We present the discovery of sub-stellar mass companions to six giant stars by the ongoing Penn State-Torun Planet Search conducted with the Hobby-Eberly Telescope. Each system has a single planet, with minimum masses ranging from 0.9 to 5.3 MJ and orbits ranging from 0.9 to 5.6 years, the longest period yet found by our survey. Three other stars

We use Hubble Space Telescope (HST) and ground-based imaging to study the multiple populations of 47 Tucanae (47 Tuc), combining high-precision photometry with calculations of synthetic spectra. Using filters covering a wide range of wavelengths, our HST photometry splits the main sequence into two branches, and we find that this duality is

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Different nuclear burning regimes are predicted on accreting neutron stars (NSs) depending mainly -but not only- on the amount of mass accreted on the NS per unit time and area. We present X-ray observations of a rapidly accreting 11 Hz pulsar in the globular cluster Terzan 5 that reveal four distinct thermonuclear bursting regimes. In one of them

HerMES, the Herschel/SPIRE extragalactic GTO program, is detecting high redshift sources which were once the domain of high redshift QSOs. Our most spectacular object discovered to date, from over 50 square degrees of survey area with rich ancillary data, is an extraordinarily bright submillimeter galaxy with a confirmed redshift of z=6.337, which