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Paper Citation Record · LEDGER

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era

As of 22 August 2026, this Paper Citation Record lists 100 of 205 outbound references and 0 inbound Pith citation observations for arXiv:2608.07128.

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

pith.paper-citation-record.v1
2608.07128 v1

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measured 100 of 205 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-10T14:25:54.752038Z

measured 100 of 100 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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100 of 205 outbound references displayed

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Outbound references

Observation 75986f92-c2c6-4c67-b361-643b15eaa5c4 · outbound

This paper cites JWST COMPASS: A NIRSpec G395H Transmission Spectrum of the Super-Earth GJ 357 b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era JWST COMPASS: A NIRSpec G395H Transmission Spectrum of the Super-Earth GJ 357 b

Reference 1

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source=arxiv_source observed=2026-08-10T14:25:54.274838Z digest=sha256:594dfa98b72b8c2abbc7599e33cee0dab5e8d4bd6aa1bd5a51cd6c2ff063607c

Observation b3c08189-fe0f-40c0-98b4-960f34936156 · outbound

This paper cites The impact of atmospheric circulation on the chemistry of the hot Jupiter HD 209458b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The impact of atmospheric circulation on the chemistry of the hot Jupiter HD 209458b

Reference 2

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no resolver link, observed 2026-08-10T14:25:54.280344Z

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source=arxiv_source observed=2026-08-10T14:25:54.280344Z digest=sha256:d4272a59daff8d9b3b1c25cec270c6788b5996286d1080c507d63cdf69e2f8ca

Observation 164495e2-f67e-45d1-a2c1-f3ff1dcf1647 · outbound

This paper cites Early Release Science of the exoplanet WASP-39b with JWST NIRCam.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Early Release Science of the exoplanet WASP-39b with JWST NIRCam

Reference 3

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source=arxiv_source observed=2026-08-10T14:25:54.285617Z digest=sha256:d10599017784eee03a7d376ab9f8adbf89f18309fee02d5231c4e5c4dd5783cf

Observation 7a1190ca-1aac-4ed4-bff5-2724df5c6710 · outbound

This paper cites Escaping Helium and a Highly Muted Spectrum Suggest a Metal-Enriched Atmosphere on Sub-Neptune GJ3090b from JWST Transit Spectroscopy.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Escaping Helium and a Highly Muted Spectrum Suggest a Metal-Enriched Atmosphere on Sub-Neptune GJ3090b from JWST Transit Spectroscopy

Reference 4

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no resolver link, observed 2026-08-10T14:25:54.290632Z

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source=arxiv_source observed=2026-08-10T14:25:54.290632Z digest=sha256:1206493305ae39dd859ca6281504e463124b869f02ae49723cb1aeac3c14bde6

Observation d0285597-f3a7-4185-8a44-69a31c1c4f1e · outbound

This paper cites Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94Ab using JWST NIRSpec/G395H.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94Ab using JWST NIRSpec/G395H

Reference 5

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source=arxiv_source observed=2026-08-10T14:25:54.295430Z digest=sha256:aa54c368cd93a4389bd18963150f6a938b6be5b370113dbd8f1ebb0d23cd1d93

Observation afdfecfe-7a7c-4ab2-a2c9-e8c2cb404ea3 · outbound

This paper cites The tidal deformation and atmosphere of WASP-12b from its phase curve.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The tidal deformation and atmosphere of WASP-12b from its phase curve

Reference 6

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source=arxiv_source observed=2026-08-10T14:25:54.300579Z digest=sha256:04e231c1168c42d8cae4a4b1fbb27ac9ff7fa68386cd67d563917ac365f7566c

Observation 99d4b599-6281-4477-b829-30877079d3e5 · outbound

This paper cites TauREx III: A fast, dynamic and extendable framework for retrievals.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era TauREx III: A fast, dynamic and extendable framework for retrievals

Reference 7

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source=arxiv_source observed=2026-08-10T14:25:54.306266Z digest=sha256:16ce1c3fa244b6606c07934b7536889fd42a53276b719748a30fc5b5997b3e60

Observation 26783708-63b6-463d-9676-8b1ee3d08f4a · outbound

This paper cites JWST COMPASS: The first near- to mid-infrared transmission spectrum of the hot super-Earth L 168-9 b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era JWST COMPASS: The first near- to mid-infrared transmission spectrum of the hot super-Earth L 168-9 b

Reference 8

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source=arxiv_source observed=2026-08-10T14:25:54.311551Z digest=sha256:4cb67eaae1e44b09ecfd6b6d553ea724181667928adf407c56466bb20489dc9f

Observation 602c9f4f-09b8-4abd-ad66-95ded1dc892c · outbound

This paper cites Early Release Science of the Exoplanet WASP-39b with JWST NIRSpec G395H.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Early Release Science of the Exoplanet WASP-39b with JWST NIRSpec G395H

Reference 9

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source=arxiv_source observed=2026-08-10T14:25:54.316427Z digest=sha256:a931b729c651e26a125f7d71ad74034e01259128da66d4509eadfcf9ccb35ce3

Observation b1538ce6-6489-48f6-adb3-3ec72610b438 · outbound

This paper cites JWST COMPASS: NIRSpec/G395H Transmission Observations of the Super-Earth TOI-836b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era JWST COMPASS: NIRSpec/G395H Transmission Observations of the Super-Earth TOI-836b

Reference 10

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source=arxiv_source observed=2026-08-10T14:25:54.321203Z digest=sha256:51b9419f0691c4e8f07f69cd018e685ac6e96c38d0856f79fd922dbb28da13d6

Observation 331bea49-b7c0-4540-9622-a10d1dfa8c73 · outbound

This paper cites New study of the line profiles of sodium perturbed by H2.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era New study of the line profiles of sodium perturbed by H2

Reference 11

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no resolver link, observed 2026-08-10T14:25:54.325914Z

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source=arxiv_source observed=2026-08-10T14:25:54.325914Z digest=sha256:60345710f801ad85da0e1a385f5c0a29d14cbbbaff25c794a48e5b77de161da0

Observation 7aae1f0f-c23b-43ff-9d7e-4ae1b806ec6a · outbound

This paper cites Three sub-Jupiter-mass planets: WASP-69b & WASP-84b transit active K dwarfs and WASP-70Ab transits the evolved primary of a G4+K3 binary.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Three sub-Jupiter-mass planets: WASP-69b & WASP-84b transit active K dwarfs and WASP-70Ab transits the evolved primary of a G4+K3 binary

Reference 12

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no resolver link, observed 2026-08-10T14:25:54.331024Z

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source=arxiv_source observed=2026-08-10T14:25:54.331024Z digest=sha256:6513272548e5eef035425be533c9a7cdeb1d29834efbf3db643ba5559d5a8e43

Observation b38321e4-a720-4496-90d0-1fe1a85d6336 · outbound

This paper cites Error estimation in astronomy: A guide.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Error estimation in astronomy: A guide

Reference 13

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no resolver link, observed 2026-08-10T14:25:54.335808Z

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source=arxiv_source observed=2026-08-10T14:25:54.335808Z digest=sha256:d1a659d7ffb0b8c60d0a8eeb3b7cabee3f425c4f811c9ae47fa3b9b6a3aa56ea

Observation 17b3fdba-0d09-48f1-80c6-3ed50a5b16ba · outbound

This paper cites H- Opacity and Water Dissociation in the Dayside Atmosphere of the Very Hot Gas Giant WASP-18 b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era H- Opacity and Water Dissociation in the Dayside Atmosphere of the Very Hot Gas Giant WASP-18 b

Reference 14

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no resolver link, observed 2026-08-10T14:25:54.341584Z

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source=arxiv_source observed=2026-08-10T14:25:54.341584Z digest=sha256:b4faec32af2673a1cc08493512495694377c7d73e40b0aa295f8bcf6dc1d2b6f

Observation 89fb61d2-24da-46d1-807e-1b3fda4a745a · outbound

This paper cites Nested sampling for physical scientists.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Nested sampling for physical scientists

Reference 15

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no resolver link, observed 2026-08-10T14:25:54.346526Z

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source=arxiv_source observed=2026-08-10T14:25:54.346526Z digest=sha256:8559b22b043c7a68d658661743b5db1ececf29647c7e72605552d80b4ce96e6a

Observation 87df5dae-1858-498f-9ad3-b4281f1f091e · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 16

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source=arxiv_source observed=2026-08-10T14:25:54.351328Z digest=sha256:0d4819befd2d6ccf80ea6962bf6b0841eef17a9d69938429a0064642d159f5de

Observation b2dac6d6-9e37-44c9-8461-d7d4ca28335b · outbound

This paper cites The chemical make-up of the Sun: A 2020 vision.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The chemical make-up of the Sun: A 2020 vision

Reference 17

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no resolver link, observed 2026-08-10T14:25:54.355834Z

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source=arxiv_source observed=2026-08-10T14:25:54.355834Z digest=sha256:7f5105b79df63ce9d63ceefcf150939f97d111ab2970c0db1fcef71248aefba9

Observation 280e9017-bec7-491a-999e-4419431c069c · outbound

This paper cites ExoMol molecular line lists - XVI: The rotation-vibration spectrum of hot H$_2$S.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era ExoMol molecular line lists - XVI: The rotation-vibration spectrum of hot H$_2$S

Reference 18

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source=arxiv_source observed=2026-08-10T14:25:54.360764Z digest=sha256:1f54812238443cdb27f4307e00fd311c5d676978c8f256e22acf6035a1065562

Observation df806ee0-8cf8-497a-b206-6b5aa750689e · outbound

This paper cites Grid of Pseudo-2D Chemistry Models for Tidally-Locked Exoplanets. I. The Role of Vertical and Horizontal Mixing.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Grid of Pseudo-2D Chemistry Models for Tidally-Locked Exoplanets. I. The Role of Vertical and Horizontal Mixing

Reference 19

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source=arxiv_source observed=2026-08-10T14:25:54.365512Z digest=sha256:95677470f711518a2e4e4ca74fa7dcd916fb09a7d4bb5520ec672486708df2c4

Observation 672a08d5-9379-41cf-a700-bce7b514f4e5 · outbound

This paper cites Grid of pseudo-2D chemistry models for tidally locked exoplanets -- II. The role of photochemistry.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Grid of pseudo-2D chemistry models for tidally locked exoplanets -- II. The role of photochemistry

Reference 20

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no resolver link, observed 2026-08-10T14:25:54.370055Z

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source=arxiv_source observed=2026-08-10T14:25:54.370055Z digest=sha256:2ed68f7ce1464138b59afe3f240de0ca9f8b67e4a93b62f9669912e37a68ed46

Observation 896316ad-8b31-45a0-9792-91ec1a67ec4d · outbound

This paper cites Kinetic and photochemical disequilibrium in the potentially carbon-rich atmosphere of the warm-Jupiter WASP-69b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Kinetic and photochemical disequilibrium in the potentially carbon-rich atmosphere of the warm-Jupiter WASP-69b

Reference 21

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source=arxiv_source observed=2026-08-10T14:25:54.374564Z digest=sha256:2f310936ec461cb41a71d21cd99226bcc59455c09c4e6d45fdc41289b8b06ad8

Observation a5b2e82d-d136-4998-bdea-6bc9cd631d5f · outbound

This paper cites A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b

Reference 22

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no resolver link, observed 2026-08-10T14:25:54.379266Z

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source=arxiv_source observed=2026-08-10T14:25:54.379266Z digest=sha256:e737dfc0af5c4a35066bd622a99848b75583ca7f35ab50adb9ab2ce315fabab1

Observation efab2b39-9a65-4709-ab00-cc656d3627f4 · outbound

This paper cites ExoMol line lists III: An improved hot rotation-vibration line list for HCN and HNC.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era ExoMol line lists III: An improved hot rotation-vibration line list for HCN and HNC

Reference 23

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no resolver link, observed 2026-08-10T14:25:54.384408Z

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source=arxiv_source observed=2026-08-10T14:25:54.384408Z digest=sha256:bff9730d78521e7bc792f6fa044e344ac31b5e1f7fd72cc82b653fb9c4d034ec

Observation 4e80aa68-1e55-47f6-99c1-f8b4dc414807 · outbound

This paper cites ExoMol molecular line lists V: The ro-vibrational spectra of NaCl and KCl.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era ExoMol molecular line lists V: The ro-vibrational spectra of NaCl and KCl

Reference 24

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source=arxiv_source observed=2026-08-10T14:25:54.389280Z digest=sha256:9884d47274c6c52c21d8e04f7f214dc07209f801f20efebccf3f919e8e8b444e

Observation 1a67f4c4-a5bd-49e0-9dfb-95f9f8df5c42 · outbound

This paper cites The GAPS Programme at TNG LV. Multiple molecular species in the atmosphere of HAT-P-11 b and review of the HAT-P-11 planetary system.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The GAPS Programme at TNG LV. Multiple molecular species in the atmosphere of HAT-P-11 b and review of the HAT-P-11 planetary system

Reference 25

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no resolver link, observed 2026-08-10T14:25:54.394004Z

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source=arxiv_source observed=2026-08-10T14:25:54.394004Z digest=sha256:60aa49a410087efa0940d14dac476720c6e52a952bf1be0e1bce27a64d39bd3e

Observation b0f96f12-6ec5-4a78-849f-4a490fb70c16 · outbound

This paper cites Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

Reference 26

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source=arxiv_source observed=2026-08-10T14:25:54.398890Z digest=sha256:f2660c0661d554a7855b6f8de7fd0c8034acef3f5ed5946ad7fe6fb391a107d8

Observation 33a8d599-8447-49d1-aa72-3692b476b8dd · outbound

This paper cites Evidence for a volcanic atmosphere on the sub-Earth L98-59b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Evidence for a volcanic atmosphere on the sub-Earth L98-59b

Reference 27

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source=arxiv_source observed=2026-08-10T14:25:54.403573Z digest=sha256:14e65bd1a149fd241b7b67988e294c61c117b7996c03cfde02f9ff8cea20142d

Observation 78a349f1-56a5-428f-96ca-e17b3280af61 · outbound

This paper cites JWST Reveals CH$_4$, CO$_2$, and H$_2$O in a Metal-rich Miscible Atmosphere on a Two-Earth-Radius Exoplanet.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era JWST Reveals CH$_4$, CO$_2$, and H$_2$O in a Metal-rich Miscible Atmosphere on a Two-Earth-Radius Exoplanet

Reference 28

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source=arxiv_source observed=2026-08-10T14:25:54.408406Z digest=sha256:261b1f635e9eafc6265cb29198d5030d74f44808cb75d33fcd49602fa9fe5ff4

Observation dee20f49-ed9a-4f98-a146-90481f1f0341 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 29

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no resolver link, observed 2026-08-10T14:25:54.413121Z

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source=arxiv_source observed=2026-08-10T14:25:54.413121Z digest=sha256:6217df08613dc99b6b5e773007aa77ebdf8aa19441463bd98b3fb7fa508ba621

Observation 13c9d415-a672-4c64-9ed8-45b53b83df7d · outbound

This paper cites TEA: A Code for Calculating Thermochemical Equilibrium Abundances.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era TEA: A Code for Calculating Thermochemical Equilibrium Abundances

Reference 30

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source=arxiv_source observed=2026-08-10T14:25:54.418044Z digest=sha256:66a3bc44bd20bbff2fcc63a829d2575b51f1416cc22a35c8df691b7d1aa41e0f

Observation 3efbea9f-3876-41ab-8052-8dc88c5aa145 · outbound

This paper cites Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396

Reference 31

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source=arxiv_source observed=2026-08-10T14:25:54.422745Z digest=sha256:c03565e5b2ad8ae6ed6a394bc910c1db3c216907fcb86da5bfa6c6f0faf80cf1

Observation 20fd4b2a-2d77-45b6-8ebe-f33af7765600 · outbound

This paper cites The GAPS Programme with HARPS-N@TNG XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The GAPS Programme with HARPS-N@TNG XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

Reference 32

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source=arxiv_source observed=2026-08-10T14:25:54.427736Z digest=sha256:d073f6a5b6a2411e0d29216b949f4b7dec3cb8c89546e7147df8cb9f270a7979

Observation 8cefd7d1-6f1d-41ca-8d43-ab9a81630bec · outbound

This paper cites Reports on Progress in Physics , year = 2016, month = mar, volume =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Reports on Progress in Physics , year = 2016, month = mar, volume =

Reference 33

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source=arxiv_source observed=2026-08-10T14:25:54.432479Z digest=sha256:8f91b1426655ca691396cab451bca23d26de373851a05f05fc2839ff65e01772

Observation 2a64ed13-f640-4f41-b410-f5c466c81c0a · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 34

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no resolver link, observed 2026-08-10T14:25:54.437417Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.437417Z digest=sha256:bcc6a38f75f923a941eff9ec58dd49ced67a1ac46a08b8e512e15065aa5668c5

Observation 5d38549b-207f-4d2e-8a87-9e949e4b8011 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 35

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unresolved
no resolver link, observed 2026-08-10T14:25:54.441903Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.441903Z digest=sha256:81a55c5e785130f07c8cf832bc23f2b7c7e70bd9210ab9e944d290fdd58fdb27

Observation 22f549f8-af29-493c-9601-dde4fefc9da3 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 36

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unresolved
no resolver link, observed 2026-08-10T14:25:54.446312Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.446312Z digest=sha256:e3deff5604076951d0a79258927c35ee83ce4c50cce570c59bb46f9a98053cf6

Observation 2a06693c-9d28-4eb6-be6e-d1d5bfdc116b · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 37

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unresolved
no resolver link, observed 2026-08-10T14:25:54.450889Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.450889Z digest=sha256:c88f01fc581bff108c393bc64be403d7ce49516b5861aa25bcdc389653c2a47e

Observation cdd172b2-6e80-4140-b21c-ae01499a2e05 · outbound

This paper cites an unresolved cited work.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Unresolved cited work

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.455327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.455327Z digest=sha256:468c40d9b5549208c95125af9dcd0ba357912d18110ec4e04a0bd1223da9c64a

Observation eebe6202-5840-44e7-b887-5acac485abf0 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.459870Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.459870Z digest=sha256:ca1594055009474d94d243e17d91a39ab437c9bf31217db7645ea133bfdc3d2d

Observation 8ed03c4c-fcbc-4092-9e08-dcf79f5f791c · outbound

This paper cites ExoMol line lists -- LVI: The SO line list, MARVEL analysis of experimental transition data and refinement of the spectroscopic model.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era ExoMol line lists -- LVI: The SO line list, MARVEL analysis of experimental transition data and refinement of the spectroscopic model

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.464312Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.464312Z digest=sha256:00ae6dfd0449cf780b9b4914a78de9bf68269abd2e5adc23e0c90938ab8e0e81

Observation c2fdc3cb-109b-465f-9c3b-4418d115c14d · outbound

This paper cites X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.469159Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.469159Z digest=sha256:fc213459d8cf3b6ecc232ccb28a298b6285608b98169f01f41378a4123508f23

Observation 5f59103c-a1ee-4d6d-9c8d-7eb0c66cb749 · outbound

This paper cites 2005 , month =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era 2005 , month =

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.473576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.473576Z digest=sha256:633e43d9b9515046e0e8b21bcb2cffb41bb1cf1a195a8c7a1d7df3cd816fa747

Observation a3395cd3-03bf-45bf-aef8-beb077cd9a9a · outbound

This paper cites The Near-Infrared and Optical Spectra of Methane Dwarfs and Brown Dwarfs.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The Near-Infrared and Optical Spectra of Methane Dwarfs and Brown Dwarfs

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.478569Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.478569Z digest=sha256:a5fd41f3cf9aff128d139afad85bd5fb22502f0885dd473891434cb02bf864c0

Observation 0303f3c5-2d57-4f0e-9e5f-1541f7a90f76 · outbound

This paper cites Theoretical Spectra and Light Curves of Close-in Extrasolar Giant Planets and Comparison with Data.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Theoretical Spectra and Light Curves of Close-in Extrasolar Giant Planets and Comparison with Data

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.483197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.483197Z digest=sha256:dbd8de64217b7d9a93f8bdf0ecec3317e50a8c63b13dbf6652f2096d9348805a

Observation 47b5164f-bcc3-43dd-9da3-87f804b57037 · outbound

This paper cites The GAPS Programme at TNG XXXIX -- Multiple molecular species in the atmosphere of the warm giant planet WASP-80 b unveiled at high resolution with GIANO-B.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The GAPS Programme at TNG XXXIX -- Multiple molecular species in the atmosphere of the warm giant planet WASP-80 b unveiled at high resolution with GIANO-B

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.488025Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.488025Z digest=sha256:773bad9b37b84775f8ac7efe9742c35f4354a3aea8cbf6eaac520f18c4399287

Observation 2d100521-b4ab-491e-b36d-dc43f975553c · outbound

This paper cites an unresolved cited work.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Unresolved cited work

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.493261Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.493261Z digest=sha256:9704e0aa353e0e5f6db5ce95c3ef6f3179ec13476d1d49240e2c9d5cec0fdcc5

Observation b071a4fb-b8ad-41e8-a992-a4c906913ab5 · outbound

This paper cites A Benchmark JWST Near-Infrared Spectrum for the Exoplanet WASP-39b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era A Benchmark JWST Near-Infrared Spectrum for the Exoplanet WASP-39b

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.498155Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.498155Z digest=sha256:53c5b037b20f76915784a11e16365fa71cb12183d197bf71fb3b228b2f1b8cd1

Observation 08d46fb6-5d32-46d1-a74f-00217fd7fec0 · outbound

This paper cites Nature Astronomy , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Nature Astronomy , keywords =

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.502936Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.502936Z digest=sha256:8e47f26e5ef9879906a945928c56c0c4ce56c311c4769e40a2bc86f42578f8a8

Observation 004e7aa1-2102-4a38-afd1-13f1b3d2b2a8 · outbound

This paper cites Towards a more complex description of chemical profiles in exoplanets retrievals: A 2-layer parameterisation.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Towards a more complex description of chemical profiles in exoplanets retrievals: A 2-layer parameterisation

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.507576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.507576Z digest=sha256:77826540f34c4ec857ad91f296b0d4a546221a27a73e0885f0038a8a582d86ad

Observation f5fcbf71-b108-4373-8767-f3c9f0caf640 · outbound

This paper cites Detection of Planetary Transits Across a Sun-like Star.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Detection of Planetary Transits Across a Sun-like Star

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.512650Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.512650Z digest=sha256:74b5c29a44d5199cedaf9973586d28a94bf57a9d230d4b77c7a7a96a71de592b

Observation 54ff635b-1e61-4fd7-9199-8458438d3c82 · outbound

This paper cites an unresolved cited work.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Unresolved cited work

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.517324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.517324Z digest=sha256:68aa906df7121332a382d85636498f7f81d9efee049494e537612562b3ed25e8

Observation 9743623b-5b04-4ded-a002-a29638bcead3 · outbound

This paper cites Marvel analysis of the measured high-resolution rovibrational spectra of H2S.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Marvel analysis of the measured high-resolution rovibrational spectra of H2S

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.522594Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.522594Z digest=sha256:07dfae6e2b4ecc3d305daf52d4183572a7b1344aec9b13b13fbf346eff9a0d96

Observation 819fa324-c4c9-4c30-82d9-b137560cb1e1 · outbound

This paper cites ExoMol molecular line lists -- XXXVII: spectra of acetylene.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era ExoMol molecular line lists -- XXXVII: spectra of acetylene

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.527705Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.527705Z digest=sha256:491e7ad6abb8c2130347b7a3ba31daae0db1346bf3d290666ca975f5b0076bd3

Observation 650a7863-53ad-4074-832e-914fb588c459 · outbound

This paper cites ExoMol molecular line lists XXXV: a rotation-vibration line list for hot ammonia.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era ExoMol molecular line lists XXXV: a rotation-vibration line list for hot ammonia

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.532718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.532718Z digest=sha256:d7fb6b198a8dfc1ec823dd697f3c0eab8f8ee76d1c786df009f56631924b36ba

Observation 545b133f-6bf7-4082-9c31-28460deb0572 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.537781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.537781Z digest=sha256:d9f6b405024292d6f27c51677150b9f548ed9403eb577623c54c6ca944e46f9a

Observation e37c8089-224d-48e5-871c-20b49ad6fa22 · outbound

This paper cites an unresolved cited work.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Unresolved cited work

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.542303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.542303Z digest=sha256:ff99b8efeb3e6e31c25d0ce1daeb58d8ef1881080a7993bce8d8647fa39280d9

Observation 06042c16-fde2-4612-ad83-ee3160a0d50a · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.546851Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.546851Z digest=sha256:924bc0507066528387c50a8379d97e36eb1b18736608084de5ec1a820df7b78e

Observation 954c2d04-30ec-4a1c-90ed-c1074216395c · outbound

This paper cites An Algorithm to Compress Line-transition Data for Radiative-transfer Calculations.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era An Algorithm to Compress Line-transition Data for Radiative-transfer Calculations

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.551676Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.551676Z digest=sha256:f9537af09e09d77741b69bba48fee298579f92e61c6ac2d78b8396b56b483dc2

Observation 5778db8d-8755-456d-ac96-3382432b902f · outbound

This paper cites doi:10.5281/zenodo.2547042 , publisher =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era doi:10.5281/zenodo.2547042 , publisher =

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.556934Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.556934Z digest=sha256:73ea13c7d8dfe4aefb7b6e328471e2c05d8a57a91509c5b0beead645cba56631

Observation 7544e68c-4bf0-4367-ab0e-d0ec101ad322 · outbound

This paper cites Gen TSO: A General JWST Simulator for Exoplanet Times-series Observations.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Gen TSO: A General JWST Simulator for Exoplanet Times-series Observations

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.561777Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.561777Z digest=sha256:957edf7a4ec85ec6a9603218743e9153ea6fae9dabc0a83099a62dfd50c338e1

Observation 82573643-45b1-45fd-8f4e-069076cf7235 · outbound

This paper cites The Pyrat Bay Framework for Exoplanet Atmospheric Modeling: A Population Study of Hubble/WFC3 Transmission Spectra.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The Pyrat Bay Framework for Exoplanet Atmospheric Modeling: A Population Study of Hubble/WFC3 Transmission Spectra

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.566530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.566530Z digest=sha256:239cc178844cb27407ef155d2800f9892dbba775938b2bbab6b55d2d55447dc2

Observation 0c2cbfc4-a5a7-476a-a5f6-9e769206b210 · outbound

This paper cites On Correlated-noise Analyses Applied To Exoplanet Light Curves.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era On Correlated-noise Analyses Applied To Exoplanet Light Curves

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.571566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.571566Z digest=sha256:23992f868f58c0cdef60e631c1baed563313220e5c93b11a6caf6b132839c795

Observation 3939d3aa-4a07-4b98-81a2-2f257780ce0b · outbound

This paper cites Toward More Reliable Analytic Thermochemical-equilibrium Abundances.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Toward More Reliable Analytic Thermochemical-equilibrium Abundances

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.576610Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.576610Z digest=sha256:e23cb3ceeb3699c51bf6d827ec4f2b83fd1fa5dd1032a4beb100493d93dda2d8

Observation e9f4281b-236b-460c-b987-501a3d3af65c · outbound

This paper cites TOI-837 b: characterisation, formation and evolutionary history of an infant warm Saturn-mass planet.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era TOI-837 b: characterisation, formation and evolutionary history of an infant warm Saturn-mass planet

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.581505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.581505Z digest=sha256:dae184469eff44ee8503ea1bb1e9016019818bb6746eae099c7a60d2f069d4d8

Observation 335c4667-7107-4568-a526-d201d303ad91 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.586226Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.586226Z digest=sha256:122d3c9cb6bca01ec0eb5c35ea53769f2e94de21378564477bb24974ce1ac1d6

Observation 8468b904-dc61-43b2-acdc-f0fe68ab9af2 · outbound

This paper cites Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.590824Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.590824Z digest=sha256:0845e194ad86443c3734ee88c9c4418a5dd31d9868d5362dddae8e693f09b2d0

Observation 0c8c5c95-5b6e-41d7-b216-1a1fbd94e8d2 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.595568Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.595568Z digest=sha256:06aedf2fd440ceb1b7d51204505de3aa9c648afd38aaf506d4bb244f202a7729

Observation eed07b74-32ca-496c-8d60-9e8589de75ca · outbound

This paper cites The Effects of Consistent Chemical Kinetics Calculations on the Pressure-Temperature Profiles and Emission Spectra of Hot Jupiters.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The Effects of Consistent Chemical Kinetics Calculations on the Pressure-Temperature Profiles and Emission Spectra of Hot Jupiters

Reference 68

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unresolved
no resolver link, observed 2026-08-10T14:25:54.600146Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.600146Z digest=sha256:07cb0fbbbd1488ae5535167c28702745a5d7eedd7c3311884f2caea33de13413

Observation 08aef448-69f5-4d7d-8300-30b4bf700f6a · outbound

This paper cites Line Intensities and Molecular Opacities of the FeH $F^4\Delta_i-X^4\Delta_i$ Transition.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Line Intensities and Molecular Opacities of the FeH $F^4\Delta_i-X^4\Delta_i$ Transition

Reference 69

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unresolved
no resolver link, observed 2026-08-10T14:25:54.604893Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.604893Z digest=sha256:0805a0a8e7f67ecb84aff54ec7b5730ee4e814aa3a68b5e9dadc527f1068050c

Observation 4fbb4fda-92ae-4b05-9ace-2dabfa3c85c4 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.609692Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.609692Z digest=sha256:7b98dac140cb155b6cdd64b66d8dadea545b04fcd5a950c5ff01476e79d12b14

Observation 52e09524-fe44-44f4-92ee-bf34219198e4 · outbound

This paper cites Spectroscopic Time-series Performance of JWST/NIRSpec from Commissioning Observations.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Spectroscopic Time-series Performance of JWST/NIRSpec from Commissioning Observations

Reference 71

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no resolver link, observed 2026-08-10T14:25:54.614948Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.614948Z digest=sha256:cc6744f5e1454b128d64bdea95a5fa2bc49c2221694aa3f0d21feb5abdd85675

Observation fe2877e0-5fa4-453c-970b-6aa7ac484465 · outbound

This paper cites Inhomogeneous terminators on the exoplanet WASP-39 b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Inhomogeneous terminators on the exoplanet WASP-39 b

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.619612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.619612Z digest=sha256:f5210b57b93b3c8f061d714fffe12233ae15fa132bf385f63f42a373870a7337

Observation f6f4794e-ce19-4108-b75f-ab1b35847a8d · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.624163Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.624163Z digest=sha256:b9eeb0b318d5db6452137630b2e8d24960035a9a1bc6986e2f8478304baaffc8

Observation d1734236-47be-41a0-b438-1925e16a049f · outbound

This paper cites Early Release Science of the exoplanet WASP-39b with JWST NIRISS.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Early Release Science of the exoplanet WASP-39b with JWST NIRISS

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.629830Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.629830Z digest=sha256:f2b9ff46f15626655a0ab50e2fc629e812040ce53ea377661b9730497499fceb

Observation f405a77c-6b89-4032-ae5a-8ed41bb90f24 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.634215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.634215Z digest=sha256:12ce8762609c09b87404023f54309fbab22e715f382bd1ac9b2e93743c91c268

Observation cf864e05-9d07-4125-a43e-719d91d5bc5e · outbound

This paper cites Retrieval analysis of 38 WFC3 transmission spectra and resolution of the normalisation degeneracy.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Retrieval analysis of 38 WFC3 transmission spectra and resolution of the normalisation degeneracy

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.638639Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.638639Z digest=sha256:5e9baf516ee4ef57849b5d616f4dd36c54b8ca3e814e277d1d79f4ae93c487ad

Observation 67eb6024-aee3-4335-8238-fe066b135ee4 · outbound

This paper cites emcee: The MCMC Hammer.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era emcee: The MCMC Hammer

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.643238Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.643238Z digest=sha256:c079fe17fb3df7430c9b36b6445c6ff8f65e040fb979ff09da2d1f2e5e32c158

Observation 906705ac-9e3d-4fee-bee7-3556d18ffa8c · outbound

This paper cites Beyond Equilibrium Temperature: How the Atmosphere/Interior Connection Affects the Onset of Methane, Ammonia, and Clouds in Warm Transiting Giant Planets.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Beyond Equilibrium Temperature: How the Atmosphere/Interior Connection Affects the Onset of Methane, Ammonia, and Clouds in Warm Transiting Giant Planets

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.647859Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.647859Z digest=sha256:79e7149ce7dcc918da1a187e076216c49bb625d50dec9e3421a79cee96fd766a

Observation aec0796a-7802-4918-bc9c-24e61d89feb1 · outbound

This paper cites Non-local thermodynamic equilibrium effects determine the upper atmospheric temperature structure of the ultra-hot Jupiter KELT-9b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Non-local thermodynamic equilibrium effects determine the upper atmospheric temperature structure of the ultra-hot Jupiter KELT-9b

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.653019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.653019Z digest=sha256:f01639834ea997ed1d5038b67458f1f9e4ccc4d8dbae757aa734a829b16a7297

Observation f47ebbdd-7163-4f96-b766-f24c0b8049d9 · outbound

This paper cites The GAPS programme at TNG. XLV. HI Balmer lines transmission spectroscopy and NLTE atmospheric modelling of the ultra-hot Jupiter KELT-20b/MASCARA-2b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The GAPS programme at TNG. XLV. HI Balmer lines transmission spectroscopy and NLTE atmospheric modelling of the ultra-hot Jupiter KELT-20b/MASCARA-2b

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.657737Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.657737Z digest=sha256:a5a52f7afa40bc09e3618ad67597635ec6142863383cff2b17c3f27edad9b84a

Observation b23af136-4222-455d-b6d4-41907a86ec85 · outbound

This paper cites NLTE atmospheric modelling of the ultra-hot Jupiter WASP-178b and comparison with UV and optical observations.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era NLTE atmospheric modelling of the ultra-hot Jupiter WASP-178b and comparison with UV and optical observations

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.662510Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.662510Z digest=sha256:b0ea17ee7249b5d32bce398e688ae34a8017cb5cc8ad2817bba8ff2e934e5801

Observation 65c02924-6339-4022-8829-553bb758d568 · outbound

This paper cites Transmission spectroscopy of WASP-52 b with JWST NIRISS: Water and helium atmospheric absorption, alongside prominent star-spot crossings.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Transmission spectroscopy of WASP-52 b with JWST NIRISS: Water and helium atmospheric absorption, alongside prominent star-spot crossings

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.667214Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.667214Z digest=sha256:11e8c76c540be65adf5c61b93eb153799f44dfb2a1d4466bc0798f7534635f4b

Observation 86007df2-3923-4e70-ad79-78052de9e436 · outbound

This paper cites Hydrogen sulfide and metal-enriched atmosphere for a Jupiter-mass exoplanet.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Hydrogen sulfide and metal-enriched atmosphere for a Jupiter-mass exoplanet

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.671921Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.671921Z digest=sha256:1b1c1689aafe129b47739c25539aac653cb88160ae7c6fafa02a9d93acfec586

Observation 6c851c0f-bb98-4ab6-944e-e47ecd68cc9d · outbound

This paper cites The California Kepler Survey VII. Precise Planet Radii Leveraging Gaia DR2 Reveal the Stellar Mass Dependence of the Planet Radius Gap.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The California Kepler Survey VII. Precise Planet Radii Leveraging Gaia DR2 Reveal the Stellar Mass Dependence of the Planet Radius Gap

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.676770Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.676770Z digest=sha256:2e1e7c93e509a1f31d0a3e3f65117bc69977f40f7d3b45af04e4b923962b46c8

Observation f1c5374f-498a-4ab2-931b-d2da4db6d542 · outbound

This paper cites JWST measurements of $^{13}$C, $^{18}$O and $^{17}$O in the atmosphere of super-Jupiter VHS 1256 b.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era JWST measurements of $^{13}$C, $^{18}$O and $^{17}$O in the atmosphere of super-Jupiter VHS 1256 b

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.681665Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.681665Z digest=sha256:19aae5a4d9a10a7f632cc7795b194d4e58ac52a3953872fdc1b9785c660aab3e

Observation abaed2d0-a7be-4f86-8f81-e49ffe42985f · outbound

This paper cites The ESO SupJup Survey V: Exploring Atmospheric Variability and Orbit of the Super-Jupiter AB Pictoris b with CRIRES+.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The ESO SupJup Survey V: Exploring Atmospheric Variability and Orbit of the Super-Jupiter AB Pictoris b with CRIRES+

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.686453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.686453Z digest=sha256:af22118493b31e63ef879142bf8c5e3602bea25b059dbfc3b1762eae359ba341

Observation b701cb81-0cad-4ebe-85d3-a0524d05c7b4 · outbound

This paper cites The KELT-7b atmospheric thermal-inversion conundrum revisited with CHEOPS, TESS, and additional data.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The KELT-7b atmospheric thermal-inversion conundrum revisited with CHEOPS, TESS, and additional data

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.691332Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.691332Z digest=sha256:bf15b3180da6cb4948907b7ed0b881aa72ac585ed53cf9e2a8cbac342bf3cf07

Observation 9da5f65e-2fa7-4153-b469-813eba387b4a · outbound

This paper cites Five carbon- and nitrogen-bearing species in a hot giant planet's atmosphere.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Five carbon- and nitrogen-bearing species in a hot giant planet's atmosphere

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.696196Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.696196Z digest=sha256:2a656f9021797ad8c8d8d93025cb5c50aa290fae69e8ae02e668d3d6809446cc

Observation f4fa2b1e-b0c3-4625-a545-cb31ea21ac07 · outbound

This paper cites an unresolved cited work.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Unresolved cited work

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.700908Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.700908Z digest=sha256:c59822bd22543b597ed67e4d07a859da0241c65842f78a1231f728398cba9522

Observation 258e4815-2d2e-4126-89de-b758be8a5748 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.705387Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.705387Z digest=sha256:1103d2f4a65f6f3668a48b5cc44050b760d989624608942dd1709b6c8caa6b18

Observation 2615458e-b809-4559-906d-42859054738b · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 91

Resolution
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no resolver link, observed 2026-08-10T14:25:54.709853Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.709853Z digest=sha256:a9b8f347a4ec576cb9f9b03232bb2ab88d39d8d4f9b19239897165b64d2edb77

Observation 53275126-b92c-4411-9273-b23cc361d15c · outbound

This paper cites 1994 , url=.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era 1994 , url=

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.714209Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.714209Z digest=sha256:c0ac9dba54b748cd85251e05b047c960bf0b8d372afdc2ff8113b516d730e1f2

Observation 9ef91222-4d9f-4217-8ff7-aeecf9cf2d0f · outbound

This paper cites ExoMol molecular line lists XXXVI: $X\ {}^2\Pi - X\ {}^2\Pi$ and $A\ {}^2\Sigma^+ - X\ {}^2\Pi$ transitions of SH.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era ExoMol molecular line lists XXXVI: $X\ {}^2\Pi - X\ {}^2\Pi$ and $A\ {}^2\Sigma^+ - X\ {}^2\Pi$ transitions of SH

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.718644Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.718644Z digest=sha256:9a92260a50b8b16ac62070ff8b06e5897ac37b640481043f6d9645fe2ab77cf4

Observation 605978a2-0f27-455f-b46d-0c310c061a38 · outbound

This paper cites an unresolved cited work.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Unresolved cited work

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.723365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.723365Z digest=sha256:7fb497b26383c91ebd3f891090069963dac4f296187d583f2ea298e20bfe6d6b

Observation b3b373a6-69b4-4cdd-ade4-22a17dd678cd · outbound

This paper cites Hints of a sulfur-rich atmosphere around the 1.6 R$_{\oplus}$ Super-Earth L98-59 d from JWST NIRSpec G395H transmission spectroscopy.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era Hints of a sulfur-rich atmosphere around the 1.6 R$_{\oplus}$ Super-Earth L98-59 d from JWST NIRSpec G395H transmission spectroscopy

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.728369Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.728369Z digest=sha256:189588f9908fac276d9bd04e1b0c5400ed76e70346f88ac1dc995937697f749f

Observation 00c224c7-0408-4fe3-8669-b1083972b1e1 · outbound

This paper cites HELIOS-K: An Ultrafast, Open-source Opacity Calculator for Radiative Transfer.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era HELIOS-K: An Ultrafast, Open-source Opacity Calculator for Radiative Transfer

Reference 96

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unresolved
no resolver link, observed 2026-08-10T14:25:54.733263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.733263Z digest=sha256:4609ba92e6b26329898534f52b15c8a6f706d8fb23edaa21f639f7cc70f0d4fc

Observation 82cb5772-263f-413a-af89-977393997ef0 · outbound

This paper cites On the radiative equilibrium of irradiated planetary atmospheres.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era On the radiative equilibrium of irradiated planetary atmospheres

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.738046Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.738046Z digest=sha256:c20b886814da6ce4bf715f3b92c390d9a0cc2d5a832bd69dd873dc4c646e81c0

Observation a30a0ca8-d813-4f4c-9fad-8c39752932af · outbound

This paper cites The GAPS Programme at TNG XXXVIII. Five molecules in the atmosphere of the warm giant planet WASP-69b detected at high spectral resolution.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era The GAPS Programme at TNG XXXVIII. Five molecules in the atmosphere of the warm giant planet WASP-69b detected at high spectral resolution

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.742664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.742664Z digest=sha256:1fb89bbf322ba68651bc2bfe54079211ab7f533c2f19464759ba9f749a70297d

Observation 546687d4-c4f3-4346-a261-61a5061f0bb7 · outbound

This paper cites A grid of MARCS model atmospheres for late-type stars I. Methods and general properties.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era A grid of MARCS model atmospheres for late-type stars I. Methods and general properties

Reference 99

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unresolved
no resolver link, observed 2026-08-10T14:25:54.747393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.747393Z digest=sha256:8c7457137c535838483fad534b6c89e87f0b5012ce169bf0cb26a6f213e7f5ff

Observation db1fc477-eee3-4a7d-afa2-9b4efaf53cb6 · outbound

This paper cites , keywords =.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era , keywords =

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-10T14:25:54.752038Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T14:25:54.752038Z digest=sha256:f7c8508c07abc0e8e22495308429cac2030cdb058ea06e7add8f2d31414f8961

Pith citing papers

No inbound Pith citation observations are available.