output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 1994 · astro-phShow all

7 papers · 2 filters

astro-ph1994★ 1 cited

Extragalactic Large-Scale Structures behind the Southern Milky Way. - I. Redshifts Obtained at the SAAO in the Hydra/Antlia Extension

Renee C. Kraan-Korteweg, Tony P. Fairall, Chantal Balkowksi

Spectroscopic observations have been carried out for galaxies in the Milky Way with the 1.9 m telescope of the South African Astronomical Observatory (SAAO). The galaxies were sele…

astro-ph1994

Surveys for Z>1 Field Galaxies; David Crampton

C. L. Morbey, O. Le Fevre, F. Hammer +3

In the course of the comprehensive CFRS redshift survey to I = 22.5 with the CFHT MOS/SIS spectrograph, we have observed ~25 field galaxies with z > 1. However, it is clear that al…

astro-ph1994★ 4 cited

Preliminary Results from the ESO Slice Project (ESP)

G. Vettolani, E. Zucca, A. Cappi +18

We present the first results of a galaxy redshift survey, ESO Slice Project (ESP), we are accomplishing as an ESO Key-Project over about 30 square degrees in a region near the Sout…

astro-ph1994★ 18 cited

A search for the associations of distant radio-bright quasars with Abell clusters: an effect of gravitational amplification bias ?

Xiang-Ping Wu, Jinlin Han

The theory predicts that the effect of gravitational lensing by the matter associated with clusters of galaxies can magnify background sources, leading to an enhancement of source…

astro-ph1994★ 184 cited

Isocurvature Perturbations in Multiple Inflationary Models

D. Polarski, A. A. Starobinsky

Dynamics of long-wave isocurvature perturbations during an inflationary stage in multiple (multi-component) inflationary models is calculated analytically for the case where scalar…

astro-ph1994★ 39 cited

Confrontation of Double-Inflationary Models with Observations

P. Peter, D. Polarski, A. A. Starobinsky

We consider double-inflationary models with two noninteracting scalar fields, a light scalar field with potential and a heavy scalar field with…