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| SHARDS 20008777 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST13:42:54 |
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 |
|---|---|---|---|---|---|---|---|---|---|
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. | ||
|
2015ApJ...803...34B
|
16 | D | 1 | 10313 | 1045 | UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields. | BOUWENS R.J., ILLINGWORTH G.D., OESCH P.A., et al. | ||
|
2018ApJS..237...12O
|
16 | D | 1 | 25243 | 42 | HDUV: the Hubble Deep UV Legacy Survey. | OESCH P.A., MONTES M., REDDY N., et al. | ||
|
2018MNRAS.478.3740A
|
16 | D | 1 | 1561 | 2 | A simultaneous search for high-z LAEs and LBGs in the SHARDS survey. | ARRABAL HARO P., RODRIGUEZ ESPINOSA J.M., MUNOZ-TUNON C., et al. | ||
|
2020MNRAS.495.1807A
|
16 | D | 1 | 1551 | ~ | Differences and similarities of stellar populations in LAEs and LBGs at z ∼ 3.4-6.8. | ARRABAL HARO P., RODRIGUEZ ESPINOSA J.M., MUNOZ-TUNON C., et al. | ||
| 2021MNRAS.502.4558C | 17 | D | 2 | 36 | 9 | Probing the existence of a rich galaxy overdensity at z = 5.2. | CALVI R., DANNERBAUER H., ARRABAL HARO P., et al. | ||
|
2021ApJS..257...68S
|
17 | D | 1 | 9083 | 17 | The Spitzer/IRAC Legacy over the GOODS fields: full-depth 3.6, 4.5, 5.8, and 8.0 µm mosaics and photometry for >9000 galaxies at z ∼ 3.5-10 from the GOODS Reionization Era wide-Area Treasury from Spitzer (GREATS). | STEFANON M., LABBE I., OESCH P.A., et al. | ||
| 2025MNRAS.537..788H | 47 | X | 1 | 9 | ~ | Mapping dusty galaxy growth at z > 5 with FRESCO: detection of Hα in submm galaxy HDF850.1 and the surrounding overdense structures. | HERARD-DEMANCHE T., BOUWENS R.J., OESCH P.A., et al. |
