MétaCan
Menu
← Back to cohort
Record W3081509667 · doi:10.1093/mnras/staa2139

Erratum: Atmospheric mass loss from high velocity giant impacts

2020· erratum· en· W3081509667 on OpenAlexaff
Almog Yalinewich, Hilke E. Schlichting

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2020
Typeerratum
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsCanadian Institute for Theoretical Astrophysics
Fundersnot available
KeywordsPhysicsAstrophysicsAstronomy

Abstract

fetched live from OpenAlex

We report and correct a mistake with the numerical results presented in the original paper (Yalinewich & Schlichting 2019). In the original paper, we tracked the velocities in the wrong positions: instead of a series of points on the surface of the planet, the velocity was tracked on a series of points below the surface. Therefore, although there was no error with the simulation itself, there was a mistake in the diagnostic function. In order to correct this mistake we ran the simulations again, this time with the diagnostics properly implemented. Below we discuss the affected parts in the original paper and present the corrected results and figures where relevant. Corrected version of fig. 2 in the original paper. The ground velocity measured perpendicular to the surface of the target at different latitudes for different impactor sizes. The velocity is normalised by the impact velocity, and the radius of the impactor is normalised by the radius of the target. The top panel shows the results in a linear scale, while the bottom panel shows the same results in a logarithmic scale. Corrected version of fig. 2 in the original paper. The ground velocity measured perpendicular to the surface of the target at different latitudes for different impactor sizes. The velocity is normalised by the impact velocity, and the radius of the impactor is normalised by the radius of the target. The top panel shows the results in a linear scale, while the bottom panel shows the same results in a logarithmic scale. Corrected version of fig. 4 in the original paper. A comparison between the universal curve (equation 1) and the numerical results for the case Ri/Rt = 0.05. Corrected version of fig. 4 in the original paper. A comparison between the universal curve (equation 1) and the numerical results for the case Ri/Rt = 0.05. Corrected version of fig. 8 in the original paper. Fraction of the atmosphere lost as a result of a giant collision, as a function of the mass and velocity of the impactor. The radius of the impactor is normalised by the radius of the target, and the velocity is normalised by the escape velocity. The bottom panel zooms in on the small impactor to target size regime and displays the mass loss in a logarithmic scale. Corrected version of fig. 8 in the original paper. Fraction of the atmosphere lost as a result of a giant collision, as a function of the mass and velocity of the impactor. The radius of the impactor is normalised by the radius of the target, and the velocity is normalised by the escape velocity. The bottom panel zooms in on the small impactor to target size regime and displays the mass loss in a logarithmic scale. The corrected results yield lower ground velocities at the same latitude, and hence the atmospheric mass loss is somewhat lower compared with the previous results. Therefore, whereas our previous results consistently predicted higher atmospheric mass loss compared to other numerical simulations, the corrected results presented here yield slightly lower net loss than reported by other studies. Overall, the differences between the old and new results is relatively small, and the main conclusions of the original paper remain unchanged.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.010
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: Not applicable
GenreCandidate signal: Other · Consensus signal: none
Teacher disagreement score0.042
Threshold uncertainty score0.141

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.010
Meta-epidemiology (narrow)0.0020.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0030.002
Science and technology studies0.0030.001
Scholarly communication0.0020.001
Open science0.0010.001
Research integrity0.0040.004
Insufficient payload (model declined to judge)0.0420.031

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.007
GPT teacher head0.198
Teacher spread0.191 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designNot applicable
Domainnot available
GenreOther

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations1
Published2020
Admission routes1
Has abstractno

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicGamma-ray bursts and supernovae→French-language works237,207→