2003 QZ30
Available from the Minor Planet Center.
Available from the Minor Planet Center.
Available from the Minor Planet Center.
Available from the Minor Planet Center.
Lyα emitters (LAEs) are seen everywhere in the redshift domain
from local to z ~ 7. Far-infrared (FIR) counterparts of LAEs at
different epochs could provide direct clues on dust content, extinction,
and spectral energy distribution (SED) for these galaxies. We search for
FIR counterparts of LAEs that are optically detected in the GOODS-North
field at redshift z ~ 2.2 using data from the Herschel Space Telescope
with the Photodetector Array Camera and Spectrometer (PACS). The LAE
candidates were isolated via color-magnitude diagram using the
medium-band photometry from the ALHAMBRA Survey,…
Available from the Minor Planet Center.
Available from the Minor Planet Center.
Ly-alpha emitters (LAEs) are seen everywhere in the redshift domain from
local to z~7. Far-infrared (FIR) counterparts of LAEs at different
epochs could provide direct clues on dust content, extinction, and
spectral energy distribution (SED) for these galaxies. We search for FIR
counterparts of LAEs that are optically detected in the GOODS-North
field at redshift z~2.2 using data from the Herschel Space Telescope
with the Photodetector Array Camera and Spectrometer (PACS). The LAE
candidates were isolated via color-magnitude diagram using the
medium-band photometry from the ALHAMBRA Survey,…
Not Available