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| 2dFGRS TGN327Z157 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST14:42:06 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2003MNRAS.344..307L 
|
63299 | 194 | The Millennium Galaxy Catalogue: 16 ≤BMGC< 24 galaxy counts and the calibration of the local galaxy luminosity function. | LISKE J., LEMON D.J., DRIVER S.P., et al. | |||||
|
2011MNRAS.416..727C
|
15 | D | 1 | 3386 | 57 | The Padova–Millennium galaxy and group catalogue (PM2GC): the group-finding method and the PM2GC catalogues of group, binary and single field galaxies. | CALVI R., POGGIANTI B.M. and VULCANI B. | ||
|
2013MNRAS.432.3141C
|
15 | D | 1 | 3210 | 26 | The impact of global environment on galaxy mass functions at low redshift. | CALVI R., POGGIANTI B.M., VULCANI B., et al. | ||
|
2016AJ....151...78P
|
428 | 135 | Jellyfish galaxy candidates at low redshift. | POGGIANTI B.M., FASANO G., OMIZZOLO A., et al. | |||||
|
2019MNRAS.482..881P
|
16 | D | 1 | 1808 | 10 | The strong correlation between post-starburst fraction and environment. | PACCAGNELLA A., VULCANI B., POGGIANTI B.M., et al. | ||
|
2020AJ....159..167L
|
16 | D | 1 | 640 | 53 | The AMUSING++ nearby galaxy compilation. I. Full sample characterization and galactic-scale outflow selection. | LOPEZ-COBA C., SANCHEZ S.F., ANDERSON J.P., et al. | ||
| 2021ApJ...914...27V | 268 | D | X C | 6 | 42 | 16 | GASP. XXXIII. The ability of Spatially resolved data to distinguish among the different physical mechanisms affecting galaxies in low-density environments. | VULCANI B., POGGIANTI B.M., MORETTI A., et al. | |
|
2021ApJ...923...28F
|
17 | D | 1 | 85 | 10 | GASP and MaNGA surveys shed light on the enigma of the gas metallicity gradients in disk galaxies. | FRANCHETTO A., MINGOZZI M., POGGIANTI B.M., et al. | ||
| 2026ApJ..1000..110S | 50 | X | 1 | 118 | ~ | Selecting Post-starburst Galaxies Based on Star Formation History. | STARECHESKI S., FRENCH K.D., VILLANUEVA V., et al. |
