E. Daddi
About
In The Last Decade
E. Daddi
234 papers receiving 12.8k citations
Hit Papers
Peers
Comparison fields: 5 of 55
- Astronomy and Astrophysics 13.0k
- Instrumentation 7.4k
- Nuclear and High Energy Physics 1.4k
- Statistical and Nonlinear Physics 354
- Ecology 350
Countries citing papers authored by E. Daddi
This map shows the geographic impact of E. Daddi's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by E. Daddi with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. Daddi more than expected).
Fields of papers citing papers by E. Daddi
This network shows the impact of papers produced by E. Daddi. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by E. Daddi. The network helps show where E. Daddi may publish in the future.
Co-authorship network of co-authors of E. Daddi
This figure shows the co-authorship network connecting the top 25 collaborators of E. Daddi. A scholar is included among the top collaborators of E. Daddi based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with E. Daddi. E. Daddi is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 12 | |
| 2 | 1 | |
| 3 | 2 | |
| 4 | 13 | |
| 5 | 17 | |
| 6 | The Evolving Interstellar Medium of Star-forming Galaxies, as Traced by Stardust* | 28 |
| 7 | The infrared-radio correlation of star-forming galaxies is strongly M?-dependent but nearly redshift-invariant since z ~ 4 | 7 |
| 8 | 20 | |
| 9 | 12 | |
| 10 | Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z~2 | 4 |
| 11 | 25 | |
| 12 | 10 | |
| 13 | 34 | |
| 14 | The galaxy’s gas content regulated by the dark matter halo mass results in a superlinear M BH–M ⋆ Relation | 11 |
| 15 | COLDz: shape of the CO luminosity function at high redshift sand the cold gas history of the universe | 32 |
| 16 | 31 | |
| 17 | 31 | |
| 18 | 20 | |
| 19 | The morphologies of massive galaxies from z ~ 3-witnessing the two channels of bulge growth | 49 |
| 20 | 14 |
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.