Showing 1–20 of 24 results
/ Date/ Name
Jan 9, 2014The Qatar Exoplanet SurveyNov 4, 2007A new wavelet-based approach for the automated treatment of large sets of lunar occultation dataJul 16, 2008Milliarcsecond angular resolution of reddened stellar sources in the vicinity of the Galactic Center. II. Additional observationsDec 4, 2009The Fabra-ROA Baker-Nunn Camera at Observatori Astronòmic del Montsec: a wide-field imaging facility for exoplanet transit detectionOct 19, 2022TFAW survey II: 6 Newly Validated Planets and 13 Planet Candidates from K2Sep 27, 2011Status of Telescope Fabra ROA at Montsec: Optical Observations for Space Surveillance & TrackingSep 27, 2011The Fabra-ROA Telescope at Montsec (TFRM): A Fully Robotic Wide-field Telescope for Space Surveillance and TrackingNov 23, 2012Telescope Fabra ROA Montsec: a new robotic wide-field Baker-Nunn facilitySep 20, 2012A catalog of near-IR sources found unresolved with milliarcsecond resolutionJul 16, 2008Milliarcsecond angular resolution of reddened stellar sources in the vicinity of the Galactic CenterNov 19, 2014Detrending algorithms in large time-series: Application to TFRM-PSES dataJan 9, 2015Evidence of coupling between the thermal and nonthermal emission in the gamma-ray binary LS I +61 303Feb 21, 2017TFAW: wavelet-based signal reconstruction to reduce photometric noise in time-domain surveysJan 15, 2002LS 5039: a runaway microquasar ejected from the galactic planeApr 6, 2006New observational techniques and analysis tools for wide field CCD surveys and high resolution astrometryMar 4, 2004Application of fast CCD drift scanning to speckle imaging of binary starsAug 27, 2001CCD drift-scan imaging lunar occultations: a feasible approach for sub-meter class telescopesJan 30, 2004Infrared and visual lunar occultations measurements of stellar diameters and new binary stars detections at the Calar Alto 1.5m telescopeDec 19, 2024Enhancing the detection of low-energy M dwarf flares: Wavelet-based denoising of CHEOPS dataJul 15, 2010New high-sensitivity, milliarcsecond resolution results from routine observations of lunar occultations at the ESO VLT