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| GOODS-MUSIC 16883 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST01:41:34 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2011AJ....141...14S 
|
15 | D | 2 | 51 | 28 | Hubble Space Telescope WFC3 Early Release Science: emission-line galaxies from infrared grism observations. | STRAUGHN A.N., KUNTSCHNER H., KUMMEL M., et al. | ||
|
2011ApJ...743..146C
|
15 | D | 1 | 4132 | 61 | Active and passive galaxies at z ∼ 2: rest-frame optical morphologies with WFC3. | CAMERON E., CAROLLO C.M., OESCH P.A., et al. | ||
| 2012AJ....144...28X | 15 | D | 2 | 15 | 25 | Metallicities of emission-line galaxies from HST ACS PEARS and HST WFC3 ERS grism spectroscopy at 0.6 < z < 2.4. | XIA L., MALHOTRA S., RHOADS J., et al. | ||
| 2014A&A...564A..19C | 16 | D | 1 | 25 | 7 | Modelling galaxy spectra at redshifts 0.2 ≤ z ≤ 2.3 by the [OII]/Hβ and [OIII]/Hβ line ratios. | CONTINI M. | ||
|
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. | ||
|
2015AJ....149..178M
|
16 | D | 1 | 1020 | 31 | A WFC3 grism emission line redshift catalog in the GOODS-South field. | MORRIS A.M., KOCEVSKI D.D., TRUMP J.R., 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. |
