J1144–4308

Source: Wikipedia, the free encyclopedia.
SMSS J114447.77–430859.3
Approximate location of SMSS J114447.77–430859.3 in the sky (circled)
Observation data (Epoch J2000)
ConstellationCentaurus
Right ascension11h 44m 47.76096s[1]
Declination−43° 08′ 59.4276″[1]
Redshift0.83[2]
Other designations
2MASS J11444776-4308594[1]
See also: Quasar, List of quasars

SMSS J114447.77–430859.3 or J1144 or J1144–4308 is a very bright (unbeamed)

Southern Cross (Crux). The SkyMapper Southern Survey (SMSS) was used to ascertain its spectral properties.[2]

J1144 was identified during a search for

binary stars.[2][3] Despite being relatively bright, it had escaped classification as a quasar in earlier searches, which avoided the crowded fields near the galactic equator.[4]

After examining various data sets, the study group determined that J1144 is the most intrinsically luminous quasar known over the last ~9 Gyr of cosmic history, having a luminosity 8 times greater than 3C 273 in Virgo.[2]

According to the lead researcher Dr Christofer Onken, of the Australian National University: While black holes are themselves not visible; their gravity is so great that not even light can escape them, they are observable because of the matter that swirls around them.

References

  1. ^ a b c "SMSS J114447.77-430859.3". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2022-11-03.
  2. ^
    S2CID 249538461
    .
  3. ABC News Online
    , 2022-06-15
  4. ^ "Fastest-growing black hole of the last 9 billion years". cosmosmagazine.com. 2022-06-15. Retrieved 2022-06-15.