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| SN 2019ofm , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST17:09:33 |
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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...905...58D 
|
1457 | D | S X C | 34 | 68 | 64 | The Zwicky Transient Facility Census of the Local Universe. I. Systematic search for calcium-rich gap transients reveals three related spectroscopic subclasses. | DE K., KASLIWAL M.M., TZANIDAKIS A., et al. | |
|
2022MNRAS.509.5275S
|
43 | X | 1 | 544 | 8 | The ZTF-BTS Type Ia supernovae luminosity function is consistent with a single progenitor channel for the explosions. | SHARON A. and KUSHNIR D. | ||
| 2022ApJ...925L..12K | 46 | X | 1 | 6 | 19 | Discovery of a Double-detonation Thermonuclear Supernova Progenitor. | KUPFER T., BAUER E.B., VAN ROESTEL J., et al. | ||
| 2023ApJ...946...83L | 348 | X C | 7 | 23 | 4 | SN 2020jgb: A Peculiar Type Ia Supernova Triggered by a Helium-shell Detonation in a Star-forming Galaxy. | LIU C., MILLER A.A., POLIN A., et al. | ||
| 2023ApJ...958..178L | 44 | X | 1 | 19 | ~ | SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation. | LIU C., MILLER A.A., BOOS S.J., et al. | ||
| 2024ApJ...972..194Y | 18 | D | 3 | 53 | ~ | SN 2022oqm: A Bright and Multipeaked Calcium-rich Transient. | YADAVALLI S.K., VILLAR V.A., IZZO L., et al. | ||
| 2024RAA....24i5009H | 45 | X | 1 | 24 | ~ | The Energy Sources and the Explosion Mechanism of Ca-rich Supernova PTF 10iuv. | HUANG Q.-P., WANG S.-Q., WANG T., et al. | ||
| 2025MNRAS.537.1015T | 93 | F | 1 | 19 | ~ | SN 2023xwi: forbidden line emission in the peak spectrum of a Ca-strong transient. | TOUCHARD-PAXTON C.-G., FROHMAIER C., PURSIAINEN M., et al. | ||
| 2025PASP..137k4207S | 19 | D | 2 | 19 | ~ | Characterizing the Host Galaxies and Delay Times of Ca-rich Gap Transients versus 91bg-like SNe and Normal Type Ia SNe. | SCHERBAK P., POLIN A., KASLIWAL M., et al. |
