Results 81 to 90 of about 44,112 (114)
A summary for GWAS phenotypes and covariates for 991 Tibetan individuals included in our GWAS.
A summary for GWAS phenotypes and covariates for 991 Tibetan individuals included in our GWAS.
Geoff Childs (3966869) +8 more
core +1 more source
Construction of a kit of reference strains for rapid genetic mapping in Bacillus subtilis 168. [PDF]
Dedonder RA +5 more
europepmc +1 more source
Baseline characteristics of randomised participants by randomised and analysed group (n = 1,010 and 991).
Anne-Maree Kenan (3687613) +17 more
core +1 more source
Chorismate mutase and 3-deoxy-D-arabino-heptulosonate 7-phosphate synthase of the methylotrophic actinomycete Amycolatopsis methanolica. [PDF]
Euverink GJ +3 more
europepmc +1 more source
Mean (and Standard Deviation) or Percentage of Relevant Variables by Year of Cycle (n = 991).
Mean (and Standard Deviation) or Percentage of Relevant Variables by Year of Cycle (n = 991).
Ronny Westerman (471272) +2 more
core +1 more source
A Geodetic and Astrometric VLBI Experiment at 22/43/88/132 GHz
Extending geodetic and astrometric Very Long Baseline Interferometry (VLBI) observations from traditional centimeter wavebands to millimeter wavebands offers numerous scientific potentials and benefits. However, it was considered quite challenging due to
Shuangjing Xu +16 more
doaj +1 more source
The radar circular polarization ratio (CPR) is an indicator of near-surface, wavelength-scale complexity. Interestingly, previous surveys also noted an association between near-Earth asteroid (NEA) disk-integrated CPR and spectral taxonomic class ...
Edgard G. Rivera-Valentín +9 more
doaj +1 more source
Post-new-horizons Orbits and Masses for the Satellites of Pluto
We report on ephemerides for the satellites of Pluto based on the large set of astrometric measurements. Our orbit fit yielded the following masses with 1 σ uncertainties: GM _Pluto = 869.3 ± 0.4 km ^3 s ^−2 , GM _Charon = 106.1 ± 0.3 km ^3 s ^−2 , GM ...
Marina Brozović, Robert A. Jacobson
doaj +1 more source
Validation of a Third Planet in the LHS 1678 System
The nearby LHS 1678 (TOI-696) system contains two confirmed planets and a wide-orbit, likely brown-dwarf companion, which orbit an M2 dwarf with a unique evolutionary history. The host star occupies a narrow “gap” in the Hertzsprung–Russell diagram lower
Michele L. Silverstein +26 more
doaj +1 more source
On the Rigidly Precessing, Eccentric Gas Disk Orbiting the White Dwarf SDSS J1228+1040
Metal pollution onto white dwarfs is a widespread phenomenon that remains puzzling. Some of these white dwarfs also harbor gaseous debris disks. Emission lines from these disks open a unique window to the physical properties of the polluting material ...
Olcay Ates Goksu +2 more
doaj +1 more source

