Citations per year, relative to S. B. Pandey S. B. Pandey (= 1×)
peers
E. Maiorano
Countries citing papers authored by S. B. Pandey
Since
Specialization
Citations
This map shows the geographic impact of S. B. Pandey'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 S. B. Pandey with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. B. Pandey more than expected).
This network shows the impact of papers produced by S. B. Pandey. 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 S. B. Pandey. The network helps show where S. B. Pandey may publish in the future.
Co-authorship network of co-authors of S. B. Pandey
This figure shows the co-authorship network connecting the top 25 collaborators of S. B. Pandey.
A scholar is included among the top collaborators of S. B. Pandey 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 S. B. Pandey. S. B. Pandey is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Gupta, Rahul, S. B. Pandey, Amit Kumar, et al.. (2021). GRB 210204A: observations with the 3.6m Devasthal Optical Telescope and possible jet break. GRB Coordinates Network. 29490. 1.1 indexed citations
Gupta, Rahul, et al.. (2020). GRB 210120A : 1.3m DFOT optical observations.. GRB Coordinates Network. 29345. 1.
7.
Castro‐Tirado, A. J., Yi-Ming Hu, A. F. Valeev, et al.. (2019). GRB 190114C: refined redshift by the 10.4m GTC.. GRB Coordinates Network. 23708. 1.6 indexed citations
8.
Misra, Kuntal, et al.. (2018). GRB 180418A: Imaging of the optical afterglow with the 1.3 m DFOT=.. GCN. 22663. 1.
Castro‐Tirado, A. J., R. Cunniffe, R. Sánchez-Ramírez, et al.. (2014). GRB140703A: 10.4m GTC redshift.. GCN. 16505. 1.2 indexed citations
12.
Sagar, R. & S. B. Pandey. (2012). GRB afterglow observations from ARIES Nainital and their importance. 5. 1.2 indexed citations
13.
Zheng, WeiKang, F. Yuan, J. Vinkó, et al.. (2010). Discovery of a Supernova Candidate. ATel. 2468. 1.1 indexed citations
14.
Pandey, S. B., W. Zheng, F. Yuan, & C. Akerlof. (2009). GRB 090902B: ROTSE-III detection of optical afterglow.. GRB Coordinates Network. 9878. 1.
15.
Schady, P. & S. B. Pandey. (2006). GRB061007: Swift UVOT followup observations.. GCN. 5719. 1.1 indexed citations
16.
Jelínek, M., A. de Ugarte Postigo, A. J. Castro‐Tirado, et al.. (2005). GRB 051109a: Bootes R & I-band detection of the early afterglow.. GRB Coordinates Network. 4227. 1.1 indexed citations
17.
Postigo, A. de Ugarte, M. Jelínek, S. Vítek, et al.. (2005). GRB 051221B: Bootes optical observations.. GCN. 4379. 1.1 indexed citations
18.
Pandey, S. B., D. K. Sahu, L. Resmi, et al.. (2003). Optical observations of the bright long duration peculiar GRB 021004 afterglow. Bulletin of the Astronomical Society of India. 31. 19–36.5 indexed citations
19.
Sagar, R., S. B. Pandey, V. Mohan, D. Bhattacharya, & A. J. Castro‐Tirado. (2001). GRB 000926 and its optical afterglow : Another possible evidence for non-isotropic emission. 29. 1–13.2 indexed citations
20.
Sagar, R., et al.. (2000). GRB 000301C with peculiar afterglow emission. CERN Bulletin. 28. 499–513.4 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.