Results 191 to 200 of about 3,124 (236)

Satellite Laser-Ranging as a Probe of Fundamental Physics. [PDF]

Sci Rep, 2019
Ciufolini I, Matzner R, Paolozzi A, Pavlis EC, Sindoni G, Ries J, Gurzadyan V, Koenig R.   +7 more
europepmc   +1 more source

Gravitational waves from dark domain walls

Christiansen Ø, Adamek J, Hassani F, Mota DF.   +3 more
europepmc   +1 more source

Multi-messenger gravitational lensing. [PDF]

Philos Trans A Math Phys Eng Sci
Smith GP, Baker T, Birrer S, Collins CE, Ezquiaga JM, Goyal S, Hannuksela OA, Hemanta P, Hendry MA, Janquart J, Keitel D, Levan AJ, Lo RKL, More A, Nicholl M, Pastor-Marazuela I, Ponte Pérez AI, Ubach H, Uronen LE, Wright M, Zumalacarregui M, Bianco F, Çalişkan M, Chan JCL, Colangeli E, Gompertz BP, Haines CP, Hayes EE, Hu B, Lamb GP, Liu A, Mandhai S, Narola H, Nguyen QL, Poon JSC, Ryczanowski D, Seo E, Shajib AJ, Shan X, Tanvir N, Vujeva L.   +40 more
europepmc   +1 more source

Dipolar Recoupling in Rotating Solids. [PDF]

Chem Rev
Ladizhansky V, Palani RS, Mardini M, Griffin RG.   +3 more
europepmc   +1 more source

Sleep restriction and age effects on distinct aspects of cognition in adolescents. [PDF]

Sleep
Campbell IG, Kurinec CA, Zhang ZY, Cruz-Basilio A, Figueroa JG, Bottom VB, Whitney P, Hinson JM, Van Dongen HPA.   +8 more
europepmc   +1 more source

Cathepsin S Is More Abundant in Serum of Mycobacterium avium subsp. paratuberculosis-Infected Dairy Cows. [PDF]

Metabolites
Duda HC, von Toerne C, Korbonits L, Didier A, Scholz AM, Märtlbauer E, Hauck SM, Deeg CA.   +7 more
europepmc   +1 more source

Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6−1125

Nina Gusinskaia, Amruta Jaodand, J. W. T. Hessels, Slavko Bogdanov, Adam T. Deller, J. C. A. Miller‐Jones, T D Russell, Alessandro Patruno, Anne M. Archibald   +8 more
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A millisecond pulsar

Nature, 1982
The radio properties of 4C21.53 have been an enigma for many years. First, the object displays interplanetary scintillations (IPS) at 81 MHz, indicating structure smaller than 1 are s, despite its low galactic latitude (−0.3°)1. IPS modulation is rare at low latitudes because of interstellar angular broadening. Second, the source has an extremely steep
Backer, D. C., Kulkarni, Shrinivas R., Heiles, Carl, Davis, M. M., Goss, W. M.   +4 more
openaire   +2 more sources