L. W. Neuschaefer

536 total citations
16 papers, 291 citations indexed

About

L. W. Neuschaefer is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, L. W. Neuschaefer has authored 16 papers receiving a total of 291 indexed citations (citations by other indexed papers that have themselves been cited), including 13 papers in Astronomy and Astrophysics, 11 papers in Instrumentation and 5 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in L. W. Neuschaefer's work include Astronomy and Astrophysical Research (11 papers), Galaxies: Formation, Evolution, Phenomena (10 papers) and Adaptive optics and wavefront sensing (5 papers). L. W. Neuschaefer is often cited by papers focused on Astronomy and Astrophysical Research (11 papers), Galaxies: Formation, Evolution, Phenomena (10 papers) and Adaptive optics and wavefront sensing (5 papers). L. W. Neuschaefer collaborates with scholars based in United States, Germany and United Kingdom. L. W. Neuschaefer's co-authors include Rogier A. Windhorst, K. U. Ratnatunga, R. E. Griffiths, Stefano Casertano, Myungshin Im, David C. Koo, J. P. Huchra, Karl Glazebrook, Keith Matthews and P. D. Barthel and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

L. W. Neuschaefer

16 papers receiving 285 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
L. W. Neuschaefer United States 11 270 155 36 21 21 16 291
N. Scoville United States 2 309 1.1× 184 1.2× 34 0.9× 29 1.4× 25 1.2× 3 327
A. P. Oates United Kingdom 6 338 1.3× 145 0.9× 44 1.2× 30 1.4× 14 0.7× 12 363
S. K. Okumura Japan 8 401 1.5× 122 0.8× 37 1.0× 24 1.1× 10 0.5× 19 429
M. G. M. Cawson United States 6 378 1.4× 223 1.4× 22 0.6× 21 1.0× 9 0.4× 12 387
M. D. Gladders United States 9 346 1.3× 169 1.1× 67 1.9× 32 1.5× 15 0.7× 20 365
Thomas J. Broadhurst United States 7 352 1.3× 214 1.4× 38 1.1× 27 1.3× 10 0.5× 9 366
V. Le Brun France 10 423 1.6× 204 1.3× 61 1.7× 31 1.5× 21 1.0× 18 434
C. Rité Germany 11 518 1.9× 281 1.8× 72 2.0× 27 1.3× 11 0.5× 16 524
O. Le Fèvre France 3 419 1.6× 252 1.6× 36 1.0× 32 1.5× 26 1.2× 4 439
M. Kümmel Germany 8 208 0.8× 128 0.8× 29 0.8× 19 0.9× 13 0.6× 20 222

Countries citing papers authored by L. W. Neuschaefer

Since Specialization
Citations

This map shows the geographic impact of L. W. Neuschaefer'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 L. W. Neuschaefer with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites L. W. Neuschaefer more than expected).

Fields of papers citing papers by L. W. Neuschaefer

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by L. W. Neuschaefer. 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 L. W. Neuschaefer. The network helps show where L. W. Neuschaefer may publish in the future.

Co-authorship network of co-authors of L. W. Neuschaefer

This figure shows the co-authorship network connecting the top 25 collaborators of L. W. Neuschaefer. A scholar is included among the top collaborators of L. W. Neuschaefer 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 L. W. Neuschaefer. L. W. Neuschaefer is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

16 of 16 papers shown
1.
Tyson, J. A., Philippe Fischer, Puragra Guhathakurta, et al.. (1998). Deep Optical Imaging of the Bright Seyfert Galaxy NGC 5548: A Long, Very Low Surface Brightness Tail. The Astronomical Journal. 116(1). 102–110. 16 indexed citations
2.
Griffiths, R. E., K. U. Ratnatunga, Stefano Casertano, et al.. (1997). The HST medium deep survey: Progress towards resolution of the faint blue galaxy problem. 36. 355–361. 1 indexed citations
3.
Neuschaefer, L. W., Myungshin Im, K. U. Ratnatunga, R. E. Griffiths, & Stefano Casertano. (1997). Evidence for Galaxy Interactions/Mergers from Medium Deep Survey WFPC2 Data. The Astrophysical Journal. 480(1). 59–71. 31 indexed citations
4.
Roche, N., K. U. Ratnatunga, R. E. Griffiths, Myungshin Im, & L. W. Neuschaefer. (1996). Angular sizes and luminosity evolution of faint galaxies. Monthly Notices of the Royal Astronomical Society. 282(4). 1247–1273. 14 indexed citations
5.
Neuschaefer, L. W. & Rogier A. Windhorst. (1995). The angular two-point correlation function of galaxies down to B[SUB]J[/SUB] less than or approximately = 26 magnitudes on less than or approximately = 10 arcmins scales. The Astrophysical Journal. 439. 14–14. 10 indexed citations
6.
Neuschaefer, L. W. & Rogier A. Windhorst. (1995). Observation and reduction methods of deep Palomar 200 inch 4-Shooter mosaics. The Astrophysical Journal Supplement Series. 96. 371–371. 11 indexed citations
7.
Casertano, Stefano, K. U. Ratnatunga, R. E. Griffiths, et al.. (1995). Structural Parameters of Faint Galaxies from Prerefurbishment Hubble Space Telescope Medium Deep Survey Observations. The Astrophysical Journal. 453. 599–599. 26 indexed citations
8.
Neuschaefer, L. W., K. U. Ratnatunga, R. E. Griffiths, Stefano Casertano, & Myungshin Im. (1995). Galaxy Clustering Statistics of Hubble Space Telescope Medium Deep Survey WF/PC Images. The Astrophysical Journal. 453. 559–559. 11 indexed citations
9.
Neuschaefer, L. W., K. U. Ratnatunga, R. E. Griffiths, & F. Valdés. (1995). Detection, Photometry, and Completeness of FOCAS Catalogs for the HST Medium-Deep Survey. Publications of the Astronomical Society of the Pacific. 107. 590–590. 2 indexed citations
10.
Ratnatunga, K. U., et al.. (1994). Calibration of HST wide field camera for quantitative analysis of faint galaxy images. The Astronomical Journal. 108. 2362–2362. 13 indexed citations
11.
Windhorst, Rogier A., et al.. (1994). Removing cosmic-ray hits from multiorbit HST Wide Field Camera images. Publications of the Astronomical Society of the Pacific. 106. 798–798. 28 indexed citations
12.
Griffiths, R. E., Stefano Casertano, K. U. Ratnatunga, et al.. (1994). The morphology of faint galaxies in Medium Deep Survey images using WFPC2. The Astrophysical Journal. 435. L19–L19. 58 indexed citations
13.
Windhorst, Rogier A., P. C. Schmidtke, S. M. Pascarelle, et al.. (1994). Hubble Space Telescope Medium Deep Survey. 2: Deconvolution of Wide Field Camera field galaxy images in the 13 hour + 43 deg field. The Astronomical Journal. 107. 930–930. 9 indexed citations
14.
Windhorst, Rogier A., David Burstein, L. W. Neuschaefer, et al.. (1991). The discovery of a young radio galaxy at Z = 2.390 - Probing initial star formation at Z less than approximately 3.0. The Astrophysical Journal. 380. 362–362. 47 indexed citations
15.
Neuschaefer, L. W., Rogier A. Windhorst, & Alan Dressler. (1991). The galaxy two-point correlation function down to V - 26 magnitudes on 0.5-deg scales. The Astrophysical Journal. 382. 32–32. 9 indexed citations
16.
Windhorst, Rogier A., et al.. (1990). The evolution of weak radio galaxies at radio and optical wavelengths.. NASA Technical Reports Server (NASA). 10. 389–403. 5 indexed citations

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.

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