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| PUDG R15 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST20:14:18 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2020ApJ...890..105H | 16 | D | 1 | 57 | 15 | The PIPER survey. I. An initial look at the intergalactic globular cluster population in the Perseus cluster. | HARRIS W.E., BROWN R.A., DURRELL P.R., et al. | ||
| 2022MNRAS.510..946G | 17 | D | 1 | 16 | 11 | Ultra-diffuse galaxies in the perseus cluster: comparing galaxy properties with globular cluster system richness. | GANNON J.S., FORBES D.A., ROMANOWSKY A.J., et al. | ||
| 2023MNRAS.518.3653G | 104 | D | S | 2 | 32 | 2 | Keck spectroscopy of the coma cluster ultra-diffuse galaxy Y358: dynamical mass in a wider context. | GANNON J.S., FORBES D.A., BRODIE J.P., et al. | |
| 2023MNRAS.526.4735F | 409 | D | X F | 9 | 35 | ~ | The star formation histories of quiescent ultra-diffuse galaxies and their dependence on environment and globular cluster richness. | FERRE-MATEU A., GANNON J.S., FORBES D.A., et al. | |
| 2024MNRAS.529.4914P | 179 | X C | 3 | 19 | ~ | Origin of the correlation between stellar kinematics and globular cluster system richness in ultradiffuse galaxies. | PFEFFER J., JANSSENS S.R., BUZZO M.L., et al. | ||
| 2024MNRAS.531.1856G | 18 | D | 1 | 46 | ~ | A Catalogue and analysis of ultra-diffuse galaxy spectroscopic properties. | GANNON J.S., FERRE-MATEU A., FORBES D.A., et al. | ||
| 2025MNRAS.536.1217F | 65 | D | X | 2 | 25 | ~ | Why do some ultra diffuse Galaxies have rich globular cluster systems? | FORBES D.A., BUZZO M.L., FERRE-MATEU A., et al. | |
| 2025ApJ...984..147L | 19 | D | 1 | 48 | ~ | Discovery of Two Ultra-diffuse Galaxies with Unusually Bright Globular Cluster Luminosity Functions via a Mark-dependently Thinned Point Process (MATHPOP). | LI D., EADIE G.M., BROWN P.E., et al. | ||
| 2025MNRAS.544.3094G | 19 | D | 1 | 24 | ~ | Ultra-diffuse, ultra-different: observed versus simulated ultra-diffuse galaxies live in fundamentally different haloes. | GANNON J.S., DI CINTIO A., FORBES D.A., et al. |