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相关论文: Quasi-Simultaneous Two Band Optical Micro-Variabil…

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We present optical light curves of 19 radio quiet (RQ) broad absorption line (BAL) QSOs and study their rapid variability characteristics. Systematic CCD observations, aided by a careful data analysis procedure, have allowed us to clearly…

宇宙学与河外天体物理 · 物理学 2015-05-20 Ravi Joshi , Hum Chand , Alok C. Gupta , Paul J. Wiita

We present the results of an optical multi-band (BVR) photometric monitoring program of 22 core-dominated radio-loud quasars (CRLQs) and 22 radio-quiet quasars (RQQs). The aim was to compare the properties of microvariability in both types…

宇宙学与河外天体物理 · 物理学 2015-05-13 A. Ramirez , J. A. de Diego , D. Dultzin , J. -N. Gonzalez-Perez

We present the first results from a pilot programme to monitor the short term optical variability in Broad Absorption Line system QSOs. Intra-night optical variations of ~5% were detected on time scales of ~ one hour in QSOs 0846+156 and…

天体物理学 · 物理学 2009-10-30 G. C. Anupama , Arati Chokshi

The detection of rapid variability on a time-scale of hours in radio-quiet quasars (RQQSOs) could be a powerful discriminator between starburst, accretion disc and relativistic jet models of these sources. This paper contains an account of…

天体物理学 · 物理学 2009-10-30 M. Rabbette , B. McBreen , N. Smith , S. Steel

This paper presents results of a search for short-term variability in the optical band of selected high-luminosity, high-redshift radio-quiet quasars. Each quasar has been monitored typically for 2 - 4 hours with a time resolution of 2 - 5…

天体物理学 · 物理学 2009-11-10 R. Bachev , A. Strigachev , E. Semkov

In the present paper we report the detection of intra-night variability in some of the RQQSOs and one LDQ. To study intra-night variability, we carried out photometric monitoring of seven RQQSOs and one LDQ in Johnson V-passband using 1.2…

天体物理学 · 物理学 2007-05-23 A. C. Gupta , U. C. Joshi

We report on the second installment of an X-ray monitoring project of seven luminous radio-quiet quasars (RQQs). New {\sl Chandra} observations of four of these, at $4.10\leq z\leq4.35$, yield a total of six X-ray epochs, per source, with…

高能天体物理现象 · 物理学 2017-10-18 Ohad Shemmer , W. N. Brandt , Maurizio Paolillo , Shai Kaspi , Cristian Vignali , Paulina Lira , Donald P. Schneider

The long-term variability of a sample of 149 optically selected QSOs in the field of the Selected Area 94 has been studied in the R-band. The relations between variability and luminosity and between variability and redshift have been…

天体物理学 · 物理学 2007-05-23 S. Cristiani , S. Trentini , F. La Franca , P. Andreani

Strong lensed quasi-stellar objects (QSOs) are valuable probes of the universe in numerous aspects. Two of these applications, reverberation mapping and measuring time delays for determining cosmological parameters, require the source QSOs…

星系天体物理 · 物理学 2023-08-02 Yoon Chan Taak , Tommaso Treu

We present initial results from an exploratory X-ray monitoring project of two groups of comparably luminous radio-quiet quasars (RQQs). The first consists of four sources at 4.10 <= z <= 4.35, monitored by Chandra, and the second is a…

In this paper we present results of a short-term optical monitoring of 13 blazars. The objects were monitored mostly in the R-band for a total of ~ 160 hours between 2006 and 2011. We study the nature of the short-term variations and show…

高能天体物理现象 · 物理学 2013-11-21 R. Bachev , E. Semkov , A. Strigachev , Alok C. Gupta , Haritma Gaur , B. Mihov , S. Boeva , L. Slavcheva-Mihova

We study systematically the ~0.1-1200 Hz quasi-periodic oscillations (QPOs) and broad noise components observed in the power spectra of non-pulsing neutron-star and black-hole low-mass X-ray binaries. We show that among these components we…

天体物理学 · 物理学 2009-10-31 Dimitrios Psaltis , Tomaso Belloni , Michiel van der Klis

We present an analysis of quasar variability from data collected during a photometric monitoring of 50 objects carried out at CNPq/Laboratorio Nacional de Astrofisica, Brazil, between March 1993 and July 1996. A distinctive feature of this…

天体物理学 · 物理学 2009-10-31 A. Garcia , L. Sodre , F. J. Jablonski , R. J. Terlevich

We discuss 6 GHz JVLA observations covering a volume-limited sample of 178 low redshift ($0.2 < z < 0.3$) optically selected QSOs. Our 176 radio detections fall into two clear categories: (1) About $20$\% are radio-loud QSOs (RLQs) having…

星系天体物理 · 物理学 2016-11-15 K. I. Kellermann , J. J. Condon , A. E. Kimball , R. A. Perley , Zeljko Ivezic

Millihertz quasi-periodic oscillations (mHz QPOs) observed in neutron-star low-mass X-ray binaries (NS LMXBs) are generally explained as marginally stable thermonuclear burning on the neutron star surface. We report the discovery of mHz…

高能天体物理现象 · 物理学 2020-10-28 Kaho Tse , Duncan K. Galloway , Yi Chou , Alexander Heger , Hung-En Hsieh

We report on the optical spectroscopic analysis of a sample of 99 low-luminosity quasi-stellar objects (LLQSOs) at $z\leq 0.06$ base the Hamburg/ESO QSO survey (HES). The LLQSOs presented here offer the possibility of studying the faint end…

星系天体物理 · 物理学 2015-08-19 E. Tremou , M. Garcia-Marin , J. Zuther , A. Eckart , M. Valencia-Schneider , M. Vitale , C. Shan

Although well established for BL Lac objects and radio-loud quasars, the occurrence of intra-night optical variability (INOV) in radio-quiet quasars is still debated, primarily since only a handful of INOV events with good statistical…

天体物理学 · 物理学 2007-06-01 A. Goyal , Gopal-Krishna , Ram Sagar , G. C. Anupama , D. K. Sahu

Based on a recently started programme, we report the first search for intranight optical variability among radio-quiet weak-line-quasars (RQWLQs). Eight members of this class were observed on 13 nights in the R-band, such that each source…

宇宙学与河外天体物理 · 物理学 2020-04-08 Gopal-Krishna , Ravi Joshi , Hum Chand

We present three new Chandra X-ray epochs along with new ground-based optical-UV observations as the third installment in a time-series analysis of four high-redshift ($z\sim4.1-4.4$) radio-quiet quasars (RQQs). In total, we present nine…

The recent detection of the quasi-stellar object (QSO) VIKING J231818.3$-$311346 (hereafter VIK J2318$-$3113) at redshift $z=6.44$ in the Rapid ASKAP Continuum Survey (RACS) uncovered its radio-loud nature, making it one of the most distant…

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