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Record W3209047804 · doi:10.1017/pasa.2021.31

[no title]

2021· article· en· W3209047804 on OpenAlexafffund
I. Kamp, Mitsuhiko Honda, Hideko Nomura, M. Audard, D. Fedele, L. B. F. M. Waters, Yuri Aikawa, Andrea Banzatti, J. E. Bowey, M. Bradford, C. Dominik, Kenji Furuya, E. Habart, Daisuke Ishihara, Doug Johnstone, Grant M. Kennedy, M. Kim, Quentin Kral, S. Lai, Bengt Larsson, M. K. McClure, A. Miotello, Munetake Momose, Takao Nakagawa, David A. Naylor, B. Nisini, Shota Notsu, Takashi Onaka, É. Pantin, L. Podio, P. Riviére-Marichalar, W. R. M. Rocha, Peter Roelfsema, T. Shimonishi, Ya‐Wen Tang, M. Takami, Ryo Tazaki, S. Wolf, M. C. Wyatt, N. Ysard

Bibliographic record

VenueUvA-DARE (University of Amsterdam) · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of LethbridgeHerzberg Institute of Astrophysics
FundersMinistry of Science and Technology, TaiwanAgenzia Spaziale ItalianaNederlandse Organisatie voor Wetenschappelijk OnderzoekUniversiteit LeidenJapan Society for the Promotion of ScienceMinistry of Education, Culture, Sports, Science and TechnologyRIKENNatural Sciences and Engineering Research Council of CanadaEuropean Commission
KeywordsSpicaPhysicsAstronomyAstrophysicsAstrobiology

Abstract

fetched live from OpenAlex

In this era of spatially resolved observations of planet-forming disks with Atacama Large Millimeter Array (ALMA) and large ground-based telescopes such as the Very Large Telescope (VLT), Keck, and Subaru, we still lack statistically relevant information on the quantity and composition of the material that is building the planets, such as the total disk gas mass, the ice content of dust, and the state of water in planetesimals. SPace Infrared telescope for Cosmology and Astrophysics (SPICA) is an infrared space mission concept developed jointly by Japan Aerospace Exploration Agency (JAXA) and European Space Agency (ESA) to address these questions. The key unique capabilities of SPICA that enable this research are (1) the wide spectral coverage $10{-}220 μm$ , (2) the high line detection sensitivity of $(1{-}2) × 10^{-19} W m^{-2}$ with $R ∼ 2 000{-}5 000$ in the far-IR (SAFARI), and $10^{-20} W m^{-2}$ with $R ∼ 29 000$ in the mid-IR (SPICA Mid-infrared Instrument (SMI), spectrally resolving line profiles), (3) the high far-IR continuum sensitivity of 0.45 mJy (SAFARI), and (4) the observing efficiency for point source surveys. This paper details how mid- to far-IR infrared spectra will be unique in measuring the gas masses and water/ice content of disks and how these quantities evolve during the planet-forming period. These observations will clarify the crucial transition when disks exhaust their primordial gas and further planet formation requires secondary gas produced from planetesimals. The high spectral resolution mid-IR is also unique for determining the location of the snowline dividing the rocky and icy mass reservoirs within the disk and how the divide evolves during the build-up of planetary systems. Infrared spectroscopy (mid- to far-IR) of key solid-state bands is crucial for assessing whether extensive radial mixing, which is part of our Solar System history, is a general process occurring in most planetary systems and whether extrasolar planetesimals are similar to our Solar System comets/asteroids. We demonstrate that the SPICA mission concept would allow us to achieve the above ambitious science goals through large surveys of several hundred disks within $∼\!2.5$ months of observing time.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow), Insufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.084
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.010
GPT teacher head0.186
Teacher spread0.176 · 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 teacher head, not a consensus.

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

Citations8
Published2021
Admission routes2
Has abstractyes

Explore more

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