|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| EIS-DEEP CDFS-3 Ks 1 564 , the SIMBAD biblio (7 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST08:21:36 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2003AJ....126..539A 
|
960 | 736 | The Chandra Deep Field North Survey. XIII. 2 Ms point-source catalogs. | ALEXANDER D.M., BAUER F.E., BRANDT W.N., et al. | |||||
|
2006A&A...452..119O
|
3542 | 8 | ESO imaging survey: infrared observations of CDF-S and HDF-S. | OLSEN L.F., MIRALLES J.-M., DA COSTA L., et al. | |||||
|
2008ApJ...680..130C
|
15 | D | 1 | 1013 | 61 | Mid-infrared properties and color selection for X-Ray-detected active galactic nuclei in the MUSYC Extended Chandra Deep Field-South. | CARDAMONE C.N., URRY C.M., DAMEN M., et al. | ||
|
2012MNRAS.425.2116C
|
15 | D | 3 | 7382 | 55 | The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS spectroscopic survey of the Chandra Deep Field-South. | COOPER M.C., YAN R., DICKINSON M., et al. | ||
|
2014ApJS..214...24S
|
16 | D | 1 | 66903 | 733 | 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses. | SKELTON R.E., WHITAKER K.E., MOMCHEVA I.G., et al. | ||
|
2016ApJ...830...51S
|
16 | D | 1 | 67524 | 168 | The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. | STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al. | ||
|
2018MNRAS.475.5133R
|
16 | D | 1 | 11242 | 2 | Testing the hierarchical assembly of massive galaxies using accurate merger rates out to z ∼ 1.5. | RODRIGUES M., PUECH M., FLORES H., et al. |
