LSQ 14an , the SIMBAD biblio

LSQ 14an , the SIMBAD biblio (34 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST21:40:45

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2014ATel.5718....1L 39           X         1 9 6 PESSTO spectroscopic classification of optical transients. LEGET P.-F., LE GUILLOU L., FLEURY M., et al.
2016ApJ...828L..18N 49           X         1 9 85 Superluminous supernova SN 2015bn in the nebular phase: evidence for the engine-powered explosion of a stripped massive star. NICHOLL M., BERGER E., MARGUTTI R., et al.
2016ApJ...831..144L 685   K   S   X C       15 14 54 PS1-14bj: a hydrogen-poor superluminous supernova with a long rise and slow decay. LUNNAN R., CHORNOCK R., BERGER E., et al.
2017ApJ...835...13J 1937   K A S   X C       46 22 99 Long-duration superluminous supernovae at late times. JERKSTRAND A., SMARTT S.J., INSERRA C., et al.
2017ApJ...842...26L 81             C       1 26 23 A Monte Carlo approach to magnetar-powered transients. I. Hydrogen-deficient superluminous supernovae. LIU L.-D., WANG S.-Q., WANG L.-J., et al.
2017MNRAS.466.2633S 44           X         1 13 44 Supernova ejecta with a relativistic wind from a central compact object: a unified picture for extraordinary supernovae. SUZUKI A. and MAEDA K.
2017MNRAS.468.4642I 4671   K A D S   X C F     113 35 37 Complexity in the light curves and spectra of slow-evolving superluminous supernovae. INSERRA C., NICHOLL M., CHEN T.-W., et al.
2017ApJ...845...85L viz 82           X         2 47 77 Analyzing the largest spectroscopic data set of hydrogen-poor super-luminous supernovae. LIU Y.-Q., MODJAZ M. and BIANCO F.B.
2017MNRAS.470.3566C 384       D     X   F     9 22 54 Superluminous supernova progenitors have a half-solar metallicity threshold. CHEN T.-W., SMARTT S.J., YATES R.M., et al.
2017ApJ...850...55N 61       D     X         2 41 176 The magnetar model for Type I superluminous supernovae. I. Bayesian analysis of the full multicolor light-curve sample with MOSFiT. NICHOLL M., GUILLOCHON J. and BERGER E.
2018MNRAS.473.1258S 100       D         F     4 75 131 Cosmic evolution and metal aversion in superluminous supernova host galaxies. SCHULZE S., KRUHLER T., LELOUDAS G., et al.
2018ApJ...854..175I 82             C       1 48 19 A statistical approach to identify superluminous supernovae and probe their diversity. INSERRA C., PRAJS S., GUTIERREZ C.P., et al.
2018A&A...611A..45R 82           X         2 47 13 Search for γ-ray emission from superluminous supernovae with the Fermi-LAT. RENAULT-TINACCI N., KOTERA K., NERONOV A., et al.
2018MNRAS.478..110S 41           X         1 16 6 Broad-band emission properties of central engine-powered supernova ejecta interacting with a circumstellar medium. SUZUKI A. and MAEDA K.
2018ApJ...864...45M viz 141       D     X         4 37 58 Results from a systematic survey of X-ray emission from hydrogen-poor superluminous SNe. MARGUTTI R., CHORNOCK R., METZGER B.D., et al.
2018ApJ...865....9B 82           X         2 18 9 The Type I superluminous supernova PS16aqv: lightcurve complexity and deep limits on radioactive ejecta in a fast event. BLANCHARD P.K., NICHOLL M., BERGER E., et al.
2019ApJ...871..102N 1064       D S   X C       24 20 55 Nebular-phase spectra of superluminous supernovae: physical insights from observational and statistical properties. NICHOLL M., BERGER E., BLANCHARD P.K., et al.
2019A&A...621A.141D 612     A     X C       14 16 33 Simulations of light curves and spectra for superluminous Type Ic supernovae powered by magnetars. DESSART L.
2019RAA....19...63W 42           X         1 28 3 The Energy Sources of Superluminous Supernovae. WANG S.-Q., WANG L.-J. and DAI Z.-G.
2019ApJ...881...87G viz 43           X         1 20 27 SN 2016iet: the pulsational or pair instability explosion of a low-metallicity massive CO core embedded in a dense hydrogen-poor circumstellar medium. GOMEZ S., BERGER E., NICHOLL M., et al.
2020A&A...634A.107Y 17       D               2 144 39 Present-day mass-metallicity relation for galaxies using a new electron temperature method. YATES R.M., SCHADY P., CHEN T.-W., et al.
2020ApJ...892...28K 170           X         4 20 ~ SN 2010kd: photometric and spectroscopic analysis of a slow-decaying superluminous supernova. KUMAR A., PANDEY S.B., KONYVES-TOTH R., et al.
2020ApJ...904...74G 17       D               1 145 ~ FLEET: a redshift-agnostic machine learning pipeline to rapidly identify hydrogen-poor superluminous supernovae. GOMEZ S., BERGER E., BLANCHARD P.K., et al.
2021ApJ...909...24K 17       D               2 93 ~ Photospheric velocity gradients and ejecta masses of hydrogen-poor superluminous supernovae: proxies for distinguishing between fast and slow events. KONYVES-TOTH R. and VINKO J.
2021MNRAS.502.2120F 131           X C       2 23 16 SN 2017gci: a nearby Type I Superluminous Supernova with a bumpy tail. FIORE A., CHEN T.-W., JERKSTRAND A., et al.
2021ApJ...912...21E 235       D S   X         5 125 18 Late-time radio and millimeter observations of superluminous supernovae and long gamma-ray bursts: implications for central engines, fast radio bursts, and obscured star formation. EFTEKHARI T., MARGALIT B., OMAND C.M.B., et al.
2021MNRAS.507.1229P 87               F     1 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.
2022MNRAS.517.2056G 421       D     X C F     8 30 9 SN 2020wnt: a slow-evolving carbon-rich superluminous supernova with no O II lines and a bumpy light curve. GUTIERREZ C.P., PASTORELLO A., BERSTEN M., et al.
2022ApJ...940...69K 287       D     X         7 32 2 Premaximum Spectroscopic Diversity of Hydrogen-poor Superluminous Supernovae. KONYVES-TOTH R.
2022ApJ...941..107G 45           X         1 238 16 Luminous Supernovae: Unveiling a Population between Superluminous and Normal Core-collapse Supernovae. GOMEZ S., BERGER E., NICHOLL M., et al.
2023ApJ...951...34T 47           X         1 19 3 Supernova 2020wnt: An Atypical Superluminous Supernova with a Hidden Central Engine. TINYANONT S., WOOSLEY S.E., TAGGART K., et al.
2023NatAs...7..779L 233           X C       4 16 ~ A superluminous supernova lightened by collisions with pulsational pair-instability shells. LIN W., WANG X., YAN L., et al.
2023ApJ...954...44K 19       D               2 29 ~ Type W and Type 15bn Subgroups of Hydrogen-poor Superluminous Supernovae: Premaximum Diversity, Postmaximum Homogeneity? KONYVES-TOTH R. and SELI B.
2024A&A...683A.223S viz 1670       D     X C F     32 28 ~ 1100 days in the life of the supernova 2018ibb The best pair-instability supernova candidate, to date. SCHULZE S., FRANSSON C., KOZYREVA A., et al.

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