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| [MII2017] LAE02 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:33:50 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2004AJ....128..569M | 2 | 39 | 299 | A SUBARU search for Lyα blobs in and around the protocluster region at redshift z = 3.1. | MATSUDA Y., YAMADA T., HAYASHINO T., et al. | ||||
| 2005MNRAS.363.1398G | 47 | 79 | A submillimetre survey of Lyman α haloes in the SA22 protocluster at z= 3.1. | GEACH J.E., MATSUDA Y., SMAIL I., et al. | |||||
| 2009ApJ...692.1561W | 15 | D | 1 | 50 | 27 | Spitzer observations of extended Lyman-α clouds in the SSA22 field. | WEBB T.M.A., YAMADA T., HUANG J.-S., et al. | ||
| 2009ApJ...693.1579Y | 76 | C | 1 | 22 | 87 | Extended Lyα nebulae at z ≃ 2.3: an extremely rare and strongly clustered population? | YANG Y., ZABLUDOFF A., TREMONTI C., et al. | ||
| 2009ApJ...700....1G | 38 | X | 1 | 38 | 106 | The Chandra deep protocluster survey: Lyα blobs are powered by heating, not cooling. | GEACH J.E., ALEXANDER D.M., LEHMER B.D., et al. | ||
| 2011ApJ...728...59C | 15 | D | 1 | 23 | 26 | Polycyclic aromatic hydrocarbon emission within Lyα blobs. | COLBERT J.W., SCARLATA C., TEPLITZ H., et al. | ||
| 2013MNRAS.430.2768T | 15 | D | 1 | 44 | 15 | Obscured star formation in Lyα blobs at z = 3.1. | TAMURA Y., MATSUDA Y., IKARASHI S., et al. | ||
| 2016MNRAS.460.4075H | 16 | D | 2 | 38 | 9 | The average submillimetre properties of Lyman α blobs at z = 3. | HINE N.K., GEACH J.E., MATSUDA Y., et al. | ||
2017MNRAS.465..316M 
|
294 | D | X C | 7 | 34 | 17 | Searching for candidates of Lyman continuum sources - revisiting the SSA22 field. | MICHEVA G., IWATA I., INOUE A.K., et al. | |
| 2017ApJ...850..178A | 16 | D | 1 | 45 | 7 | Deep submillimeter and radio observations in the SSA22 field. I. Powering sources and the Lyα escape fraction of Lyα blobs. | AO Y., MATSUDA Y., HENKEL C., et al. |
