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| GOODS J033248.52-274517.7 , the SIMBAD biblio (7 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST20:21:35 |
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 |
|---|---|---|---|---|---|---|---|---|---|
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. | ||
|
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. | ||
|
2016ApJS..225...27M
|
16 | D | 1 | 19341 | 548 | The 3D-HST survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for ∼ 100,000 galaxies. | MOMCHEVA I.G., BRAMMER G.B., VAN DOKKUM P.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. | ||
| 2018ApJ...861....7F | 16 | D | 1 | 53 | 41 | ALMA 26 arcmin2 survey of GOODS-S at one millimeter (ASAGAO): average morphology of high-z dusty star-forming galaxies in an exponential disk (n ≃ 1). | FUJIMOTO S., OUCHI M., KOHNO K., et al. | ||
| 2021MNRAS.503.5329H | 17 | D | 1 | 46 | 5 | Integral field spectroscopy of luminous infrared main-sequence galaxies at cosmic noon. | HOGAN L., RIGOPOULOU D., MAGDIS G.E., et al. |
