Results 51 to 60 of about 2,376 (130)
Galaxy bimodality versus stellar mass and environment [PDF]
I. K. Baldry +13 more
core +1 more source
Astro-COLIBRI: Empowering Citizen Scientists in Multi-Messenger Astrophysics
International audienceIn the era of real-time astronomy, citizen scientists play an increasingly important role in the discovery and follow-up of transient astrophysical phenomena.
Schüssler, Fabian +4 more
core +1 more source
Laboratory astrophysics : investigation of planetary and astrophysical maser emission
This paper describes a model for cyclotron maser emission applicable to planetary auroral radio emission, the stars UV Ceti and CU Virginus, blazar jets and astrophysical shocks.
Ronald K +27 more
core +1 more source
Astro-COLIBRI: A Comprehensive Platform for Real-Time Multi-Messenger Astrophysics
International audienceThe detection of transient phenomena such as Gamma-Ray Bursts (GRBs), Fast Radio Bursts (FRBs), stellar flares, novae, and supernovae, alongside novel cosmic messengers like high-energy neutrinos and gravitational waves, has ...
Schüssler, Fabian +4 more
core +1 more source
Generating artificial light curves: revisited and updated
The production of artificial light curves with known statistical and variability properties is of great importance in astrophysics. Consolidating the confidence levels during cross-correlation studies, understanding the artefacts induced by sampling ...
McHardy, I. M. +2 more
core +1 more source
Deep learning and alignment of spatially resolved single-cell transcriptomes with Tangram. [PDF]
Biancalani T +21 more
europepmc +1 more source
Timing analysis of the isolated neutron star RX J0720.4-3125 revisited
We present a reanalysis of the X-ray data for RX J0720.4-3125 presented in our previous paper, Zane et al., using more data recently available from XMM-Newton and Chandra.
Zane, S +11 more
core
Hawking radiation in optics and beyond. [PDF]
Aguero-Santacruz R, Bermudez D.
europepmc +1 more source
Shedding new light on sterile neutrinos from XENON1T experiment. [PDF]
Shakeri S, Hajkarim F, Xue SS.
europepmc +1 more source
We use a two-temperature hydrodynamical formulation to determine the temperature and density structures of the post-shock accretion flows in magnetic cataclysmic variables (mCVs) and calculate the corresponding X-ray spectra.
Wu, K, Ramsay, G, Cropper, M, Saxton, CJ
core

