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| BoRG 0440-5244 682 , the SIMBAD biblio (7 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST04:10:53 |
Sort references on where and how often the object is cited
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2012ApJ...760..108B | 16 | D | 1 | 40 | 154 | The Brightest of Reionizing Galaxies survey: constraints on the bright end of the z ∼ 8 luminosity function. | BRADLEY L.D., TRENTI M., OESCH P.A., et al. | ||
2013MNRAS.432.2696M 
|
15 | D | 1 | 209 | 345 | A new multifield determination of the galaxy luminosity function at z = 7-9 incorporating the 2012 Hubble ultra-deep field imaging. | McLURE R.J., DUNLOP J.S., BOWLER R.A.A., 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. | ||
| 2015MNRAS.453.3068B | 484 | D | X C F | 11 | 9 | 7 | A spectroscopically confirmed z = 1.327 galaxy-scale deflector magnifying a z ∼ 8 Lyman-break galaxy in the Brightest of Reionizing Galaxies survey. | BARONE-NUGENT R.L., SONNENFELD A., WYITHE J.S.B., et al. | |
| 2016ApJ...823..143R | 19 | D | 1 | 32 | 204 | z ≳ 7 galaxies with red Spitzer/IRAC [3.6]-[4.5] colors in the full CANDELS data set: The brightest-known galaxies at z∼ 7-9 and a probable spectroscopic confirmation at z=7.48. | ROBERTS-BORSANI G.W., BOUWENS R.J., OESCH P.A., et al. | ||
| 2022ApJ...927..236R | 60 | D | X | 2 | 75 | 30 | The Physical Properties of Luminous z >= 8 Galaxies and Implications for the Cosmic Star Formation Rate Density from ∼0.35 deg2 of (Pure-)Parallel HST Observations. | ROBERTS-BORSANI G., MORISHITA T., TREU T., et al. | |
| 2023MNRAS.524.5454L | 17 | D | 1 | 33 | ~ | The UV luminosity functions of bright z > 8 galaxies: determination from ∼0.41 deg2 of HST observations along ∼300 independent sightlines. | LEETHOCHAWALIT N., ROBERTS-BORSANI G., MORISHITA T., et al. |
