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| CANDELS EGS F160W J141914.2+525018.3 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST04:03:54 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2014ApJS..214...24S 
|
15 | D | 1 | 97940 | 733 | 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses. | SKELTON R.E., WHITAKER K.E., MOMCHEVA I.G., et al. | ||
|
2017ApJS..229...32S
|
16 | D | 1 | 37883 | 113 | CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS Extended Groth Strip. | STEFANON M., YAN H., MOBASHER B., et al. | ||
| 2022ApJ...927..170T | 491 | D | X C | 11 | 12 | 76 | On the Stellar Populations of Galaxies at z = 9-11: The Growth of Metals and Stellar Mass at Early Times. | TACCHELLA S., FINKELSTEIN S.L., BAGLEY M., et al. | |
| 2022ApJ...928...52F | 232 | D | X | 6 | 32 | 68 | A Census of the Bright z = 8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields. | FINKELSTEIN S.L., BAGLEY M., SONG M., et al. | |
| 2022ApJ...930..104L | 128 | X C | 2 | 32 | 30 | Searching for Islands of Reionization: A Potential Ionized Bubble Powered by a Spectroscopic Overdensity at z = 8.7. | LARSON R.L., FINKELSTEIN S.L., HUTCHISON T.A., et al. | ||
| 2022MNRAS.517.5104C | 51 | X | 1 | 4 | 34 | The far-ultraviolet continuum slope as a Lyman Continuum escape estimator at high redshift. | CHISHOLM J., SALDANA-LOPEZ A., FLURY S., et al. | ||
| 2023ApJ...946L..13F | 177 | X C | 3 | 38 | 132 | CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST. | FINKELSTEIN S.L., BAGLEY M.B., FERGUSON H.C., et al. | ||
| 2024MNRAS.529..855W | 134 | X | 3 | 53 | ~ | Insight from JWST/Near Infrared Camera into galaxy overdensities around bright Lyman-alpha emitters during reionization: implications for ionized bubbles at z ∼ 9. | WHITLER L., STARK D.P., ENDSLEY R., et al. |
