Dale D. Kocevski et al 2015 ApJ 814 104

Heavily obscured AGN are found to be twice as likely to be hosted by late-type galaxies relative to unobscured AGN, and three times as likely to exhibit signatures of mergers or interactions.

Francesca Valsecchi et al 2015 ApJ 813 101

Simulations with MESA demonstrate that mass loss through Roche-lobe overflow could transform a hot Jupiter into a lower-mass planet (such as a hot Neptune or super Earth).

C. R. Nugent et al 2015 ApJ 814 117

Preliminary properties are reported for 7956 asteroids detected in the first year of the NEOWISE Reactivation mission. 201 of these are near-Earth asteroids; the rest are Main-Belt or Mars-crossing.

Chiara M. F. Mingarelli et al 2015 ApJ 814 L20

Radio transients resulting from the coalescence of a neutron star and a black hole may form a sub-population of fast radio bursts, distinguishable by a double peak with a precursor.

L. Fossati et al 2015 ApJ 812 L35

Observations of a sample of stars with transiting hot Jupiters support the theory that stars’ chromospheric activity may be masked if they are orbited by hot Jupiters with low surface gravity.

N. G. Rudraswami et al 2015 ApJ 814 78

Bulk chemical analyses of 1133 Antarctica micrometeorites suggest that 65% of meteorites lose <20% of their original mass, and 20% lose 20-60% of their original mass, during atmospheric entry.