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| [DGI99] J164457+4626.0 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST06:58:08 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 1994AJ....107.1303H | 1 | 21 | 151 | Two extremely red galaxies. | HU E.M. and RIDGWAY S.E. | ||||
| 1997MNRAS.290L..43C | 2 | 2 | 22 | On the dust extinction in high-z galaxies and the case of extremely red objects. | CIMATTI A., BIANCHI S., FERRARA A., et al. | ||||
| 1998A&A...333...43F | 20 | 3 | Imaging around PC 1643+4631A at the Lyman limit. | FERRERAS I., BENITEZ N. and MARTINEZ-GONZALEZ E. | |||||
| 1999ApJ...519..610D | 4 | 14 | 174 | Observations of a z = 1.44 dusty, ultraluminous galaxy and implications for deep submillimeter surveys. | DEY A., GRAHAM J.R., IVISON R.J., et al. | ||||
| 2000A&A...364...26M | 63 | 63 | The morphology of Extremely Red Objects. | MORIONDO G., CIMATTI A. and DADDI E. | |||||
| 2000ApJ...539..570G | 9 | 2 | Infrared observations of three extremely red objects. | GLASSMAN T.M. and LARKIN J.E. | |||||
| 2002A&A...381L...1E | 1 | 6 | 29 | ISOCAM mid-infrared detection of HR10: A distant clone of Arp 220 at z = 1.44. | ELBAZ D., FLORES H., CHANIAL P., et al. | ||||
| 2002A&A...383..440M | 25 | 25 | Search for sub-mm, mm and radio continuum emission from extremely red objects. | MOHAN N.R., CIMATTI A., ROETTGERING H.J.A., et al. | |||||
| 2002MNRAS.334..262H | 9 | 6 | Deep optical imaging of the field of PC 1643+4631A&B - I. Spatial distributions and the counts of faint galaxies. | HAYNES T., COTTER G., BAKER J.C., et al. | |||||
| 2005MNRAS.360..685C | 22 | 3 | Vigorous star formation in a bulge-dominated extremely red object at z= 1.34. | COTTER G., SIMPSON C. and BOLTON R.C. | |||||
2008A&A...477...55H 
|
74 | X | 2 | 36 | 5 | EROs found behind lensing clusters. II. Empirical properties, classification, and SED modelling based on multi-wavelength observations. | HEMPEL A., SCHAERER D., EGAMI E., et al. |
