Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
First Results from the X‐Ray and Optical Survey of theChandraDeep Field South
2001297 citationsR. Giacconi, P. Rosati et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of G. Hasinger'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 G. Hasinger with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Hasinger more than expected).
This network shows the impact of papers produced by G. Hasinger. 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 G. Hasinger. The network helps show where G. Hasinger may publish in the future.
Co-authorship network of co-authors of G. Hasinger
This figure shows the co-authorship network connecting the top 25 collaborators of G. Hasinger.
A scholar is included among the top collaborators of G. Hasinger 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 G. Hasinger. G. Hasinger is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Lehmann, I., G. Hasinger, Maarten Schmidt, et al.. (2001). The ROSAT Deep Survey. Astronomy and Astrophysics. 371(3). 833–857.100 indexed citations
10.
Giacconi, R., P. Rosati, P. Tozzi, et al.. (2001). First Results from the X‐Ray and Optical Survey of theChandraDeep Field South. The Astrophysical Journal. 551(2). 624–634.297 indexed citations breakdown →
Hasinger, G. & N. E. White. (1998). X‐ray Surveys Workshop. Astronomische Nachrichten. 319(1-2). 1–2.3 indexed citations
15.
Sołtan, A. & G. Hasinger. (1994). The angular correlation function of the soft X-ray background.. A&A. 288. 77–88.1 indexed citations
16.
Motch, C., G. Hasinger, & W. Pietsch. (1994). Discovery of a luminous galactic supersoft X-ray source in the ROSAT all-sky survey. 284(3). 827–838.1 indexed citations
17.
Alpar, M. A., G. Hasinger, J. Shaham, & Sophia Yancopoulos. (1992). 6 Hz quasiperiodic oscillations from low-mass X-ray binaries - The sound of an accretion disk?. OpenMETU (Middle East Technical University). 257(2). 627–631.
Predehl, P., G. Hasinger, & F. Verbunt. (1991). ROSAT discovery of bright X-ray sources in globular clusters Ter 6 and NGC 6652. 246(1).1 indexed citations
20.
Hasinger, G.. (1987). A classification of fast quasi-periodic X-ray oscillators: Is 6 Hz a fundamental frequency?. NASA STI/Recon Technical Report N. 87. 28000.2 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.