346 citations · 2.6k across the 41 of their papers we have counts for
41 papers
Candidate ram-pressure stripped galaxies in six low-redshift clusters revealed from ultraviolet imaging
Koshy George, B. M. Poggianti, A. Omizzolo +12
The assembly of galaxy clusters is understood to be a hierarchical process with a continuous accretion of galaxies over time, which increases the cluster size and mass. Late-type g…
Clustercentric distance or local density? It depends on galaxy morphology
B. Vulcani, B. M. Poggianti, M. Gullieuszik +6
Determining which between projected local density and distance from the cluster center plays a major role in regulating morphological fractions in clusters is a longstanding debate…
UV and H HST observations of 6 GASP jellyfish galaxies
Marco Gullieuszik, Eric Giunchi, Bianca M. Poggianti +17
Star-forming, H-emitting clumps are found embedded in the gaseous tails of galaxies undergoing intense ram-pressure stripping in galaxy clusters, so-called jellyfish galaxies. T…
Ultraviolet imaging observations of three jellyfish galaxies: Star formation suppression in the centre and ongoing star formation in stripped tails
Koshy George, B. M. Poggianti, Neven Tomičić +13
Spiral galaxies undergo strong ram-pressure effects when they fall into the galaxy cluster potential. As a consequence, their gas is stripped to form extended tails within which st…
Observing ram pressure at work in intermediate redshift clusters with MUSE: the case of Abell 2744and Abell 370
A. Moretti, M. Radovich, B. M. Poggianti +11
Ram pressure stripping has been proven to be effective in shaping galaxy properties in dense environments at low redshift. The availability of MUSE observations of a sample of dist…
The Luminosity Function of bright QSOs at z~4 and implications for the cosmic ionizing background
K. Boutsia, A. Grazian, F. Fontanot +8
Based on results by recent surveys, the number of bright quasars at redshifts z>3 is being constantly revised upwards. Current consensus is that at bright magnitudes ($M_{1450}\le…