[PDF] Top 20 RAiSE II: resolved spectral evolution in radio AGN
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RAiSE II: resolved spectral evolution in radio AGN
... The radio AGN counts at z < 1 are dominated by faint low-powered FR-I class objects (Willman et ...FR-I radio source is not physically based, and simply specifies that the location of the surface ... See full document
18
RAiSE III: 3C radio AGN energetics and composition
... monochromatic radio luminosities are highly uncertain due to confounding variables and a lack of knowledge about some aspects of the physics of active galactic nuclei ...powerful radio sources based on ... See full document
19
Donoso, Emilio (2010): Evolution of Radio Galaxies Across Cosmic Time. Dissertation, LMU München: Fakultät für Physik
... low-luminosity radio AGN produced by weakly accreting black holes at low redshifts, to a population of high-luminosity radio AGN that may be produced by strongly accreting black holes at high ... See full document
150
The redshift evolution of major merger triggering of luminous AGN : a slight enhancement at z∼2
... of AGN lies in the low surface brightness of the fea- tures being searched for compared to the high intensity emission from the ...differently resolved at different redshifts; the shape asymmetry works ... See full document
17
Observation of Tungsten Line Emissions in Wavelength Range of 10 – 500 Å in Large Helical Device
... 500 Å observed with EUV_Short and EUV_Long spec- trometers are carefully identified based on NIST atomic spectra database and previous studies [8, 15, 16], as shown in Figs. 3 (a) - 3 (o). The shot number, central ... See full document
6
A systematic search for changing look quasars in SDSS
... Emerging or disappearing BELs have been discovered in sev- eral relatively local AGN (Khachikian & Weedman 1971; Tohline & Osterbrock 1976; Penston & Perez 1984; Cohen et al. 1986; Aretxaga et al. ... See full document
16
School Desegregation, Law and Order, and Litigating Social Justice in Alabama, 1954 1973
... two radio-loud relativistic jets, traveling away from the black hole and perpendicular to the accretion ...of radio galaxies, while AGN without jets are observed as ...the AGN if viewed from ... See full document
298
Kakkad, Darshan Mahesh (2017): Ionized and molecular gas studies to unveil AGN feedback. Dissertation, LMU München: Fakultät für Physik
... in AGN Narrow Line Region using S7 survey: Our SINFONI work motivated a systematic study of the electron density in the NLR of AGN host galaxies, which was the basis of chap- ter ...the AGN host ... See full document
175
X-ray spectra of the RIXOS source sample
... inferred spectral slope seen in the IR, giving rise to claims that there is a power law of energy index 1 underlying the observed spectrum from the IR to X-ray range ... See full document
24
Airborne measurements of particulate organic matter by proton-transfer-reaction mass spectrometry (PTR-MS): a pilot study
... Abstract. Herein we report on the first successful airborne deployment of the CHemical Analysis of AeRosol ONline (CHARON) particle inlet which allowed us to measure the chemical composition of atmospheric submicrometer ... See full document
12
Complex spectral evolution in a BCS superconductor, ZrB12
... To calculate the x-ray photoemission spectrum, we have multiplied the partial density of states obtained by the band structure calculations by the corresponding photoemission cross sections for Al Kaenergy. These ... See full document
7
A radio-controlled trencher for accurate installation of shallow ditches and pipelines
... the target and maintains grade by operating the radio control to raise or lower the target (and thus the cutter head) in relation to the line of sight.. The transit operator makes adjust[r] ... See full document
5
The case for electron re acceleration at galaxy cluster shocks
... more radio galaxies (B and C, see ...the radio galaxies (source B) is embedded within the relic ...The spectral index map and the 325 MHz image (SI and ...The spectral index steepens along the ... See full document
20
Broadcast Partners DRM tuner
... 40 Radio Sweden German Flevo 1300-1500 Mon-Fri 9410 62 NE & C Europe 33 BBCWS English Rampisham 1305-1455 daily 5975 290 W Europe 40 T-Systems German Juelich 1330-1400 daily 9815 ND Europe 40 Radio ... See full document
7
Cosmic evolution of radio sources in ATLAS
... D. L. Clements, A. Conley, L. Conversi, A. Cooray, H. Dannerbauer, M. Dick- inson, H. Dominguez, C. D. Dowell, J. S. Dunlop, E. Dwek, S. Eales, D. Farrah, N. F. Schreiber, M. Fox, A. Franceschini, W. Gear, R. Genzel, J. ... See full document
213
Characterization of Passive Spectral Regrowth in Radio Frequency Systems.
... Passive spectral regrowth is difficult to predict theoretically, because the small interaction or coupling involved is often approximated out as insignificant to make governing equations tractable and ...of ... See full document
164
Host guest complexes of baicalein and silybin with C hexylpyrogallol[4]arene: Determination of the stoichiometry and the mode of binding
... In order to confirm the inclusion complexation of baicalein with C-HPA are studied by the time–resolved fluorescence spectroscopy. Fig. SI 4 shows that the time-resolved spectrum of baicalein in water, low ... See full document
12
CANDELS: Elevated black hole growth in the progenitors of compact quiescent galaxies at z ∼ 2
... Our parent sample of massive galaxies is drawn from HST / WFC3 F160W ( H-band ) selected catalogs in four of the fi ve CANDELS fi elds ( Grogin et al. 2011; Koekemoer et al. 2011 ) . This includes the Great Observatories ... See full document
13
Radio Loud AGN Unification: Connecting Jets and Accretion
... Fermi-detected AGN (large symbols) show that alignment plays a strong effect in the gamma-ray ...FR II sources appear to drop directly below the powerful FSRQ sources, FR I radio galaxies appear to ... See full document
8
Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the $Kepler$ 2 Observations
... color evolution of SN 2018oh is similar to that of the comparison ...color evolution of the SN is ...Ca II H&K and iron-group elements (IGEs) absorption at shorter ...color evolution due ... See full document
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