Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002apj...578l..19i&link_type=abstract
The Astrophysical Journal, Volume 578, Issue 1, pp. L19-L22.
Astronomy and Astrophysics
Astronomy
13
Cosmology: Observations, Cosmology: Early Universe, Galaxies: Formation, Galaxies: High-Redshift, Galaxies: Individual (Hero J171411.91+501541.8)
Scientific paper
Hyper extremely red objects (HEROs) are objects that are very red in near-IR colors (J-K>~3). They are speculated to be intrinsically red galaxies at z>~2 or Lyman break galaxies at z>10. We report the discovery of a HERO in the field that includes a known radio galaxy, 53W002, and a possible cluster of galaxies both at z=2.39. The HERO, which we name HERO J171411.91+501541.8, or 53W002-HERO1 for brevity, is visible in the Hubble Space Telescope Near-Infrared Camera and Multi-Object Spectrometer H-band data and deep K'-band data from the Subaru Telescope (K'~=21.5 mag) but not visible in B-, V-, I-, and J-band images (J-K>4.45, 2 σ). Its spectral energy distribution is consistent with that of a dusty star-forming or old galaxy at z~=2.4, which may suggest that 53W002-HERO1 is a member of the group of galaxies associated with 53W002. Alternatively, the HERO could be at z~=12.5, if its red color is due to the redshifted Lyman break. If 53W002-HERO1 is an old galaxy at z~2.4, the implied stellar age is ~2-3 Gyr, meaning that stars in the HERO formed at the reionization epoch of z>~10.
Im Myungshin
Kajisawa Masaru
Tanaka Ichi
Yamada Toru
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