Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies | Paper Citation Record

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

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This paper cites Research Notes of the American Astronomical Society , keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Research Notes of the American Astronomical Society , keywords =

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Unresolved cited work

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This paper cites 1987, MNRAS, 225, 155, doi: 10.1093/mnras/225.1.155.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 1987, MNRAS, 225, 155, doi: 10.1093/mnras/225.1.155

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This paper cites Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources

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Observation 7ab2ab01-5b48-4224-9f0e-9e9739aaf9a5 · outbound

This paper cites Jiang, F.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Jiang, F

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

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This paper cites The role of mergers and halo spin in shaping galaxy morphology.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The role of mergers and halo spin in shaping galaxy morphology

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

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This paper cites G., Vega-Ferrero, J., et al.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies G., Vega-Ferrero, J., et al

Reference 10

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This paper cites Stellar masses of SDSS-III BOSS galaxies at z~0.5 and constraints to galaxy formation models.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Stellar masses of SDSS-III BOSS galaxies at z~0.5 and constraints to galaxy formation models

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

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 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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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies NIHAO XXI: The emergence of Low Surface Brightness galaxies

Reference 14

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This paper cites A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417

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This paper cites R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607

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This paper cites At the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies At the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores

Reference 17

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This paper cites Discovery of disc truncations above the galaxies' mid-plane in Milky Way-like galaxies.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Discovery of disc truncations above the galaxies' mid-plane in Milky Way-like galaxies

Reference 18

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

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This paper cites Star formation thresholds and galaxy edges: why and where.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Star formation thresholds and galaxy edges: why and where

Reference 20

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This paper cites The Gaia mission.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The Gaia mission

Reference 21

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This paper cites Summary of the content and survey properties.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Summary of the content and survey properties

Reference 22

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Total Galaxy Magnitudes and Effective Radii from Petrosian Magnitudes and Radii

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The Thirteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey MApping Nearby Galaxies at Apache Point Observatory

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies HyperLEDA. III. The catalogue of extragalactic distances

Reference 26

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies archivePrefix = "arXiv", eprint =

Reference 27

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Theoretical Challenges in Galaxy Formation

Reference 28

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This paper cites Edge-on disk galaxies in the SDSS DR6: Fractions of bulgeless and other disk galaxies.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Edge-on disk galaxies in the SDSS DR6: Fractions of bulgeless and other disk galaxies

Reference 29

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies How Do Disks Survive Mergers?

Reference 30

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Annales d'Astrophysique , year = 1948, month = jan, volume =

Reference 31

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 32

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Bulgeless Giant Galaxies Challenge our Picture of Galaxy Formation by Hierarchical Clustering

Reference 33

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Our Milky Way as a Pure-Disk Galaxy -- A Challenge for Galaxy Formation

Reference 34

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Unresolved cited work

Reference 35

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This paper cites A concise reference to (projected) Sersic R^{1/n} quantities, including Concentration, Profile Slopes, Petrosian indices, and Kron Magnitudes.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies A concise reference to (projected) Sersic R^{1/n} quantities, including Concentration, Profile Slopes, Petrosian indices, and Kron Magnitudes

Reference 36

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies On The Robustness of z=0-1 Galaxy Size Measurements Through Model and Non-Parametric Fits

Reference 37

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The ATLAS$^{\rm{3D}}$ project - XXV: Two-dimensional kinematic analysis of simulated galaxies and the cosmological origin of fast and slow rotators

Reference 38

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since $z=3$

Reference 39

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 2024, A&A, 682, A110, doi: 10.1051/0004-6361/202346133

Reference 40

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The Sloan Digital Sky Survey: Technical Summary

Reference 41

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 42

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback

Reference 43

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 44

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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Sparse Image and Signal Processing : Wavelets, Curvelets, Morphological Diversity , isbn =

Reference 45

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This paper cites and Shibahashi , H.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies and Shibahashi , H

Reference 46

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Observation 5fab2231-a435-4d27-a935-f30c3ec072a2 · outbound

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

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Minor mergers and the size evolution of elliptical galaxies

Reference 47

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.853471Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation ca12a8db-388b-4d40-a828-25eedea5ee23 · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 48

Resolution: verified fuzzy; raw_fallback, observed 2026-05-20T15:13:32.443613Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 8c13cdca-7009-465a-8183-d98f1dd61f54 · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 49

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.847679Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation b358ccb8-3c3a-4f61-b54f-8ec7553efe8f · outbound

This paper cites an unresolved cited work.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Unresolved cited work

Reference 50

Resolution: unresolved; raw_fallback, observed 2026-05-20T15:13:32.441653Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 0db163a6-a7b4-481b-87d8-50f2dd78f32d · outbound

This paper cites 2020, A&A, 639, A14, doi: 10.1051/0004-6361/202038015.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 2020, A&A, 639, A14, doi: 10.1051/0004-6361/202038015

Reference 51

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.844762Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation fb59e1f5-be85-4ea3-a381-04264de8c73c · outbound

This paper cites an unresolved cited work.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Unresolved cited work

Reference 52

Resolution: unresolved; raw_fallback, observed 2026-05-20T15:13:32.449203Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation adb09c67-7eb7-4d08-9df9-28c8c9f15d53 · outbound

This paper cites 10.1051/0004-6361/202555288.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 10.1051/0004-6361/202555288

Reference 53

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.768473Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation de44f4e3-7a0e-44ef-9c35-288333a47322 · outbound

This paper cites 10.1051/0004-6361/202557194.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 10.1051/0004-6361/202557194

Reference 54

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.992992Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 27f13dd9-b5cd-4da9-96bb-e3e8ccd1297d · outbound

This paper cites 10.1051/0004-6361/202556875.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 10.1051/0004-6361/202556875

Reference 55

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.866367Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 698c21d5-b8fe-405f-b740-46a6f191d025 · outbound

This paper cites A universal angular momentum profile for galactic halos.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies A universal angular momentum profile for galactic halos

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.842616Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation b80a6964-759a-456e-93b0-be686d017b74 · outbound

This paper cites Removing Internal Reflections from Deep Imaging Datasets.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Removing Internal Reflections from Deep Imaging Datasets

Reference 57

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.831163Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation cc2928ae-61e5-4bcd-a053-5322e1ecd2e0 · outbound

This paper cites Beyond 31 mag/arcsec^2: the low surface brightness frontier with the largest optical telescopes.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Beyond 31 mag/arcsec^2: the low surface brightness frontier with the largest optical telescopes

Reference 58

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.788635Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation fb8b5b4e-081a-4d8c-90c5-db62376ee84a · outbound

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

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Noise Based Detection and Segmentation of Nebulous Objects

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.834204Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 764b35bf-2938-4834-9baf-375f4b5b9da3 · outbound

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

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Carving out the low surface brightness universe with NoiseChisel

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-05-20T08:58:09.779586Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation a2272516-2bac-435c-bdcc-70472df4af5d · outbound

This paper cites Mathematical Morphology - Theory and Applications , doi =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Mathematical Morphology - Theory and Applications , doi =

Reference 61

Resolution: verified fuzzy; raw_fallback, observed 2026-05-20T15:13:32.438660Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 4468fa61-4236-48f2-9364-efe319643018 · outbound

This paper cites I., 1987, @doi [ ] 10.1093/mnras/226.4.747 , http://adsabs.harvard.edu/abs/1987MNRAS.226..747J 226, 747.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies I., 1987, @doi [ ] 10.1093/mnras/226.4.747 , http://adsabs.harvard.edu/abs/1987MNRAS.226..747J 226, 747

Reference 62

Resolution: metadata mismatch; doi, observed 2026-05-20T08:58:09.799594Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation e9fbb40b-a3b0-4e77-804f-199a6947f7ce · outbound

This paper cites doi:10.5281/zenodo.3478575 , version =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies doi:10.5281/zenodo.3478575 , version =

Reference 63

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.828448Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation ab3876cb-02b8-4013-89b3-1a4ce6c40415 · outbound

This paper cites On the Uncertainties of Stellar Mass Estimates via Colour Measurements.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies On the Uncertainties of Stellar Mass Estimates via Colour Measurements

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.837590Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 660fe102-b707-44cc-8c55-ef7b9e48f35c · outbound

This paper cites Color Profiles of Spiral Galaxies: Clues on Outer-Disk Formation Scenarios.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Color Profiles of Spiral Galaxies: Clues on Outer-Disk Formation Scenarios

Reference 65

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.821516Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 637c01b8-5ba0-49bc-b880-8049f8eacb60 · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 66

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.826637Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation ecb74f10-c818-4cb5-96ab-0b151cece115 · outbound

This paper cites The Absolute Magnitude of the Sun in Several Filters.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The Absolute Magnitude of the Sun in Several Filters

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.996476Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation a8f12640-afb9-42a7-866c-44bd95f6401f · outbound

This paper cites 10.1051/0004-6361/202554290.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 10.1051/0004-6361/202554290

Reference 68

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.816015Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 3ab3da19-30c5-4b4e-a112-6c21895386ed · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 69

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.814218Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 3ec2ffb9-4aa6-47c7-814d-b4c34b914877 · outbound

This paper cites The Dependence of Quenching upon the Inner Structure of Galaxies at 0.5<z< 0.8 in the DEEP2/AEGIS Survey.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The Dependence of Quenching upon the Inner Structure of Galaxies at 0.5<z< 0.8 in the DEEP2/AEGIS Survey

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.972382Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 1285430f-9a0b-4c96-b352-b999eb3eac2d · outbound

This paper cites Dense cores in galaxies out to z=2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fields.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Dense cores in galaxies out to z=2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fields

Reference 71

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.875794Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 66a42bfa-4d31-42d8-a6d1-2216b34e8f7a · outbound

This paper cites Evidence for Mature Bulges and an Inside-out Quenching Phase 3 Billion Years After the Big Bang.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Evidence for Mature Bulges and an Inside-out Quenching Phase 3 Billion Years After the Big Bang

Reference 72

Resolution: metadata mismatch; local_arxiv, observed 2026-05-20T08:58:09.818628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation ec35aa4b-f53a-454c-b7ac-3427831cbd83 · outbound

This paper cites The intrinsic characteristics of galaxies on the SFR-stellar mass plane at 1.2<z<4: I. the correlation between stellar age, central density and position relative to the main sequence.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The intrinsic characteristics of galaxies on the SFR-stellar mass plane at 1.2<z<4: I. the correlation between stellar age, central density and position relative to the main sequence

Reference 73

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.824542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 04f4eeac-9727-45a9-bd7a-c8a21fe6d9a1 · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 74

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.839735Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation b932844c-d747-47db-ad05-2c445a5e6914 · outbound

This paper cites Strong bimodality in the host halo mass of central galaxies from galaxy-galaxy lensing.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Strong bimodality in the host halo mass of central galaxies from galaxy-galaxy lensing

Reference 75

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.850538Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation bdcec721-17e0-4fe2-b92c-2af3bee067db · outbound

This paper cites and Shibahashi , H.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies and Shibahashi , H

Reference 76

Resolution: metadata mismatch; arxiv_id, observed 2026-05-20T08:58:09.858882Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation e30c21f8-863e-4319-bae2-1d79f284a209 · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 77

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.985239Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 5601b195-aa17-4e10-a98c-0d5f238ef6ec · outbound

This paper cites Monthly Notices of the Royal Astronomical Society , volume =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Monthly Notices of the Royal Astronomical Society , volume =

Reference 78

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.809528Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 42458e68-81f2-4d11-aa84-59e900c83b6e · outbound

This paper cites Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence

Reference 79

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.791814Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 2e6faca7-45f5-4633-a73f-9da48dbbc4be · outbound

This paper cites Morphological quenching of star formation: making early-type galaxies red.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Morphological quenching of star formation: making early-type galaxies red

Reference 80

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.802430Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 6e116c1a-f321-4831-9d7f-2ffd5fc515e6 · outbound

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

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD

Reference 81

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.797356Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 8caa1d0c-65e3-4146-9c15-7740ed1f1d56 · outbound

This paper cites Jiang, F.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Jiang, F

Reference 82

Resolution: metadata mismatch; arxiv_id, observed 2026-05-20T08:58:09.983025Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d3e874fd-dbd9-4d6a-b9c3-982f4b1432c6 · outbound

This paper cites The size evolution of galaxies since z~3: combining SDSS, GEMS and FIRES.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The size evolution of galaxies since z~3: combining SDSS, GEMS and FIRES

Reference 83

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.759916Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation f3ee8dcb-0893-4774-a106-9f646b060980 · outbound

This paper cites eprint =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies eprint =

Reference 84

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.762050Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 05349c20-7229-4719-a332-980cc0b5003d · outbound

This paper cites An Explanation for the Observed Weak Size Evolution of Disk Galaxies.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies An Explanation for the Observed Weak Size Evolution of Disk Galaxies

Reference 85

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.764819Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 73ba2a01-586e-490f-8443-36f595d38aea · outbound

This paper cites an unresolved cited work.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Unresolved cited work

Reference 86

Resolution: unresolved; raw_fallback, observed 2026-05-20T15:13:32.445498Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation eea2aa15-63e1-4ff3-a7de-6046aaf82d41 · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 87

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.977368Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 6fb6bdc9-0048-43c9-a41e-dee52350b079 · outbound

This paper cites A., De Marco O., Barlow M.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies A., De Marco O., Barlow M

Reference 88

Resolution: metadata mismatch; arxiv_id, observed 2026-05-20T08:58:09.975473Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d9ae8126-4583-458e-9abb-4cbd0b9d3fbe · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 89

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.770653Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 1ce7cbda-1812-4997-bb4d-39ef0f5b63be · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 90

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.752993Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation dea1ad57-fdd9-4c3e-915d-1be85b3e9aa8 · outbound

This paper cites Formation and Environmental Context of Giant Bulgeless Disk Galaxies in the Early Universe: Insights from Cosmological Simulations.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Formation and Environmental Context of Giant Bulgeless Disk Galaxies in the Early Universe: Insights from Cosmological Simulations

Reference 91

Resolution: verified exact; arxiv_id, observed 2026-05-20T08:58:09.773898Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 9ad75c89-45f2-4aff-8b41-e94d5c340baa · outbound

This paper cites 1996, A&AS, 117, 393, doi: 10.1051/aas:1996164.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies 1996, A&AS, 117, 393, doi: 10.1051/aas:1996164

Reference 92

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.751094Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 832ed684-76fa-4d88-a952-08fe3d9a6f77 · outbound

This paper cites Astrometry.net: Blind astrometric calibration of arbitrary astronomical images.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Astrometry.net: Blind astrometric calibration of arbitrary astronomical images

Reference 93

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.776888Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 72c09fb3-e3bf-4506-af8c-763f40aa4b25 · outbound

This paper cites Astronomical Data Analysis Software and Systems XV , year = 2006, editor =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Astronomical Data Analysis Software and Systems XV , year = 2006, editor =

Reference 94

Resolution: verified fuzzy; raw_fallback, observed 2026-05-20T15:13:32.444017Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation da3e37ed-8c89-475a-bf48-6f91e9f8e30e · outbound

This paper cites Physica , year = 1934, month = may, volume =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies Physica , year = 1934, month = may, volume =

Reference 95

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.755067Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 44ec6b58-df10-4b80-aeee-3ffc40af8bd9 · outbound

This paper cites M., Rom \'a n , J., Knapen , J.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies M., Rom \'a n , J., Knapen , J

Reference 96

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.783697Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 8ff8d5fc-a991-4405-8909-190daa6f063f · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 97

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.785492Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d4b46afb-9d21-4ddf-9cb1-c6c19f79c0d9 · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 98

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.747311Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation ff94c39e-6f78-4930-b52d-00cd166ad82f · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 99

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.749144Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d33b287a-e82c-4024-9d49-3a98608629ea · outbound

This paper cites keywords =.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies keywords =

Reference 100

Resolution: verified exact; doi, observed 2026-05-20T08:58:09.757214Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Coverage vector

Reference resolution

Outbound references

Pith citing papers