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| SA 22- , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST17:29:19 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1989PAZh...15..462B | 17 | 2 | UBVR-magnitudes of high luminosity stars in Kapteyn selected areas. | BERDNIKOV L.N. and PAVLOVSKAYA E.D. | |||||
| 1991PAZh...17..505B | 24 | 0 | The study of interstellar absorption in the galactic longitude range 65-165. | BERDNIKOV L.N. and PAVLOVSKAJA E.D. | |||||
| 2004ApJ...611..725B | 11 | 8 | 268 | Clustering of submillimeter-selected galaxies. | BLAIN A.W., CHAPMAN S.C., SMAIL I., et al. | ||||
2004ApJ...616...71S 
|
95 | 168 | The rest-frame optical properties of SCUBA galaxies. | SMAIL I., CHAPMAN S.C., BLAIN A.W., et al. | |||||
| 2014MNRAS.443.2695S | 117 | X | 3 | 30 | 89 | A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS. | STOTT J.P., SOBRAL D., SWINBANK A.M., et al. | ||
| 2015ApJ...806..189K | 351 | X C | 8 | 6 | 7 | Linking galaxies to dark matter halos at z ∼ 1 : dependence of galaxy clustering on stellar mass and specific star formation rate. | KIM J.-W., IM M., LEE S.-K., et al. | ||
| 2015ApJ...813L..35K | 297 | A | X C | 7 | 8 | 21 | Discovery of a faint quasar at z ∼ 6 and implications for cosmic reionization. | KIM Y., IM M., JEON Y., et al. | |
| 2019MNRAS.487.4856M | 42 | X | 1 | 12 | 23 | The kiloparsec-scale gas kinematics in two star-forming galaxies at z ∼ 1.47 seen with ALMA and VLT-SINFONI. | MOLINA J., IBAR E., SMAIL I., et al. | ||
| 2022ApJ...926..230N | 43 | X | 1 | 42 | 8 | The Magellan M2FS Spectroscopic Survey of High-z Galaxies: Lyα Emitters at z ≃ 6.6 and the Evolution of Lyα Luminosity Function over z ≃ 5.7-6.6. | NING Y., JIANG L., ZHENG Z.-Y., et al. | ||
| 2024MNRAS.529.2290S | 45 | X | 1 | 19 | ~ | Obscured star formation in clusters at z = 1.6-2.0: massive galaxy formation and the reversal of the star formation-density relation. | SMAIL I. |
