activity
20062016
most citedThe rise of SN2014J in the nearby galaxy M82

132 citations · 395 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2016★ 21 cited

Post-maximum near infrared spectra of SN 2014J: A search for interaction signatures

D. J. Sand, E. Y. Hsiao, D. P. K. Banerjee +7

We present near infrared (NIR) spectroscopic and photometric observations of the nearby Type Ia SN 2014J. The seventeen NIR spectra span epochs from +15.3 to +92.5 days after -b…

astro-ph.SR2015

Near Infrared studies of the carbon-monoxide and dust forming nova V5668 Sgr

D. P. K. Banerjee, Mudit K. Srivastava, N. M. Ashok +1

We present near-infrared (NIR) observations of Nova V5668 Sgr, discovered in outburst on 2015 March 15.634 UT, between 2d to 107d after outburst. NIR spectral features are used to…

astro-ph.EP2014★ 5 cited

Lately Exposed Amorphous Water Ice on Comet 49P/Arend-Rigaux

B. Sivaraman, V. Venkataraman, A. Kalyaan +2

Comet 49P/ Arend-Rigaux, thought to be a low activity comet since the 1980's was found to be active in its recent apparitions. Recent analysis of the data obtained from Spitzer obs…

astro-ph.HE2014★ 102 cited

The peculiar extinction law of SN2014J measured with The Hubble Space Telescope

R. Amanullah, A. Goobar, J. Johansson +10

The wavelength-dependence of the extinction of Type Ia SN2014J in the nearby galaxy M82 has been measured using UV to near-IR photometry obtained with the Hubble Space Telescope, t…

astro-ph.GA2014★ 76 cited

Early Observations and Analysis of the Type Ia SN 2014J in M82

G. H. Marion, D. J. Sand, E. Y. Hsiao +23

We present optical and near infrared (NIR) observations of the nearby Type Ia SN 2014J. Seventeen optical and twenty-three NIR spectra were obtained from 10 days before (10d) to…

astro-ph.HE2014★ 36 cited

Near-IR studies of recurrent nova V745 Scorpii during its 2014 outburst

D. P. K. Banerjee, Vishal Joshi, V. Venkataraman +4

The recurrent nova (RN) V745 Scorpii underwent its third known outburst on 2014 February 6. Infrared monitoring of the eruption on an almost daily basis, starting from 1.3d after d…