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| MUSE-WIDE 156065339 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST16:06:02 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2012A&A...547A..51G | 15 | D | 1 | 115 | 62 | The size-luminosity relation at z=7 in CANDELS and its implication on reionization. | GRAZIAN A., CASTELLANO M., FONTANA A., et al. | ||
| 2013MNRAS.429..150L | 15 | D | 1 | 36 | 30 | Constraining the bright-end of the UV luminosity function for z ∼ 7-9 galaxies: results from CANDELS/GOODS-south. | LORENZONI S., BUNKER A.J., WILKINS S.M., 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. | ||
|
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. | ||
| 2018A&A...619A.147P | 16 | D | 1 | 73 | 67 | CANDELSz7: a large spectroscopic survey of CANDELS galaxies in the reionization epoch. | PENTERICCI L., VANZELLA E., CASTELLANO M., et al. | ||
|
2021A&A...654A..80S
|
17 | D | 1 | 2058 | 14 | Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4. | SCHMIDT K.B., KERUTT J., WISOTZKI L., 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. | ||
|
2022A&A...659A.183K
|
17 | D | 1 | 1923 | 13 | Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep. | KERUTT J., WISOTZKI L., VERHAMME A., et al. |
