Every reference with a DOI in the deposited reference list resolved to a known
work in Crossref or DataCite at the dated check, and none carried a retraction,
withdrawal, or removal notice.
The 74 checked references that resolve
resolves10.1016/0370-2693(88)91651-6Detection of the neutrino signal from SN 1987A in the LMC using the INR Baksan underground scintillation telescope
resolves10.1086/166565Why did the progenitor of SN 1987A undergo the blue-red-blue evolution?
resolves10.1086/169114Theoretical light curve of SN 1987A and mixing of hydrogen and nickel in the ejecta
resolves10.1086/308588Radiation Hydrodynamics of SN 1987A. I. Global Analysis of the Light Curve for the First 4 Months
resolves10.1111/j.1365-2966.2010.16611.xSupernova radiative-transfer modelling: a new approach using non-local thermodynamic equilibrium and full time dependence
resolves10.1038/nature11473Hard-X-ray emission lines from the decay of 44Ti in the remnant of supernova 1987A
resolves10.1126/science.aaa2259<sup>44</sup>
Ti gamma-ray emission lines from SN1987A reveal an asymmetric explosion
resolves10.1086/185002The composite image of Sanduleak -69 deg 202, candidate precursor to supernova 1987 A in the Large Magellanic Cloud
resolves10.1086/167545Asymmetric envelope expansion of supernova 1987A
resolves10.1093/mnras/stx818The quest for blue supergiants: binary merger models for the evolution of the progenitor of SN 1987A
resolves10.1088/0004-637X/757/1/69PROGENITOR-EXPLOSION CONNECTION AND REMNANT BIRTH MASSES FOR NEUTRINO-DRIVEN SUPERNOVAE OF IRON-CORE PROGENITORS
resolves10.1088/0004-637X/806/2/275PUSHING CORE-COLLAPSE SUPERNOVAE TO EXPLOSIONS IN SPHERICAL SYMMETRY. I. THE MODEL AND THE CASE OF SN 1987A
resolves10.3847/0004-637X/818/2/124A TWO-PARAMETER CRITERION FOR CLASSIFYING THE EXPLODABILITY OF MASSIVE STARS BY THE NEUTRINO-DRIVEN MECHANISM
resolves10.3847/1538-4357/aae7c9PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. II. Explodability and Remnant Properties
resolves10.1086/498224Composition of the Innermost Core‐Collapse Supernova Ejecta
resolves10.3847/1538-4357/aae7d2PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. III. Nucleosynthesis Yields
resolves10.1088/0004-637X/801/2/90THE LANDSCAPE OF THE NEUTRINO MECHANISM OF CORE-COLLAPSE SUPERNOVAE: NEUTRON STAR AND BLACK HOLE MASS FUNCTIONS, EXPLOSION ENERGIES, AND NICKEL YIELDS
resolves10.3847/0004-637X/831/1/98GENERAL-RELATIVISTIC THREE-DIMENSIONAL MULTI-GROUP NEUTRINO RADIATION-HYDRODYNAMICS SIMULATIONS OF CORE-COLLAPSE SUPERNOVAE
resolves10.3847/0004-637X/825/1/6PROGENITOR-DEPENDENT EXPLOSION DYNAMICS IN SELF-CONSISTENT, AXISYMMETRIC SIMULATIONS OF NEUTRINO-DRIVEN CORE-COLLAPSE SUPERNOVAE
resolves10.1093/mnrasl/sly059A full general relativistic neutrino radiation-hydrodynamics simulation of a collapsing very massive star and the formation of a black hole
resolves10.1088/1361-6471/aaed51The impact of different neutrino transport methods on multidimensional core-collapse supernova simulations
resolves10.3847/2041-8213/aaa967The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12–40 M<sub>⊙</sub>
resolves10.3847/1538-4357/aaac29Simulations of Core-collapse Supernovae in Spatial Axisymmetry with Full Boltzmann Neutrino Transport
resolves10.3847/1538-4357/aa9ce8Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
resolves10.3847/1538-4357/aa9d97Nucleosynthesis in the Innermost Ejecta of Neutrino-driven Supernova Explosions in Two Dimensions
resolves10.1051/0004-6361/200913106Protoneutron star evolution and the neutrino-driven wind in general relativistic neutrino radiation hydrodynamics simulations
resolves10.1103/PhysRevLett.96.142502Neutrino-Induced Nucleosynthesis of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>A</mml:mi><mml:mo>></mml:mo><mml:mn>64</mml:mn></mml:math>Nuclei: The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>ν</mml:mi><mml:mi>p</mml:mi></mml:math>Process
resolves10.1086/503891Nucleosynthesis in Early Supernova Winds. II. The Role of Neutrinos
resolves10.1086/313304The Accuracy, Consistency, and Speed of an Electron‐Positron Equation of State Based on Table Interpolation of the Helmholtz Free Energy
resolves10.1088/0004-637X/783/2/125TOWARD CONNECTING CORE-COLLAPSE SUPERNOVA THEORY WITH OBSERVATIONS. I. SHOCK REVIVAL IN A 15<i>M</i><sub>☉</sub>BLUE SUPERGIANT PROGENITOR WITH SN 1987A ENERGETICS
resolves10.1086/304253<i>Hubble Space Telescope</i>Spectrum of SN 1987A at an Age of 8 Years: Radioactive Luminescence of Cool Gas
resolves10.1086/341728Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
resolves10.1086/323946Nucleosynthesis of Zinc and Iron Peak Elements in Population III Type II Supernovae: Comparison with Abundances of Very Metal Poor Halo Stars
resolves10.3847/1538-4357/aa76deImplications for Post-processing Nucleosynthesis of Core-collapse Supernova Models with Lagrangian Particles
resolves10.3847/1538-4357/aa72deProduction and Distribution of <sup>44</sup>Ti and <sup>56</sup>Ni in a Three-dimensional Supernova Model Resembling Cassiopeia A
The 7 references without a DOI — listed, not checked
no DOI — not checkedPossible detection of a neutrino signal on 23 February 1987 at the Baksan underground scintillation telescope of the Institute of nuclear research
no DOI — not checkedHydrodynamic study of supernova 1987A—near the peak luminosity
no DOI — not checkedAstrometry of SN 1987A and Sanduleak-69 202
no DOI — not checkedA common envelope model for SN 1987A
no DOI — not checkedA merger model for SN 1987 A
no DOI — not checkedBinaries at low metallicity: ranges for case A, B and C mass transfer
no DOI — not checkedNeutrino signal from proto-neutron star evolution: effects of opacities from charged current neutrino interactions and inverse neutron decay
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