154 citations
- American Association of Variable Star ObserversUS16 papers
- Kyoto UniversityJP13 papers
- British Astronomical AssociationGB12 papers
- Crimean Astrophysical ObservatoryUA12 papers
- Lomonosov Moscow State UniversityRU11 papers
- Rolling Hills ObservatoryUS11 papers
- Astronomical Institute of the Slovak Academy of SciencesSK10 papers
- Slovak Academy of SciencesSK10 papers
- Vihorlat ObservatorySK10 papers
- Bundesdeutsche Arbeitsgemeinschaft für Veränderliche SterneDE9 papers
- Osaka Kyoiku UniversityJP9 papers
- Universidad de HuelvaES9 papers
5 papers · 1 filter
Orbital periods of cataclysmic variables identified by the SDSS. III. Time-series photometry obtained during the 2004/5 International Time Project on La Palma
M. Dillon, B. T. Gaensicke, A. Aungwerojwit +7
We present time resolved CCD photometry of 15 cataclysmic variables (CVs) identified by the Sloan Digital Sky Survey (SDSS). The data were obtained as part of the 2004/05 Internati…
Radio-to-UV monitoring of AO 0235+164 by the WEBT and Swift during the 2006--2007 outburst
C. M. Raiteri, M. Villata, V. M. Larionov +2
The blazar AO 0235+164 was claimed to show a quasi-periodic behaviour in the radio and optical bands. Moreover, an extra emission component contributing to the UV and soft X-ray fl…
The reflecting surface of the MAGIC-II Telescope
D. Bastieri, J. Arnold, C. Baixeras +19
The MAGIC Collaboration is building a second telescope, MAGIC II, improving the design of the current MAGIC Telescope. MAGIC II is being built at 85 m of distance from MAGIC I, and…
A Survey Searching for the Epoch of Assembling of Hubble Types
Duilia F. de Mello, Anna Pasquali
We have started a survey of galaxies at intermediate redshifts using the HST-STIS parallel fields. Our main goal is to analyse the morphology of faint galaxies in order to estimate…
The Nature of Submm-Detected Galaxies
Duilia de Mello, T. Wiklind, C. Leitherer +1
We present high resolution VLT spectra of 2 submm-detected galaxies. Diagnostic stellar absorption lines (Starburst99) are used to analyse their stellar population. SMM J14011+0252…