Classification of Flat Spectrum Radio Quasars by Optical Activity Types

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
A. M. Mickaelian, H. V. Abrahamyan, G. M. Paronyan, G. A. Mikayelyan, A. G. Sukiasyan, V. K. Mkrtchyan
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引用次数: 0

Abstract

We have carried out a spectral classification by the activity types for a subsample of blazars from the BZCAT v.5 Catalogue, namely the Flat Spectrum Radio Quasars (FSRQ) candidates, designated in the catalogue as BZQ subtype objects. The classification is based on the Sloan Digital Sky Survey (SDSS) homogeneous medium-resolution optical spectroscopy and along with the standard BPT-type diagnostic diagrams, we have applied our newly introduced fine classification scheme with subtypes of quasars and considering many more features. Out of 1909 BZQ objects, 618 having SDSS spectra were classified, resulting in 445 broad-line QSOs, 19 narrow-line QSOs, 138 broad-line Seyferts, 8 narrow-line Seyferts, and 2 Emission-line galaxies without a proper classification. We have calculated the absolute magnitudes and luminosities for all objects to distinguish QSOs from Seyferts, as defined by the Catalogue of QSOs and Active Galaxies, -22m.25 separation limit. This way 148 objects changed their BZCAT subtypes between BZQ to BZG, and also 6 BZQ objects to BZU.

按光学活动类型对平谱射电类星体进行分类
我们对BZCAT v.5目录中的一个子样本,即平谱射电类星体(FSRQ)候选者,进行了活动类型的光谱分类,在目录中被指定为BZQ子类型天体。该分类是基于斯隆数字巡天(SDSS)的同质中分辨率光学光谱,并结合标准的 BPT 类型诊断图,应用了我们新引入的类星体亚型精细分类方案,并考虑了更多的特征。在1909个BZQ天体中,我们对618个具有SDSS光谱的天体进行了分类,其中包括445个宽线类星体、19个窄线类星体、138个宽线塞弗体、8个窄线塞弗体和2个没有正确分类的发射线星系。我们计算了所有天体的绝对星等和亮度,以便按照《QSO和活动星系目录》中-22m.25的分离极限来区分QSO和Seyfer。这样就有148个天体的BZCAT子类型从BZQ变为了BZG,还有6个BZQ天体变为了BZU。
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来源期刊
Astrophysics
Astrophysics 地学天文-天文与天体物理
CiteScore
0.90
自引率
20.00%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Astrophysics (Ap) is a peer-reviewed scientific journal which publishes research in theoretical and observational astrophysics. Founded by V.A.Ambartsumian in 1965 Astrophysics is one of the international astronomy journals. The journal covers space astrophysics, stellar and galactic evolution, solar physics, stellar and planetary atmospheres, interstellar matter. Additional subjects include chemical composition and internal structure of stars, quasars and pulsars, developments in modern cosmology and radiative transfer.
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