Pushpa Khare

1.3k total citations
41 papers, 771 citations indexed

About

Pushpa Khare is a scholar working on Astronomy and Astrophysics, Instrumentation and Statistical and Nonlinear Physics. According to data from OpenAlex, Pushpa Khare has authored 41 papers receiving a total of 771 indexed citations (citations by other indexed papers that have themselves been cited), including 35 papers in Astronomy and Astrophysics, 17 papers in Instrumentation and 3 papers in Statistical and Nonlinear Physics. Recurrent topics in Pushpa Khare's work include Stellar, planetary, and galactic studies (27 papers), Galaxies: Formation, Evolution, Phenomena (24 papers) and Astrophysics and Star Formation Studies (18 papers). Pushpa Khare is often cited by papers focused on Stellar, planetary, and galactic studies (27 papers), Galaxies: Formation, Evolution, Phenomena (24 papers) and Astrophysics and Star Formation Studies (18 papers). Pushpa Khare collaborates with scholars based in India, United States and France. Pushpa Khare's co-authors include Donald G. York, Varsha P. Kulkarni, J. T. Lauroesch, Céline Péroux, Joseph D. Meiring, R. Srianand, Arlin Crotts, G. Vladilo, D. E. Welty and James W. Truran and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

Pushpa Khare

37 papers receiving 759 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Pushpa Khare India 18 751 152 87 33 21 41 771
Milan Raičević Netherlands 6 605 0.8× 186 1.2× 165 1.9× 22 0.7× 12 0.6× 7 632
Toru Misawa Japan 13 480 0.6× 100 0.7× 109 1.3× 20 0.6× 10 0.5× 35 508
Rob P. Olling United States 11 730 1.0× 236 1.6× 96 1.1× 33 1.0× 29 1.4× 15 739
Sandhya M. Rao United States 18 1.3k 1.8× 300 2.0× 238 2.7× 36 1.1× 24 1.1× 32 1.3k
G. Vettolani Italy 12 429 0.6× 180 1.2× 124 1.4× 20 0.6× 29 1.4× 28 457
Hai Fu United States 18 650 0.9× 228 1.5× 86 1.0× 38 1.2× 9 0.4× 36 682
R. J. Cool United States 8 502 0.7× 237 1.6× 101 1.2× 21 0.6× 9 0.4× 12 511
P. Mazzei Italy 14 710 0.9× 332 2.2× 97 1.1× 30 0.9× 11 0.5× 70 736
H. Hippelein Germany 15 637 0.8× 249 1.6× 92 1.1× 37 1.1× 10 0.5× 45 670
Samantha M. Benincasa Canada 11 522 0.7× 152 1.0× 58 0.7× 13 0.4× 13 0.6× 15 548

Countries citing papers authored by Pushpa Khare

Since Specialization
Citations

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

Fields of papers citing papers by Pushpa Khare

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Pushpa Khare. 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 Pushpa Khare. The network helps show where Pushpa Khare may publish in the future.

Co-authorship network of co-authors of Pushpa Khare

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

All Works

20 of 20 papers shown
1.
Khare, Pushpa. (2013). Quasar absorption lines: an overview. Bulletin of the Astronomical Society of India. 41(1). 41. 1 indexed citations
2.
York, Donald G., Lorrie A. Straka, Michael Bishof, et al.. (2012). Galaxies with background QSOs - I. A search for strong galactic Hα lines. Monthly Notices of the Royal Astronomical Society. 423(4). 3692–3708. 17 indexed citations
3.
Meiring, Joseph D., J. T. Lauroesch, L. Haberzettl, et al.. (2010). SOAR imaging of sub-damped Lyman α systems at z < 1. Monthly Notices of the Royal Astronomical Society. 410(4). 2516–2525. 10 indexed citations
4.
Meiring, Joseph D., Varsha P. Kulkarni, J. T. Lauroesch, et al.. (2009). New Magellan Inamori Kyocera Echelle Observations ofz< 1.5 sub-damped Lyman α systems. Monthly Notices of the Royal Astronomical Society. 393(4). 1513–1530. 24 indexed citations
5.
Wild, Vivienne, Guinevere Kauffmann, Simon D. M. White, et al.. (2008). Narrow associated quasi-stellar object absorbers: clustering, outflows and the line-of-sight proximity effect. Monthly Notices of the Royal Astronomical Society. 388(1). 227–241. 70 indexed citations
6.
Meiring, Joseph D., Varsha P. Kulkarni, J. T. Lauroesch, et al.. (2008). The chemical compositions of 10 new sub-DLAs and strong Lyman-limit systems atz≲ 1.5. Monthly Notices of the Royal Astronomical Society. 384(3). 1015–1033. 31 indexed citations
7.
Péroux, Céline, Varsha P. Kulkarni, Joseph D. Meiring, et al.. (2006). The most metal-rich intervening quasar absorber known. Springer Link (Chiba Institute of Technology). 42 indexed citations
8.
Vladilo, G., M. Centurión, S. A. Levshakov, et al.. (2006). Extinction and metal column density of HI regions up to redshiftz$\mathsf{\simeq 2}$. Astronomy and Astrophysics. 454(1). 151–164. 39 indexed citations
9.
Péroux, Céline, Joseph D. Meiring, Varsha P. Kulkarni, et al.. (2006). Metal-rich damped/subdamped Lyman   quasar absorbers at z < 1. Monthly Notices of the Royal Astronomical Society. 372(1). 369–380. 38 indexed citations
10.
Khare, Pushpa, Varsha P. Kulkarni, J. T. Lauroesch, et al.. (2005). Evolution of metals and dust in the universe. Bulletin of the Astronomical Society of India. 33(2). 219. 1 indexed citations
11.
Khare, Pushpa, et al.. (2001). Unified model for quasar absorption line systems. Springer Link (Chiba Institute of Technology).
12.
Khare, Pushpa, et al.. (1999). Chemical Enrichment at High Redshifts. The Astrophysical Journal. 510(2). 597–604. 2 indexed citations
13.
Khare, Pushpa, et al.. (1997). The ionization and abundance of C and Si in QSO absorbers. SOKENDAI (Graduate University for Advanced Studies). 2 indexed citations
14.
Khare, Pushpa. (1995). Quasar absorption lines.. 23. 19–39.
15.
Srianand, R. & Pushpa Khare. (1994). Evolutionary properties of Ly   clouds. Monthly Notices of the Royal Astronomical Society. 271(1). 81–93. 7 indexed citations
16.
Srianand, R. & Pushpa Khare. (1993). Halo model for MG II absorption lines in the spectra of quasars. The Astrophysical Journal. 413. 486–486. 6 indexed citations
17.
Khare, Pushpa & Narayan Rana. (1993). Chemical evolution of the high redshift galaxies. Journal of Astrophysics and Astronomy. 14(2). 83–95.
18.
Acharya, M. R. & Pushpa Khare. (1993). Differential evolution of Lyman alpha lines. Journal of Astrophysics and Astronomy. 14(2). 97–102. 1 indexed citations
19.
Khare, Pushpa. (1986). Comment on ‘‘Time variation of fundamental constants, primordial nucleosynthesis, and the size of extra dimensions.’’. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 34(6). 1936–1937. 7 indexed citations
20.
Khare, Pushpa & B. B. Deo. (1983). Neutrino degeneracy and the primordial abundance of helium and deuterium. Journal of Astrophysics and Astronomy. 4(4). 301–306. 1 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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