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Optical Spectra of Candidate International Celestial Reference Frame (ICRF) Flat-spectrum Radio Sources. III
被引:5
|作者:
Titov, O.
[1
]
Pursimo, T.
[2
]
Johnston, Helen M.
[3
]
Stanford, Laura M.
[1
]
Hunstead, Richard W.
[3
]
Jauncey, David L.
[4
]
Zenere, Katrina A.
[5
]
机构:
[1] Geosci Australia, POB 378, Canberra, ACT 2601, Australia
[2] Nord Opt Telescope, Nord Opt Telescope Apartado 474E-38700, Santa Cruz De La Palma, Santa Cruz De T, Spain
[3] Univ Sydney, Sydney Inst Astron, Sch Phys, Sydney, NSW 2006, Australia
[4] CSIRO Astron & Space Sci, ATNF & Mt Stromlo Observ, Cotter Rd, Weston, ACT 2611, Australia
[5] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia
基金:
美国安德鲁·梅隆基金会;
美国国家科学基金会;
关键词:
BL Lacertae objects: general;
galaxies: active;
quasars: emission lines;
radio continuum: general;
reference systems;
KILOMETER ARRAY PATHFINDER;
BASE-LINE INTERFEROMETRY;
DIGITAL-SKY-SURVEY;
PROPER MOTIONS;
ASTROMETRY;
ABSORPTION;
GALAXY;
D O I:
10.3847/1538-3881/aa61fd
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
In extending our spectroscopic program, which targets sources drawn from the International Celestial Reference Frame ( ICRF) Catalog, we have obtained spectra for similar to 160 compact, flat-spectrum radio sources and determined redshifts for 112 quasars and radio galaxies. A further 14 sources with featureless spectra have been classified as BL Lac objects. Spectra were obtained at three telescopes: the 3.58m European Southern Observatory New Technology Telescope, and the two 8.2m Gemini telescopes in Hawaii and Chile. While most of the sources are powerful quasars, a significant fraction of radio galaxies is also included from the list of non-defining ICRF radio sources.
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