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| LEDA 1354027 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST03:12:43 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2003A&A...412...45P 
|
15 | D | 1 | 956189 | 750 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
| 2011CBET.2931....1B | 39 | T | O X | 1 | 2 | Supernova 2011io. | BALANUTSA P. and LIPUNOV V. | ||
| 2014ApJ...784..105W | 15 | D | 1 | 163 | 17 | SweetSpot: near-infrared observations of 13 type Ia supernovae from a new NOAO survey probing the nearby smooth Hubble flow. | WEYANT A., WOOD-VASEY W.M., ALLEN L., et al. | ||
| 2011ATel.3783....1B | 114 | T | X | 2 | 2 | 1 | MASTER bright SuperNova in PGC 1354027. | BALANUTSA P., LIPUNOV V., TYURINA N., et al. | |
|
2020AJ....159..167L
|
16 | D | 1 | 640 | 53 | The AMUSING++ nearby galaxy compilation. I. Full sample characterization and galactic-scale outflow selection. | LOPEZ-COBA C., SANCHEZ S.F., ANDERSON J.P., et al. | ||
|
2020MNRAS.498.4790K
|
16 | D | 1 | 2220 | 47 | A census of ultraluminous X-ray sources in the local Universe. | KOVLAKAS K., ZEZAS A., ANDREWS J.J., et al. | ||
|
2021ApJ...923..197P
|
17 | D | 1 | 441 | ~ | Are Type Ia supernovae in rest-frame H brighter in more massive galaxies? | PONDER K.A., WOOD-VASEY W.M., WEYANT A., et al. | ||
|
2022ApJ...925..115H
|
17 | D | 1 | 420 | ~ | The Dependence of the Type Ia Supernova Host Bias on Observation or Fitting Technique. | HAND J., LIU S., GALBANY L., et al. | ||
|
2023ApJS..269....3M
|
17 | D | 1 | 356397 | ~ | Siena Galaxy Atlas 2020. | MOUSTAKAS J., LANG D., DEY A., et al. | ||
|
2025A&A...699A.366C
|
19 | D | 1 | 688 | ~ | The EDGE-CALIFA Survey: An integral field unit-based integrated molecular gas database for galaxy evolution studies in the Local Universe. | COLOMBO D., KALINOVA V., BAZZI Z., et al. |
