Observations taken at Calar Alto and Loiano led to the possible identification of the GRB 971227 optical counterpart. Details on the observations are presented.
An optical fiber system to perform bidimensional spectroscopy
This article describes a fiber optic system contrived to perform spectral imaging of extended objects. It consists of two fiber bundles mounted simultaneously...
We present the first results of an observational project aimed at producing a database of nearby face-on spiral galaxies in the optical. The project is being...
An optical supernova associated with the X-ray flash XRF 060218
Long-duration γ-ray bursts (GRBs) are associated with type Ic supernovae that are more luminous than average and that eject material at very high velocities...
An optical time-resolved spectroscopic study of SS Cygni. 1: Quiescence
In this work we analyze time-resolved spectra of SS Cygni in quiescence. The geometrical and orbital fundamental parameters of the system are determined. When...
An optical time-resolved spectroscopic study of SS Cygni. II. Outburst.
Time resolved spectra of SS Cyg corresponding to different outburst types are analyzed. Some evidence has been found for an increase of the mass transfer rate...
An optical transmission spectrum of the giant planet WASP-36 b
We present broad-band photometry of five transits in the planetary system WASP-36, totalling 17 high-precision light curves. Four of the transits were...
An Optical-Near-IR Study of a Triplet of Super Star Clusters in the Starburst Core of M82
We present HST/STIS optical and Gemini/NIFS near-IR IFU spectroscopy and archival Hubble Space Telescope (HST) imaging of the triplet of super star clusters (A1...
An optimized Hβ index for disentangling stellar population ages
We have defined a new Hβ absorption index definition, Hβo, which has been optimized as an age indicator for old and intermediate age stellar populations. Rather...