Pith. sign in

Paper Citation Record · LEDGER

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels

As of 23 August 2026, this Paper Citation Record lists 100 of 119 outbound references and 6 inbound Pith citation observations for arXiv:2505.22186.

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

pith.paper-citation-record.v1
2505.22186 v2

Coverage vector

measured 100 of 119 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T13:20:54.676964Z

measured 106 of 106 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 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T20:44:03.718689Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

100 of 119 outbound references displayed

  • verified exact0
  • verified fuzzy27
  • unresolved73
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation 57d54978-f3ed-4c08-86ca-029b2bad8e9f · outbound

This paper cites , " * write output.state after.block = add.period write newline.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels , " * write output.state after.block = add.period write newline

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:43.556899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:43.556899Z digest=sha256:f87f3e847de99c0884d7bd70fc43094eae31c3d021adb16609e0f0de06aed871

Observation 9ef9e9de-c4c8-40a7-ab0e-35189cbee5de · outbound

This paper cites write newline.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels write newline

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:43.610065Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:43.610065Z digest=sha256:0a7e79cff2cfe021254b1eaffce86ce132960869f49ef7f79c5eb486ba8a2695

Observation 599cc4b1-0864-48e6-808b-a6759dfa73c7 · outbound

This paper cites L., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels L., et al

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:43.670402Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:43.670402Z digest=sha256:c96f437c5a15ef397f001107efcddd64277d762937d83de071666233d08c466d

Observation 59597a7e-55a2-4931-a1d1-17b709d3d40e · outbound

This paper cites & Foreman-Mackey , D.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels & Foreman-Mackey , D

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:43.794959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:43.794959Z digest=sha256:4d2e937b097818cb84f64005e6b9bc7aa9ab4362d8988683ff9d711c2a877ec1

Observation df546a97-b25e-4dc7-bf1e-572a34e4d113 · outbound

This paper cites K., Gao , P., Adams Redai , J., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels K., Gao , P., Adams Redai , J., et al

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:43.968609Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:43.968609Z digest=sha256:a8e9ee28851c7b7e8865291cb1d5d3b9c5c7c744741b0e51485f0341f76e1e01

Observation c343a4a1-e0bb-4c8e-99aa-47033f9dfb8a · outbound

This paper cites 2011, in Astronomical Society of the Pacific Conference Series, Vol.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2011, in Astronomical Society of the Pacific Conference Series, Vol

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:44.100287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:44.100287Z digest=sha256:dd03e7ee9c068c569deb136786966efd87c181846dad87ac6112c8caec92974b

Observation bb6f34ab-8fe9-4f58-bb1f-a1cc014e0715 · outbound

This paper cites 2018, in Handbook of Exoplanets, ed.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2018, in Handbook of Exoplanets, ed

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:44.245824Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:44.245824Z digest=sha256:7069b69a3503cc1029b0793068c46fe23da67cd15009c6bf6f39b964004a3467

Observation 3f6e86ec-2fbc-4a09-b959-ceec39dcd4f7 · outbound

This paper cites M., Lim , P.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels M., Lim , P

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:44.332820Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:44.332820Z digest=sha256:e0ad4530117f09cd6dc5c2f18a85eb62fd11b490d16c47db0ba9b6e13f154364

Observation 9e7c6953-a56f-433d-9ad7-949b34532925 · outbound

This paper cites C., Buchhave , L.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels C., Buchhave , L

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:44.419600Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:44.419600Z digest=sha256:c8af3cd0d0895f110bb62b06f29db1fc01a673c487c6947013f8cf0ce5669ab7

Observation ecc65d56-4818-4739-9f9a-69ef6a3539ea · outbound

This paper cites K., Gressier, A., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels K., Gressier, A., et al

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:44.519852Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:44.519852Z digest=sha256:6645250f9db50a4ea0c98d2a9fc2181b5efe66c8dced1371890f6e11ebb9aeb2

Observation 4b9c6ae1-bd5e-47dd-a456-3b129278a1a3 · outbound

This paper cites J., Tennyson , J., Harris , G.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels J., Tennyson , J., Harris , G

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:44.580691Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:44.580691Z digest=sha256:bbe6af94d3feb35f949282fe057ca21300e3c7ba4d4971ac35655fb93c8c6888

Observation 6fe0175f-fba2-4d0d-ba2d-9fdadcc54509 · outbound

This paper cites J., Crouzet , N., Cubillos , P.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels J., Crouzet , N., Cubillos , P

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:44.676875Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:44.676875Z digest=sha256:24fa0ca6015a85052e5831ffae6ac24191c1419c919cdcf0b870062a2cc379a5

Observation dcf56849-2c49-433b-8cb7-6c2df5cbea79 · outbound

This paper cites A., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels A., et al

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:44.772589Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:44.772589Z digest=sha256:c355dd655a7f69a6ec2daec344f1d75093f85ce11b300d3a801a3e5b1c83b714

Observation 21a51a91-423f-494d-a596-536ac6c42f17 · outbound

This paper cites 2018, JAX : composable transformations of P ython+ N um P y programs.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2018, JAX : composable transformations of P ython+ N um P y programs

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:44.905652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:44.905652Z digest=sha256:fc5a41bc5427cd88ad691a820c7455244d4f4041df8f8d39081eba8a95639496

Observation d79baf17-d5ca-44d9-afc1-8e359091d98e · outbound

This paper cites 2024, astropy/photutils: 1.13.0.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2024, astropy/photutils: 1.13.0

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:45.016872Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:45.016872Z digest=sha256:c027847a5de69fb61b435b83921be218817a625e4ca5ef4d03871884c77d4829

Observation 5546990f-27bf-4344-b8bd-1a47c7532c8b · outbound

This paper cites 2024 a , , 960, L3.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2024 a , , 960, L3

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:45.122758Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:45.122758Z digest=sha256:ebd37e98f6e9ad44419daa05999723afaa05e9a7f1ace431b473021f8a7b08dd

Observation a49a9c40-ef76-4ebd-8cd9-5c756bc89313 · outbound

This paper cites J., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels J., et al

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:45.225435Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:45.225435Z digest=sha256:444b205abe2f80018a81016f2dbe618ed503596d6b37a8365c35cc78145f6db1

Observation 2ce15e29-f51a-4aab-8337-0092abf8f53b · outbound

This paper cites E., Megeath , S.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels E., Megeath , S

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:45.361790Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:45.361790Z digest=sha256:fd33d7ad0d395181fbe7604a8356e59a5b4148c4e5e4be55ba1efe6d385505bb

Observation b08e9c11-2bf1-42c8-9762-ff564a84bc94 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:45.491661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:45.491661Z digest=sha256:6f0ff6f4fe45d1c09d664242f206a856e997ec7ab426eff541025694dccfa70e

Observation fa0623a3-9660-4daa-865e-3df408bf2a84 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:45.528346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:45.528346Z digest=sha256:1ee8b6b170c6d8168d2d7cf26a681b2539b2ed1cdf3c631de8c39e91bf701a77

Observation 4d55e97a-7d96-44cb-a9f8-bb50d83a63d3 · outbound

This paper cites 2024, , 968, L22.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2024, , 968, L22

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:45.694047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:45.694047Z digest=sha256:703acb8acaef78306a09cc929f73ae6719c7b4f1bc88d9dc5f61f8167c05dcb3

Observation 8e9129f1-8f2a-4be3-86af-4f87da913917 · outbound

This paper cites 2015, , 805, 132.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2015, , 805, 132

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:45.797421Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:45.797421Z digest=sha256:5051c25c6778e294de79f8fb800416042f70c238e666aaa36996504cad25105e

Observation f9dd45ed-c9b9-473e-a576-23b4c3758912 · outbound

This paper cites 2016, , 532, 207.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2016, , 532, 207

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:45.892424Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:45.892424Z digest=sha256:179e5e83903c9e125aad49011deadd5cc9d7e6db60ce82007da81f4b03ddb059

Observation 9972618b-e7e8-45bd-bb44-45d1c2bb453f · outbound

This paper cites G., Shivaei , I., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels G., Shivaei , I., et al

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.034249Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.034249Z digest=sha256:5d52892a24eb431a9c13b0e952a33f7539041d74689df76a784abcb6e6eb0463

Observation 55e7275b-23e2-4024-bf03-f19db97fefd1 · outbound

This paper cites A., Irwin , J.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels A., Irwin , J

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.142498Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.142498Z digest=sha256:0efc874b536f263ae5fbcdf9c578bd030b184d016aeeffac58afc4643633fd6a

Observation c49d1cc8-072b-494d-8863-605bd4e4c1cb · outbound

This paper cites 2024, in EGU General Assembly Conference Abstracts, EGU General Assembly Conference Abstracts, 20183.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2024, in EGU General Assembly Conference Abstracts, EGU General Assembly Conference Abstracts, 20183

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.244407Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.244407Z digest=sha256:9717048177667ad5ec27e6af0049f8ecf6dafaa52297f8c4efff161df16fce11

Observation c37072e8-14da-4077-8faf-03fdf5edd68b · outbound

This paper cites S., & Agol, E.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels S., & Agol, E

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.380544Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.380544Z digest=sha256:ef6dc7a908c5981a8cd85c7747fa2af7284dd374123c75e448b3d52804de4b69

Observation 9a5a70f6-2af2-4fd6-869b-8ca8e548c2a2 · outbound

This paper cites P., Sprague , A.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels P., Sprague , A

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.480093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.480093Z digest=sha256:f08aab6580b2ec9900005bd7ad756f737ab885466a2ebe7c307265559e9970d1

Observation de44ceff-9af8-4b12-bf73-3d24407c3a9f · outbound

This paper cites 2022, TransitSpectroscopy.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2022, TransitSpectroscopy

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.573513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.573513Z digest=sha256:4de30e2f72084572e84ba4237d238b6c55bbb0d48fe6dbcbddea23fe91c61871

Observation 5540d1ed-6151-46db-8ce6-aeb3d4707ea5 · outbound

This paper cites 2019, , 490, 2262–2283.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2019, , 490, 2262–2283

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.652546Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.652546Z digest=sha256:1ba07f9977b371f8f59c57fae5031b26be2145cc78bce6ed647b15cbf5e78937

Observation 0e93e5ff-5a9a-402b-9e40-4361ef34fb72 · outbound

This paper cites M., Aigrain, S., Gibson, N., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels M., Aigrain, S., Gibson, N., et al

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.704444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.704444Z digest=sha256:3ba605f3d37bd6c3b6d8bccf038077ee34bbd6fa8c41b9a978b194a59d630b85

Observation 16ef69ad-e9c9-4437-9379-ede402469678 · outbound

This paper cites 2016, The Journal of Open Source Software, 1, 24.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2016, The Journal of Open Source Software, 1, 24

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.829532Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.829532Z digest=sha256:53475e0a014e5a8b6eed574a77bcfe3ac06c73a41828bf81d28e6b18a4e62247

Observation 561c5029-f61f-4392-804c-96323f350734 · outbound

This paper cites 2017, , 154, 220.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2017, , 154, 220

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:46.952451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:46.952451Z digest=sha256:45d1cba20f0b0ec3e72a8587418861b45dcbc92463bcbfd51177fff07fa4e282

Observation bc641659-45b8-484e-a3fb-a10935a0d24f · outbound

This paper cites 2021, exoplanet: Gradient-based probabilistic inference for exoplanet data & other astronomical time series.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2021, exoplanet: Gradient-based probabilistic inference for exoplanet data & other astronomical time series

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.032860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.032860Z digest=sha256:190a2a999468995ee58fafacfdbc9121b199dec3991810bf1378b649e675cb48

Observation 9f4b7dc9-bd82-410a-94ad-f07d43f89b53 · outbound

This paper cites P., Foreman-Mackey , D., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels P., Foreman-Mackey , D., et al

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.180305Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.180305Z digest=sha256:38a90fb385e30752d4da824318a4c0d74d080193739cefdcef91b429524506e1

Observation b35e32f8-b435-49ba-b560-bbccda52e561 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.252220Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.252220Z digest=sha256:34731432bd0913091172ac2a0ef3ff269a589016beb807082c2f1e371968fb7e

Observation 86172b9c-d46c-4c63-93fe-2ae9da1e7179 · outbound

This paper cites 2004, , 611, 1005.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2004, , 611, 1005

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.382407Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.382407Z digest=sha256:6b177122165ec6036367040dd48ead4a8cc8100400af976dc4768e4bdc41d302

Observation 992a82bd-2226-4f3c-9a4b-8e12fb9a3726 · outbound

This paper cites & Rubin , D.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels & Rubin , D

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.424000Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.424000Z digest=sha256:0065ecc79d2e00cae8cd43fbe212d6293dc46323059c48517d463bd77a10805c

Observation 018d9a77-a498-4e5f-a3b0-42ba44ee1cf1 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.514451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.514451Z digest=sha256:57514d0020413e5c4c34633ecaf6610be9c23e8fc0e04c3906ae76f15018e1c2

Observation c2386fa6-3dd0-444d-8a9a-bdfc551b70da · outbound

This paper cites P., Aigrain , S., Barstow , J.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels P., Aigrain , S., Barstow , J

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.567534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.567534Z digest=sha256:653c76f488d03ebc58582aa435d2e2ad6fb382361b21d345ffde93328cd9c351

Observation 6a81f202-efcc-47eb-9d02-23765a1378f2 · outbound

This paper cites P., Aigrain , S., Roberts , S., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels P., Aigrain , S., Roberts , S., et al

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.639988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.639988Z digest=sha256:af742a910e6cbfdd0bd024d083b6b89f1a9b50c6ea573ce9e1bbb0ac82042ba9

Observation 68efb0f8-47f5-41f9-a24e-401db7cfbe14 · outbound

This paper cites H., Bauwens , E., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels H., Bauwens , E., et al

Reference 42

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:09.064886Z

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=2026-08-07T13:20:47.729540Z digest=sha256:5a1ea7fb5a19a7380d734a1fd67b3f62ee6747487e0ceb8ff87215d29d200a44

Observation 773417db-26b3-4522-90f4-41d1d233ed54 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 43

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:21:08.905454Z

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=2026-08-07T13:20:47.792530Z digest=sha256:ec9da7764bd48d4196e2829630ab26c88fe2053767301b648574e2d5c00c9a82

Observation 824a3593-74d1-4599-b1a4-e6bc4e0b06d5 · outbound

This paper cites E., Rothman , L.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels E., Rothman , L

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.870867Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.870867Z digest=sha256:a8f6cf50698d2f1dd2d33b8c3752edc176cb214b1e9788115a69000922f978fd

Observation a25b1f0f-a064-4186-9e91-2945f2378da1 · outbound

This paper cites D., Sloan , G.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels D., Sloan , G

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:47.961971Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:47.961971Z digest=sha256:7a84bde785b2de009903a2f8bc5a7c6a14062a6475204dee0691acbe183d1a9d

Observation f5d90510-0719-42e9-beb9-99e06f6452df · outbound

This paper cites P., Bell , T.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels P., Bell , T

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:48.032047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:48.032047Z digest=sha256:337c78fdb263a5bc6dd9279b8bd6b1617645a6dacf78a03aae70cac7b4416679

Observation 5b07f39f-ae09-467c-8b71-de51549955c2 · outbound

This paper cites H., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels H., et al

Reference 47

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:08.692057Z

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=2026-08-07T13:20:48.181816Z digest=sha256:4f17ee6ea4deb77c79f702e4b490571bb48135227840bd4fbc81750b066b1a78

Observation 1d02a5d2-78f3-4d71-94bd-7d69b2a6ac62 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:48.299244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:48.299244Z digest=sha256:53cdfc50f16eda0b20618d33417e036fc4c862ef892dd9ee14c518af65ea2ee0

Observation cb055d87-57c3-4935-b5df-be8f68d7fb65 · outbound

This paper cites M., Lichtenberg , T., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels M., Lichtenberg , T., et al

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:48.408514Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:48.408514Z digest=sha256:7cb0c3af15af3e8f7b098760dd6d1a171a834d72913e342408fdf5a3114fb6ce

Observation 825af487-152d-4918-a4db-25aa710dc159 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 50

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:21:08.486734Z

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=2026-08-07T13:20:48.618638Z digest=sha256:8d472af2586f6ddadfdb8bba88bb21689d0ee85f22c71030e1bb2ed5777bd0bf

Observation 8f13650e-5ca3-46ea-9258-fd7099ce4fb5 · outbound

This paper cites 1993, Theory of Reflectance and Emittance Spectroscopy, Topics in Remote Sensing (Cambridge University Press).

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 1993, Theory of Reflectance and Emittance Spectroscopy, Topics in Remote Sensing (Cambridge University Press)

Reference 51

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:08.311219Z

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=2026-08-07T13:20:48.748237Z digest=sha256:acacac9b311a65056335860d41698e94fece47593800e2d140d7e3a1b62d0a27

Observation 6f3c778e-e6af-4416-a613-b82b274c5672 · outbound

This paper cites R., Millman, K.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels R., Millman, K

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:48.881584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:48.881584Z digest=sha256:37903162849197190f6a16e56816955d1b4cda7e98b1c95db1f003409b6db53d

Observation 83c70937-a62b-4df8-a83a-10b48e398a7c · outbound

This paper cites 2024, exoplanet-dev/jaxoplanet: Astronomical time series analysis with JAX.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2024, exoplanet-dev/jaxoplanet: Astronomical time series analysis with JAX

Reference 53

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:08.101014Z

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=2026-08-07T13:20:49.031916Z digest=sha256:382495a897aaf096396db1cf24fdbf66c3224133f623115876fc2d2f2c4ba199

Observation f484a396-aea1-4996-bb00-3a106d66ae9c · outbound

This paper cites M., & Kitzmann , D.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels M., & Kitzmann , D

Reference 54

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:07.959330Z

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=2026-08-07T13:20:49.149272Z digest=sha256:a167a84f6c6054a138dabb8b526631125bab2f57a5416d91b11f41e85059c896

Observation 5e4f6ac3-7b34-47f5-88a4-7efacaacee33 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 55

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:21:07.804246Z

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=2026-08-07T13:20:49.265444Z digest=sha256:349c384eca04c55447941b915a66aa89e91ce3e356b197158a966203b63683bc

Observation 1dd50fc1-1480-42cd-9a60-c0f0062da19c · outbound

This paper cites 1986, , 98, 609.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 1986, , 98, 609

Reference 56

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:07.642406Z

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=2026-08-07T13:20:49.370072Z digest=sha256:14471eec1008d807e7d8d65adb411b92c92baaa61f9c0acf4f6712d6371eab9d

Observation 20ea0471-fcde-4502-aa83-aadb65948bbd · outbound

This paper cites 2024, , 630, 609.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2024, , 630, 609

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:49.536973Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:49.536973Z digest=sha256:bdfec7b5fdb2a633f715c77618629476275054aef0e6a5b30bac69a222ce810c

Observation ab32ac1c-e9dd-459b-ad8a-4f52f66418c7 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:49.696753Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:49.696753Z digest=sha256:2c323b9e66912469705c141a0f6683f472da97600878c66c985bd040ff73d3dd

Observation 8695db2d-e3e6-4a74-93bd-1c9feadceaa4 · outbound

This paper cites & Kempton , E.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels & Kempton , E

Reference 59

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:07.518519Z

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=2026-08-07T13:20:49.832173Z digest=sha256:56bd2c7d5b9b11b1c71e39234f73c663701002bd82b619ef89c92e3adf95fd1c

Observation 7caa29b8-ec46-44e3-8d9e-8983091ebe1b · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:50.007514Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:50.007514Z digest=sha256:ea577dbe2273498df211ab7841c811251a2fa69b1baf32ed8a800aa4321486e9

Observation ee121d4c-f1f7-47b1-9bd8-f537fcb2eec8 · outbound

This paper cites G., Krick , J.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels G., Krick , J

Reference 61

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:07.337968Z

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=2026-08-07T13:20:50.166679Z digest=sha256:927f9c1bd387c343efcd2d26d8d9a26cf4ca5dbd2b560fb9f4e2a233cdafcf96

Observation e29dcc79-de15-405f-b614-541075fa2f71 · outbound

This paper cites S., Kjærulff, U., & Kong, A.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels S., Kjærulff, U., & Kong, A

Reference 62

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:07.203846Z

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=2026-08-07T13:20:50.228952Z digest=sha256:f5588ecef9b0b1ad34169dfafeb800e93cbcef671aaacd40a247fb1a0941c968

Observation de0543d0-d990-4e07-bcc5-3630780f49de · outbound

This paper cites 1997, Icarus, 129, 450.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 1997, Icarus, 129, 450

Reference 63

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:06.986575Z

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=2026-08-07T13:20:50.275995Z digest=sha256:a228506a8702de28895d7852249ac53ac945ecbe151b6ca50065abaa45a5bb72

Observation 731b74b7-eaa3-449b-999e-cf01bef42781 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 64

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:21:06.845164Z

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=2026-08-07T13:20:50.347855Z digest=sha256:e35d0fd949519c6b44a3aca1ec5d61dc335196841f3912c9b32c0036e2b77115

Observation d41c416f-d82d-4f5c-ac21-c80e57aaf1c9 · outbound

This paper cites A., Charbonneau , D., Allen , L.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels A., Charbonneau , D., Allen , L

Reference 65

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:06.665455Z

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=2026-08-07T13:20:50.440644Z digest=sha256:f7db24a0004b60d861998a590bf03763c21eb82203d2f4d5d5e437a009afd7a2

Observation 0e10a751-0150-4a25-bf84-e3814c00a676 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:50.560932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:50.560932Z digest=sha256:24a59378f9ba7e1ea6582e53fcdb5818c1111b3c64713422ce879575afc55347

Observation 61d1478c-8e7e-4d26-b548-15eea2aa3d3c · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 67

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:21:06.396200Z

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=2026-08-07T13:20:50.657571Z digest=sha256:921024014bfa912eef8275ff62adfdcac0e73c3e5e46b1611b10a84c2c07f91b

Observation 0074599b-ae53-4952-a061-8616686eee76 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 68

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:21:06.104656Z

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=2026-08-07T13:20:50.749987Z digest=sha256:2f31657099866b59588df49b009e95cbb2944fa43f1087cf29633fe71541a4aa

Observation fbe26f81-b1b6-432b-a9fc-7af2e81e5b4a · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 69

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:21:05.912240Z

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=2026-08-07T13:20:50.837043Z digest=sha256:981e321b378194805df581e41f8067bbf618de08d2386a827c0f99d874752ec6

Observation 0d32b2e6-3618-4bea-9de3-28af97be2d57 · outbound

This paper cites 2019, Journal of Open Source Software, 4, 1143.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2019, Journal of Open Source Software, 4, 1143

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:50.921645Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:50.921645Z digest=sha256:1333a706a05d3b7596b4f5d5ec1e0b89d213e0ebe8a07b85d026b4726dc3054c

Observation 19a60831-9687-46b2-a4f8-ec8166c5ca51 · outbound

This paper cites & Barnes , R.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels & Barnes , R

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:50.995648Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:50.995648Z digest=sha256:55bd9aaf2f44d44092f62db8635ed67f6bfa4bde0ad1d7f4249016afab5980fa

Observation 6efcee86-da14-4065-9439-cc15be1814f9 · outbound

This paper cites S., Eastman , J.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels S., Eastman , J

Reference 72

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:05.668139Z

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=2026-08-07T13:20:51.101866Z digest=sha256:1c2b35ab71b76f330d8292a10a582c59c8744c7827d08b5849d26942b4aef3fe

Observation cdd21295-f22a-4384-9b70-0f945ca88bc8 · outbound

This paper cites M., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels M., et al

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:51.289550Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:51.289550Z digest=sha256:81f238f9b19251dbf5efb2cdc3317da25d2c6a825a74a21a0b4f75e4184fdce0

Observation 5326656d-4fd7-4c4c-a34c-bbe615e28741 · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 74

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:21:05.421026Z

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=2026-08-07T13:20:51.401028Z digest=sha256:550a71cddd2cfd178e012f8ec5d44bffd2b50fae1f5d6222a21c884d08d49058

Observation 605797de-281f-4689-b68e-eecf26041e18 · outbound

This paper cites M., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels M., et al

Reference 75

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:05.217661Z

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=2026-08-07T13:20:51.539667Z digest=sha256:212df583606b3fae51bd1e431d0e62fda2a4d00e3da1ad0a199bf1cdb4aadfa3

Observation bddc4586-56d2-4056-ac9d-4f2766f8c8fa · outbound

This paper cites & Agol , E.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels & Agol , E

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:51.649416Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:51.649416Z digest=sha256:8a6ac8d57f55fe1d2ce88a96968f7495eed5686ebc7cf14fa5ccb7bd8bb023c6

Observation 09e2a907-08d0-4f76-ae9f-47406c46616e · outbound

This paper cites S., Hu , R., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels S., Hu , R., et al

Reference 77

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:05.032023Z

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=2026-08-07T13:20:51.810507Z digest=sha256:00c6455dce2a3dc57a00553c0498026aae903c8ee931b12c578e430e85de6209

Observation 42eee69a-9f50-4599-85e1-bf35273fa478 · outbound

This paper cites Hot Rocks Survey II: The thermal emission of TOI-1468 b reveals a hot bare rock.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Hot Rocks Survey II: The thermal emission of TOI-1468 b reveals a hot bare rock

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:51.881976Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:51.881976Z digest=sha256:343ef4393dfcda3d00e08a6989bfa3e924b9a2c953e2b1e8660094c41c0d0a60

Observation f4656c83-837e-42bc-a635-71af9ad88800 · outbound

This paper cites A., Astudillo-Defru , N., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels A., Astudillo-Defru , N., et al

Reference 79

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:04.880850Z

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=2026-08-07T13:20:51.973353Z digest=sha256:7ad9ff14010f4be3209c649a99cffe37a25f5c238e1dd29ff0917b90a3761b7b

Observation 4b604a90-69cf-46f3-9d5d-d41ac1e9b883 · outbound

This paper cites C., Ninkov , Z., & Forrest , W.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels C., Ninkov , Z., & Forrest , W

Reference 80

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:04.731312Z

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=2026-08-07T13:20:52.042850Z digest=sha256:04f3d07ecf1e53c0ff8057c2e5a9ccccdf9b0493e39bc47ba999b2a773aec627

Observation 145d57c4-1675-4852-b50b-c8bcd2ea002f · outbound

This paper cites 2015, , 808, 56.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2015, , 808, 56

Reference 81

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:04.584146Z

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=2026-08-07T13:20:52.127901Z digest=sha256:d30e2edc46e14609f2a589a8cd9e9754fe5cc94d62d64a728ae67c7907efd3c3

Observation 1fe05c8f-dfeb-478d-b9ab-f2b840faaf48 · outbound

This paper cites P., & Tinetti , G.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels P., & Tinetti , G

Reference 82

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:04.482825Z

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=2026-08-07T13:20:52.254262Z digest=sha256:30ce739a587fde8f52fa66c967ee09e7ec481bbf4feb6a84eaf37336ef6a3450

Observation e57fee6f-8549-48d7-8164-4606384b1ea3 · outbound

This paper cites P., Tinetti , G., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels P., Tinetti , G., et al

Reference 83

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:04.249419Z

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=2026-08-07T13:20:52.335748Z digest=sha256:9dad38ffd531290e62125d8a2440c5abcfa136d5c8e664a88186b146bc25ac0a

Observation 6445e785-a5ee-4bed-b1b7-07124141d6f4 · outbound

This paper cites E., Dicken , D., Argyriou , I., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels E., Dicken , D., Argyriou , I., et al

Reference 84

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:03.930095Z

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=2026-08-07T13:20:52.449911Z digest=sha256:0e8f1585e8d24325e7a4074791a7e4706fa4117bb73593efc8aa71bea913065a

Observation c0c3d8c9-eaca-474c-88b5-a8330b61032c · outbound

This paper cites E., Dicken, D., Argyriou, I., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels E., Dicken, D., Argyriou, I., et al

Reference 85

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:03.680150Z

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=2026-08-07T13:20:52.565983Z digest=sha256:6b8c01f2f9b933d2ae4b3ad94b405cf6f8244dc43f5a5f851b5c4de86044b123

Observation 62ac1885-fdc0-4b82-9d7a-25119502db4c · outbound

This paper cites an unresolved cited work.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Unresolved cited work

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:52.691132Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:52.691132Z digest=sha256:19b89625659169f6beda1f4771b0e188e18ea692bc52441c99bed2be1c0b7253

Observation 8f3d9433-cce1-4006-ac5a-c5a23782fe2e · outbound

This paper cites 2020, pandas-dev/pandas: Pandas.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2020, pandas-dev/pandas: Pandas

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:52.767636Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:52.767636Z digest=sha256:1462ba40901f88d17fdac213353c7725169b42684b8bf7805153c31a4da24dc1

Observation 51ef0980-df18-4ff0-807d-260076b438bc · outbound

This paper cites Population-level Hypothesis Testing with Rocky Planet Emission Data: A Tentative Trend in the Brightness Temperatures of M-Earths.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Population-level Hypothesis Testing with Rocky Planet Emission Data: A Tentative Trend in the Brightness Temperatures of M-Earths

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:52.867601Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:52.867601Z digest=sha256:38b5bf1dc63d161c022a3f0742ae2a7f5e615504894d6daa7db5c53c1b0e807b

Observation b31696e3-1f7c-4f16-a898-05294da1a2a7 · outbound

This paper cites The Receding Cosmic Shoreline of Mid-to-Late M Dwarfs: Measurements of Active Lifetimes Worsen Challenges for Atmosphere Retention by Rocky Exoplanets.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels The Receding Cosmic Shoreline of Mid-to-Late M Dwarfs: Measurements of Active Lifetimes Worsen Challenges for Atmosphere Retention by Rocky Exoplanets

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:53.005968Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:53.005968Z digest=sha256:a0944f86f607ddf63c7435ba928f623d124b7ee7f2aad035637b8655836ce709

Observation 4b388896-05ab-4fd1-a846-4c0218fcd90e · outbound

This paper cites A., Brandeker , A., Kitzmann , D., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels A., Brandeker , A., Kitzmann , D., et al

Reference 90

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:03.348256Z

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=2026-08-07T13:20:53.207845Z digest=sha256:1fc2e4f9c67924b878bbc9434aa4063f8d69bb7e1bd7beb2da526a0336417536

Observation b03b55bf-1f9a-48b7-83bf-a11b90c97fa8 · outbound

This paper cites & Granger, B.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels & Granger, B

Reference 91

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:03.173830Z

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=2026-08-07T13:20:53.362545Z digest=sha256:1d84a002d50c6d59c9d1bd880dd4f3bfd08751c1baea6a57d60043441039c4df

Observation a84da7b1-eb29-476b-8a9c-e89c441c8b5e · outbound

This paper cites D., Sivaramakrishnan , A., Lajoie , C.-P., et al.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels D., Sivaramakrishnan , A., Lajoie , C.-P., et al

Reference 92

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:03.043727Z

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=2026-08-07T13:20:53.515816Z digest=sha256:2df224ff46a9d858b17c15fb673ca26499cbd5c92f52f301f48d8cf3ce31700b

Observation fa4a3148-38f1-46b6-89e1-b5cd83ac3d78 · outbound

This paper cites V., Apai , D., & Giampapa , M.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels V., Apai , D., & Giampapa , M

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:53.676651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:53.676651Z digest=sha256:85f85b234510ef37da3e612ef14ef7665aa5457a9d12a41459031e7cb41b5dcc

Observation 08688e25-72af-4e75-a4c6-8c6cfcc5a859 · outbound

This paper cites 2013, in Advances in Neural Information Processing Systems, Vol.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2013, in Advances in Neural Information Processing Systems, Vol

Reference 94

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:02.972083Z

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=2026-08-07T13:20:53.833030Z digest=sha256:3b756edba0b60d401f92e227e8d22cd20e9f61f2f43fe687e86c9ad8366d1e04

Observation ac3aad1b-808a-4f24-a080-4b096df3465f · outbound

This paper cites Report of the Working Group on Strategic Exoplanet Initiatives with HST and JWST.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Report of the Working Group on Strategic Exoplanet Initiatives with HST and JWST

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:53.947044Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:53.947044Z digest=sha256:73470cd284a81ab48d788c386f742db70c4ca6d3443cd33ecc5f83d25d036445

Observation 31210914-a99b-4891-9dbe-bc1fe374c66c · outbound

This paper cites 2023, , 135, 048001.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels 2023, , 135, 048001

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:54.072244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:54.072244Z digest=sha256:06e1f1ef03cc22373fd5bfd75eed867dc524559d06fec02df583c6391efc4acf

Observation afa2ce31-5c20-47f2-b369-b56cf1c1719e · outbound

This paper cites S., Gordon , I.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels S., Gordon , I

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:54.266734Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:54.266734Z digest=sha256:fc4fcd19be7302717f22257d37640fcc18f9e657a130e66bf5f5bc8d88ce161d

Observation fb33b970-7f8f-4e7f-9d74-77eab78eb2b6 · outbound

This paper cites V., & Fonnesbeck, C.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels V., & Fonnesbeck, C

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-07T13:20:54.380684Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:20:54.380684Z digest=sha256:87e4afb5cc09947a6fe9d5026fdbdd0a29e186b492b8721c8013a6ba0c7aeb34

Observation fadb3cfd-91c4-481c-816c-5e5a1fd2d531 · outbound

This paper cites Z., Feinstein , A.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels Z., Feinstein , A

Reference 99

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:02.793796Z

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=2026-08-07T13:20:54.542689Z digest=sha256:44c3b3252b9100f791da6101f9b5dc0a9a4ba0aabf94b17e544570ddce0995b9

Observation 7d5963ef-5de1-49d8-a088-30ff888314e9 · outbound

This paper cites D., & Forget , F.

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels D., & Forget , F

Reference 100

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:21:02.462446Z

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=2026-08-07T13:20:54.676964Z digest=sha256:b366124d567dc5b408850982781280c5cde6fd3ffedc61b371da5669a9d4c72a

Pith citing papers

Observation cc851466-df76-4a76-8f72-0259cf7ac37d · inbound

Uniform Reanalysis of JWST MIRI 15{\mu}m Exoplanet Eclipse Observations using Frame-Normalized Principal Component Analysis cites this paper.

Uniform Reanalysis of JWST MIRI 15{\mu}m Exoplanet Eclipse Observations using Frame-Normalized Principal Component Analysis Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-06T20:44:03.718689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T20:44:03.718689Z digest=sha256:cae7f2c3ab518b14d786f87af07fa3ebeea87a7e9c72f5db5f4285a8ddc3d8d1

Observation e4586f15-374d-4f4e-b014-5658d6019f37 · inbound

Hydrocarbon Hazes on Temperate sub-Neptune K2-18b supported by data from the James Webb Space Telescope cites this paper.

Hydrocarbon Hazes on Temperate sub-Neptune K2-18b supported by data from the James Webb Space Telescope Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-04T17:25:29.432612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T17:25:29.432612Z digest=sha256:b32428f3af1888a9b77624c8c57e529e546f6aba4665be6d20c0df40bd291288

Observation 03f988c0-b698-47e6-952a-16aef69ab23a · inbound

Uniform Reinterpretation of Rocky Exoplanet Secondary Eclipse Observations and the Impact of Stellar and Orbital Uncertainties cites this paper.

Uniform Reinterpretation of Rocky Exoplanet Secondary Eclipse Observations and the Impact of Stellar and Orbital Uncertainties Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels

Reference 37

Resolution
verified exact
arxiv_id, observed 2026-05-10T09:38:41.815974Z

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=2026-05-10T09:35:18.981046Z digest=sha256:525d37b834bcebb0efbf3e7f92c3d7dc51898f832830712c77c4fab05d5bb74b

Observation dece9d47-c2ce-4027-a238-559527c964aa · inbound

GJ 3929 b as the First Complete Rocky Worlds DDT Data Set cites this paper.

GJ 3929 b as the First Complete Rocky Worlds DDT Data Set Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels

Reference 28

Resolution
verified exact
arxiv_id, observed 2026-07-02T20:17:21.344511Z

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=2026-06-27T20:49:13.271060Z digest=sha256:ac933e0f952a707b0985f57a8178216c5f1af4634d0a9dffc0c7602fdef6d277

Observation f978a1cb-e76b-44ac-b35c-53288265094c · inbound

GJ 3929 b as the First Complete Rocky Worlds DDT Data Set cites this paper.

GJ 3929 b as the First Complete Rocky Worlds DDT Data Set Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-04T04:51:47.763004Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T04:51:47.763004Z digest=sha256:933bc1646bd4f0bc4d8fe4dbb17912cde169ff8186866439f42f45bfb7344750

Observation a9455103-e0b0-4886-af20-c1e655a47a4e · inbound

ESCAPE: a small explorer mission to study the stellar drivers of exoplanet evolution cites this paper.

ESCAPE: a small explorer mission to study the stellar drivers of exoplanet evolution Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels

Reference 244

Resolution
unresolved
no resolver link, observed 2026-08-05T00:36:51.721488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T00:36:51.721488Z digest=sha256:c850478615a8d5fedd257759bd24599dd6abdfa3cd461bd3744f31c9336a0824