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LSQ 14bdq , the SIMBAD biblio (66 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST05:56:25 |
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 |
---|---|---|---|---|---|---|---|---|---|
2015ApJ...808L..51P | 786 | K A | S X C | 18 | 6 | 107 | Using double-peaked supernova light curves to study extended material. | PIRO A.L. | |
2015ApJ...807L..18N | 1275 | T K A | D | X C | 31 | 12 | 99 |
LSQ14bdq: a type IC super-luminous supernova with a double-peaked light curve. |
NICHOLL M., SMARTT S.J., JERKSTRAND A., et al. |
2015MNRAS.452.3869N | 255 | K | D | X | 7 | 55 | 156 | On the diversity of superluminous supernovae: ejected mass as the dominant factor. | NICHOLL M., SMARTT S.J., JERKSTRAND A., et al. |
2015MNRAS.454.2353O | 516 | K A | D | X C | 13 | 5 | 6 | Quark-Novae in massive binaries: a model for double-humped, hydrogen-poor, superluminous Supernovae. | OUYED R., LEAHY D. and KONING N. |
2014ATel.6118....1B | 39 | X | 1 | 5 | 2 | PESSTO spectroscopic classification of optical transients. | BENITEZ S., POLSHAW J., INSERRA C., et al. | ||
2016ApJ...818L...8S | 368 | X C | 8 | 7 | 51 | DES14X3taz: a Type I superluminous supernova showing a luminous, rapidly cooling initial pre-peak bump. | SMITH M., SULLIVAN M., D'ANDREA C.B., et al. | ||
2016ApJ...818...77O | 803 | K A | D | S X C | 19 | 10 | 7 | Quark-novae occurring in massive binaries : a universal energy source in superluminous supernovae with double-peaked light curves. | OUYED R., LEAHY D. and KONING N. |
2016ApJ...819...51L | 81 | C | 1 | 18 | 25 | Late time multi-wavelength observations of Swift J1644+5734: a luminous Optical/IR bump and quiescent X-ray emission. | LEVAN A.J., TANVIR N.R., BROWN G.C., et al. | ||
2016ApJ...821...36K | 272 | A | D | X | 7 | 3 | 93 | Magnetar-driven shock breakout and double-peaked supernova light curves. | KASEN D., METZGER B.D. and BILDSTEN L. |
2016MNRAS.457L..79N | 1527 | K A | D | X C F | 37 | 14 | 35 | Seeing double: the frequency and detectability of double-peaked superluminous supernova light curves. | NICHOLL M. and SMARTT S.J. |
2016ARep...60....1B | 40 | X | 1 | 50 | 21 | Scientific problems addressed by the Spektr-UV Space Project (World Space Observatory-Ultraviolet) | BOYARCHUK A.A., SHUSTOV B.M., SAVANOV I.S., et al. | ||
2016ApJ...826...39N | 408 | X C | 9 | 18 | 133 | SN 2015BN: a detailed multi-wavelength view of a nearby superluminous supernova. | NICHOLL M., BERGER E., SMARTT S.J., et al. | ||
2016ApJ...831..144L | 43 | X | 1 | 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...58V | 489 | X C | 11 | 14 | 40 | On the early-time excess emission in hydrogen-poor superluminous supernovae. | VREESWIJK P.M., LELOUDAS G., GAL-YAM A., et al. | ||
2016A&A...596A..67R | 40 | X | 1 | 60 | 14 | SN 2012aa: A transient between Type Ibc core-collapse and superluminous supernovae. | ROY R., SOLLERMAN J., SILVERMAN J.M., et al. | ||
2017ApJ...838..130S | 299 | K | X C | 6 | 4 | 63 | UV/Optical emission from the expanding envelopes of Type II supernovae. | SAPIR N. and WAXMAN E. | |
2017ApJ...840...12Y | 139 | D | X | 4 | 38 | 51 | A statistical study of superluminous supernovae using the magnetar engine model and implications for their connection with gamma-ray bursts and hypernovae. | YU Y.-W., ZHU J.-P., LI S.-Z., 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. | ||
2017A&A...602A...9C | 204 | X C | 4 | 25 | 37 | The evolution of superluminous supernova LSQ14mo and its interacting host galaxy system. | CHEN T.-W., NICHOLL M., SMARTT S.J., et al. | ||
2017MNRAS.468.4642I | 82 | X | 2 | 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 | 17 | D | 1 | 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 | 43 | X | 1 | 22 | 54 | Superluminous supernova progenitors have a half-solar metallicity threshold. | CHEN T.-W., SMARTT S.J., YATES R.M., et al. | ||
2017MNRAS.470.4241P | 124 | X C | 2 | 6 | 13 | DES15E2mlf: a spectroscopically confirmed superluminous supernova that exploded 3.5 Gyr after the big bang. | PAN Y.-C., FOLEY R.J., SMITH M., et al. | ||
2017ApJ...848....6Y | 44 | X | 1 | 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. | ||
2017A&A...605A.107C | 42 | X | 1 | 24 | 44 | GRB 161219B/SN 2016jca: A low-redshift gamma-ray burst supernova powered by radioactive heating. | CANO Z., IZZO L., DE UGARTE POSTIGO A., et al. | ||
2017ApJ...850...55N | 101 | D | X | 3 | 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. | |
2018ApJ...852...81L | 455 | X C | 10 | 32 | 93 | Hydrogen-poor superluminous supernovae from the Pan-STARRS1 Medium Deep Survey. | LUNNAN R., CHORNOCK R., BERGER E., et al. | ||
2018MNRAS.473.1258S | 100 | D | C | 3 | 75 | 131 | Cosmic evolution and metal aversion in superluminous supernova host galaxies. | SCHULZE S., KRUHLER T., LELOUDAS G., et al. | |
2018ApJ...853...57B | 208 | X C | 4 | 27 | 66 | Gaia17biu/SN 2017egm in NGC 3191: the closest hydrogen-poor superluminous supernova to date is in a "normal," massive, metal-rich spiral galaxy. | BOSE S., DONG S., PASTORELLO A., et al. | ||
2018ApJ...854...37S | 82 | X | 2 | 13 | 12 | Studying the ultraviolet spectrum of the first spectroscopically confirmed Supernova at redshift two. | SMITH M., SULLIVAN M., NICHOL R.C., 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. | ||
2018MNRAS.475.2659M | 278 | K A | X C F | 5 | 10 | 61 | The GRB-SLSN connection: misaligned magnetars, weak jet emergence, and observational signatures. | MARGALIT B., METZGER B.D., THOMPSON T.A., 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. | ||
2018ApJ...860..100D | 84 | X | 2 | 41 | 119 | Light curves of hydrogen-poor superluminous supernovae from the Palomar Transient Factory. | DE CIA A., GAL-YAM A., RUBIN A., et al. | ||
2018ApJ...865....9B | 123 | X C | 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. | ||
2018MNRAS.479.4984C | 165 | C F | 3 | 10 | 1 | Testing the magnetar scenario for superluminous supernovae with circular polarimetry. | CIKOTA A., LELOUDAS G., BULLA 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. | ||
2018MNRAS.481..894P | 42 | X | 1 | 92 | 103 | Rapidly evolving transients in the Dark Energy Survey. | PURSIAINEN M., CHILDRESS M., SMITH M., et al. | ||
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. | ||
2018A&A...620A..67A | 124 | X | 3 | 25 | 36 | A nearby super-luminous supernova with a long pre-maximum & "plateau" and strong C II features. | ANDERSON J.P., PESSI P.J., DESSART L., et al. | ||
2019ApJ...874...68C | 59 | D | X | 2 | 32 | 1 | A systematic study of superluminous supernova light-curve models using clustering. | CHATZOPOULOS E. and TUMINELLO R. | |
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...877...20W | 167 | X C | 3 | 8 | ~ | Modeling the light curves of the luminous Type Ic supernova 2007D. | WANG S.-Q., CANO Z., LI L., et al. | ||
2019MNRAS.487.2215A | 169 | X F | 3 | 26 | 67 | Superluminous supernovae from the Dark Energy Survey. | ANGUS C.R., SMITH M., SULLIVAN M., et al. | ||
2019ApJ...881...87G | 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. | ||
2020ApJ...892...28K | 43 | 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 | 17 | 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. | ||
2020MNRAS.497..318L | 43 | X | 1 | 15 | ~ | SN 2018hti: a nearby superluminous supernova discovered in a metal-poor galaxy. | LIN W.L., WANG X.F., LI W.X., 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.502.1678K | 87 | X | 2 | 51 | 12 | SN 2020ank: a bright and fast-evolving H-deficient superluminous supernova. | KUMAR A., KUMAR B., PANDEY S.B., et al. | ||
2021ApJ...910...68J | 44 | X | 1 | 7 | ~ | The effect of circumstellar matter on the double-peaked Type Ic supernovae and implications for LSQ14efd, iPTF15dtg, and SN 2020bvc. | JIN H., YOON S.-C. and BLINNIKOV S. | ||
2021ApJ...911..142L | 392 | A | D | X C | 9 | 9 | ~ | Magnetar-driven shock breakout revisited and implications for double-peaked Type I superluminous supernovae. | LIU L.-D., GAO H., WANG X.-F., et al. |
2021ApJ...912...21E | 409 | D | S X | 9 | 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. | |
2022MNRAS.512.4484F | 645 | D | X C F | 13 | 24 | 4 | Close, bright, and boxy: the superluminous SN 2018hti. | FIORE A., BENETTI S., NICHOLL M., et al. | |
2022ApJ...931...71G | 45 | X | 1 | 17 | ~ | The GALEX-PTF Experiment. II. Supernova Progenitor Radius and Energetics via Shock-cooling Modeling. | GANOT N., OFEK E.O., GAL-YAM A., et al. | ||
2022MNRAS.514.2627C | 179 | X C | 3 | 63 | 5 | A puzzle solved after two decades: SN 2002gh among the brightest of superluminous supernovae. | CARTIER R., HAMUY M., CONTRERAS C., et al. | ||
2022ApJ...933...14H | 18 | D | 1 | 35 | 28 | Bumpy Declining Light Curves Are Common in Hydrogen-poor Superluminous Supernovae. | HOSSEINZADEH G., BERGER E., METZGER B.D., et al. | ||
2022MNRAS.517.2056G | 287 | D | X C F | 5 | 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 | 108 | D | X | 3 | 32 | 2 | Premaximum Spectroscopic Diversity of Hydrogen-poor Superluminous Supernovae. | KONYVES-TOTH R. | |
2022A&A...667A..92O | 108 | D | F | 2 | 25 | 2 | Supernova double-peaked light curves from double-nickel distribution. | ORELLANA M. and BERSTEN M.C. | |
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...943...42C | 112 | D | X | 3 | 55 | 22 | The Hydrogen-poor Superluminous Supernovae from the Zwicky Transient Facility Phase I Survey. II. Light-curve Modeling and Characterization of Undulations. | CHEN Z.H., YAN L., KANGAS T., et al. | |
2023ApJ...954...44K | 47 | X | 1 | 29 | ~ | Type W and Type 15bn Subgroups of Hydrogen-poor Superluminous Supernovae: Premaximum Diversity, Postmaximum Homogeneity? | KONYVES-TOTH R. and SELI B. | ||
2023MNRAS.526.1822K | 112 | D | F | 2 | 31 | ~ | Reduction of supernova light curves by vector Gaussian processes. | KORNILOV M.V., SEMENIKHIN T.A. and PRUZHINSKAYA M.V. | |
2024ApJ...961...67T | 50 | X | 1 | 18 | ~ | Simulating Hydrogen-poor Interaction-powered Supernovae with CHIPS. | TAKEI Y., TSUNA D., KO T., et al. |