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20022023
most citedSN 2005cs in M51 II. Complete Evolution in the Optical and the Near-Infrared

258 citations · 3.5k across the 58 of their papers we have counts for

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Showing 2007Show all

7 papers · 1 filter

astro-ph2007★ 40 cited

Near-Infrared observations of the type Ib Supernova SN2006jc: evidence of interactions with dust

E. Di Carlo, C. Corsi, A. A. Arkharov +6

In the framework of a program for the monitoring of Supernovae in the Near-Infrared (NIR) carried out by the Teramo, Rome and Pulkovo observatories with the AZT-24 telescope, we ob…

astro-ph2007★ 57 cited

The infrared JHK light curves of RR Lyr

A. Sollima, C. Cacciari, A. A. Arkharov +4

We present infrared JHK time series photometry of the variable star RR Lyr, that allow us to construct the first complete and accurate infrared light curves for this star. The deri…

astro-ph2007★ 4 cited

Color Variability of the Blazar AO 0235+16

V. A. Hagen-Thorn, V. M. Larionov, C. M. Raiteri +5

Multicolor (UBVRIJHK) observations of the blazar AO 0235+16 are analyzed. The light curves were compiled at the Turin Observatory from literature data and the results of observatio…

astro-ph2007★ 70 cited

SN 2002cv: A Heavily Obscured Type Ia Supernova

N. Elias-Rosa, S. Benetti, M. Turatto +15

We present VRIJHK photometry, and optical and near-infrared spectroscopy, of the heavily extinguished Type Ia supernova (SN) 2002cv, located in NGC 3190, which is also the parent g…

astro-ph2007★ 90 cited

The Outburst of the Blazar AO 0235+164 in 2006 December: Shock-in-Jet Interpretation

V. A. Hagen-Thorn, V. M. Larionov, S. G. Jorstad +5

We present the results of polarimetric ( band) and multicolor photometric () observations of the blazar AO 0235+16 during an outburst in 2006 December. The data reveal…

astro-ph2007★ 27 cited

An infrared view of the EXor variables: on the case of V1118 ORI

D. Lorenzetti, T. Giannini, V. M. Larionov +4

We investigate the relationship between the IR observed properties of the EXor variables and the mechanisms active during their evolutionary stage. To this aim, we have constructed…