scienceCase
P116263
predicate
Indicates a relationship where something serves as, constitutes, or provides justification as a scientific case or rationale for a study, hypothesis, or investigation.
All labels observed (4)
| Label | Occurrences |
|---|---|
| scienceCase canonical | 51 |
| primaryScienceCase | 7 |
| scienceCaseDocument | 1 |
| scientificRationale | 1 |
Description generation (PDg)
The one-sentence description above was generated by prompting gpt-5.1 with the predicate name and this instruction.
Instruction
Given a predicate that represents a relationship or action between entities, generate a one-sentence description explaining its meaning. # Instructions Focus on describing the relationship, not the entities themselves. # Response Format Begin the description with \' Indicates...\'
Input
Predicate: scienceCase
Generated description
Indicates a relationship where something serves as, constitutes, or provides justification as a scientific case or rationale for a study, hypothesis, or investigation.
Sample triples (60)
| Subject | Object |
|---|---|
| LBNE experiment | study of matter–antimatter asymmetry via neutrinos ⓘ |
| LBNE experiment | proton decay searches in large underground detector ⓘ |
| LBNE experiment | detection of supernova neutrinos ⓘ |
| FEROS | search for exoplanets ⓘ |
| FEROS | characterization of exoplanet host stars ⓘ |
| FEROS | stellar activity studies ⓘ |
| FEROS | binary star orbits ⓘ |
| FEROS | stellar oscillations ⓘ |
| Mars Sample Return campaign | laboratory instruments on Earth are more capable than in-situ instruments on Mars rovers via predicate surface "scientificRationale" ⓘ |
| CHARIS | detection of young giant exoplanets ⓘ |
| CHARIS | measurement of exoplanet spectra ⓘ |
| CHARIS | study of planetary system architectures ⓘ |
| SITELLE | detailed mapping of emission lines in galaxies ⓘ |
| SITELLE | study of ionization mechanisms in nebulae ⓘ |
| SITELLE | measurement of gas velocities in extended objects ⓘ |
| SPIRou | search for Earth-like planets around cool stars ⓘ |
| SPIRou | characterization of exoplanetary systems ⓘ |
| SPIRou | investigation of star–planet interactions ⓘ |
| SPIRou | study of stellar magnetism ⓘ |
| SPIRou | study of pre-main-sequence stars ⓘ |
| SPIRou | study of young stellar objects ⓘ |
| Pan-STARRS survey | near-Earth object detection ⓘ |
| Pan-STARRS survey | asteroid discovery ⓘ |
| Pan-STARRS survey | comet discovery ⓘ |
| Pan-STARRS survey | supernova search ⓘ |
| Pan-STARRS survey | variable star studies ⓘ |
| Pan-STARRS survey | cosmology ⓘ |
| Pan-STARRS survey | Milky Way structure ⓘ |
| Pan-STARRS survey | galaxy evolution ⓘ |
| ESO ELT |
Science with the European Extremely Large Telescope
via predicate surface "scienceCaseDocument"
ⓘ
linked to:
European Extremely Large Telescope
|
| VISTA Kilo-degree Infrared Galaxy survey | measure galaxy clustering ⓘ |
| VISTA Kilo-degree Infrared Galaxy survey | constrain dark energy ⓘ |
| VISTA Kilo-degree Infrared Galaxy survey | constrain cosmological parameters ⓘ |
| VISTA Kilo-degree Infrared Galaxy survey | study galaxy stellar masses ⓘ |
| VISTA Kilo-degree Infrared Galaxy survey | study galaxy star-formation histories ⓘ |
| VISTA Kilo-degree Infrared Galaxy survey | identify high-redshift quasars ⓘ |
| ZIMPOL | characterization of scattered light from circumstellar dust ⓘ |
| ZIMPOL | mapping of circumstellar disks ⓘ |
| ZIMPOL | search for faint companions ⓘ |
| IRDIS | exoplanet imaging via predicate surface "primaryScienceCase" ⓘ |
| IRDIS | circumstellar disk imaging via predicate surface "primaryScienceCase" ⓘ |
| UltraVISTA survey | high-redshift galaxy populations ⓘ |
| UltraVISTA survey | mass assembly of galaxies ⓘ |
| UltraVISTA survey | evolution of the galaxy stellar mass function ⓘ |
| UltraVISTA survey | quiescent galaxies at high redshift ⓘ |
| UltraVISTA survey | star-forming galaxies at high redshift ⓘ |
| UltraVISTA survey | luminous and massive galaxies in the early universe ⓘ |
| UltraVISTA survey | cosmic star-formation history ⓘ |
| UltraVISTA survey | large-scale structure at high redshift ⓘ |
| VISTA Variables in the Via Lactea | distance determination using variable stars ⓘ |