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| SN 2018hpq , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST22:24:17 |
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trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2020ApJ...895...32F 
|
16 | D | 1 | 1494 | 104 | The Zwicky Transient Facility Bright Transient Survey. I. Spectroscopic classification and the redshift completeness of local galaxy catalogs. | FREMLING C., MILLER A.A., SHARMA Y., et al. | ||
|
2023ApJ...943...41C
|
17 | D | 1 | 104 | 17 | The Hydrogen-poor Superluminous Supernovae from the Zwicky Transient Facility Phase I Survey. I. Light Curves and Measurements. | CHEN Z.H., YAN L., KANGAS T., et al. | ||
|
2023ApJ...943...42C
|
17 | D | 1 | 88 | 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. | ||
| 2023A&A...672A.111P | 17 | D | 1 | 106 | 1 | Supernova search with active learning in ZTF DR3. | PRUZHINSKAYA M.V., ISHIDA E.E.O., NOVINSKAYA A.K., et al. | ||
| 2023MNRAS.524.3559C | 17 | D | 1 | 56 | ~ | Metallicity beats sSFR: the connection between superluminous supernova host galaxy environments and the importance of metallicity for their production. | CLELAND C., McGEE S.L. and NICHOLL M. | ||
| 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. | ||
| 2024MNRAS.535..471G | 287 | D | S X | 6 | 274 | ~ | The Type I superluminous supernova catalogue I: light-curve properties, models, and catalogue description. | GOMEZ S., NICHOLL M., BERGER E., et al. | |
| 2025ApJ...980..219K | 19 | D | 1 | 137 | ~ | The Bolometric Light-curve Modeling of 98 Type I Superluminous Supernovae Using the Magnetar- and the Circumstellar Interaction Models Reveals Surprisingly High Ejecta Masses. | KONYVES-TOTH R. |
