The optical counterpart of the new Fermi LAT flaring source J0109+6134 near the Galactic Plane
The position of the recently discovered transient gamma-ray source J0109+6134 (ATEL #2414) lies within the footprints of the IPHAS (Drew et al. 2005, MNRAS, 362...
We report the counterpart to the X-ray transient and black hole candidate XTE J1817-330 (ATEL #714). Our observations consist of a series of 5s and 10s g'-band...
The optical counterparts of Accreting Millisecond X-Ray Pulsars during quiescence
Using data obtained with the ESO-Very Large Telescope, we have performed a deep optical and NIR photometric study of the fields of three Accreting Millisecond X...
The Optical Properties of the Host Galaxies of FR I and FR II Radio Sources
The two Fanaroff & Riley classes of radio galaxies are defined by radio morphology, and the distinction may arise from a combination of environmental conditions...
The publication by Lloyd (1984) of new and revised data for a sample of active nuclei brought the number of published observations of 3C 345 up to over 900...
The optical, infrared and radio light curve of OJ 287 during winter 1993 - 94.
The light curves of OJ 287 at UBVRIJHK, 22 and 37 GHz are presented for the 1993/94 observing campaign. Despite the considerable optical and infrared activity...
The OPTICON A2IM Cookbook: an introduction to additive manufacture for astronomy
Additive manufacture (AM), also known as 3D printing, builds an object, layer-by-layer, from a digital design file. The primary advantage of the layer-by-layer...