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| [LFR2003] 317 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST15:27:18 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2000A&A...353...92R | 15 | 11 | Interaction rate at z∼1. | RESHETNIKOV V.P. | |||||
2000AJ....120.2747C 
|
2658 | 246 | WFPC2 observations of the Hubble Deep Field South. | CASERTANO S., DE MELLO D.F., DICKINSON M., et al. | |||||
|
2000ApJ...538..493Y
|
1617 | 44 | Photometry and photometric redshifts of faint galaxies in the Hubble Deep Field South NICMOS field. | YAHATA N., LANZETTA K.M., CHEN H.-W., et al. | |||||
|
2003AJ....125.1107L
|
15 | D | 836 | 235 | Ultradeep near-infrared ISAAC observations of the Hubble Deep Field South: observations, reduction, multicolor catalog, and photometric redshifts. | LABBE I., FRANX M., RUDNICK G., et al. | |||
|
2004MNRAS.355...82T
|
15 | D | 225 | 43 | Quantitative morphological analysis of the Hubble Deep Field North and Hubble Deep Field South - I. Early- and late-type luminosity-size relations of galaxies out to z∼ 1. | TRUJILLO I. and AGUERRI J.A.L. | |||
|
2015A&A...575A..75B
|
16 | D | 1 | 589 | 177 | The MUSE 3D view of the Hubble Deep Field South. | BACON R., BRINCHMANN J., RICHARD J., et al. | ||
| 2016A&A...591A..49C | 259 | D | X C | 6 | 35 | 71 | Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to 108M. | CONTINI T., EPINAT B., BOUCHE N., et al. | |
| 2017A&A...608A...5G | 327 | X | 8 | 20 | 54 | The MUSE Hubble Ultra Deep Field Survey. V. Spatially resolved stellar kinematics of galaxies at redshift 0.2 ≤z ≤0.8. | GUEROU A., KRAJNOVIC D., EPINAT B., et al. | ||
|
2018MNRAS.478.4293C
|
16 | D | 1 | 87 | 17 | First gas-phase metallicity gradients of 0.1 <= z <= 0.8 galaxies with MUSE. | CARTON D., BRINCHMANN J., CONTINI T., et al. |
