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| GMASS 1667 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST07:02:49 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2004ApJ...600L..93G 
|
15 | D | 1 | 7819 | 1453 | The Great Observatories Origins Deep Survey: initial results from optical and near-infrared imaging. | GIAVALISCO M., FERGUSON H.C., KOEKEMOER A.M., et al. | ||
| 2009A&A...504..331K | 15 | D | 1 | 52 | 89 | GMASS ultradeep spectroscopy of galaxies at z ∼ 2. V. Witnessing the assembly at z = 1.6 of a galaxy cluster. | KURK J., CIMATTI A., ZAMORANI G., et al. | ||
|
2011A&A...533A.119E
|
15 | D | 1 | 3965 | 926 | GOODS-Herschel: an infrared main sequence for star-forming galaxies. | ELBAZ D., DICKINSON M., HWANG H.S., et al. | ||
|
2013A&A...549A..63K
|
54 | D | X | 2 | 245 | 70 | GMASS ultradeep spectroscopy of galaxies at z ∼ 2. VII. Sample selection and spectroscopy. | KURK J., CIMATTI A., DADDI E., et al. | |
|
2014ApJS..214...24S
|
15 | D | 1 | 97940 | 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 | 67525 | 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. | ||
|
2020ApJ...905..170M
|
16 | D | 1 | 4760 | 24 | Galaxy sizes since z = 2 from the perspective of stellar mass distribution within galaxies. | MOSLEH M., HOSSEINNEJAD S., HOSSEINI-SHAHISAVANDI S.Z., et al. |
