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| COSMOS2015 1053990 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.05.09CEST14:57:06 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2007ApJS..172...29H 
|
15 | D | 1 | 1391 | 287 | The XMM-Newton wide-field survey in the COSMOS field. I. Survey description. | HASINGER G., CAPPELLUTI N., BRUNNER H., et al. | ||
|
2009A&A...497..635C
|
15 | D | 1 | 1896 | 242 | The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue. | CAPPELLUTI N., BRUSA M., HASINGER G., et al. | ||
|
2010ApJ...716..348B
|
15 | D | 1 | 1849 | 274 | The XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei. | BRUSA M., CIVANO F., COMASTRI A., et al. | ||
|
2011ApJ...742...61S
|
15 | D | 1 | 2652 | 210 | Dissecting photometric redshift for active galactic nucleus using XMM- and Chandra-COSMOS samples. | SALVATO M., ILBERT O., HASINGER G., et al. | ||
|
2012MNRAS.427.3103B
|
15 | D | 1 | 1737 | 196 | Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies. | BONGIORNO A., MERLONI A., BRUSA M., et al. | ||
|
2016ApJ...817...34M
|
16 | D | 1 | 4057 | 237 | The Chandra COSMOS legacy survey: optical/IR identifications. | MARCHESI S., CIVANO F., ELVIS M., et al. | ||
|
2016ApJ...819...62C
|
16 | D | 1 | 4017 | 337 | The Chandra Cosmos Legacy survey: overview and point source catalog. | CIVANO F., MARCHESI S., COMASTRI A., et al. | ||
|
2018ApJ...858...77H
|
16 | D | 1 | 7945 | 125 | The DEIMOS 10k spectroscopic survey catalog of the COSMOS field. | HASINGER G., CAPAK P., SALVATO M., et al. | ||
| 2020ApJ...889...32S | 17 | D | 1 | 101 | 53 | No significant evolution of relations between black hole mass and galaxy total stellar mass up to z ∼ 2.5. | SUH H., CIVANO F., TRAKHTENBROT B., et al. |
