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| NAME SXDF-E , the SIMBAD biblio (6 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:42:18 |
Sort references on where and how often the object is cited
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2008ApJ...676..163M | 14 | 20 | The Subaru/XMM-Newton Deep Survey (SXDS). V. Optically faint variable object survey. | MOROKUMA T., DOI M., YASUDA N., et al. | |||||
2008ApJS..176..301O 
|
2 | 96 | 529 | The Subaru/XMM-Newton deep survey (SXDS). IV. Evolution of Lyα emitters from z=3.1 to 5.7 in the 1 deg2 field: luminosity functions and AGN. | OUCHI M., SHIMASAKU K., AKIYAMA M., et al. | ||||
|
2010PASJ...62...91R
|
354 | D | X F | 9 | 72 | 0 | Proper motions with Subaru II. A sample in the Subaru/XMM-Newton Deep Survey Field. | RICHMOND M.W., MOROKUMA T., DOI M., et al. | |
| 2014PASJ...66...49O | 789 | D | X C | 20 | 63 | 7 | The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey. | OKUMURA J.E., IHARA Y., DOI M., et al. | |
| 2016ApJ...823...20K | 333 | D | X C | 8 | 12 | 92 | Bright and faint ends of Lyα luminosity functions at z = 2 determined by the Subaru survey: implications for AGNs, magnification bias, and ISM H I evolution. | KONNO A., OUCHI M., NAKAJIMA K., et al. | |
| 2023ApJ...958..187L | 87 | X | 2 | 7 | ~ | A Spectroscopic Survey of Lyα Emitters and Lyα Luminosity Function at Redshifts 3.7 and 4.8. | LIU W. and JIANG L. |
