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.
Nearby supernova rates from the Lick Observatory Supernova Search - II. The observed luminosity functions and fractions of supernovae in a complete sample
2011390 citationsR. Chornock, A. V. Filippenko et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of M. Modjaz'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 M. Modjaz with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Modjaz more than expected).
This network shows the impact of papers produced by M. Modjaz. 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 M. Modjaz. The network helps show where M. Modjaz may publish in the future.
Co-authorship network of co-authors of M. Modjaz
This figure shows the co-authorship network connecting the top 25 collaborators of M. Modjaz.
A scholar is included among the top collaborators of M. Modjaz 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 M. Modjaz. M. Modjaz is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Cenko, S. B., J. S. Bloom, D. A. Perley, et al.. (2010). GRB 100206A - Keck/LRIS spectroscopy.. GRB Coordinates Network. 10389. 1.1 indexed citations
10.
Perley, D. A., J. S. Bloom, M. Modjaz, et al.. (2008). GRB 070809: putative host galaxy and redshift.. GRB Coordinates Network. 7889. 1.3 indexed citations
11.
Chornock, R., J. S. Bloom, M. Modjaz, et al.. (2008). Optical Spectroscopy of the Transient ROTSE3 J115649.1+542726. ATel. 1593. 1.
12.
Miller, Adam A., J. S. Bloom, R. Chornock, et al.. (2008). Optical-NIR SED and spectroscopy of ROTSE3 J115649.1+542726. ATel. 1576. 1.
13.
Torres, M. A. P., P. G. Jonker, P. Challis, et al.. (2007). XMMSL1 J070542.7-381442 is a nova. The astronomer's telegram. 1285. 1.1 indexed citations
14.
Torres, M. A. P., D. Steeghs, P. G. Jonker, et al.. (2007). SWIFT J052522.48+241331.8 (=1RXS J052523.2+241331) is a Cataclysmic Variable. The astronomer's telegram. 1286. 1.2 indexed citations
15.
Perley, D. A., J. S. Bloom, M. Modjaz, D. Poznanski, & C. C. Thoene. (2007). GRB 070429B: probable host galaxy and redshift.. GCN. 7140. 1.3 indexed citations
16.
Kocevski, D., D. A. Perley, & M. Modjaz. (2007). GRB 071010A: continued Keck imaging.. GCN. 6885. 1.1 indexed citations
17.
Blondin, S., M. Modjaz, R. Kirshner, P. Challis, & P. Berlind. (2007). Supernova 2007U in ESO 552-65. 838. 1.
18.
Immler, S., M. Modjaz, & P. J. Brown. (2006). Detection of SN 2006jc in X-Rays with Chandra. ATel. 934. 1.
19.
Blondin, S., et al.. (2006). Supernova 2006at [resend (Url truncated in Cbet 440 by e-mailing software)]. 441. 1.1 indexed citations
20.
Modjaz, M., R. Kirshner, P. Challis, T. Matheson, & P. Berlind. (2005). Supernova 2005hg in UGC 1394. 271. 1.1 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.