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.362C .292. © 1985. The American Astronomical Society. All … We have obtained 1 Â resolution spectra with the MMT spectograph of the QSO S5 0014 + 81 (z em = 3.42) and have selected a strong Lyman absorption-line system (z abs = 3.32), in which …
arXiv:0906.0575v2 [astro-ph.CO] 14 Jul 2009 4 Jul 2017 · Fig. 1 shows the SED of S5 0014+813. The BAT data correspond to the average flux of the 3 years survey, while the UVOT and XRT data are the sum of three pointed …
Precessing Jet in the High-Redshift Blazar J0017+8135 - arXiv.org Abstract: The prominent flat-spectrum radio quasar J0017+8135 (S5 0014+81) at z = 3.366 is one of the most luminous active galactic nuclei (AGN) known. Its milliarcsecond-scale radio jet …
The blazar S5 0014+813: a real or apparent monster? The blazar S5 0014+813 L25 hole masses and large accretion rates. The recently published list of blazars detected by the Burst Alert Telescope (BAT) onboard the Swift satellite (Ajello et al. …
.33K 75L. The flat-spectrum radio source S5 0014 + 81 has been identified optically with an extremely luminous quasar having a redshift of z = 3.41 and m v = 16.5 + 0.2 mag.
arXiv:astro-ph/9610204v1 25 Oct 1996 In the light of the new results for S5 0836+71 and S5 0014+81, absorption intrinsic to the quasars is considered and discussed. The average slope obtained from the 8 ASCA spectra in the …
.5K 4L. The Astrophysical Journal, 284:L5-L8,1984 September 1 … S5 0014 + 81 is the first object at such high redshift in which Hß and [O m] have been measured separately, showing rest frame equivalent widths of 37 and 31 A, respectively. The relatively
THE ASTROPHYSICAL JOURNAL, 548:224 2001. The American … In the context of two examples (quasar S5 0014]813 and hybrid-chromosphere supergiant star a TrA), we illustrate a new highly structured model and how Bayesian posterior sampling can be …
by NuSTAR - slac.stanford.edu In this paper we report on observations of S5 0014+81 (00 17008:500+81d35m08s, z = 3:366) and B0222+185 (02 25004:700+18d46m49s, z= 2:690) by NuSTAR. These two blazars have been …
Short-termopticalvariabilityofhigh-redshiftQSO’s - arXiv.org an accretion disc. The only exception is S5 0014+81 which has RK ≃ 250 and technically should be considered radio-loud. Any possible detection of micro-variations of this ob-ject should be …
The Billion-Light-Year Club: Extra Targets - Sky & Telescope of the viewing instrument. Right ascension and declination are for equinox 2000.0.
The blazar S5 0014 813: a real or apparent monster? The blazar S5 0014 +813 L25 holemassesandlargeaccretionrates.Therecentlypublishedlist ofblazarsdetectedbytheBurstAlertTelescope(BAT)onboard the Swift satellite ...
.52K The .302 © 1986. The American Astronomical Society. All … The most luminous quasar known, S5 0014 + 81, was found as a flat-spectrum radio source in the MPIfR 5 GHz S5-Survey (Kühr et al. 1981) and was identified on Palomar Observatory Sky …
Hard X-ray Properties of NuSTAR Blazars - arXiv.org We investigated the spectral shapes of the sources using single power-law, broken power-law and log-parabola models. We also studies the co-relation between the soft and the hard emission …
Finder Chart - Quasar „S5 0014+81“ - spacewalk-telescopes.de Finder Chart - Quasar „S5 0014+81“ 00 17 08.5 // +81 35 08.1 Christian Busch, Spacewalk Telescopes – 2. Finder Chart - Quasar „S5 0014+81“ 00 17 08.5 // +81 35 08.1 Christian …
81, 60001098002 - aanda.org S5 0014 + 81, 60001098002 5×10-1 keV 1 10 2×10-4-3 -1-0.5 0 0.5-20 -15 -10 -5 0 5 10 15 20 ZDCF Lag (ks) -4 10-5-4 5×10 keV (Photons cm-2 s-1) Unfolded Spectrum 5 10 50 0.5 1 1.5 2 …
Quantum Plus - S5 2024 SPECIFICATIONS / OPTIONS Shelf in A/C compartment or above storage drawer (above drawer not available on Quantum models). Faceted body design for ultimate off-road ability and aerodynamics. Reduced fuel …
List of most massive black holes - ResearchGate This is a list of the most massive known black holes, measured in units of solar masses (M☉), or the mass of the Sun (approx. 2 ×1030 kilograms).
BROADBAND OBSERVATIONS OF HIGH REDSHIFT BLAZARS … We present a multi-wavelength study of four high redshift blazars, S5 0014+81 (z=3.37), CGRaBS J0225+1846 (z=2.69), BZQ J1430+4205 (z=4.72), and 3FGL J1656.2−3303 (z=2.40) using …
The Astrophysical Journal, in Press arXiv:1410.1751v2 [astro … ), such as S5 0014+81 (Osmer et al. 1994), SDSS J1701+6412 (Hewett & Wild2010), and HS 1946+7658 (Lu et al.1996). These quasars have SMBH masses of ˘few 109 M or higher, if they …