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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 OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.

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

fetched live from OpenAlex

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.

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 categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.544
Threshold uncertainty score0.302

Codex and Gemma teacher scores by category

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

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 head0.027
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