Image Details

Choose export citation format:

NICER Magnetar Burst Catalog

  • Authors: Che-Yen Chu, Chin-Ping Hu, Teruaki Enoto, George A. Younes, Rachael Stewart, Zaven Arzoumanian, Wynn C. G. Ho, Zorawar Wadiasingh, Andrea Sanna, Sebastien Guillot, Gaurava K. Jaisawal, Matthew G. Baring, Marlon L. Bause, Tolga Güver, Chryssa Kouveliotou, Alex Van Kooten, Keith C. Gendreau

Che-Yen Chu et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 7.

Distribution of blackbody emission radius R (top) and emission radius R versus temperature kT (bottom). Different histograms represent the magnetar groups defined in Figure 2, as indicated in the legend. The unshaded red histogram shows Swift J1555.2−5402 assuming a distance of 10 kpc, while the shaded red histogram assumes a distance of 4.5 kpc. The blue curve shows the log-normal fit to the R distribution of the SGR 1935+2154 sample. In the bottom panel, red triangles represent Swift J1555.2−5402, green diamonds represent SGR 1830−0645, blue squares represent SGR 1935+2154, and black circles represent the remaining magnetars.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse