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19922026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

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170 papers · 1 filter

astro-ph2000★ 526 cited

The O-Na and Mg-Al Anticorrelations in Turn-Off and early Subgiants in Globular Clusters

R. G. Gratton, P. Bonifacio, A. Bragaglia +16

High dispersion spectra (R>40,000) for a quite large number of stars at the main sequence turn-off and at the base of the subgiant branch in NGC6397 and NGC6752 were obtained with…

astro-ph2000★ 11 cited

The Cuspy LINER Nucleus of the S0/a Galaxy NGC 2681

Michele Cappellari, Francesco Bertola, David Burstein +3

The nucleus of the bulge-dominated, multiply-barred S0/a galaxy NGC 2681 is studied in detail, using high resolution Hubble Space Telescope FOC and NICMOS imaging and FOS spectrosc…

astro-ph2000★ 19 cited

Why did Supernova 1054 shine at late times?

Jesper Sollerman, Cecilia Kozma, Peter Lundqvist

The Crab nebula is the remnant of supernova 1054 (SN 1054). The progenitor of this supernova has, based on nucleosynthesis arguments, been modeled as an 8-10 solar mass star. Here…

astro-ph2000★ 17 cited

Tunable-filter imaging of quasar fields at z~1. I. A cluster around MRC B0450-221

Joanne C. Baker, Richard W. Hunstead, Malcolm N. Bremer +3

Using a combination of multicolour broad- and narrow-band imaging techniques and follow-up spectroscopy, we have detected an overdensity of galaxies in the field of quasar MRC B045…

astro-ph2000★ 250 cited

The ROSAT-ESO Flux Limited X-Ray (REFLEX) Galaxy Cluster Survey I: The Construction of the Cluster Sample

H. Boehringer, P. Schuecker, L. Guzzo +10

We describe the construction of an X-ray flux-limited sample of galaxy clusters, the REFLEX survey catalogue, to be used for cosmological studies. The survey is based on the ROSAT…

astro-ph2000

Optical/Infrared Survey of Galaxy Clusters

Luiz da Costa, S. Arnouts, S. Bardelli +13

In this contribution the ongoing effort to build a statistical sample of clusters of galaxies over a wide range of redshifts to study the evolution of clusters and member galaxies…

astro-ph2000★ 87 cited

The Intracluster Medium in z > 1 Galaxy Clusters

S. A. Stanford, B. Holden, P. Rosati +4

The Chandra X-ray Observatory was used to obtain a 190 ks image of three high redshift galaxy clusters in one observation. The results of our analysis of these data are reported fo…

astro-ph2000★ 158 cited

The microwave background temperature at the redshift of 2.33771

R. Srianand, Patrick Petitjean, Cedric Ledoux

The Cosmic Microwave Background radiation is a fundamental prediction of Hot Big Bang cosmology. The temperature of its black-body spectrum has been measured at the present time, $…

astro-ph2000★ 111 cited

Confirmation of the existence of coherent orientations of quasar polarization vectors on cosmological scales

D. Hutsemekers, H. Lamy

In order to verify the existence of coherent orientations of quasars polarization vectors on very large scales, we have obtained new polarization measurements for a sample of quasa…

astro-ph2000★ 37 cited

MACHO 96-LMC-2: Lensing of a Binary Source in the LMC and Constraints on the Lensing Object

C. Alcock, R. A. Allsman, D. R. Alves +21

We present photometry and analysis of the microlensing alert MACHO 96-LMC-2. The ~3% photometry provided by the Global Microlensing Alert Network follow--up effort reveals a period…

astro-ph2000★ 79 cited

The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey III: The Power Spectrum

Peter Schuecker, Hans Boehringer, Luigi Guzzo +11

We present a measure of the power spectrum on scales from 15 to 800 Mpc/h using the ROSAT-ESO Flux-Limited X-Ray(REFLEX) galaxy cluster catalogue. The REFLEX survey provides a samp…

astro-ph2000★ 65 cited

The Core-Wing Anomaly of Cool Ap Stars: Abnormal Balmer Profiles

Charles R. Cowley, S. Hubrig, T. A. Ryabchikova +3

Paper by Cowley et al. The Core-Wing Anomaly Etc. The profiles of H in a number of cool Ap stars are anomalous. Broad wings, indicative of temperatures in the range 7000-8000K e…

astro-ph2000

The BMW (Brera-Multiscale-Wavelet) Catalogue of Serendipitous X-ray Sources

D. Lazzati, S. Campana, S. Covino +6

In collaboration with the Observatories of Palermo and Rome and the SAX-SDC we are constructing a multi-site interactive archive system featuring specific analysis tools. In this c…

astro-ph2000

Identification of the donor in GRS 1915+105

J. Greiner, M. J. McCaughrean, J. G. Cuby +2

We report on the results of medium-resolution spectroscopy of GRS 1915+105 in the H and K band using the 8m VLT at ESO. We clearly identify absorption bandheads from CO12 and CO13.…

astro-ph2000★ 10 cited

Linking the Metallicity Distribution of Galactic Halo Stars to the Enrichment History of the Universe

Evan Scannapieco, Tom Broadhurst

We compare the metallicity distribution of Galactic Halo stars with 3D realizations of hierarchical galaxy formation. Outflows from dwarf galaxies enrich the intergalactic medium i…

astro-ph2000★ 109 cited

The obscured mid-infrared continuum of NGC 4418: a dust- and ice-enshrouded AGN

H. W. W. Spoon, J. V. Keane, A. G. G. M. Tielens +2

We report the detection of absorption features in the 6-8 micron region superimposed on a featureless mid-infrared continuum in NGC 4418. For several of these features this is the…

astro-ph2000★ 352 cited

MACHO Project Limits on Black Hole Dark Matter in the 1-30 Solar Mass Range

The Macho collaboration, C. Alcock, R. A. Allsman +22

We report on a search for long duration microlensing events towards the Large Magellanic Cloud. We find none, and therefore put limits on the contribution of high mass objects to t…

astro-ph2000★ 4 cited

Molecular hydrogen abundance in the dust-free damped Ly-alpha galaxy at z = 3.4

S. A. Levshakov, P. Molaro, M. Centurion +3

New results from the search for H2 absorption in the damped Ly-alpha galaxy at redshift z = 3.4 toward QSO 0000-2620 (z_em = 4.1) are reported. The high-resolution (lambda/Delta la…

astro-ph2000★ 1 cited

Molecular hydrogen and the nature of damped Lyman-alpha systems

Patrick Petitjean, R. Srianand, Cédric Ledoux

We report results from our mini-survey for molecular hydrogen in eight high redshift damped Lyman-alpha (DLA) systems using the ESO Ultra-violet and Visible Spectrograph on the VLT…

astro-ph2000★ 25 cited

The LMC eclipsing binary HV 2274 revisited

M. A. T. Groenewegen, M. Salaris

We reanalyse the UV/optical spectrum and optical broad-band data of the eclipsing binary HV 2274 in the LMC, and derive its distance following the method given by Guinan et al. (19…

astro-ph2000★ 37 cited

A search for possible interactions between ejections from GRS 1915+105 and the surrounding interstellar medium

S. Chaty, L. F. Rodriguez, I. F. Mirabel +5

We have observed an extended region surrounding the first discovered galactic superluminal source GRS 1915+105, seeking evidence of interaction between the relativistic ejecta of t…

astro-ph2000★ 15 cited

Anomalous Surface Brightness Fluctuations in NGC 4489

S. Mei, D. R. Silva, P. J. Quinn

Anomalously high K-band surface brightness fluctuations (SBF) have been reported in NGC 4489 by Pahre & Mould (1994), Jensen et al. (1996) and Jensen et al. (1998). However, these…

astro-ph2000★ 374 cited

XMM-Newton observation of the Lockman Hole; I. The X-ray Data

G. Hasinger, B. Altieri, M. Arnaud +25

We report on the first deep X-ray survey with the XMM-Newton observatory during the performance verification phase. The field of the Lockman Hole, one of the best studied sky areas…

astro-ph2000★ 131 cited

Galaxy mapping with the SAURON integral-field spectrograph: The star formation history of NGC 4365

Roger L. Davies, Harald Kuntschner, Eric Emsellem +9

We report the first wide-field mapping of the kinematics and stellar populations in the E3 galaxy NGC 4365. The velocity maps extend previous long-slit work. They show two independ…