SDSS J151451.78+311654.0
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| SDSS J151451.78+311654.0 | |
|---|---|
 The quasar, SDSS J151451.78+311654.0 as seen from Sloan Digital Sky Survey | |
| Observation data (J2000.0 epoch) | |
| Constellation | Corona Borealis |
| Right ascension | 15h 14m 51.78s |
| Declination | +31d 16m 54.07s |
| Redshift | 2.130612 |
| Heliocentric radial velocity | 638,741 km/s |
| Distance | 10.660 Gly (light travel time distance} |
| Apparent magnitude (V) | 0.057 |
| Apparent magnitude (B) | 0.075 |
| Surface brightness | 17.2 |
| Characteristics | |
| Type | BAL |
| Other designations | |
| PGC 1939926, CSO 1085, 2MASS J15145178+3116540, 2CXO J151451.7+311654, LQAC 228+031 003 | |
SDSS J151451.78+311654.0 also known as CSO 1085, is a quasar located in the constellation of Corona Borealis. At the redshift of 2.13, the object is located 10.6 billion light-years from Earth.[1]
Characteristics
[edit]SDSS J151451.78+311654.0 is classified as a radio-quiet luminous quasar.[2]
References
[edit]- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-06-22.
- ^ Timlin, John D.; Brandt, W. N.; Ni, Q.; Luo, B.; Pu, Xingting; Schneider, D. P.; Vivek, M.; Yi, W. (2020-02-01). "The correlations between optical/UV broad lines and X-ray emission for a large sample of quasars". Monthly Notices of the Royal Astronomical Society. 492 (1): 719–741. arXiv:1912.02189. Bibcode:2020MNRAS.492..719T. doi:10.1093/mnras/stz3433. ISSN 0035-8711.