[PDF] Top 20 Cosmic downsizing of powerful radio galaxies to low radio luminosities
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Cosmic downsizing of powerful radio galaxies to low radio luminosities
... of radio lu- minosities and redshifts from which the cosmic evolution of the radio galaxy population can be read ...erent radio source popu- lations ...the luminosities and redshifts ... See full document
7
Starbursts and the triggering of the activity in nearby powerful radio galaxies
... far-IR luminosities of the detected sources are well below those of ...a radio galaxy phase, the radio galaxy phase cannot be coeval with the ULIG phase in all ...in radio galaxies ... See full document
16
Donoso, Emilio (2010): Evolution of Radio Galaxies Across Cosmic Time. Dissertation, LMU München: Fakultät für Physik
... of 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 ... See full document
150
Ultimate precision in cosmic-ray radio detection — the SKA
... from the dismantled KASCADE array [15], between the SKA antenna stations (see Fig. 2). The detectors could be read out via the same kind of RF-over-fibre links that are used for the antenna readout. Assuming 4 channels ... See full document
6
Development of the radio astronomical method of cosmic particle detection for extremely high-energy cosmic ray physics and neutrino astronomy
... large radio telescopes of Australia, USA, Russia and other countries but these experiments only put upper limits to the EHE cosmic rays ...nanosecond radio pulses from the Moon in a wider interval of ... See full document
6
Optical emission lines in radio sources of intermediate power
... In th e previous ch ap ter we discussed th e collection and reduction of the radio d a ta an d p resen ted th e results. L ittle discussion of th e ir significance or in te rre la tio n was presented. We rem edy ... See full document
418
The environments of luminous radio galaxies and type-2 quasars
... 2-Jy radio galaxies at intermedi- ate redshifts ...type-2 radio-quiet quasars at ...the powerful radio galaxies (PRGs) and 75 per cent of the type-2 quasars] show tidal features ... See full document
20
First joint observations of space weather events over Mexico
... The cosmic ray observatory can detect flux variations caused by solar activity, for example, when a coronal mass ejection (CME) strikes the Earth and produces a sudden re- duction in galactic cosmic ray ... See full document
14
A radio and infrared investigation of Seyfert galaxies in the local universe
... be radio-loud using the radio only criterion discussed in Drake ...(blue) luminosities) > 10 are considered radio-loud, the newly identified radio-excess PGC 029778 is right at this ... See full document
197
Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization
... We present HST/WFC3 observations of MASOSA ob- served as part of HST program 14699 (PI: Sobral) on March 6 2018. Observations were performed for two or- bits with the F110W and F160W filters. During each orbit, four ... See full document
26
Radio detection of extensive air showers - Measurements of the properties of cosmic rays with the radio technique — past, present, future
... LOFAR has a very dense antenna spacing in its core [25], which is very useful to examine details of the radio emission processes in the atmosphere. There is now consensus that the bulk of the radiation originates ... See full document
7
Radio and optical observations of a complete sample of E and SO galaxies
... recent radio continuum surveys of "normal" ...that radio emission from galaxies is of two types, "compact" flat-spectrum sources which are confined to the nucleus and ... See full document
365
CO(1-0) detection of molecular gas in the massive Spiderweb Galaxy (z=2)
... central radio galaxy, there are indications that a substantial fraction of this gas is associated with satellite galaxies or spread across the intergalactic medium on scales of tens of ... See full document
7
Precision measurements of cosmic rays up to the highest energies with a large radio array at the Pierre Auger Observatory
... *Sub project #3: Deployment of the radio detectors – PI, PD 1+2, PhD students 1+2, engineer + external. The PI has coordinated the deployment of 125 RDs for AERA and is experienced to work in the harsh envi- ... See full document
9
Numerical simulation of oblique ionospheric heating by powerful radio waves
... Figure 3 shows the three-dimensional results after 180 s heating. Three magnetic meridian planes are selected to show the results, which intersect the ground 20 km west of the heating facility, at the heater, and 20 km ... See full document
12
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
Cosmic ray acceleration to ultrahigh energy in radio galaxies
... The origin of ultrahigh energy cosmic rays (UHECRs) has been a mystery for decades. Various subclasses of active galactic nuclei (AGN) have been frequently discussed as possible sources [e.g. 1–4], but ... See full document
6
Comptonization of the cosmic microwave background by relativistic plasma
... of galaxies or at the accretion shock where the matter is falling onto a ...of galaxies and are called ‘cluster radio relics’ (for reviews, see Jaffe 1992 and Fer- etti & Giovannini ...cluster ... See full document
15
A re establishing jet during an X ray re brightening of the Be/X ray binary Swift J0243 6+6124
... (new) radio epochs (1 and 2) showed an increase in radio flux, which then decayed, apparently unaccompanied by a similarly significant event in ...the radio spectrum at the time of this observation, ... See full document
11
Trojans in Wireless Sensor Networks
... Seyfert-like galaxies, with the initial assumption being that those objects that demonstrated the greatest g -ray emission and/or radio loudness would also show the most blazar-like ... See full document
434
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