Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
Paper Citation Record · LEDGER
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation
As of 9 August 2026, this Paper Citation Record lists 52 of 52 outbound references and 0 inbound Pith citation observations for arXiv:2607.06339.
A citation records a reference. It does not transfer a finding from one paper to another.
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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
52 of 52 outbound references displayed
- verified exact43
- verified fuzzy4
- unresolved2
- parse uncertain0
- malformed identifier0
- metadata mismatch3
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation ff110036-2146-4759-b8b0-666997f64560 · outbound
This paper cites , keywords =.
Reference 1
- Resolution
- verified exact
- doi, observed 2026-07-08T09:54:50.689105Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 03fd5899-f617-4ceb-adc9-e2543552f058 · outbound
This paper cites The EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation The EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities
Reference 2
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.805792Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation ebb9f970-24d3-41b0-9f0c-940c82915fe3 · outbound
This paper cites Astronomy & Astrophysics , volume=.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Astronomy & Astrophysics , volume=
Reference 3
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-08T09:54:50.964890Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 459f1520-7767-45ef-990a-0d48d6cf2b0f · outbound
This paper cites New Methods for Finding Activity-Sensitive Spectral Lines: Combined Visual Identification and an Automated Pipeline Find a Set of 40 Activity Indicators.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation New Methods for Finding Activity-Sensitive Spectral Lines: Combined Visual Identification and an Automated Pipeline Find a Set of 40 Activity Indicators
Reference 4
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.774743Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 11e303c3-0bf5-4851-98b5-5db2be9423da · outbound
This paper cites The spectral impact of magnetic activity on disk-integrated HARPS-N solar observations: exploring new activity indicators.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation The spectral impact of magnetic activity on disk-integrated HARPS-N solar observations: exploring new activity indicators
Reference 5
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.685702Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation af753e47-64f5-4798-b8ae-b0c30d0da796 · outbound
This paper cites The Changing Face of $\alpha$ Centauri B: Probing plage and stellar activity in K-dwarfs.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation The Changing Face of $\alpha$ Centauri B: Probing plage and stellar activity in K-dwarfs
Reference 6
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.770537Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation a2acfa62-4c29-4d70-90a8-f9f42991967b · outbound
This paper cites keywords =.
Reference 7
- Resolution
- verified exact
- doi, observed 2026-07-08T09:54:50.781880Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation ea45eed5-b5fa-440d-93d2-a74537a35684 · outbound
This paper cites SPECIES I: Spectroscopic Parameters and atmosphEric ChemIstriEs of Stars.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation SPECIES I: Spectroscopic Parameters and atmosphEric ChemIstriEs of Stars
Reference 8
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.778818Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 534b44f9-589e-48f9-8c10-75966135575f · outbound
This paper cites The PLATO Mission.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation The PLATO Mission
Reference 9
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-08T09:54:50.854411Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 630fd436-8b4e-4e08-b3eb-bdbb19f860dd · outbound
This paper cites A Gaussian process framework for modelling stellar activity signals in radial velocity data.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation A Gaussian process framework for modelling stellar activity signals in radial velocity data
Reference 10
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.850474Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 2b01258a-b4d7-4f8a-b43b-9c8e00ae5fb7 · outbound
This paper cites R., Lockwood , G.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation R., Lockwood , G
Reference 11
- Resolution
- verified exact
- doi, observed 2026-07-08T09:54:50.719553Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 98d7cb94-cfce-4b7e-accd-345f002daa6d · outbound
This paper cites Analysis of the public HARPS/ESO spectroscopic archive -- Ca II H&K time series for the HARPS radial velocity database.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Analysis of the public HARPS/ESO spectroscopic archive -- Ca II H&K time series for the HARPS radial velocity database
Reference 12
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.842349Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation f1e24e0c-ea95-46ea-be1e-e4dce4adc7d0 · outbound
This paper cites ESPRESSO@VLT -- On-sky performance and first results.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation ESPRESSO@VLT -- On-sky performance and first results
Reference 13
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.809392Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 8b481f4c-52ef-4c41-b8ed-f08b6435a3b6 · outbound
This paper cites , keywords =.
Reference 14
- Resolution
- verified exact
- doi, observed 2026-07-08T09:54:50.817266Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 83e1129e-f75e-4376-ade8-1e606f63a15a · outbound
This paper cites HARPS-N Solar Radial-Velocity Variations Are Dominated By Large, Bright Magnetic Regions.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation HARPS-N Solar Radial-Velocity Variations Are Dominated By Large, Bright Magnetic Regions
Reference 15
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.739121Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation abe02e43-de15-4ac1-88b0-12445d9823bd · outbound
This paper cites Activity time series of old stars from late F to early K. IV. Limits of the correction of radial velocities using chromospheric emission.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Activity time series of old stars from late F to early K. IV. Limits of the correction of radial velocities using chromospheric emission
Reference 16
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.826848Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 21a04f65-8179-48ee-a5e0-3ef0ae72dc69 · outbound
This paper cites Unexpectedly strong effect of supergranulation on the detectability of Earth twins orbiting Sun-like stars with radial velocities.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Unexpectedly strong effect of supergranulation on the detectability of Earth twins orbiting Sun-like stars with radial velocities
Reference 17
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.821977Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation b8dda00b-ab92-496f-be34-46d066a9e3bc · outbound
This paper cites Activity time series of old stars from late F to early K IV. Diagnosis from photometry.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Activity time series of old stars from late F to early K IV. Diagnosis from photometry
Reference 18
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.858744Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation f564da1e-7ab5-4366-bd4e-7c8449035b09 · outbound
This paper cites Confrontation between modelled solar integrated observables and direct observations I. Radial velocities and convective blueshift.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Confrontation between modelled solar integrated observables and direct observations I. Radial velocities and convective blueshift
Reference 19
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.846633Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 2210acf0-add3-4a6c-8d76-5c3825149825 · outbound
This paper cites and Desort, M.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation and Desort, M
Reference 20
- Resolution
- verified exact
- doi, observed 2026-07-08T09:54:50.680894Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 721e810c-634d-4c5f-ad5b-90734010af73 · outbound
This paper cites The Messenger , year = 2003, month = dec, volume =.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation The Messenger , year = 2003, month = dec, volume =
Reference 21
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-08T09:54:50.976005Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation d1253bb9-e9b7-4444-b070-58c0615b1ea8 · outbound
This paper cites an unresolved cited work.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Unresolved cited work
Reference 22
- Resolution
- unresolved
- raw_fallback, observed 2026-07-08T09:54:50.972477Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 009e1543-dad1-4761-af29-6bbc4ff0a035 · outbound
This paper cites The magnetically quiet solar surface dominates HARPS-N solar RVs during low activity.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation The magnetically quiet solar surface dominates HARPS-N solar RVs during low activity
Reference 23
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.867259Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation d33d5395-c154-4a2f-8415-2a7e626f5fc1 · outbound
This paper cites Investigating stellar activity through eight years of Sun-as-a-star observations.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Investigating stellar activity through eight years of Sun-as-a-star observations
Reference 24
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.798754Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 89882a24-19c7-4c29-910d-7893fda9f242 · outbound
This paper cites Revisiting $\epsilon$ Eridani with NEID: Identifying New Activity-Sensitive Lines in a Young K Dwarf Star.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Revisiting $\epsilon$ Eridani with NEID: Identifying New Activity-Sensitive Lines in a Young K Dwarf Star
Reference 25
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.786074Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation ecac4cf9-ac59-4dfa-b8dd-8a9c56d30849 · outbound
This paper cites Optimizing exoplanet transit searches around low-mass stars with inclination constraints.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Optimizing exoplanet transit searches around low-mass stars with inclination constraints
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.753117Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation ffc750e4-2947-41cd-8e5b-1cf46c2b360f · outbound
This paper cites The Sun as a planet-host star: Proxies from SDO images for HARPS radial-velocity variations.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation The Sun as a planet-host star: Proxies from SDO images for HARPS radial-velocity variations
Reference 27
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.676365Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation cb2e82f9-9356-4384-945f-5564f2bce0e7 · outbound
This paper cites On the Feasibility of Intense Radial Velocity Surveys for Earth-twin Discoveries.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation On the Feasibility of Intense Radial Velocity Surveys for Earth-twin Discoveries
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.707562Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation eedc47fa-af83-4990-bfa8-bcdbfe43ed05 · outbound
This paper cites keywords =.
Reference 29
- Resolution
- verified exact
- doi, observed 2026-07-08T09:54:50.716270Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 816fb32d-a4a0-4435-bb85-1653cd8debcf · outbound
This paper cites Measuring precise radial velocities on individual spectral lines. I. Validation of the method and application to mitigate stellar activity.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Measuring precise radial velocities on individual spectral lines. I. Validation of the method and application to mitigate stellar activity
Reference 30
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.794972Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation d877455b-0d7a-4c6f-a650-b727973f188e · outbound
This paper cites Radial-Velocity Fitting Challenge. II. First results of the analysis of the data set.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Radial-Velocity Fitting Challenge. II. First results of the analysis of the data set
Reference 31
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.734396Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation d7a57487-b40b-4b8c-bbbc-6ea9ce40a27f · outbound
This paper cites Stellar surface information from the Ca II H&K lines I. Intensity profiles of the solar activity components.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Stellar surface information from the Ca II H&K lines I. Intensity profiles of the solar activity components
Reference 32
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.757364Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 577845c0-f37f-4447-868e-9d215479f0bf · outbound
This paper cites YARARA: Significant improvement of RV precision through post-processing of spectral time-series.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation YARARA: Significant improvement of RV precision through post-processing of spectral time-series
Reference 33
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.694441Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 058eadc3-3ca1-41d5-a697-e01d1c071717 · outbound
This paper cites Extreme Precision Radial Velocity Working Group Final Report.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Extreme Precision Radial Velocity Working Group Final Report
Reference 34
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-08T09:54:50.698680Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 56cca205-d639-4207-b9b4-bff8f5c81648 · outbound
This paper cites Long-term stellar activity variations and their effect on radial-velocity measurements.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Long-term stellar activity variations and their effect on radial-velocity measurements
Reference 35
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.761218Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 96059ce0-eb6d-4c05-93d4-0d2e17e4545a · outbound
This paper cites Separating planetary reflex Doppler shifts from stellar variability in the wavelength domain.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Separating planetary reflex Doppler shifts from stellar variability in the wavelength domain
Reference 36
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.790593Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation a4a38e12-c398-4e08-a931-efbd82cb2c7f · outbound
This paper cites Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum
Reference 37
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.834721Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation aa83ad02-8d08-4737-9b45-df9d3e5dbf0a · outbound
This paper cites Precise Doppler Monitoring of Barnard's Star.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Precise Doppler Monitoring of Barnard's Star
Reference 38
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.729482Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 8fd54cf0-bd40-43bc-a2b9-84d7577311e1 · outbound
This paper cites Machine Learning 45(1), 5–32 (Oct 2001).
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Machine Learning 45(1), 5–32 (Oct 2001)
Reference 39
- Resolution
- verified exact
- doi, observed 2026-07-08T09:54:50.801961Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 32d4ff71-5f05-4b51-89b0-bf84c600369d · outbound
This paper cites Three-dimensional simulations of near-surface convection in main-sequence stars. IV. Effect of small-scale magnetic flux concentrations on centre-to-limb variation and spectral lines.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Three-dimensional simulations of near-surface convection in main-sequence stars. IV. Effect of small-scale magnetic flux concentrations on centre-to-limb variation and spectral lines
Reference 40
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.766327Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 6c9e31ff-56e3-4f46-9872-bd3f09d6e58c · outbound
This paper cites Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations
Reference 41
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.863182Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation f221d3a6-6d09-4d25-b63c-63ac1351e909 · outbound
This paper cites Plato Mission Conference 2021 , year = 2021, month = oct, eid =.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Plato Mission Conference 2021 , year = 2021, month = oct, eid =
Reference 42
- Resolution
- verified exact
- doi, observed 2026-07-08T09:54:50.837674Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 27eab946-3272-41b7-867d-3a85c8e26c7d · outbound
This paper cites Stellar signal components seen in HARPS and HARPS-N solar radial velocities.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Stellar signal components seen in HARPS and HARPS-N solar radial velocities
Reference 43
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.725058Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation cb4efe61-42f2-4582-b124-91e01a6a4a13 · outbound
This paper cites , keywords =.
Reference 44
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-08T09:54:50.961607Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 683fac34-bb5e-495a-b346-a3b5f0a59986 · outbound
This paper cites The effects of granulation and supergranulation on Earth-mass planet detectability in the habitable zone around F6-K4 stars.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation The effects of granulation and supergranulation on Earth-mass planet detectability in the habitable zone around F6-K4 stars
Reference 45
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.712562Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 98759d01-ecbc-4adc-85c1-8875dcb5e0a0 · outbound
This paper cites Gaussian Process regression for astronomical time-series.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Gaussian Process regression for astronomical time-series
Reference 46
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.744623Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 134f0673-8bb9-4d50-a64e-483098a8f368 · outbound
This paper cites an unresolved cited work.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Unresolved cited work
Reference 47
- Resolution
- unresolved
- raw_fallback, observed 2026-07-08T09:54:50.979645Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 1bc53e8a-f55e-49bc-a9e7-5edba5caaa25 · outbound
This paper cites No planet for HD 166435.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation No planet for HD 166435
Reference 48
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.749357Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 1fd3b47b-91c7-48a4-b3d7-fc654805daa0 · outbound
This paper cites 2025 , pages =.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation 2025 , pages =
Reference 49
- Resolution
- metadata mismatch
- doi, observed 2026-07-08T09:54:50.830008Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation cf2c844a-fe5d-457a-84f7-c3f6d8a93b7d · outbound
This paper cites Unsigned magnetic flux proxy from solar optical intensity spectra.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Unsigned magnetic flux proxy from solar optical intensity spectra
Reference 50
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.702899Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation d41cda48-4df0-45c9-856b-c7eba493eb18 · outbound
This paper cites and Watson, Christopher, A.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation and Watson, Christopher, A
Reference 51
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-08T09:54:50.968860Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 493805dc-3b46-4970-8198-d3dc977d7b12 · outbound
This paper cites Sensitivity of spectral lines to granulation: The Sun.
Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Sensitivity of spectral lines to granulation: The Sun
Reference 52
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T09:54:50.813548Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Pith citing papers
No inbound Pith citation observations are available.