Disk-Jet quenching of the Galactic Black Hole Swift J1753.5-0127
(2016)
HIRAX: A probe of dark energy and radio transients
Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 9906 (2016) 99065x-99065x-11
Engineering and science highlights of the KAT-7 radio telescope
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 460:2 (2016) 1664-1679
Relative likelihood for life as a function of cosmic time
Journal of Cosmology and Astroparticle Physics Institute of Physics 2016 (2016) 040
Abstract:
Is life most likely to emerge at the present cosmic time near a star like the Sun? We address this question by calculating the relative formation probability per unit time of habitable Earth-like planets within a fixed comoving volume of the Universe, dP (t)/dt, starting from the first stars and continuing to the distant cosmic future. We conservatively restrict our attention to the context of “life as we know it” and the standard cosmological model, ΛCDM. We find that unless habitability around low mass stars is suppressed, life is most likely to exist near ∼ 0.1M ⊙ stars ten trillion years from now. Spectroscopic searches for biosignatures in the atmospheres of transiting Earth-mass planets around low mass stars will determine whether present-day life is indeed premature or typical from a cosmic perspective.MeerLICHT and BlackGEM: custom-built telescopes to detect faint optical transients
Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 9906 (2016) 990664-990664-9