H. Bushouse
About
In The Last Decade
H. Bushouse
63 papers receiving 1.0k citations
Peers
Comparison fields: 5 of 42
- Astronomy and Astrophysics 982
- Instrumentation 364
- Nuclear and High Energy Physics 157
- Electrical and Electronic Engineering 80
- Atomic and Molecular Physics, and Optics 78
Countries citing papers authored by H. Bushouse
This map shows the geographic impact of H. Bushouse'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 H. Bushouse with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites H. Bushouse more than expected).
Fields of papers citing papers by H. Bushouse
This network shows the impact of papers produced by H. Bushouse. 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 H. Bushouse. The network helps show where H. Bushouse may publish in the future.
Co-authorship network of co-authors of H. Bushouse
This figure shows the co-authorship network connecting the top 25 collaborators of H. Bushouse. A scholar is included among the top collaborators of H. Bushouse 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 H. Bushouse. H. Bushouse is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Title | Journal | Authors | Indexed citations |
|---|---|---|---|---|
| 1 | Multiwavelength Observations of Sgr A*. II. 2019 July 21 and 26 | The Astrophysical Journal | Joseph M. Michail, F. Yusef‐Zadeh et al. | 3 |
| 2 | The JWST Calibration Pipeline | AAS | Christine Chen, James Muzerolle et al. | 5 |
| 3 | WFC3/UVIS Charge Injection Behavior: Results of an Initial Test | H. Bushouse, S. Baggett et al. | 2 | |
| 4 | IR Detector Timing and Persistence | Knox S. Long, Thomas Wheeler et al. | 1 | |
| 5 | WFC3/IR Bad Pixel Table: Update Using Cycle 17 Data | B. Hilbert, H. Bushouse | 2 | |
| 6 | WFC3: UVIS and IR Flat Fields | Cheryl Pavlovsky, S. Baggett et al. | 1 | |
| 7 | The ground calibrations of the WFC3/UVIS G280 grism | H. Kuntschner, H. Bushouse et al. | 1 | |
| 8 | WFC3 Calibration Using Galactic Clusters | Elena Sabbi, Jason S. Kalirai et al. | 1 | |
| 9 | Calibrating the WFC3 Grisms | H. Kuntschner, H. Bushouse et al. | 2 | |
| 10 | WFC3 SMOV proposal 11552: Calibration of the G102 grism | H. Kuntschner, H. Bushouse et al. | 8 | |
| 11 | WFC3 SMOV Proposal 11445 - IR Geometric Distortion Calibration | V. Kozhurina-Platais, Colin Cox et al. | 1 | |
| 12 | WFC3 TV3 Testing: IR Science Monitor | H. Bushouse | 1 | |
| 13 | CSM Mapping of the UVIS Field-of-View | H. Bushouse, Jason S. Kalirai | 1 | |
| 14 | The WFC3/UVIS Reference Files : 2. Biases and Darks | A. R. Martel, S. Baggett et al. | 1 | |
| 15 | The TV2 ground calibrations of the WFC3 NIR grisms | H. Kuntschner, H. Bushouse et al. | 1 | |
| 16 | WFC3 UVIS Ground P-flats | Elena Sabbi, A. R. Martel et al. | 4 | |
| 17 | WFC3 IR Ground P-Flats | H. Bushouse | 4 | |
| 18 | WFC3 Thermal Vacuum Testing: IR Science Performance Monitor | H. Bushouse, O. L. Lupie | 4 | |
| 19 | WFC3 UVIS CCD Image Overscan Region Layouts | H. Bushouse | 1 | |
| 20 | News on the ISOPHOT Interactive Analysis PIA | ASPC | R. Albrecht, R. N. Hook et al. | 0 |
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.