output
19962026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2005 · astro-phShow all

38 papers · 2 filters

astro-ph2005★ 140 cited

A CH3CN and HCO+ survey towards southern methanol masers associated with star formation

C. R. Purcell, R. Balasubramanyam, M. G. Burton +32

We present the initial results of a 3-mm spectral line survey towards 83 methanol maser selected massive star-forming regions. Here we report observations of the J=5-4 and 6-5 rota…

astro-ph2005★ 13 cited

The formation of brown dwarfs

A. P. Whitworth, S. P. Goodwin

We review four mechanisms for forming brown dwarfs: (i) turbulent fragmentation (producing very low-mass prestellar cores); (ii) gravitational instabilities in discs; (iii) dynamic…

astro-ph2005★ 15 cited

An investigation of the submillimeter background radiation using SCUBA and Spitzer

S. Dye, S. A. Eales, M. L. N. Ashby +8

We investigate the redshift dependence of the contribution to the extragalactic far-infrared/sub-millimeter background from galaxies detected by the Spitzer Space Telescope at 8um…

astro-ph2005★ 33 cited

Optical/near-infrared colours of early-type galaxies and constraints on their star formation histories

P. A. James, M. Salaris, J. I. Davies +2

(abridged) We introduce and discuss the properties of a theoretical (B-K)-(J-K) integrated colour diagram for single-age, single-metallicity stellar populations. This combination o…

astro-ph2005★ 68 cited

Resolution requirements for simulating gravitational fragmentation using SPH

D. A. Hubber, S. P. Goodwin, A. P. Whitworth

Jeans showed analytically that, in an infinite uniform-density isothermal gas, plane-wave perturbations collapse to dense sheets if their wavelength, , satisfies $λ> λ_{_{\rm JE…

astro-ph2005★ 2 cited

Observational characteristics of dense cores with deeply embedded young protostars

D. Stamatellos, A. P. Whitworth, S. P. Goodwin

Class 0 objects, which are thought to be the youngest protostars, are identified in terms of NIR or radio emission and/or the presence of molecular outflows. We present combined hy…

astro-ph2005★ 49 cited

Expected coalescence rates of NS-NS binaries for laser beam interferometers

J. A. de Freitas Pacheco, T. Regimbau, S. Vincent +1

The coalescence rate of two neutron stars (NS) is revisited. For estimation of the number of bound NS-NS and the probability of their coalescence in a timescale , the galactic s…

astro-ph2005★ 341 cited

Bolocam Survey for 1.1 mm Dust Continuum Emission in the c2d Legacy Clouds. I. Perseus

M. L. Enoch, K. E. Young, J. Glenn +14

We have completed a 1.1 mm continuum survey of 7.5 sq deg of the Perseus Molecular Cloud using Bolocam at the Caltech Submillimeter Observatory. This represents the largest millime…

astro-ph2005★ 63 cited

COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses II. SDSS J0924+0219: the redshift of the lensing galaxy, the quasar spectral variability and the Einstein rings

A. Eigenbrod, F. Courbin, S. Dye +6

(Abridged) We present our VLT/FORS1 deep spectroscopic observations of the gravitationally lensed quasar SDSS J0924+0219, as well as archival HST/NICMOS and ACS images of the same…

astro-ph2005★ 6 cited

First ground-based 200-um observing with THUMPER on JCMT - sky characterisation and planet maps

D. Ward-Thompson, P. A. R. Ade, H. Araujo +19

We present observations that were carried out with the Two HUndred Micron PhotometER (THUMPER) mounted on the James Clerk Maxwell Telescope (JCMT) in Hawaii, at a wavelength of 200…

astro-ph2005★ 27 cited

A Fluctuation Analysis of the Bolocam 1.1mm Lockman Hole Survey

Philip R. Maloney, Jason Glenn, James E. Aguirre +13

We perform a fluctuation analysis of the 1.1mm Bolocam Lockman Hole Survey, which covers 324 square arcmin to a very uniform point source-filtered RMS noise level of 1.4 mJy/beam.…

astro-ph2005★ 4 cited

A Dark Galaxy in the Virgo Cluster Imaged at 21-cm

R. F. Minchin, J. I. Davies, M. J. Disney +10

Dark Matter supposedly dominates the extragalactic, yet no totally dark structure of galactic proportions has ever been convincingly identified. Earlier (Minchin et al. 2005) we su…

astro-ph2005★ 25 cited

XMM-Newton Surveys of the Canada-France Redshift Survey Fields - III: The Environments of X-ray Selected AGN at 0.4<z<0.6

T. J. Waskett, S. A. Eales, W. K. Gear +3

The environmental properties of a sample of 31 hard X-ray selected AGN are investigated, from scales of 500 kpc down to 30 kpc, and are compared to a control sample of inactive gal…

astro-ph2005★ 11 cited

Perturbations of the Yang-Mills field in the universe

Wen Zhao

It has been suggested that the Yang-Mills (YM) field can be a kind of candidate for the inflationary field at high energy scales or the dark energy at very low energy scales, which…

astro-ph2005★ 84 cited

The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- I. Survey motivation, design and data processing

A. M. J. Mortier, S. Serjeant, J. S. Dunlop +2

The SCUBA HAlf Degree Extragalactic Survey (SHADES) is a major blank-field extragalactic sub-mm survey underway at the James Clerk Maxwell telescope.SHADES aims to cover half a squ…

astro-ph2005★ 257 cited

A Measurement of the CMB <EE> Spectrum from the 2003 Flight of BOOMERANG

T. E. Montroy, P. A. R. Ade, J. J. Bock +34

We report measurements of the CMB polarization power spectra from the January 2003 Antarctic flight of BOOMERANG. The primary results come from six days of observation of a patch c…

astro-ph2005★ 123 cited

Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG

S Masi, P Ade, J Bock +41

We present the BOOMERanG-03 experiment and maps of the Stokes parameters I, Q, U of the microwave sky obtained during a 14 day balloon flight in 2003. Three regions of the southern…

astro-ph2005★ 152 cited

A measurement of the polarization-temperature angular cross power spectrum of the Cosmic Microwave Background from the 2003 flight of BOOMERANG

F Piacentini, P Ade, J Bock +34

We present a measurement of the temperature-polarization angular cross power spectrum, <TE>, of the Cosmic Microwave Background. The result is based on hours of data fro…

astro-ph2005★ 176 cited

Cosmological Parameters from the 2003 flight of BOOMERANG

C. J. MacTavish, P. A. R. Ade, J. J. Bock +35

We present the cosmological parameters from the CMB intensity and polarization power spectra of the 2003 Antarctic flight of the BOOMERANG telescope. The BOOMERANG data alone const…

astro-ph2005★ 238 cited

A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of Boomerang

W. C. Jones, P Ade, J Bock +34

We report on observations of the Cosmic Microwave Background (CMB) obtained during the January 2003 flight of Boomerang . These results are derived from 195 hours of observation wi…

astro-ph2005★ 110 cited

Upper Limits on a Stochastic Background of Gravitational Waves

LIGO Scientific Collaboration, B. Abbott

The Laser Interferometer Gravitational Wave Observatory (LIGO) has performed a third science run with much improved sensitivities of all three interferometers. We present an analys…

astro-ph2005★ 12 cited

Iron Needles in Supernova Remnants?

H L Gomez, L Dunne, S Eales +2

It has been suggested by Dwek (2004) that iron needles could explain the submillimetre emission from the Cas A supernova remnant (SNR) with only a very small total mass. We investi…

astro-ph2005★ 210 cited

The HIPASS Catalogue: III - Optical Counterparts & Isolated Dark Galaxies

Marianne T. Doyle, M. J. Drinkwater, D. J. Rohde +38

We present the largest catalogue to date of optical counterparts for HI radio-selected galaxies, Hopcat. Of the 4315 HI radio-detected sources from the HI Parkes All Sky Survey (Hi…

astro-ph2005★ 135 cited

Limits on the primordial stellar multiplicity

Simon P. Goodwin, Pavel Kroupa

Most stars - especially young stars - are observed to be in multiple systems. Dynamical evolution is unable to pair stars efficiently, which leads to the conclusion that star-formi…