activity
20112017
most citedIdentification of the feature that causes the I-band secondary maximum of a type Ia supernova

25 citations · 87 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR20179 cited

Carrington cycle 24: The solar chromospheric emission in a historical and stellar perspective

K. -P. Schroder, M. Mittag, J. H. M. M. Schmitt +3

We present the solar S-index record of cycle 24, obtained by the TIGRE robotic telescope facility and its high-resolution spectrograph HEROS (R20,000), which measures the…

astro-ph.HE20177 cited

Study of the variability of Nova V5668 Sgr, based on high resolution spectroscopic monitoring

D. Jack, J. de J. Robles Pérez, I. De Gennaro Aquino +9

We present results of our dense spectroscopic monitoring of Nova V5668 Sgr. Starting on March 19 in 2015, only a few days after discovery, we have obtained a series of spectra with…

astro-ph.HE201519 cited

Time series of high resolution spectra of SN 2014J observed with the TIGRE telescope

D. Jack, M. Mittag, K. -P. Schroder +6

We present a time series of high resolution spectra of the Type Ia supernova 2014J, which exploded in the nearby galaxy M82. The spectra were obtained with the HEROS echelle spectr…

astro-ph.HE201525 cited

Identification of the feature that causes the I-band secondary maximum of a type Ia supernova

D. Jack, E. Baron, P. H. Hauschildt

We obtained a time series of spectra covering the secondary maximum in the I-band of the bright Type Ia supernova 2014J in M82 with the TIGRE telescope. Comparing the observations…

astro-ph.IM20128 cited

A 3D radiative transfer framework IX. Time dependence

D. Jack, P. H. Hauschildt, E. Baron

Context. Time-dependent, 3D radiation transfer calculations are important for the modeling of a variety of objects, from supernovae and novae to simulations of stellar variability…

astro-ph.SR201119 cited

Theoretical light curves of type Ia supernovae

D. Jack, P. H. Hauschildt, E. Baron

Aims. We present the first theoretical SN Ia light curves calculated with the time-dependent version of the general purpose model atmosphere code PHOENIX. Our goal is to produce li…