Emission lines properties of the radio-loud quasar LAMOST J1131+3114

Z. X. Shi; G. Comte; G. Comte; A. L. Luo; Y. H. Zhao; J. K. Zhao; J. K. Zhao; T. D. Oswalt; F. C. Wu

doi:10.1051/0004-6361/201321750

Emission lines properties of the radio-loud quasar LAMOST J1131+3114

Z. X. Shi
, G. Comte
, G. Comte
, A. L. Luo
, Y. H. Zhao
, J. K. Zhao
, J. K. Zhao
, T. D. Oswalt
, F. C. Wu

Chinese Academy of Sciences
Aix-Marseille University
Florida Institute of Technology

Research output: Contribution to journal › Article › peer-review

Original language	American English
Journal	Astronomy and Astrophysics
Volume	564
DOIs	https://doi.org/10.1051/0004-6361/201321750
State	Published - Apr 1 2014
Externally published	Yes

Disciplines

Astrophysics and Astronomy
Physics

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10.1051/0004-6361/201321750License: Unspecified

Cite this

@article{ec5c3921350b405788d1ba9dff4576ed,

title = "Emission lines properties of the radio-loud quasar LAMOST J1131+3114",

author = "Shi, \{Z. X.\} and G. Comte and G. Comte and Luo, \{A. L.\} and Zhao, \{Y. H.\} and Zhao, \{J. K.\} and Zhao, \{J. K.\} and Oswalt, \{T. D.\} and Wu, \{F. C.\}",

note = "The radio-loud quasar LAMOST J1131+3114 (Ton 580, B2 1128+315), showing asymmetrical profile in Hβ and [O III] lines, has been selected from the LAMOST Pilot Survey for further study. We present an analysis of its emission lines by means of multiple Gaussian fitting, performed on LAMOST, Apache Point Observatory, and archival spectra.",

year = "2014",

month = apr,

day = "1",

doi = "10.1051/0004-6361/201321750",

language = "American English",

volume = "564",

journal = "Astronomy and Astrophysics",

issn = "1432-0746",

publisher = "EDP Sciences",

}

TY - JOUR

T1 - Emission lines properties of the radio-loud quasar LAMOST J1131+3114

AU - Shi, Z. X.

AU - Comte, G.

AU - Luo, A. L.

AU - Zhao, Y. H.

AU - Zhao, J. K.

AU - Oswalt, T. D.

AU - Wu, F. C.

N1 - The radio-loud quasar LAMOST J1131+3114 (Ton 580, B2 1128+315), showing asymmetrical profile in Hβ and [O III] lines, has been selected from the LAMOST Pilot Survey for further study. We present an analysis of its emission lines by means of multiple Gaussian fitting, performed on LAMOST, Apache Point Observatory, and archival spectra.

PY - 2014/4/1

Y1 - 2014/4/1

UR - https://ui.adsabs.harvard.edu/abs/2014A&A...564A..89S/abstract

U2 - 10.1051/0004-6361/201321750

DO - 10.1051/0004-6361/201321750

M3 - Article

SN - 1432-0746

VL - 564

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

ER -

Emission lines properties of the radio-loud quasar LAMOST J1131+3114

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