We describe the results of an ongoing survey of X-ray selected symbiotics in the Galactic bulge, begun with the Galactic Bulge Survey and now extended to the wider bulge using the Chandra Source Catalog. Chandra's sensitivity and source localization are well suited to finding symbiotic X-ray binaries (SyXBs) containing neutron stars accreting from

CXB3 is a symbiotic binary star candidate identified by the Galactic Bulge Survey using X-ray observations by the Chandra X-ray Observatory. Using new Chandra observations, we demonstrate X-ray variability CXB3 with observations showing it usually in a quiescent state with a factor-of-six flare-like event in the last observation. Spectra of CXB3 we

We report the discovery of two planetary systems, namely G 264-012, an M 4.0 dwarf with two terrestrial planets (M b sin i=2.50 −0.30 +0.29 M ⊕ and M c sin i=3.75 −0.47 +0.48 M ⊕), and Gl 393, a bright M 2.0 dwarf with one terrestrial planet (M b sini = 1.71 ± 0.24M ⊕). Although both stars were proposed to belong to young stellar kinematic groups