239 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Osservatorio Astronomico della Regione Autonoma Valle d'AostaIT32 papers
- National Institute for AstrophysicsIT21 papers
- Osservatorio Astrofisico di TorinoIT20 papers
- Osservatorio Astrofisico di CataniaIT18 papers
- Max Planck Institute for Radio AstronomyDE17 papers
- Evgeni Kharadze Georgian National Astrophysical ObservatoryGE16 papers
- Pulkovo ObservatoryRU16 papers
- Center for Astrophysics Harvard & SmithsonianUS15 papers
- St Petersburg UniversityRU14 papers
- University of Colorado DenverUS14 papers
- University of TurkuFI14 papers
- Astronomical Observatory of RomeIT13 papers
4 papers · 1 filter
Calibration of systematics in constraining modified gravity models with galaxy cluster mass profiles
L. Pizzuti, B. Sartoris, S. Borgani +1
Joint lensing and dynamical mass profile determinations of galaxy clusters are an excellent tool to constrain modification of gravity at cosmological scales. However, search for ti…
Investigating the multiwavelength behaviour of the flat spectrum radio quasar CTA 102 during 2013-2017
F. D'Ammando, C. M. Raiteri, M. Villata +94
We present a multiwavelength study of the flat-spectrum radio quasar CTA 102 during 2013-2017. We use radio-to-optical data obtained by the Whole Earth Blazar Telescope, 15 GHz dat…
The beamed jet and quasar core of the distant blazar 4C 71.07
C. M. Raiteri, M. Villata, M. I. Carnerero +5
The object 4C 71.07 is a high-redshift blazar whose spectral energy distribution shows a prominent big blue bump and a strong Compton dominance. We present the results of a two-yea…
Physical characterization of NEA Large Super-Fast Rotator (436724) 2011 UW158
A. Carbognani, B. L. Gary, J. Oey +2
Asteroids of size larger than 0.15 km generally do not have periods smaller than 2.2 hours, a limit known as cohesionless spin barrier. This barrier can be explained by the cohesio…