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Record W2738252206 · doi:10.1089/ast.2016.1543

Infrared Spectrometer for ExoMars: A Mast-Mounted Instrument for the Rover

2017· article· en· W2738252206 on OpenAlexaff
Oleg Korablev, Yurii Dobrolensky, Н. А. Евдокимова, Anna Fedorova, R. O. Kuzmin, Sergei N. Mantsevich, E. A. Cloutis, John Carter, F. Poulet, J. Flahaut, A. D. Griffiths, M. Gunn, Nicole Schmitz, Javier Martín‐Torres, María‐Paz Zorzano, Д. С. Родионов, Jorge L. Vago, A. Yu. Titov, Nikita A. Vyazovetsky, Аlexander Trokhimovskiy, A. G. Sapgir, Yurii K. Kalinnikov, Alexei A. Shapkin, A. Yu. Ivanov

Bibliographic record

VenueAstrobiology · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsUniversity of Winnipeg
FundersScience and Technology Facilities Council
KeywordsSpectrometerRemote sensingMartian surfaceMars Exploration ProgramContext (archaeology)Imaging spectrometerEnvironmental scienceAstrobiologyGeologyMartianOpticsPhysics

Abstract

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ISEM (Infrared Spectrometer for ExoMars) is a pencil-beam infrared spectrometer that will measure reflected solar radiation in the near infrared range for context assessment of the surface mineralogy in the vicinity of the ExoMars rover. The instrument will be accommodated on the mast of the rover and will be operated together with the panoramic camera (PanCam), high-resolution camera (HRC). ISEM will study the mineralogical and petrographic composition of the martian surface in the vicinity of the rover, and in combination with the other remote sensing instruments, it will aid in the selection of potential targets for close-up investigations and drilling sites. Of particular scientific interest are water-bearing minerals, such as phyllosilicates, sulfates, carbonates, and minerals indicative of astrobiological potential, such as borates, nitrates, and ammonium-bearing minerals. The instrument has an ∼1° field of view and covers the spectral range between 1.15 and 3.30 μm with a spectral resolution varying from 3.3 nm at 1.15 μm to 28 nm at 3.30 μm. The ISEM optical head is mounted on the mast, and its electronics box is located inside the rover's body. The spectrometer uses an acousto-optic tunable filter and a Peltier-cooled InAs detector. The mass of ISEM is 1.74 kg, including the electronics and harness. The science objectives of the experiment, the instrument design, and operational scenarios are described. Key Words: ExoMars—ISEM—Mars—Surface—Mineralogy—Spectroscopy—AOTF—Infrared. Astrobiology 17, 542–564. 1. Introduction 2. Science Objectives 2.1. Contribution to overall rover mission science 2.2. Synergies with other instruments 2.3. The method 2.3.1. Spectral range 2.3.2. Spectral resolution 2.4. Potentially detectable mineral groups 2.4.1. Phyllosilicates 2.4.2. Carbonates 2.4.3. Sulfates 2.4.4. Silica 2.4.5. Igneous minerals 2.4.6. Ferrous oxides/hydroxides 2.4.7. Organic compounds—PAHs 2.4.8. Perchlorates and chlorides 2.4.9. Oxalates 2.4.10. Water ice 2.4.11. Nitrates 2.4.12. Phosphates 2.4.13. Borates 2.4.14. Ammonium‐bearing minerals 2.5. Atmospheric studies (aerosol, gaseous content) 3. Instrument Description 3.1. Instrument concept 3.2. The optical box 3.3. The electronics box 3.4. The calibration target 4. Measurement Scenario 4.1. The experiment cycle 4.2. Operations on the surface 4.3. Resources required 4.4. Measurement performance, examples, comparison with state of the art 4.4.1. Spectral range and spectral resolution 4.4.2. Signal‐to‐noise ratio estimation 4.4.3. Estimation of detection capabilities 4.5. Environmental requirements and characterization 5. Conclusions Acknowledgments Author Disclosure Statement References

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: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.023
Threshold uncertainty score0.076

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0230.010

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 head0.027
GPT teacher head0.271
Teacher spread0.244 · 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 designBench or experimental
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".

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Citations76
Published2017
Admission routes1
Has abstractyes

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