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Record W7005877273

Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer

2019· article· en· W7005877273 on OpenAlexfundno aff

Bibliographic record

VenueLeiden Repository (Leiden University) · 2019
Typearticle
Languageen
FieldEconomics, Econometrics and Finance
TopicDiverse Scientific and Economic Studies
Canadian institutionsnot available
FundersLawrence Livermore National LaboratoryJapan Aerospace Exploration AgencyEurostarsJapan Society for the Promotion of ScienceCanadian Space AgencyScience Mission DirectorateGoddard Space Flight CenterMagyar Tudományos AkadémiaSLAC National Accelerator LaboratorySmithsonian Astrophysical ObservatoryCentre National d’Etudes SpatialesMinistry of Education, Culture, Sports, Science and TechnologyNational Aeronautics and Space AdministrationEuropean Space AgencyScience and Technology Facilities CouncilStrongNederlandse Organisatie voor Wetenschappelijk OnderzoekNatural Sciences and Engineering Research Council of CanadaSmithsonian Institution
KeywordsCrab NebulaSpectrometerThermalNebulaHyperspectral imaging
DOInot available

Abstract

fetched live from OpenAlex

The Crab nebula originated from a core-collapse supernova (SN) explosion observed in 1054 A. D. When viewed as a supernova remnant (SNR), it has an anomalously low observed ejecta mass and kinetic energy for an Fe-core collapse SN.Intensive searches were made for a massive shell that solves this discrepancy, but none has been detected.An alternative idea is that the SN 1054 is an electron-capture (EC) explosion with a lower explosion energy by an order of magnitude than Fe-core collapse SNe.In the X-rays, imaging searches were performed for the plasma emission from the shell in the Crab outskirts to set a stringent upper limit to the X-ray emitting mass.However, the extreme brightness of the source hampers access to its vicinity.We thus employed spectroscopic technique using the X-ray micro-calorimeter onboard the Hitomi satellite.By exploiting its superb energy resolution, we set an upper limit for emission or absorption features from yet undetected thermal plasma in the 2-12 keV range.We also re-evaluated the existing Chandra and XMM-Newton data.By assembling these results, a new upper limit was obtained for the X-ray plasma mass of < ∼ 1 M for a wide range of assumed shell radius, size, and plasma temperature both in and out

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)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.007
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0030.002
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0070.001

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 head0.014
GPT teacher head0.165
Teacher spread0.150 · 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 designObservational
Domainnot available
GenreEmpirical

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

Citations0
Published2019
Admission routes1
Has abstractno

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