Matthew A. Malkan
About
In The Last Decade
Matthew A. Malkan
215 papers receiving 8.9k citations
Hit Papers
Peers
Comparison fields: 5 of 67
- Astronomy and Astrophysics 9.0k
- Nuclear and High Energy Physics 2.6k
- Instrumentation 2.3k
- Atomic and Molecular Physics, and Optics 395
- Electrical and Electronic Engineering 192
Countries citing papers authored by Matthew A. Malkan
This map shows the geographic impact of Matthew A. Malkan'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 Matthew A. Malkan with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Matthew A. Malkan more than expected).
Fields of papers citing papers by Matthew A. Malkan
This network shows the impact of papers produced by Matthew A. Malkan. 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 Matthew A. Malkan. The network helps show where Matthew A. Malkan may publish in the future.
Co-authorship network of co-authors of Matthew A. Malkan
This figure shows the co-authorship network connecting the top 25 collaborators of Matthew A. Malkan. A scholar is included among the top collaborators of Matthew A. Malkan 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 Matthew A. Malkan. Matthew A. Malkan is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 6 | |
| 2 | 0 | |
| 3 | 0 | |
| 4 | 10 | |
| 5 | 3 | |
| 6 | 3 | |
| 7 | Spectroscopically Confirmed Lyα Emitters from Redshift 5 to 7 behind 10 Galaxy Cluster Lenses | 26 |
| 8 | Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies. I. Sample Overview and Clumpy Structure in Molecular Outflows on 500 pc Scales | 30 |
| 9 | The Mass Relations between Supermassive Black Holes and Their Host Galaxies at 1 < z < 2 with HST-WFC3 | 91 |
| 10 | Far-infrared dust properties of highly dust-obscured active galactic nuclei from the AKARI and WISE all-sky surveys | 3 |
| 11 | Spatially Resolved Spectroscopic Study of nearby Seyfert Galaxies: Implications for a Population of “Missed” Seyferts at High-z | 4 |
| 12 | The Grism Lens-Amplified Survey from Space (GLASS). VIII. The Influence of the Cluster Properties on Hα Emitter Galaxies at 0.3 < z < 0.7 | 6 |
| 13 | 39 | |
| 14 | THE GRISM LENS-AMPLIFIED SURVEY from SPACE (GLASS). VII. the DIVERSITY of the DISTRIBUTION of STAR FORMATION in CLUSTER and FIELD GALAXIES at 0.3 ≤ z ≤ 0.7 | 22 |
| 15 | THE METAL ABUNDANCES ACROSS COSMIC TIME ( ) SURVEY. I. OPTICAL SPECTROSCOPY IN THE SUBARU DEEP FIELD | 9 |
| 16 | BROAD Hβ EMISSION-LINE VARIABILITY IN A SAMPLE OF 102 LOCAL ACTIVE GALAXIES | 42 |
| 17 | Clustering of the AKARI NEP deep field 24iμ/im selected galaxies | 6 |
| 18 | 31 | |
| 19 | AN EMPIRICAL DETERMINATION OF THE INTERGALACTIC BACKGROUND LIGHT USING NEAR-INFRARED DEEP GALAXY SURVEY DATA OUT TO 5 μm AND THE GAMMA-RAY OPACITY OF THE UNIVERSE | 8 |
| 20 | The soft X-ray spectral shape of X-ray-weak seyfert galaxies | 9 |
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.