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| ASASSN -14lt , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:46:28 |
| 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.6802....1K | 116 | X | 3 | 2 | 1 | ASAS-SN Discovery of A Probable Supernova in IC 0299. | KIYOTA S., HOLOIEN T.W.-S., STANEK K.Z., et al. | ||
| 2014ATel.6804....1B | 155 | T | X | 3 | 4 | ~ |
Asiago spectroscopic classification of ASASSN-14lt and PSN J09525558+4250511. |
BENETTI S., OCHNER P., TOMASELLA L., et al. | |
| 2014ATel.6813....1Z | 116 | T | X | 2 | 3 | 1 |
Spectroscopic Confirmation of ASASSN-14lt as a Type Ia Supernova. |
ZHANG J. | |
|
2017MNRAS.464.2672H |
16 | D | 1 | 171 | 29 | The ASAS-SN bright supernova catalogue - I. 2013-2014. | HOLOIEN T.W.-S., STANEK K.Z., KOCHANEK C.S., et al. | ||
| 2019PASP..131a4001P | 16 | D | 1 | 416 | 58 | Carnegie Supernova Project-II: extending the near-infrared Hubble diagram for Type Ia supernovae to z ∼ 0.1. | PHILLIPS M.M., CONTRERAS C., HSIAO E.Y., et al. | ||
|
2019MNRAS.484.3785B |
16 | D | 1 | 918 | 27 | The relative specific Type Ia supernovae rate from three years of ASAS-SN. | BROWN J.S., STANEK K.Z., HOLOIEN T.W.-S., et al. | ||
|
2020MNRAS.493.1044T |
16 | D | 1 | 116 | 49 | Nebular spectra of 111 Type Ia supernovae disfavour single-degenerate progenitors. | TUCKER M.A., SHAPPEE B.J., VALLELY P.J., et al. | ||
| 2021MNRAS.501.3122C | 17 | D | 1 | 116 | ~ | The delay time distribution of supernovae from integral-field spectroscopy of nearby galaxies. | CASTRILLO A., ASCASIBAR Y., GALBANY L., et al. | ||
| 2024ApJ...967...20M | 18 | D | 3 | 243 | ~ | Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and II. | MORRELL N., PHILLIPS M.M., FOLATELLI G., et al. | ||
| 2024ApJ...969...80C | 242 | D | X | 6 | 317 | ~ | Type Ia Supernova Progenitor Properties and their Host Galaxies. | CHAKRABORTY S., SADLER B., HOEFLICH P., et al. |