SN 2014ad , the SIMBAD biblio

SN 2014ad , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST20:38:02


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Title First 3 Authors
2017ApJ...835..140M 16       D               1 194 134 Ejection of the massive hydrogen-rich envelope timed with the collapse of the stripped SN 2014C. MARGUTTI R., KAMBLE A., MILISAVLJEVIC D., et al.
2017MNRAS.469.1897S 4224 T   A D S   X C       102 50 5 The evolution of the 3D shape of the broad-lined Type Ic
SN 2014ad.
STEVANCE H.F., MAUND J.R., BAADE D., et al.
2018MNRAS.475.2591S 5227 T K A D     X C F     125 22 10 Broad-line Type Ic supernova
SN 2014ad.
SAHU D.K., ANUPAMA G.C., CHAKRADHARI N.K., et al.
2017MNRAS.472.1770B 81           X         2 17 12 The imprints of the last jets in core collapse supernovae. BEAR E., GRICHENER A. and SOKER N.
2018MNRAS.473.3776K 552       D     X C F     12 20 8 ASASSN-16fp (SN 2016coi): a transitional supernova between Type Ic and broad-lined Ic. KUMAR B.
2018MNRAS.479.4535S 41           X         1 11 5 Probing the rotational velocity of Galactic WO stars with spectropolarimetry. STEVANCE H.F., IGNACE R., CROWTHER P.A., et al.
2018A&A...617A.105J 41           X         1 48 11 Host galaxies of SNe Ic-BL with and without long gamma-ray bursts. JAPELJ J., VERGANI S.D., SALVATERRA R., et al.
2018ApJ...867..147W 82               F     1 14 4 Spectroscopy of the Type Ic supernova SN 2017iuk associated with low-redshift GRB 171205A. WANG J., ZHU Z.P., XU D., et al.
2019ApJ...879...89M 1572 T   A S   X C       35 18 ~ Constraints on the environment and energetics of the broad-line Ic
SN2014ad from deep radio and X-ray observations.
MARONGIU M., GUIDORZI C., MARGUTTI R., et al.
2019ApJ...880L..22W 17       D               1 31 ~ Optimal classification and outlier detection for stripped-envelope core-collapse supernovae. WILLIAMSON M., MODJAZ M. and BIANCO F.B.
2020A&A...639L..11I 44           X         1 13 23 Broad-line type Ic SN 2020bvc. Signatures of an off-axis gamma-ray burst afterglow. IZZO L., AUCHETTL K., HJORTH J., et al.
2020MNRAS.497.3770G 102       D         F     6 54 ~ Optical studies of two stripped-envelope supernovae - SN 2015ap (Type Ib) and SN 2016P (Type Ic). GANGOPADHYAY A., MISRA K., SAHU D.K., et al.
2021ApJ...908...75B 192       D     X C       4 556 32 The radio luminosity-risetime function of core-collapse supernovae. BIETENHOLZ M.F., BARTEL N., ARGO M., et al.
2021MNRAS.505.3950G 104       D         F     2 37 ~ Understanding the extreme luminosity of DES14X2fna. GRAYLING M., GUTIERREZ C.P., SULLIVAN M., et al.
2021ApJ...918...89A 104       D       C       3 59 31 The nickel mass distribution of stripped-envelope supernovae: implications for additional power sources. AFSARIARDCHI N., DROUT M.R., KHATAMI D.K., et al.
2021MNRAS.507.1229P 218           X   F     4 39 18 Photometric, polarimetric, and spectroscopic studies of the luminous, slow-decaying Type Ib SN 2012au. PANDEY S.B., KUMAR A., KUMAR B., et al.
2022ApJ...927...61K viz 18       D               1 46 1 Investigating the Observational Properties of Type Ib Supernova SN 2017iro. KUMAR B., SINGH A., SAHU D.K., et al.
2022ApJ...925..175S 108       D       C       8 117 18 Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae. SHAHBANDEH M., HSIAO E.Y., ASHALL C., et al.
2022ApJ...931..153S 63       D     X         2 84 5 Constraints on the Explosion Timescale of Core-collapse Supernovae Based on Systematic Analysis of Light Curves. SAITO S., TANAKA M., SAWADA R., et al.
2022ApJ...937...40K 5223 T   A S   X C       114 22 4 Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type Ic
Supernova 2014ad.
KWOK L.A., WILLIAMSON M., JHA S.W., et al.
2023ApJ...944L..49W 47           X         1 21 1 SN 2019ewu: A Peculiar Supernova with Early Strong Carbon and Weak Oxygen Features from a New Sample of Young SN Ic Spectra. WILLIAMSON M., VOGL C., MODJAZ M., et al.
2023MNRAS.522.2267M 47           X         1 7 ~ Diagnosing the ejecta properties of engine-driven supernovae from observables in their initial phase. MAEDA K., SUZUKI A. and IZZO L.

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