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J. M. Coloma

Researcher at INAF

Publications -  19
Citations -  1112

J. M. Coloma is an academic researcher from INAF. The author has contributed to research in topics: Blazar & Asteroid. The author has an hindex of 15, co-authored 19 publications receiving 1043 citations.

Papers
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The unprecedented optical outburst of the quasar 3C 454.3 - The WEBT campaign of 2004–2005

M. Villata, +94 more
TL;DR: In this article, a large multi-wavelength campaign was organized by the Whole Earth Blazar Telescope (WEBT) to follow the emission behavior of the radio quasar 3C 454.3.
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The WEBT BL Lacertae Campaign 2001 and its extension. Optical light curves and colour analysis 1994-2002

M. Villata, +74 more
TL;DR: In this paper, the authors present UBVRI light curves obtained by the Whole Earth Blazar Telescope (WEBT) from 1994 to 2002, including the last, extended BL Lac 2001 campaign.
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Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution

Josef Hanus, +118 more
TL;DR: In this article, the authors compared the observed pole latitude distribution of all asteroids with known convex shape models with the simulated pole latitude distributions and presented 119 new asteroid shape models derived from combined dense and sparse-in-time photometry.
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The radio delay of the exceptional 3C 454.3 outburst - Follow-up WEBT observations in 2005–2006

TL;DR: In this paper, the authors investigated the expected correlation and time delays between the optical and radio emissions in order to derive information on the variability mechanisms and jet structure of the blazar 3C 454.3.
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Another look at the BL Lacertae flux and spectral variability:Observations by GASP-WEBT, XMM- Newton, and Swift in 2008-2009

TL;DR: In this paper, the authors investigated the role of the helical jet model in the broad-band emission and variability properties of BL Lacertae, and showed that the jet geometry can play an extremely important role in the source's flux and spectral v ariability.