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| iPTF 16bad , the SIMBAD biblio (34 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST02:10:37 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2017ApJ...848....6Y | 1788 | K A | D | X C | 45 | 23 | 91 | Hydrogen-poor superluminous supernovae with late-time Hα emission: three events from the intermediate Palomar Transient Factory. | YAN L., LUNNAN R., PERLEY D.A., et al. |
| 2017ApJ...850...55N | 18 | D | 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. | ||
| 2017ApJ...850..148W | 159 | X C | 3 | 11 | 6 | Modeling the most luminous supernova associated with a gamma-ray burst, SN 2011kl. | WANG S.-Q., CANO Z., WANG L.-J., et al. | ||
| 2018ApJ...854..175I | 16 | D | 1 | 48 | 19 | A statistical approach to identify superluminous supernovae and probe their diversity. | INSERRA C., PRAJS S., GUTIERREZ C.P., et al. | ||
| 2018ApJ...856...59L | 41 | X | 1 | 7 | 11 | A multiple ejecta-circumstellar medium interaction model and its implications for superluminous supernovae iPTF15esb and iPTF13dcc. | LIU L.-D., WANG L.-J., WANG S.-Q., et al. | ||
| 2018NatAs...2..887L | 1 | 14 | 14 | A UV resonance line echo from a shell around a hydrogen-poor superluminous supernova. | LUNNAN R., FRANSSON C., VREESWIJK P.M., et al. | ||||
| 2018ApJ...867..113M | 16 | D | 2 | 37 | 11 | Systematic investigation of the fallback accretion-powered model for hydrogen-poor superluminous supernovae. | MORIYA T.J., NICHOLL M. and GUILLOCHON J. | ||
| 2018ApJ...869..166V | 16 | D | 1 | 58 | 6 | Superluminous supernovae in LSST: rates, detection metrics, and light-curve modeling. | VILLAR V.A., NICHOLL M. and BERGER E. | ||
| 2019A&A...624A.143K | 42 | X | 1 | 63 | 71 | Highly luminous supernovae associated with gamma-ray bursts. I. GRB 111209A/SN 2011kl in the context of stripped-envelope and superluminous supernovae. | KANN D.A., SCHADY P., OLIVARES F.E., et al. | ||
| 2019ApJ...882..102G | 309 | A | X C | 7 | 11 | ~ | A simple analysis of Type I superluminous supernova peak spectra: composition, expansion velocities, and dynamics. | GAL-YAM A. | |
| 2020ApJ...892...28K | 41 | X | 1 | 20 | ~ | SN 2010kd: photometric and spectroscopic analysis of a slow-decaying superluminous supernova. | KUMAR A., PANDEY S.B., KONYVES-TOTH R., et al. | ||
| 2020ApJ...897..114B | 16 | D | 1 | 67 | ~ | The pre-explosion mass distribution of hydrogen-poor superluminous supernova progenitors and new evidence for a mass-spin correlation. | BLANCHARD P.K., BERGER E., NICHOLL M., et al. | ||
| 2020ApJ...904...74G | 16 | 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 | 1 | 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.502.1678K | 84 | X | 2 | 51 | 12 | SN 2020ank: a bright and fast-evolving H-deficient superluminous supernova. | KUMAR A., KUMAR B., PANDEY S.B., et al. | ||
| 2021MNRAS.504L..51S | 84 | X | 2 | 7 | ~ | Binary pathways to SLSNe-I: SN 2017gci. | STEVANCE H.F. and ELDRIDGE J.J. | ||
| 2021ApJ...912...21E | 226 | 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. | |
|
2021ApJS..255...29S |
17 | D | 1 | 893 | 63 | The Palomar Transient Factory core-collapse supernova host-galaxy sample. I. Host-galaxy distribution functions and environment dependence of core-collapse supernovae. | SCHULZE S., YARON O., SOLLERMAN J., et al. | ||
| 2021MNRAS.506.4819P | 376 | X C | 8 | 21 | 3 | SN 2019hcc: a Type II supernova displaying early O II lines. | PARRAG E., INSERRA C., SCHULZE S., et al. | ||
| 2022MNRAS.510.3701S | 43 | X | 1 | 17 | 15 | An environmental analysis of the Type Ib SN 2019yvr and the possible presence of an inflated binary companion. | SUN N.-C., MAUND J.R., CROWTHER P.A., et al. | ||
| 2022MNRAS.512.4484F | 468 | X C F | 9 | 24 | 4 | Close, bright, and boxy: the superluminous SN 2018hti. | FIORE A., BENETTI S., NICHOLL M., et al. | ||
| 2022MNRAS.513.2965H | 43 | X | 1 | 12 | ~ | Two years of optical and NIR observations of the superluminous supernova UID 30901 discovered by the UltraVISTA SN survey. | HUEICHAPAN E.D., CONTRERAS C., CARTIER R., et al. | ||
|
2022ApJ...933...14H |
102 | D | C | 2 | 35 | 28 | Bumpy Declining Light Curves Are Common in Hydrogen-poor Superluminous Supernovae. | HOSSEINZADEH G., BERGER E., METZGER B.D., et al. | |
| 2022ApJ...938...84D | 85 | X | 2 | 34 | 6 | Radio Analysis of SN2004C Reveals an Unusual CSM Density Profile as a Harbinger of Core Collapse. | DEMARCHI L., MARGUTTI R., DITTMAN J., et al. | ||
| 2022A&A...666A..30P | 468 | X C | 10 | 43 | 14 | SN 2018bsz: A Type I superluminous supernova with aspherical circumstellar material. | PURSIAINEN M., LELOUDAS G., PARASKEVA E., et al. | ||
|
2022ApJ...939..105B |
230 | D | S X | 5 | 121 | 10 | Seven Years of Coordinated Chandra-NuSTAR Observations of SN 2014C Unfold the Extreme Mass-loss History of Its Stellar Progenitor. | BRETHAUER D., MARGUTTI R., MILISAVLJEVIC D., et al. | |
| 2022ApJ...941..107G | 43 | X | 1 | 238 | 16 | Luminous Supernovae: Unveiling a Population between Superluminous and Normal Core-collapse Supernovae. | GOMEZ S., BERGER E., NICHOLL M., et al. | ||
| 2020RNAAS...4..235B | 41 | X | 1 | 4 | ~ | Six Years of Luminous X-Ray Emission from the Strongly Interacting Type-Ib SN2014C Captured by Chandra and NuSTAR. | BRETHAUER D., MARGUTTI R., MILISAVLJEVIC D., et al. | ||
| 2023ApJ...954L..45M | 44 | X | 1 | 14 | ~ | Luminous Radio Emission from the Superluminous Supernova 2017ens at 3.3 yr after Explosion. | MARGUTTI R., BRIGHT J.S., MATTHEWS D.J., et al. | ||
| 2024MNRAS.52711970A | 45 | X | 1 | 32 | ~ | A precursor plateau and pre-maximum [O II] emission in the superluminous SN2019szu: a pulsational pair-instability candidate. | AAMER A., NICHOLL M., JERKSTRAND A., et al. | ||
| 2024ApJ...961..169H | 18 | D | 1 | 110 | ~ | An Extensive Hubble Space Telescope Study of the Offset and Host Light Distributions of Type I Superluminous Supernovae. | HSU B., BLANCHARD P.K., BERGER E., et al. | ||
| 2024A&A...685A..20G | 358 | X C F | 6 | 24 | ~ | SN 2020zbf: A fast-rising hydrogen-poor superluminous supernova with strong carbon lines. | GKINI A., LUNNAN R., SCHULZE S., et al. | ||
| 2024MNRAS.535..471G | 197 | D | S X | 4 | 274 | ~ | The Type I superluminous supernova catalogue I: light-curve properties, models, and catalogue description. | GOMEZ S., NICHOLL M., BERGER E., et al. | |
| 2025ApJ...986...84T | 140 | X C | 2 | 4 | ~ | Stellar Tidal Disruptions by Newborn Neutron Stars or Black Holes: A Mechanism for Hydrogen-poor (Super)luminous Supernovae and Fast Blue Optical Transients. | TSUNA D. and LU W. |