Figure A2 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

JADES: Resolving the Stellar Component and Filamentary Overdense Environment of Hubble Space Telescope (HST)-dark Submillimeter Galaxy HDF850.1 at z = 5.18

Authors: Fengwu Sun, Jakob M. Helton, Eiichi Egami, Kevin N. Hainline, George H. Rieke, Christopher N. A. Willmer, Daniel J. Eisenstein, Benjamin D. Johnson, Marcia J. Rieke, Brant Robertson, Sandro Tacchella, Stacey Alberts, William M. Baker, Rachana Bhatawdekar, Kristan Boyett, Andrew J. Bunker, Stephane Charlot, Zuyi Chen, Jacopo Chevallard, Emma Curtis-Lake, A. Lola Danhaive, Christa DeCoursey, Zhiyuan Ji, Jianwei Lyu, Roberto Maiolino, Wiphu Rujopakarn, Lester Sandles, Irene Shivaei, Hannah Übler, Chris Willott, Joris Witstok

Fengwu Sun et al 2024 The Astrophysical Journal 961 .

Provider: AAS Journals

Caption: Figure A2.

Top: NIRCam images of GN10 in the F090W–F444W band. The brightness of GN10 in each band is noted in the lower right corner of each panel (unit: AB mag). Image sizes are 3″ × 3″ (north up, east left). The last panel shows the true-color NIRCam image. Bottom: NIRCam grism spectrum of GN10 (similar to those in Figures 6 and A1). Images are rotated to align with the dispersion direction. Hα and [N II] λ6583 line can be detected at z = 5.303, which are indicated by vertical red lines in 2D spectrum.

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions