T. G. Phillips
About
In The Last Decade
T. G. Phillips
218 papers receiving 6.6k citations
Hit Papers
Peers
Comparison fields: 5 of 119
- Astronomy and Astrophysics 5.4k
- Spectroscopy 2.4k
- Atmospheric Science 1.6k
- Atomic and Molecular Physics, and Optics 1.5k
- Electrical and Electronic Engineering 805
Countries citing papers authored by T. G. Phillips
This map shows the geographic impact of T. G. Phillips'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 T. G. Phillips with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. G. Phillips more than expected).
Fields of papers citing papers by T. G. Phillips
This network shows the impact of papers produced by T. G. Phillips. 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 T. G. Phillips. The network helps show where T. G. Phillips may publish in the future.
Co-authorship network of co-authors of T. G. Phillips
This figure shows the co-authorship network connecting the top 25 collaborators of T. G. Phillips. A scholar is included among the top collaborators of T. G. Phillips 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 T. G. Phillips. T. G. Phillips is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 12 | |
| 3 | Development of the 2nd Generation Redshift(z) and Early Universe Spectrometer and the Detailed Study of Far-IR Fine-Structure Lines in High-z Galaxies | 1 |
| 4 | First detections of the [NII] 122 {\mu}m line at z>0.04: Demonstrating the utility of the line for studying galaxies at high redshift | 1 |
| 5 | 32 | |
| 6 | 28 | |
| 7 | SHARC II, a Second Generation 350 Micron Camera for the Caltech Submillimeter Observatory | 1 |
| 8 | The FIRST Mission | 2 |
| 9 | New molecular species in comet C/1995 O1 (Hale-Bopp) observed with the Caltech Submillimeter Observatory | 6 |
| 10 | A Submillimeter/Far-IR Heterodyne Receiver for SOFIA | 3 |
| 11 | Recent Results from the Caltech Submillimeter Observatory | 1 |
| 12 | An 850 GHz Waveguide Receiver Using a Tuned Nb SIS Tunnel Junction Fabricated on a 1μm Si 3 N 4 Membrane | 2 |
| 13 | A 665 GHz Waveguide Receiver Using a Tuned 0.5 μm 2 Nb/AlO x /Nb SIS Tunnel Junction | 1 |
| 14 | 40 | |
| 15 | Josephson-Effect Mixers using Shunted Nb and NbN Tunnel Junctions | 1 |
| 16 | The Starburst Properties of M82, M83, and IC342 | 2 |
| 17 | The Caltech Submillimeter Observatory | 1 |
| 18 | 1 | |
| 19 | Rotational Excitation of Molecules by Electrons in Interstellar Clouds. | 1 |
| 20 | Search for Interstellar HDO | 1 |
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.