:37.932570Z digest=sha256:c0a5c15adaf67d0cab7b4e59bc82a3ecd8470c943d0757d4f25ffdd120a29365

Observation ff10b4a1-6eae-4f37-90ab-f9b328b9f328 · outbound

This paper cites A remarkably large depleted core in the Abell 2029 BCG IC 1101.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy A remarkably large depleted core in the Abell 2029 BCG IC 1101

Reference 81

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source=arxiv_source observed=2026-08-01T23:42:37.936970Z digest=sha256:680dceaae7bf8b5ac5ced5986249b394f6c24cd9c8343904ffea2cb6b6e6a302

Observation d7a16d9d-f502-4b2a-9fc9-a73d3ebb9caf · outbound

This paper cites CIRS: Cluster Infall Regions in the Sloan Digital Sky Survey I. Infall Patterns and Mass Profiles.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy CIRS: Cluster Infall Regions in the Sloan Digital Sky Survey I. Infall Patterns and Mass Profiles

Reference 82

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source=arxiv_source observed=2026-08-01T23:42:37.941661Z digest=sha256:6dd9d8c30799bfea26ee80af3ea28972886c92029180668d7389048638b0ff23

Observation 18a46670-8750-4419-ab08-d3bf0f8e67ef · outbound

This paper cites Disentangling satellite galaxy populations using orbit tracking in simulations.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Disentangling satellite galaxy populations using orbit tracking in simulations

Reference 83

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source=arxiv_source observed=2026-08-01T23:42:37.946109Z digest=sha256:9fc07234a293dd36cce966b290eff859593f1d0ade9dd30d3bbcc80546e1a38e

Observation 8712b96c-9b7f-4ddc-a828-96c9b30d8a29 · outbound

This paper cites Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias

Reference 84

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source=arxiv_source observed=2026-08-01T23:42:37.950621Z digest=sha256:f75a838317ab066b7c06665fb23d781bd9613fbcfb75943d9daf1cfb28b4b58a

Observation f9314f17-b81e-4f60-8b93-c43a01ac559d · outbound

This paper cites Statistical Tools for Classifying Galaxy Group Dynamics.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Statistical Tools for Classifying Galaxy Group Dynamics

Reference 85

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source=arxiv_source observed=2026-08-01T23:42:37.955311Z digest=sha256:af5280edcbfb8e81a444d3c67500e07a326c2833e6ef8c1b509721152e7ecc33

Observation d67933a5-7ae6-411f-8efa-2bd50ec39927 · outbound

This paper cites The mass accretion rate of galaxy clusters: a measurable quantity.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The mass accretion rate of galaxy clusters: a measurable quantity

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source=arxiv_source observed=2026-08-01T23:42:37.960057Z digest=sha256:0f28d06364027f5cc09ca765d2f34ec380381b504b974c798dddb5e545af5b9b

Observation ba89314b-c840-45bb-9cf7-50ffddce96f8 · outbound

This paper cites arXiv e-prints , keywords =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy arXiv e-prints , keywords =

Reference 87

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source=arxiv_source observed=2026-08-01T23:42:37.965116Z digest=sha256:ac1e04d3b236084ae2fb5cac128878f137f6ad8b36e68e2f5c8c83a22e8caf76

Observation 3ff5d0b4-ccfd-46a6-9ac6-cb8874eca0ae · outbound

This paper cites , keywords =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

Reference 88

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source=arxiv_source observed=2026-08-01T23:42:37.969485Z digest=sha256:a8202330aebfa6bf7ab374d165ad9c9baf0f73a4e76a8923763e0d75895b9ccc

Observation a99d06d0-3faf-4c41-8291-b419c131ce8d · outbound

This paper cites First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 90

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source=arxiv_source observed=2026-08-01T23:42:37.978382Z digest=sha256:c3ee241a5fbdea58a50636466c2f881897d2c1808f2110c18c486697b69c2f0f

Observation 98b133f3-3f2e-433e-8dc9-2f0d74690ec3 · outbound

This paper cites Accreted or Not Accreted? The Fraction of Accreted Mass in Galaxies from Simulations and Observations.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Accreted or Not Accreted? The Fraction of Accreted Mass in Galaxies from Simulations and Observations

Reference 91

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source=arxiv_source observed=2026-08-01T23:42:37.982977Z digest=sha256:826c7bfadccf11c28c0ccd653d6392b586456b91eb83fc81480e1457076bc6d3

Observation bf476c1d-5b1b-497d-be9f-835af84dfc8a · outbound

This paper cites The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function

Reference 92

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source=arxiv_source observed=2026-08-01T23:42:37.987978Z digest=sha256:ee433a6746f6d572e13b9e0457b9d583d52ff3d92c29a8bcef12d73872655745

Observation 238c3a5b-1c8d-4b2a-a226-8c0f17b10f00 · outbound

This paper cites , keywords =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

Reference 93

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source=arxiv_source observed=2026-08-01T23:42:37.993081Z digest=sha256:d119fc9276ec0900945c7d511022491976353de636b0787265e4d02762d8fd98

Observation 4bdd18b9-8ee7-476c-a9a2-085acc0a0fdf · outbound

This paper cites , keywords =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , keywords =

Reference 94

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source=arxiv_source observed=2026-08-01T23:42:37.997494Z digest=sha256:c1842ceedd2e897450d471162f90b36056e5a2d707996a043fe65413823b86c2

Observation c3be24c5-7b64-4d1a-9bd7-ca2cc2798422 · outbound

This paper cites Clocking the formation of today's largest galaxies: Wide field integral spectroscopy of Brightest Cluster Galaxies and their surroundings.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Clocking the formation of today's largest galaxies: Wide field integral spectroscopy of Brightest Cluster Galaxies and their surroundings

Reference 95

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source=arxiv_source observed=2026-08-01T23:42:38.001946Z digest=sha256:a72883c1c317d092c9cbc15778217806b958f156ea2592a8a5b2e82a1b459705

Observation d3e5bf55-49c1-4fad-bcfa-afc7de946122 · outbound

This paper cites , year = 2024, month = jun, volume =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy , year = 2024, month = jun, volume =

Reference 96

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source=arxiv_source observed=2026-08-01T23:42:38.006617Z digest=sha256:0b7718b7b4a0331724c32a187f7d14bdd1cb191028ec5a807fb52da54cb444cd

Observation a01a3721-9e5d-473e-abfd-5a91b2378383 · outbound

This paper cites Stellar splashback: the edge of the intracluster light.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Stellar splashback: the edge of the intracluster light

Reference 97

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source=arxiv_source observed=2026-08-01T23:42:38.011036Z digest=sha256:2a8c223da9f5e0d5ade668aec5fd201a9c19a46d19006e3f754de8e325ea4687

Observation 228939b0-355d-45d9-b478-3845fcbffe72 · outbound

This paper cites Surface photometry of BCGs and intracluster stars in Lambda-CDM.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Surface photometry of BCGs and intracluster stars in Lambda-CDM

Reference 98

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source=arxiv_source observed=2026-08-01T23:42:38.015963Z digest=sha256:ceb0742a8a735c0fb5f19d0627a06c46a57fa5a51f11b216a289d35bc786d219

Observation 6a44c459-6f74-4a6a-98f8-6efa1b55c3dc · outbound

This paper cites A new era of intracluster light studies with JWST.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy A new era of intracluster light studies with JWST

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source=arxiv_source observed=2026-08-01T23:42:38.021169Z digest=sha256:e18fc20de1304582f3a4bc44705bac1aa9a2210269a5870191bfbcf77701c5ff

Observation e34a73e6-82f9-425f-aca3-e12b70d7511e · outbound

This paper cites Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution , year = 2004, editor =.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution , year = 2004, editor =

Reference 100

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source=arxiv_source observed=2026-08-01T23:42:38.026086Z digest=sha256:07639141c1ac7ac06a0d0dda24b6700fea2f79696543c55ab465d87921513bfc

Observation e3520fcc-224b-45f7-85a4-62679f174080 · outbound

This paper cites The Formation and Evolution of Intracluster Light.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The Formation and Evolution of Intracluster Light

Reference 101

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source=arxiv_source observed=2026-08-01T23:42:38.031041Z digest=sha256:edc3a41c47763f97ee68f21fedf6d2de8066946ae7f9977d6f223f1c28cf1f1e

Observation 9e621a7e-bd7a-411e-a69e-51700a8e1fe4 · outbound

This paper cites First joint MUSE, HST, and JWST spectro-photometric analysis of the intracluster light: the case of the relaxed cluster RX J2129.7+0005.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy First joint MUSE, HST, and JWST spectro-photometric analysis of the intracluster light: the case of the relaxed cluster RX J2129.7+0005

Reference 102

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source=arxiv_source observed=2026-08-01T23:42:38.036031Z digest=sha256:7aeaf0d278a8e246edf92cd6a6ee54c752cb24028b3f6b86678acd6956409ff1

Observation 63a61614-d91f-45ac-8dfb-1abe8e3643ed · outbound

This paper cites Intracluster light: a luminous tracer for dark matter in clusters of galaxies.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Intracluster light: a luminous tracer for dark matter in clusters of galaxies

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source=arxiv_source observed=2026-08-01T23:42:38.041242Z digest=sha256:174b97a080e5a4dc64a8dfa8bc6cbbbe23a1d1dad49e07ab15ccaf484cc0b392

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