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| SN 2017bzc , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST12:56:58 |
| 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...851L..48Y | 16 | D | 2 | 50 | 13 | An empirical limit on the kilonova rate from the DLT40 One day cadence Supernova survey. | YANG S., VALENTI S., CAPPELLARO E., et al. | ||
| 2019MNRAS.483.1114B | 934 | A | D | S X C | 22 | 25 | 4 | Narrow transient absorptions in late-time optical spectra of type Ia supernovae: evidence for large clumps of iron-rich ejecta? | BLACK C.S., FESEN R.A. and PARRENT J.T. |
|
2019MNRAS.484.1899H |
16 | D | 1 | 584 | 39 | The ASAS-SN bright supernova catalogue - IV. 2017. | HOLOIEN T.W.-S., BROWN J.S., VALLELY P.J., et al. | ||
|
2020MNRAS.491.2902F |
552 | K | D | X C | 13 | 68 | 46 | Sub-Chandrasekhar progenitors favoured for Type Ia supernovae: evidence from late-time spectroscopy. | FLORS A., SPYROMILIO J., TAUBENBERGER S., et al. |
| 2017ATel10165....1P | 119 | X | 3 | 3 | ~ | BOSS discovery of 3 probable nearby supernovae | PARKER S., MARPLES P., BOCK G., et al. | ||
| 2017ATel10240....1M | 40 | X | 1 | 17 | ~ | Spectral classification of optical transients with du Pont telescope. | MORRELL N., SHAPPEE B., DROUT M., et al. | ||
|
2022AJ....163...14B |
17 | D | 1 | 285 | ~ | Galaxian contamination in Galactic reddening maps. | BROWN P.J. and WALKER T. | ||
|
2022ApJS..259...53C |
17 | D | 1 | 291 | 15 | The First Data Release of CNIa0.02-A Complete Nearby (Redshift <0.02) Sample of Type Ia Supernova Light Curves. | CHEN P., DONG S., KOCHANEK C.S., et al. | ||
| 2022A&A...660A..96B | 178 | K | O X C | 3 | 2 | 16 | Stable nickel production in type Ia supernovae: A smoking gun for the progenitor mass? | BLONDIN S., BRAVO E., TIMMES F.X., et al. | |
|
2025A&A...698A.305M |
19 | D | 3 | 115 | ~ | Supernovae at distances <40 Mpc I. Catalogues and fractions of supernovae in a complete sample. | MA X., WANG X., MO J., et al. |