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SUMMARY:Asiago Supernova Catalogue objects subsample characteristics
DTSTART;VALUE=DATE-TIME:20161011T121500Z
DTEND;VALUE=DATE-TIME:20161011T124500Z
DTSTAMP;VALUE=DATE-TIME:20260722T162544Z
UID:indico-contribution-513@cern.ch
DESCRIPTION:Speakers: Alexander Lyapin (National Research Nuclear Universi
 ty "MEPhI")\nThe homogeneous subsample characteristics understanding is ne
 cessary for the investigation of any astrophysical objects redshift distri
 bution\, for example\, gamma-ray bursts. The type Ia supernovae considered
  as a homogeneous subsample because of suggestion that these luminous even
 ts might be used as standard candles for cosmological measurements occurs 
 since the earliest studies of supernovae in 1938. The parameters of our Me
 tagalaxy Ω and ? were determine due sample of Ia supernovae from the Supe
 rnova Cosmology Project analysis in 1998. Since then more than 4000 supern
 ovae were added. \n\nThe results of the redshift distribution analysis for
  supernova from the catalog are presented in this work. The ability to use
  an analyzed dataset as homogeneous subsample also is discussed.\n\nhttps:
 //indico.particle.mephi.ru/event/4/contributions/513/
LOCATION:Milan Hotel Hall of the 2nd floor
URL:https://indico.particle.mephi.ru/event/4/contributions/513/
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