Statements (60)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:nebula
|
| gptkbp:bfsLayer |
5
|
| gptkbp:bfsParent |
gptkb:Messier_101
gptkb:the_Sunflower_Galaxy gptkb:Messier_83 |
| gptkbp:analysis |
data analysis performed by astronomers
|
| gptkbp:apparent_magnitude |
maximum magnitude of about -19.5
brightness peaked in April 1994 |
| gptkbp:associated_with |
cosmological studies
|
| gptkbp:collaborations |
collaborated with international teams
involved collaborative research efforts involved multiple astronomical observatories part of collaborative projects in astronomy fostered scientific collaboration across institutions |
| gptkbp:collection |
data collection involved multiple instruments
|
| gptkbp:community |
part of the global research community
|
| gptkbp:community_engagement |
engaged the astronomical community
|
| gptkbp:community_involvement |
involved in outreach activities for public engagement
|
| gptkbp:composed_of |
produced elements like iron and nickel
|
| gptkbp:conference |
presented at scientific conferences
|
| gptkbp:conservation_efforts |
remnant not yet detected
|
| gptkbp:constellation |
supernova remnants studied in later years
|
| gptkbp:discovered_by |
gptkb:Robert_Kirshner
|
| gptkbp:distance |
approximately 15 million light-years
used for measuring cosmic distances |
| gptkbp:education |
educational impact on astronomy students
|
| gptkbp:events |
follow-up observations conducted for years after
follow-up studies continued for years |
| gptkbp:future_plans |
future research opportunities identified
|
| gptkbp:has_spectral_type |
Type Ia spectrum
|
| gptkbp:historical_significance |
historical significance in the study of supernovae
|
| gptkbp:hosts |
NGC 4526
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1994ae
|
| gptkbp:impact |
influenced studies on dark energy
significant scientific impact on astrophysics |
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
observational records maintained for analysis |
| gptkbp:legacy |
legacy in supernova research
|
| gptkbp:length |
around 1994
|
| gptkbp:lighting |
light curve observed
declined after peak brightness light curve analysis provided insights light curve fitting used for analysis |
| gptkbp:located_in |
galaxy NGC 4526
|
| gptkbp:notable_for |
contribution to distance measurement of galaxies
|
| gptkbp:provides_information_on |
data sharing among researchers encouraged
|
| gptkbp:publishes |
data published in scientific journals
numerous publications resulting from observations |
| gptkbp:receives_funding_from |
funded by various research grants
|
| gptkbp:redshift |
0.0034
|
| gptkbp:related_model |
tested theoretical models of supernova explosions
|
| gptkbp:research |
spectroscopy revealed chemical composition
utilized various observational techniques part of extensive observational campaigns photometric and spectroscopic data collected |
| gptkbp:research_focus |
important for understanding supernova mechanics
|
| gptkbp:scientific_classification |
classified as a supernova in the 1990s
|
| gptkbp:type |
gptkb:Type_Ia_supernova
|
| gptkbp:universe |
has cosmological implications for universe expansion
|
| gptkbp:year_created |
1994-04-02
|