Per Barth Lilje
Lilje, Per B.
Lilje, Per Barth
VIAF ID: 68818197 (Personal)
Permalink: http://viaf.org/viaf/68818197
Preferred Forms
- 100 1 0 ‡a Lilje, Per B.
- 100 1 _ ‡a Lilje, Per B.
- 100 1 _ ‡a Lilje, Per B.
- 100 1 _ ‡a Lilje, Per B.
-
- 100 0 _ ‡a Per Barth Lilje
4xx's: Alternate Name Forms (15)
Works
Title | Sources |
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Deep imaging of the double quasar 0957+561 - new constraints on H₀ | |
Frontiers of astrophysics : proceedings of the Rosseland Centenary Symposium, Oslo, 16-17 June, 1994 | |
Hva vet vi om universets tilblivelse og skjebne? | |
INCREASING EVIDENCE FOR HEMISPHERICAL POWER ASYMMETRY IN THE FIVE-YEARWMAPDATA | |
Large-scale structures in the universe | |
Den lokale gruppe, den lokale superhop og tidevannskrefter | |
Planck 2013 results. XXV. Searches for cosmic strings and other topological defects | |
Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies | |
Planck intermediate results L. Evidence of spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB B-mode analysis | |
Planck intermediate results: LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II | |
Planck intermediate results: LVII. Joint Planck LFI and HFI data processing | |
Planck intermediate results VI. The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters | |
Planck intermediate results XLIX. Parity-violation constraints from polarization data | |
Planck intermediate results XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth | |
Planck intermediate results XXIX. All-sky dust modelling with Planck, IRAS, and WISE observations | |
Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope | |
Planck intermediate results XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE | |
Planck intermediate results XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes | |
Planck intermediate results XXXI. Microwave survey of Galactic supernova remnants | |
Planck intermediate results: XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust | |
Planck2018 results | |
Planckearly results. V. The Low Frequency Instrument data processing | |
Planckearly results. VII. The Early Release Compact Source Catalogue | |
Planckearly results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations | |
Planckearly results. XIX. All-sky temperature and dust optical depth fromPlanckand IRAS. Constraints on the “dark gas” in our Galaxy | |
Planckearly results. XX. New light on anomalous microwave emission from spinning dust grains | |
Planckearly results. XXI. Properties of the interstellar medium in the Galactic plane | |
Planckpre-launch status: ThePlanckmission | |
Power asymmetry in cosmic microwave background fluctuations from full sky to sub-degree scales: is the universe isotropic? | |
Power Spectrum Estimation from High‐Resolution Maps by Gibbs Sampling | |
The radiative transfer equations for Compton scattering of polarized low frequency radiation on a hot electron gas | |
Radio--optical alignments in a low radio luminosity sample | |
The radio--optical correlation in steep-spectrum quasars | |
Radio-quiet quasar environments at 0.5 <= z <= 0.8 | |
Solar cycle variations of sunspot temperatures | |
Spectrophotometric and Weak Lensing Survey of a Supercluster and Typical Field Region. I. Spectroscopic Redshift Measurements | |
Testing for Non‐Gaussianity in theWilkinson Microwave Anisotropy ProbeData: Minkowski Functionals and the Length of the Skeleton | |
The tidal velocity field in the Local Supercluster | |
THE TWO- AND THREE-POINT CORRELATION FUNCTIONS OF THE POLARIZED FIVE-YEARWMAPSKY MAPS | |
Weak gravitational lensing by a sample of X-ray luminous clusters of galaxies |