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| HSCS J021745-052842 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST13:22:49 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2005ApJ...620L...1O | 2 | 25 | 206 | The discovery of primeval large-scale structures with forming clusters at redshift 6. | OUCHI M., SHIMASAKU K., AKIYAMA M., et al. | ||||
2008ApJS..176..301O 
|
17 | D | 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. | |||
| 2017ApJ...838L..22D | 16 | D | 2 | 12 | 12 | Constraining C III] emission in a sample of five luminous z = 5.7 galaxies. | DING J., CAI Z., FAN X., et al. | ||
|
2017MNRAS.472..772M
|
16 | D | 2 | 48 | 66 | Spectroscopic properties of luminous Ly α emitters at z ~= 6-7 and comparison to the Lyman-break population. | MATTHEE J., SOBRAL D., DARVISH B., et al. | ||
| 2018NatAs...2..962J | 16 | D | 1 | 47 | 40 | A giant protocluster of galaxies at redshift 5.7. | JIANG L., WU J., BIAN F., et al. | ||
| 2019A&A...623A.157S | 2 | 27 | 57 | Predicting Lyα escape fractions with a simple observable. Lyα in emission as an empirically calibrated star formation rate indicator. | SOBRAL D. and MATTHEE J. | ||||
| 2019ApJ...883..142H | 16 | D | 1 | 89 | 67 | SILVERRUSH. VIII. Spectroscopic identifications of early large-scale structures with protoclusters over 200 Mpc at z ∼ 6-7: strong associations of dusty star-forming galaxies. | HARIKANE Y., OUCHI M., ONO Y., et al. | ||
|
2020ApJ...903....4N
|
16 | D | 1 | 265 | ~ | The Magellan M2FS spectroscopic survey of high-redshift galaxies: a sample of 260 Lyα emitters at redshift z ≃ 5.7. | NING Y., JIANG L., ZHENG Z.-Y., et al. | ||
|
2021ApJ...911...78O
|
17 | D | 1 | 181 | 17 | SILVERRUSH X: machine learning-aided selection of 9318 LAEs at z = 2.2, 3.3, 4.9, 5.7, 6.6, and 7.0 from the HSC SSP and CHORUS survey data. | ONO Y., ITOH R., SHIBUYA T., et al. |
