Image Details

Choose export citation format:

A GLIMPSE of Intermediate Mass Black Holes in the Epoch of Reionization: Witnessing the Descendants of Direct Collapse?

  • Authors: Qinyue Fei, Seiji Fujimoto, Rohan P. Naidu, John Chisholm, Hakim Atek, Gabriel Brammer, Yoshihisa Asada, Danielle A. Berg, Volker Bromm, Lukas J. Furtak, Jenny E. Greene, Tiger Yu-Yang Hsiao, Junehyoung Jeon, Vasily Kokorev, Jorryt Matthee, Priyamvada Natarajan, Richard Pan, Johan Richard, Alberto Saldana-Lopez, Daniel Schaerer, Marta Volonteri, Adi Zitrin

Qinyue Fei et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure A3.

Accuracy of our BH mass measurement. Top: output BH masses compared to the input BH masses. Bottom: the difference between output and input BH masses (﹩{\rm{\Delta }}\mathrm{log}{M}_{{\rm{BH}}}=\mathrm{log}{M}_{{\rm{BH}},{\rm{output}}}-\mathrm{log}{M}_{{\rm{BH}},{\rm{input}}}﹩) compared to the input BH masses. Colored data points denote sources with SNRHα,broad > 5 while gray circles represent those with lower SNR. The color of each data point denotes the input magnification for our sources. The circles represent the mean values of data points in each 0.3 dex bin of the output MBH. The black dashed line denotes the 1:1 line, and the black dotted lines represent 0.3 dex.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse