SwePub
Sök i SwePub databas

  Extended search

Träfflista för sökning "WFRF:(Cooray V.) "

Search: WFRF:(Cooray V.)

  • Result 1-50 of 82
Sort/group result
   
EnumerationReferenceCoverFind
1.
  • Pezzotta, A., et al. (author)
  • Euclid preparation XLI. Galaxy power spectrum modelling in real space
  • 2024
  • In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 687
  • Journal article (peer-reviewed)abstract
    • We investigate the accuracy of the perturbative galaxy bias expansion in view of the forthcoming analysis of the Euclid spectroscopic galaxy samples. We compare the performance of a Eulerian galaxy bias expansion using state-of-the-art prescriptions from the effective field theory of large-scale structure (EFTofLSS) with a hybrid approach based on Lagrangian perturbation theory and high-resolution simulations. These models are benchmarked against comoving snapshots of the flagship I N-body simulation at z = (0.9, 1.2, 1.5, 1.8), which have been populated with H alpha galaxies leading to catalogues of millions of objects within a volume of about 58 h(-3) Gpc(3). Our analysis suggests that both models can be used to provide a robust inference of the parameters (h, omega c) in the redshift range under consideration, with comparable constraining power. We additionally determine the range of validity of the EFTofLSS model in terms of scale cuts and model degrees of freedom. From these tests, it emerges that the standard third-order Eulerian bias expansion - which includes local and non-local bias parameters, a matter counter term, and a correction to the shot-noise contribution - can accurately describe the full shape of the real-space galaxy power spectrum up to the maximum wavenumber of k(max) = 0.45 h Mpc(-1), and with a measurement precision of well below the percentage level. Fixing either of the tidal bias parameters to physically motivated relations still leads to unbiased cosmological constraints, and helps in reducing the severity of projection effects due to the large dimensionality of the model. We finally show how we repeated our analysis assuming a volume that matches the expected footprint of Euclid, but without considering observational effects, such as purity and completeness, showing that we can get constraints on the combination (h, omega c) that are consistent with the fiducial values to better than the 68% confidence interval over this range of scales and redshifts.
  •  
2.
  •  
3.
  •  
4.
  •  
5.
  •  
6.
  •  
7.
  •  
8.
  •  
9.
  • Gao, L, et al. (author)
  • Simulation of streamer discharges as finitely conducting channels
  • 1999
  • In: IEEE TRANSACTIONS ON DIELECTRICS AND ELECTRICAL INSULATION. - : IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC. - 1070-9878. ; 6:1, s. 35-42
  • Journal article (other academic/artistic)abstract
    • This paper presents a two-dimensional simulation of positive streamers in air at atmospheric pressure in a quasi-uniform electric field. A streamer is assumed to consist of a hemispherical tip and a finitely conducting cylindrical channel with a constant
  •  
10.
  •  
11.
  •  
12.
  •  
13.
  • Roman, F, et al. (author)
  • Comparison of the breakdown of rod-plane gaps with floating electrode
  • 1998
  • In: IEEE TRANSACTIONS ON DIELECTRICS AND ELECTRICAL INSULATION. - : IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC. - 1070-9878. ; 5:4, s. 622-624
  • Journal article (other academic/artistic)abstract
    • The possible influence of a metal body in a lightning protection system was determined by comparing the electrical breakdown probability of two symmetrical sphere-rod gaps, one conventional and the other with a floating electrode, i.e. a rod with a series
  •  
14.
  • Roman, F, et al. (author)
  • Corona from floating electrodes
  • 1996
  • In: JOURNAL OF ELECTROSTATICS. - : ELSEVIER SCIENCE BV. - 0304-3886. ; 37:1-2, s. 67-78
  • Journal article (other academic/artistic)abstract
    • It is not unusual to have insulated conducting objects located close to the conductors of a Lightning Protection System. However, the separation of these objects from the Lightning Protection System could vary from a few millimetres to some centimetres. W
  •  
15.
  •  
16.
  • Roman, F, et al. (author)
  • Increase in the visual corona from floating electrodes
  • 1999
  • In: JOURNAL OF ELECTROSTATICS. - : ELSEVIER SCIENCE BV. - 0304-3886. ; 45:4, s. 243-254
  • Journal article (other academic/artistic)abstract
    • The corona and streamer discharges on a floating metallic rod located close to a high-voltage electrode were investigated under the application of both positive and negative 300/3000 mu s switching impulses. The distance between the floating rod and the h
  •  
17.
  •  
18.
  •  
19.
  •  
20.
  •  
21.
  •  
22.
  • Akyuz, M, et al. (author)
  • Characteristics of laser-triggered electric discharges in air
  • 2005
  • In: IEEE Transactions on Dielectrics and Electrical Insulation. - 1070-9878. ; 12:5, s. 1060-1070
  • Journal article (peer-reviewed)abstract
    • An experiment of laser-triggered electric discharges has been conducted in a uniform background electric field. By focusing the beam of a pulsed Nd-YAG laser (wavelength 532 nm, pulse duration 5 ns) in a narrow (15 mm) plane-parallel air gap exposed to a dc voltage, streamer discharges and disruptive discharges were triggered.. The laser energy and the background electric field strength were varied in the ranges 0-180 mJ and 0.8-1.4 MV/m, respectively, and the laser plasma was induced either close to the anode, close to the cathode or mid-gap. From images of the electrode gap and from current measurements, the occurrence of and time to the streamer discharge and the disruptive discharge were determined. No distinct level was found of either the laser energy or the plasma energy for the transition from one discharge case to another, even if the general trend was that the energy required for a certain discharge case was reduced when increasing the background electric field. These and other observations make the method of laser triggering a less suitable method for studies of streamer initiation and streamer propagation, but revealed several interesting features of laser-triggered electric discharges.
  •  
23.
  •  
24.
  •  
25.
  •  
26.
  • Bakx, Tom, 1990, et al. (author)
  • A dusty protocluster surrounding the binary galaxy HerBS-70 at z = 2.3
  • 2024
  • In: Monthly Notices of the Royal Astronomical Society. - 0035-8711 .- 1365-2966. ; 530:4, s. 4578-4596
  • Journal article (peer-reviewed)abstract
    • We report on deep SCUBA-2 observations at 850 μm and NOrthern Extended Millimetre Array (NOEMA) spectroscopic measurements at 2 mm of the environment surrounding the luminous, massive (M∗ ≈ 2 × 1011 M☉) Herschel-selected source HerBS-70. This source was revealed by previous NOEMA observations to be a binary system of dusty star-forming galaxies at z = 2.3, with the east component (HerBS-70E) hosting an active galactic nucleus. The SCUBA-2 observations detected, in addition to the binary system, 21 sources at >3.5σ over an area of ∼25 square comoving Mpc with a sensitivity of 1σ850 = 0.75 mJy. The surface density of continuum sources around HerBS-70 is three times higher than for field galaxies. The NOEMA spectroscopic measurements confirm the protocluster membership of three of the nine brightest sources through their CO(4–3) line emission, yielding a volume density 36 times higher than for field galaxies. All five confirmed sub-mm galaxies in the HerBS-70 system have relatively short gas depletion times (80−500 Myr), indicating the onset of quenching for this protocluster core due to the depletion of gas. The dark matter halo mass of the HerBS-70 system is estimated around 5 × 1013 M☉, with a projected current-day mass of 1015 M☉, similar to the local Virgo and Coma clusters. These observations support the claim that DSFGs, in particular the ones with observed multiplicity, can trace cosmic overdensities.
  •  
27.
  • Bendo, G. J., et al. (author)
  • The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates
  • 2023
  • In: Monthly Notices of the Royal Astronomical Society. - 0035-8711 .- 1365-2966. ; 522:2, s. 2995-3017
  • Journal article (peer-reviewed)abstract
    • We present 101- and 151-GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500-μm flux densities >80 mJy and 250–500-μm colours consistent with z > 2, most of which are expected to be gravitationally lensed or hyperluminous infrared galaxies. Approximately half of the Herschel 500-μm sources were resolved into multiple ALMA sources, but 11 of the 15 brightest 500-μm Herschel sources correspond to individual ALMA sources. For the 37 fields containing either a single source with a spectroscopic redshift or two sources with the same spectroscopic redshift, we examined the colour temperatures and dust emissivity indices. The colour temperatures only vary weakly with redshift and are statistically consistent with no redshift-dependent temperature variations, which generally corresponds to results from other samples selected in far-infrared, submillimetre, or millimetre bands but not to results from samples selected in optical or near-infrared bands. The dust emissivity indices, with very few exceptions, are largely consistent with a value of 2. We also compared spectroscopic redshifts to photometric redshifts based on spectral energy distribution templates designed for infrared-bright high-redshift galaxies. While the templates systematically underestimate the redshifts by ∼15 per cent, the inclusion of ALMA data decreases the scatter in the predicted redshifts by a factor of ∼2, illustrating the potential usefulness of these millimetre data for estimating photometric redshifts.
  •  
28.
  • Berta, S., et al. (author)
  • z -GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies: III. Physical properties
  • 2023
  • In: Astronomy and Astrophysics. - 0004-6361 .- 1432-0746. ; 678
  • Journal article (peer-reviewed)abstract
    • The z-GAL survey observed 137 bright Herschel-selected targets with the IRAM Northern Extended Millimeter Array, with the aim to measure their redshift and study their properties. Several of them have been resolved into multiple sources. Consequently, robust spectroscopic redshifts have been measured for 165 individual galaxies in the range 0.8., <., z., <., 6.5. In this paper we analyse the millimetre spectra of the z-GAL sources, using both their continuum and line emission to derive their physical properties. At least two spectral lines are detected for each source, including transitions of 12CO, [CI], and H2O. The observed 12CO line ratios and spectral line energy distributions of individual sources resemble those of local starbursts. In seven sources the para-H2O (211-202) transition is detected and follows the IR versus H2O luminosity relation of sub-millimetre galaxies. The molecular gas mass of the z-GAL sources is derived from their 12CO, [CI], and sub-millimetre dust continuum emission. The three tracers lead to consistent results, with the dust continuum showing the largest scatter when compared to 12CO. The gas-to-dust mass ratio of these sources was computed by combining the information derived from 12CO and the dust continuum and has a median value of 107, similar to star-forming galaxies of near-solar metallicity. The same combined analysis leads to depletion timescales in the range between 0.1 and 1.0 Gyr, which place the z-GAL sources between the main sequence' of star formation and the locus of starbursts. Finally, we derived a first estimate of stellar masses "modulo possible gravitational magnification "by inverting known gas scaling relations: the z-GAL sample is confirmed to be mostly composed by starbursts, whereas ∼25% of its members lie on the main sequence of star-forming galaxies (within ±0.5 dex).
  •  
29.
  •  
30.
  • Cooray, V (author)
  • A model for negative first return strokes in lightning flashes
  • 1997
  • In: PHYSICA SCRIPTA. - : ROYAL SWEDISH ACAD SCIENCES. - 0281-1847. ; 55:1, s. 119-128
  • Journal article (other academic/artistic)abstract
    • A model is introduced to describe negative first return strokes in lightning ground hashes. The basic assumptions made are similar to those used previously to describe the subsequent return strokes. The model predictions are in general agreement with expe
  •  
31.
  • Cooray, V (author)
  • A model for positive return strokes
  • 1995
  • In: ELECTROSTATICS 1995. - : IOP PUBLISHING LTD. - 0951-3248. ; 143, s. 363-371
  • Journal article (other academic/artistic)abstract
    • A model to describe positive return strokes is presented. The basic concepts used in the model are essentially similar to those used previously to describe negative first return strokes. However, laboratory experiments indicate that the mechanism of neutr
  •  
32.
  •  
33.
  •  
34.
  •  
35.
  • Cooray, V (author)
  • Energy dissipation in lightning flashes
  • 1997
  • In: JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES. - : AMER GEOPHYSICAL UNION. ; 102:D17, s. 21401-21410
  • Journal article (other academic/artistic)abstract
    • In this paper the amounts of energy dissipation in different stages of ground flashes are estimated by electrostatic energy considerations. In the analysis the cloud is modeled using the typical charge configuration given by Malan [1963]. The leader stage
  •  
36.
  •  
37.
  •  
38.
  •  
39.
  •  
40.
  •  
41.
  •  
42.
  •  
43.
  •  
44.
  •  
45.
  •  
46.
  •  
47.
  •  
48.
  •  
49.
  •  
50.
  •  
Skapa referenser, mejla, bekava och länka
  • Result 1-50 of 82

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view