Statements (90)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:nebula
|
| gptkbp:bfsLayer |
5
|
| gptkbp:bfsParent |
gptkb:Pinwheel_Galaxy
gptkb:NGC_6685 |
| gptkbp:analysis |
data analysis ongoing
data analysis continues to yield new insights |
| gptkbp:apparent_magnitude |
maximum magnitude of about -19.3
|
| gptkbp:archives |
data archived for future research
|
| gptkbp:bomb_load |
thermonuclear explosion of a white dwarf
|
| gptkbp:collaborations |
involved multiple international collaborations
involved multiple international observatories collaborated with various astrophysical research teams involved collaborative research efforts across institutions involved collaborative efforts in the scientific community collaborative research efforts initiated inspired collaborative projects in astronomy |
| gptkbp:community_engagement |
captured public interest due to its brightness
generated public interest in astronomy engaged the astronomy community |
| gptkbp:conference |
discussed in scientific conferences
|
| gptkbp:conservation_efforts |
remnant is still being studied
remnants are still being studied remnant composition analyzed |
| gptkbp:discovered_by |
gptkb:Robert_Kirshner
|
| gptkbp:distance |
approximately 50 million light-years
approximately 60 million light-years used for measuring distances in the universe distance estimated using standard candles |
| gptkbp:education |
used in educational contexts to teach about supernovae
educational impact on astronomy students |
| gptkbp:events |
follow-up observations continued for years after discovery
follow-up observations conducted by various telescopes |
| gptkbp:future_plans |
future research planned on remnants
|
| gptkbp:has_color |
color index measured during observations
|
| gptkbp:has_spectral_type |
Type Ia spectrum
|
| gptkbp:historical_context |
historically significant supernova event
|
| gptkbp:historical_significance |
historically significant in the study of supernovae
|
| gptkbp:hosts |
NGC 4526
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1994 D
|
| gptkbp:impact |
contributed to understanding of dark energy
helped refine the value of the Hubble constant significant impact on dark energy research impactful on astrophysics research |
| gptkbp:is_essential_for |
used to measure cosmic distances
important for cosmology studies |
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
|
| gptkbp:legacy |
remains a legacy in supernova research
legacy in the study of Type Ia supernovae |
| gptkbp:length |
thermonuclear explosion
approximately 1994-03-10 |
| gptkbp:lighting |
similar to other Type Ia supernovae
light curve shows a rapid rise and decline light curve observed used for light curve fitting techniques light curve analysis provided insights into supernova behavior reached peak brightness in 1994 light curve fitting used for distance measurement light curve shape typical for Type Ia light echo phenomenon observed |
| gptkbp:located_in |
galaxy NGC 4526
|
| gptkbp:media_coverage |
received significant media coverage
|
| gptkbp:notable_feature |
one of the best-studied supernovae
|
| gptkbp:notable_work |
studied for its role in measuring cosmic distances
|
| gptkbp:provides_information_on |
data sharing among institutions
data shared among astronomers worldwide |
| gptkbp:publishes |
numerous scientific publications resulting from its study
led to numerous publications in astrophysics journals numerous scientific publications produced data published in various astronomical journals |
| gptkbp:receives_funding_from |
funded by various astronomical research grants
|
| gptkbp:redshift |
0.0034
0.0038 |
| gptkbp:related_model |
theoretical models developed based on observations
tested various theoretical models of supernova explosions |
| gptkbp:research |
utilized advanced observational techniques
extensive photometric and spectroscopic data available extensive observational data collected spectroscopy revealed details of the explosion mechanism faced observational challenges due to its distance part of a rich observational history of supernovae spectroscopy used to analyze composition observational campaigns organized part of observational history of supernovae various observational techniques employed |
| gptkbp:storage |
photometric data collected by various telescopes
photometry performed to track brightness changes |
| gptkbp:type |
gptkb:Type_Ia_supernova
|
| gptkbp:universe |
has cosmological implications for understanding the universe
significant for cosmological models |
| gptkbp:year_created |
1994-03-10
|