Elmo Tempel Eesti astronoom
Tempel, Elmo, 1980-
Tempel, Elmo
VIAF ID: 4791158915898650000006 (Personal)
Permalink: http://viaf.org/viaf/4791158915898650000006
Preferred Forms
- 100 0 _ ‡a Elmo Tempel ‡c Eesti astronoom
- 100 1 _ ‡a Tempel, Elmo
-
4xx's: Alternate Name Forms (7)
5xx's: Related Names (1)
Works
Title | Sources |
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The ALHAMBRA survey:B-band luminosity function of quiescent and star-forming galaxies at 0.2 ≤ z < 1 by PDF analysis | |
Alignment of galaxies relative to their local environment in SDSS-DR8 | |
The alignment of galaxy spin with the shear field in observations | |
The alignment of satellite galaxies and cosmic filaments: observations and simulations | |
Anatomy of luminosity functions: the 2dFGRS example | |
Assessing the reliability of the Bisous filament finder | |
Bayesian group finder based on marked point processes. Method and feasibility study using the 2MRS data set | |
Characterization of the warm-hot intergalactic medium near the Coma cluster through high-resolution spectroscopy of X Comae | |
Clustering analysis for astrophysical structures | |
The Corona Borealis supercluster: connectivity, collapse, and evolution | |
The Cosmic Ballet: spin and shape alignments of haloes in the cosmic web | |
The cosmic-ray positron excess from a local Dark Matter over-density | |
The cosmic web for density perturbations of various scales | |
Detecting filamentary pattern in the cosmic web: a catalogue of filaments for the SDSS | |
Discovery of a massive supercluster system atz~ 0.47 | |
The effect of cosmic web filaments on the properties of groups and their central galaxies | |
Environments of nearby quasars in Sloan digital sky survey | |
Evidence for indirect detection of dark matter from galaxy clusters in Fermi {gamma}-ray data | |
Evidence for spin alignment of spiral and elliptical/S0 galaxies in filaments | |
Fermi 130 GeV gamma-ray excess and dark matter annihilation in sub-haloes and in the Galactic centre | |
Fermi-LAT gamma-ray signal from Earth limb, systematic detector effects and their implications for the 130 GeV gamma-ray excess | |
Filaments from the galaxy distribution and from the velocity field in the local universe | |
Friends-of-friends galaxy group finder with membership refinement | |
From voids to filaments: environmental transformations of galaxies in the SDSS | |
Galaxies in filaments have more satellites: the influence of the cosmic web on the satellite luminosity function in the SDSS | |
Galaxy cluster mass reconstruction project – I. Methods and first results on galaxy-based techniques | |
Galaxy filaments as pearl necklaces | |
Galaxy modelling : dynamical methods and applications | |
Galaxy morphology, luminosity, and environment in the SDSS DR7 | |
Galaxy pairs align with Galactic filaments | |
Groups in the millennium simulation and in SDSS DR7 | |
Groups of galaxies in the SDSS Data Release 7. Flux- and volume-limited samples | |
Hermeian haloes: Field haloes that interacted with both the Milky Way and M31 | |
The Herschel Exploitation of Local Galaxy Andromeda (HELGA) VII. A SKIRT radiative transfer model and insights on dust heating | |
How does the grouping scheme affect the Wiener Filter reconstruction of the local Universe? | |
The influence of dark matter halo on the stellar stream asymmetry via dynamical friction | |
J-PLUS: Impact of bars on quenching timescales in nearby green valley disc galaxies | |
Kinematic modeling of distant galaxies | |
Klassikaline ja mitteparameetriline matemaatiline statistika : õpik kõrgkoolidele | |
Line-of-sight velocity dispersions and a mass-distribution model of the Sa galaxy NGC 4594 | |
The lopsided distribution of satellite galaxies | |
Meet the Laniakea supercluster | |
A method to calculate gravitational accelerations within discrete localized regions in the Milky Way | |
The miniJPAS survey | |
Missing baryons traced by the galaxy luminosity density in large-scale WHIM filaments | |
Modeling the cosmic web with the Bisous method | |
Multifrequency studies of galaxies and groups. I. Environmental effect on galaxy stellar mass and morphology | |
Multimodality in galaxy clusters from SDSS DR8: substructure and velocity distribution | |
Multimodality of rich clusters from the SDSS DR8 within the supercluster-void network | |
An optimized tiling pattern for multiobject spectroscopic surveys: application to the 4MOST survey | |
Orientation of cosmic web filaments with respect to the underlying velocity field | |
Period change of massive binaries from combined photometric and spectroscopic data in Cygnus OB2 | |
Photometric redshift galaxies as tracers of the filamentary network | |
A possible Chandra and Hubble Space Telescope detection of extragalactic WHIM towards PG 1116+215 | |
Probabilistic fibre-to-target assignment algorithm for multi-object spectroscopic surveys | |
Reliability of the detection of the baryon acoustic peak | |
SDSS DR7 superclusters. The catalogues | |
SDSS surface photometry of M31 with absorption corrections | |
The shape alignment of satellite galaxies in Local Group-like pairs from the SDSS | |
Sissejuhatus füüsikasse. Kulgliikumise kinemaatika. | |
The Sloan Great Wall. Morphology and galaxy content | |
The Sloan great wall. Rich clusters | |
Spiral arms and disc stability in the Andromeda galaxy | |
Stellar mass map and dark matter distribution in M 31 | |
Supercluster A2142 and collapse in action: infalling and merging groups and galaxy transformations | |
Taeva puudutus | |
To be or not to be: the case of the hot WHIM absorption in the blazar PKS 2155–304 sight line | |
Towards understanding the structure of voids in the cosmic web | |
Tracing galaxy evolution by their present-day luminosity function | |
Unusual A2142 supercluster with a collapsing core: distribution of light and mass | |
Wavelet analysis of the cosmic web formation | |
Кинематика поступательного движения |