Pith. sign in

Paper Citation Record · LEDGER

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models

As of 23 August 2026, this Paper Citation Record lists 47 of 47 outbound references and 3 inbound Pith citation observations for arXiv:2411.18440.

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

pith.paper-citation-record.v1
2411.18440 v2

Coverage vector

measured 47 of 47 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:16:58.602053Z

measured 50 of 50 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:16:58.520134Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-19T22:12:50.732458Z

Reference resolution

47 of 47 outbound references displayed

  • verified exact6
  • verified fuzzy17
  • unresolved24
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 20100324-205a-4949-ae31-6e782826894e · outbound

This paper cites an unresolved cited work.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Unresolved cited work

Reference 1

Resolution
unresolved
raw_fallback, observed 2026-08-12T11:16:59.873667Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.354479Z digest=sha256:44ba9114a5e45ebde28f39d14eef93bda915a8a867a1cba34d67cbdb7083f505

Observation 2558db92-a99c-411e-a998-bb70cccfabd9 · outbound

This paper cites an unresolved cited work.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Unresolved cited work

Reference 2

Resolution
unresolved
raw_fallback, observed 2026-08-12T11:16:59.851079Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.361370Z digest=sha256:b4ef2804a653bc57f5d01c053532760ab5cac543ef3e3abfca156d24eac5552e

Observation c6705125-f822-46e2-b6a2-4aba96451bfe · outbound

This paper cites Aihara et al.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Aihara et al

Reference 3

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.831031Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.366974Z digest=sha256:1746e12a8a687ab2d7e615b88133378e2cd9665a40d1a2f9a946ea0adb93bb83

Observation cb4c68c0-81c7-44a3-8f98-ef6d0b0daf9d · outbound

This paper cites Wasserstein gan.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Wasserstein gan

Reference 4

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.807403Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.372911Z digest=sha256:84be6130c4e16b524af754fde1587e1d209e11af22e44d4bef2ea199ac3febcf

Observation 5605534b-aaad-4674-a982-83a982283db4 · outbound

This paper cites Conselice.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Conselice

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.378668Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.378668Z digest=sha256:a1c6c25386c2a9736524c4c7be89eb824def538416d4b4d21236691257ea28b3

Observation be6f004e-427a-4c5f-9294-23c4629c0cb0 · outbound

This paper cites The evolution of galaxy structure over cosmic time.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models The evolution of galaxy structure over cosmic time

Reference 6

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.789376Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.384189Z digest=sha256:2a3393a05fb07f95c2f8a6c9df71df3d36aba1f2c8ec0fd19d4521a5b714fe52

Observation d67ba134-80b1-406a-9e4a-cfad76896d3e · outbound

This paper cites Diffusion Models Beat GANs on Image Synthesis.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Diffusion Models Beat GANs on Image Synthesis

Reference 7

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.768351Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.390161Z digest=sha256:6f0251d97089c3b66199b211d8c70617087bf4c26f1a5d8dee507f7f4aa490b4

Observation 83fcd2df-d074-4980-adf0-61b5f801b11d · outbound

This paper cites Jane Wang.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Jane Wang

Reference 8

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.748698Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.395368Z digest=sha256:aae9e2aefba5f906925db9f71bae7b3bc750ea713526138aa292ea1797b462ad

Observation 922ae7dc-ac94-4565-a144-b29edeeacea9 · outbound

This paper cites Galaxiesml: A dataset of galaxy images with matched redshifts.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Galaxiesml: A dataset of galaxy images with matched redshifts

Reference 9

Resolution
verified exact
raw_fallback, observed 2026-08-12T11:16:59.368455Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.400485Z digest=sha256:7083a33ce21890fe4b690168bd1b10c6bef3a617302b9f8aad3b47e4d30e6d15

Observation 6739b066-82b8-4760-a46f-de0ca8b316a9 · outbound

This paper cites GalaxiesML: an imaging and photometric dataset of galaxies for machine learning , June 2024 b.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models GalaxiesML: an imaging and photometric dataset of galaxies for machine learning , June 2024 b

Reference 10

Resolution
verified exact
doi, observed 2026-08-12T11:16:58.728247Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.405332Z digest=sha256:cd6409543a6ef6626a9c2edc424380818a0bbfaf2be51af309c413a87bc0cd1b

Observation f0dcdb3d-829a-4bec-b332-0d41c00ab3ef · outbound

This paper cites Taming transformers for high-resolution image synthesis.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Taming transformers for high-resolution image synthesis

Reference 11

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.725674Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.410616Z digest=sha256:a2bbf567ba4e7ea97d1acd15b67ca6e7ce0a0ee9ee1e240b2030e32c1e4d0256

Observation 83d9b1f1-d701-4254-afc8-419899ee4927 · outbound

This paper cites Goodfellow, Jean Pouget-Abadie, Mehdi Mirza, Bing Xu, David Warde-Farley, Sherjil Ozair, Aaron Courville, and Yoshua Bengio.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Goodfellow, Jean Pouget-Abadie, Mehdi Mirza, Bing Xu, David Warde-Farley, Sherjil Ozair, Aaron Courville, and Yoshua Bengio

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.417284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.417284Z digest=sha256:a0a8d438a4c6ef0d6a735d88ddb10dab1b60777635c5fe38e0140075e59e957c

Observation 71fe534b-0fa6-4fa9-b2fb-5491891193e9 · outbound

This paper cites Gaussian Error Linear Units (GELUs).

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Gaussian Error Linear Units (GELUs)

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.422058Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.422058Z digest=sha256:1bf0c324042d39d4612cc6c57b58cce80d0a75ab7f7a29148faa6a367976c4aa

Observation dfc4fc5b-a89a-405f-ab09-ce1199c25042 · outbound

This paper cites GANs Trained by a Two Time-Scale Update Rule Converge to a Local Nash Equilibrium.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models GANs Trained by a Two Time-Scale Update Rule Converge to a Local Nash Equilibrium

Reference 14

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.692433Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.428397Z digest=sha256:2d1fc39313c7b35fd0f83d175c3e8ab39e0b138fc28f1950e5dc09019d2afaf8

Observation 14291387-0bb6-4e67-a995-f27e47cf5007 · outbound

This paper cites Second data release of the Hyper Suprime-Cam Subaru Strategic Program.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Second data release of the Hyper Suprime-Cam Subaru Strategic Program

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.435799Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.435799Z digest=sha256:b177c34aac5a017c4ab4d02c8e6df857c66f9f179d69f63c36324ffbfc5fb7dc

Observation f767c8b4-9106-48d8-bc4c-ec9bde1647bb · outbound

This paper cites Denoising Diffusion Probabilistic Models.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Denoising Diffusion Probabilistic Models

Reference 16

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.671846Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.440905Z digest=sha256:7ed28ba80eab380890b8c4b1a579a5e98bd24a268de276c64d8a9c086dd8a82d

Observation 3115ce72-c07f-4d4a-981a-7a21cba152db · outbound

This paper cites Denoising diffusion probabilistic models.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Denoising diffusion probabilistic models

Reference 17

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.645317Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.446053Z digest=sha256:4818915ee144062f89fae4e2d05c8dac89f36219c0acb059c57874e7b0d8ce64

Observation 8e548572-fe7e-4879-a85d-dfdd4438a71e · outbound

This paper cites Better Prompt Compression Without Multi-Layer Perceptrons.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Better Prompt Compression Without Multi-Layer Perceptrons

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.451038Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.451038Z digest=sha256:9e1a2623c95870a4ed3c7123a83e211050c7e3ca6b14d6fc9bd32fecfd9f3414

Observation 1c7dbae7-a9d1-43f0-8dbb-97f325f1a675 · outbound

This paper cites Unlocking the Potential of Text-to-Image Diffusion with PAC-Bayesian Theory.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Unlocking the Potential of Text-to-Image Diffusion with PAC-Bayesian Theory

Reference 19

Resolution
verified exact
local_arxiv, observed 2026-08-12T11:16:59.219706Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.456615Z digest=sha256:49d1719f47278eb87935ce385a9ef7000acdb501a3a49461725d68af45db7044

Observation 83923430-7124-412d-9700-6d76ce73e8d0 · outbound

This paper cites Analyzing and Improving the Training Dynamics of Diffusion Models.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Analyzing and Improving the Training Dynamics of Diffusion Models

Reference 20

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.624811Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.463233Z digest=sha256:a9df9a3d97312dd4c9bb76ca5460456423f3df669eee026ce5301f6e41760f47

Observation 78416ac9-73c9-472f-8116-4f1b8aed8254 · outbound

This paper cites Auto-encoding variational bayes.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Auto-encoding variational bayes

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.468259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.468259Z digest=sha256:11b517d732f6169d64945af6b5e11bcce0b954f0d8725dae67015490e54aa22b

Observation 4fea6320-0a81-4960-a8f5-ecfa1a18cc7b · outbound

This paper cites Latent plan transformer for trajectory abstraction: Planning as latent space inference.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Latent plan transformer for trajectory abstraction: Planning as latent space inference

Reference 22

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.583238Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.473591Z digest=sha256:c14f2a28c2753b3f07e5a587ec8c110adb6a484bb8fb9f9a3876a3c41fa3d66b

Observation 4fcb3fc1-48a3-4cdd-8863-1d884410fd64 · outbound

This paper cites Kuijken et al.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Kuijken et al

Reference 23

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.564244Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.478887Z digest=sha256:0198a969828065f6fe24aa9bab3c1d832186d416c9e4a81cb41842e18c181326

Observation 5a9e660f-b244-4be1-90a6-f98b52c923f4 · outbound

This paper cites Deep generative models for galaxy image simulations.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Deep generative models for galaxy image simulations

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.483747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.483747Z digest=sha256:acbffcd62e4b05fe630b9824750201259dfeb6eb3b6026d0b48088f06ca13481

Observation 0da81623-2d34-4ed2-816f-9d68a49a4c1d · outbound

This paper cites Lastufka, M.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Lastufka, M

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.489183Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.489183Z digest=sha256:7fd1199b8e499410d0613d6e2129d92a0c0852020b14af3771d6b281f64385a8

Observation 3aa3f67e-82e1-40e8-9b64-a5f3b7f8eaa1 · outbound

This paper cites Distributionally Robust Receive Combining.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Distributionally Robust Receive Combining

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.493895Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.493895Z digest=sha256:af7fdc9c6ce4ce23250e8ca51b5e63a6c6e4cc9aa1f0e771ef6040ec0e7260ae

Observation 13c3a6dc-d8d0-458f-94c9-5b44560fbb57 · outbound

This paper cites Using Galaxy Evolution as Source of Physics-Based Ground Truth for Generative Models.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Using Galaxy Evolution as Source of Physics-Based Ground Truth for Generative Models

Reference 27

Resolution
verified exact
local_arxiv, observed 2026-08-12T11:16:59.073323Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.499457Z digest=sha256:bc7677046b2a47003dd44547756f54a5a5c11202c2b17cf00b3490d12d7de876

Observation 1af3b4c3-a948-4341-bf7a-b374c06db36a · outbound

This paper cites Rl isn't enough.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Rl isn't enough

Reference 28

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.545098Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.505144Z digest=sha256:5d9d8da523d089948a61af78190080a281827c4c56f08d5b2a5b0ee4136bc708

Observation e75ccadd-ffcb-4182-95b4-4119cbeb7934 · outbound

This paper cites an unresolved cited work.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Unresolved cited work

Reference 29

Resolution
unresolved
raw_fallback, observed 2026-08-12T11:16:59.525374Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.510396Z digest=sha256:72448232673a35670ec12fc87458583b5197ef0cd127a34277ec432448a50035

Observation 3b8e1afa-7137-4ae4-b9a8-4887c2be14eb · outbound

This paper cites Narr, Kirsten A.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Narr, Kirsten A

Reference 30

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.502755Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.515514Z digest=sha256:494bed9fc889074ff950491f41124bf82d330597a68ee7b233a979ba5c582f39

Observation 9e9171ce-9ddf-4803-94cb-976e6880e665 · outbound

This paper cites Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.520134Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.520134Z digest=sha256:09abf621b9aa2b37a1538386d2df8df9e9684c2e1e31d0bfddc7ff8fe7dcf0e8

Observation 5f00f204-a1d8-4c79-8b9c-2ba1f019aaa2 · outbound

This paper cites an unresolved cited work.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Unresolved cited work

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.524853Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.524853Z digest=sha256:f052e52dcc4bb8ba05f41692ac5a942174d277c36967b9443cb77874a7165841

Observation f580076c-de76-4624-8080-4a6d04f716f8 · outbound

This paper cites Decoupled weight decay regularization.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Decoupled weight decay regularization

Reference 33

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.474634Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.529773Z digest=sha256:8ae2f4c2f34a5070a92d4074762ecb8069d0d7b65b38a6eeddb99969e988fcab

Observation 833acd25-4d51-4a2b-a5b6-6197b50909f5 · outbound

This paper cites Lotz, Patrik Jonsson, T.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Lotz, Patrik Jonsson, T

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.534449Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.534449Z digest=sha256:339ec5b416b75139446740ad0dae72c62c22a7c7a13752cf6985b8858455e6b1

Observation a7891577-522c-4c6b-9791-1c461350e73f · outbound

This paper cites Cosmic Star-Formation History.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Cosmic Star-Formation History

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.539185Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.539185Z digest=sha256:3a35b280af127da6fd3336a1c3e4a116a722ce3d82e801067d309ead2d80b5d8

Observation d9a265e5-ae08-4bda-b9ac-0dc05e271dc5 · outbound

This paper cites Detecting outliers in astronomical images with deep generative networks.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Detecting outliers in astronomical images with deep generative networks

Reference 36

Resolution
verified exact
doi, observed 2026-08-12T11:16:58.675682Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.544392Z digest=sha256:cc65abc9e20a71402be3877e35859104c219b6b6e7d00f2ecbb375a7da0a030e

Observation 2e2dc1eb-4818-4ae3-a1ba-7b7d38470f79 · outbound

This paper cites How DREAMS are made: Emulating Satellite Galaxy and Subhalo Populations with Diffusion Models and Point Clouds.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models How DREAMS are made: Emulating Satellite Galaxy and Subhalo Populations with Diffusion Models and Point Clouds

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.549777Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.549777Z digest=sha256:bf7453a14d4279380dbf6114022668edf114fa60b74d809f4b603ab70b17858e

Observation cd2a02b8-06c7-4fbf-972d-6dc4f05ad3af · outbound

This paper cites Improved Denoising Diffusion Probabilistic Models.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Improved Denoising Diffusion Probabilistic Models

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.555634Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.555634Z digest=sha256:0628b14854ce4c0af280214843241b07e550290278c449354121b68a9a9f1230

Observation 9c69f5a5-e38b-4473-8e31-9799503811aa · outbound

This paper cites Photometric Redshifts for the Hyper Suprime-Cam Subaru Strategic Program Data Release 2.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Photometric Redshifts for the Hyper Suprime-Cam Subaru Strategic Program Data Release 2

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.561162Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.561162Z digest=sha256:a86bf5cdc03859f3291dbef067570e433c286a41ed142c6f2c15b6e5579fe71f

Observation ea8f4855-df11-4e7f-ab05-cf6e211d96c2 · outbound

This paper cites an unresolved cited work.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Unresolved cited work

Reference 40

Resolution
unresolved
raw_fallback, observed 2026-08-12T11:16:59.453854Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.566276Z digest=sha256:4d2fc36054440d3fe537a9b932f1589f6a9f2f9066ecbde455d502d11556bce5

Observation f5fa1eac-536f-452d-9ae6-3d08d16c6f96 · outbound

This paper cites Monitoring primitive interactions during the training of dnns.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Monitoring primitive interactions during the training of dnns

Reference 41

Resolution
verified exact
doi, observed 2026-08-12T11:16:58.658352Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.571225Z digest=sha256:8e906b68f26d5cfce628a6b71f5549da2353e8f5642dcf33590e3625105553a2

Observation 48a8ecb4-02ed-4da7-9957-50fca52e5a19 · outbound

This paper cites Realistic galaxy image simulation via score-based generative models.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Realistic galaxy image simulation via score-based generative models

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.575996Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.575996Z digest=sha256:c39c9045725346415b2ff4b2b25df1ab175094ccbd13edad1faf8a51f3908623

Observation 2a7b661a-5143-48dd-8298-5aeae3d1c0c3 · outbound

This paper cites Deep unsupervised learning using nonequilibrium thermodynamics.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Deep unsupervised learning using nonequilibrium thermodynamics

Reference 43

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.426189Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.580843Z digest=sha256:78664310fe16da4ef952d53187211c357a290316358200f15a514780523040b1

Observation ec8ecdd4-fa9d-431a-8361-ca4dd46bb17f · outbound

This paper cites Weiss, Niru Maheswaranathan, and Surya Ganguli.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Weiss, Niru Maheswaranathan, and Surya Ganguli

Reference 44

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T11:16:59.401463Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-12T11:16:58.586839Z digest=sha256:034dae0d917e33b223a63d3f2772436885f2f89345583b52441fc9e6d0507137

Observation 85a16c35-056c-4b84-9354-922ef8d0b578 · outbound

This paper cites Denoising Diffusion Implicit Models.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Denoising Diffusion Implicit Models

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.591721Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.591721Z digest=sha256:4629a3342d4dbb5573efd25dd6112b59cc28b8abb6fcf69eac39f96004cc9b67

Observation 01f41f1d-4588-402d-bb2c-f876f7596a00 · outbound

This paper cites Diffusion Models for Probabilistic Deconvolution of Galaxy Images.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Diffusion Models for Probabilistic Deconvolution of Galaxy Images

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.596861Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.596861Z digest=sha256:728cf42901af7af734eb29b573213bb0670a57a655cfce6800a69f61877d00ff

Observation f68b0f17-d5f9-4f7a-ad93-bc122d2aa7b0 · outbound

This paper cites Think Twice Before You Act: Improving Inverse Problem Solving With MCMC.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Think Twice Before You Act: Improving Inverse Problem Solving With MCMC

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.602053Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.602053Z digest=sha256:1c444be5684912adacd45c14af1a262d13a8edc71d8bc410c333dbbec7b33aac

Pith citing papers

Observation 9e9171ce-9ddf-4803-94cb-976e6880e665 · inbound

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models cites this paper.

Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-12T11:16:58.520134Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:16:58.520134Z digest=sha256:09abf621b9aa2b37a1538386d2df8df9e9684c2e1e31d0bfddc7ff8fe7dcf0e8

Observation 70d48cad-bee6-484d-9185-10cbfb7bee75 · inbound

Diffusion-based Galaxy Simulations for the Roman High Latitude Survey cites this paper.

Diffusion-based Galaxy Simulations for the Roman High Latitude Survey Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models

Reference 21

Resolution
metadata mismatch
arxiv_id, observed 2026-05-11T20:11:12.419379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-08T09:59:02.257428Z digest=sha256:f44ddfa0be6a0d94e8230b3711e67f83fc2d6afa0a7c97eeb638dc79998925d9

Observation 3d9e6d79-51b7-47d2-b399-abd5e79d6524 · inbound

Accelerating Redshift-Conditioned Galaxy Image Synthesis with One-step Generative Modeling cites this paper.

Accelerating Redshift-Conditioned Galaxy Image Synthesis with One-step Generative Modeling Understanding Galaxy Morphology Evolution Through Cosmic Time via Redshift Conditioned Diffusion Models

Reference 39

Resolution
verified exact
arxiv_id, observed 2026-05-19T22:12:50.735011Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-19T22:09:58.701479Z digest=sha256:3bc94b4a43f83ac1980dd215f73515ebbf846211a81abae9ba814ce0186d1960