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Weather in Bologna

Bologna
November 22, 2017, 1:49 pm
Sunny
Sunny
13°C
real feel: 15°C
current pressure: 1020 mb
humidity: 62%
wind speed: 0 m/s N
sunrise: 7:20 am
sunset: 4:42 pm
 

MAORY KICK OFF MEETING

MAORY_KoM

Image taken at the MAORY kick-off meeting in Bologna.

A new era for the Adaptive Optics. MAORY the Multi Conjugate Adaptive Optics RelaY for E-ELT entered in a new era. After the agreement signed on December 10 between INAF and ESO (which is building the telescope), on February 2 the MAORY kick-off meeting held

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V404 Cygni outburst observed at Loiano

The R light curve of V404 Cyg, obtained by BFOSC on June 20th, 2015 (observations by Ivan Bruni and Silvia Sclavi). the light curve of a nearby star, derived in the same way, is plotted for comparison (the  right-hand Y axis refers to this star).

The X-ray binary V404 Cygni underwent an outburst detected in the X-ray band by Swift on June 18, 2015. One of the components of this source is a black hole weighing about 10 solar masses, and it is the first time since 1989 that it displays such activity. Using the imager/spectrometer BFOSC at the 1.52m

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OABO news from Gaia

hort period/faint magnitude Cepheids in the Large Magellanic Cloud observed by Gaia

A press release by G. Clementini (INAF-OABO), V. Ripepi (INAF-OACN), S. Leccia (INAF-OACN), et al. was published yesterday (May 28, 2015) on the ESA Gaia web page showing results from the DPAC-CU7 pipeline on the Gaia commissioning data.

The first paper of the Gaia Science Alerts programme: “Total eclipse of the heart: The AM CVn

…→ Read More: OABO news from Gaia

Call for observing proposals at the 1.52m Cassini Telescope

Proposals may be submitted for the August 1st, 2015 – January 31st, 2016 semester.

The deadline is June 19th, 2015, at 13:00 UT.

RR Lyrae stars in the Large Magellanic Cloud as seen by Gaia

RR-LMC-GAIA-vs-OGLE-dots-To

Left panels: G-band light curves of RR Lyrae stars in the Large Magellanic Cloud observed by Gaia during the EPSL scanning. Right panels: I-band light curves obtained for the same stars by the OGLE IV survey. All light curves cover a 1.5 pulsation cycle.

During the first part of the Gaia mission in Ecliptic

…→ Read More: RR Lyrae stars in the Large Magellanic Cloud as seen by Gaia