Distant Galaxy Spectra

Distant Galaxy Spectra - IV
The redshift of the galaxy can be determined from the shift in the positions of significant emission lines from rest frequencies. From the evidence for recent star formation, the galaxy is typed as a spiral.
[NMSU, N. Vogt & UCSC/DEEP]

Photometric data on this galaxy, from the Fernández-Soto, Lanzetta & Yahil HDF-N catalog (SUNY Stony Brook).

CoordinatesX 1095.2
Y 3972.1
CoordinatesRA 12:36:48.322
DEC62:14:26.252
Total I-AB(814) 19.18
Spectroscopic redshift 0.139
Photometric redshift 0.120
Best-fit spectral type Scd
Best fit spectral energy distribution (SED, top) and redshift probability graph (bottom), spiking at z = 0.14.
Optical and IR images (8 by 8 arcsec)
BVI JHK

Aperture fluxes and errors (in nJy)
U B V I J H K
13520.00 (49.86) 34560.00 (25.65) 58880.00 (19.06) 78880.00 (30.04) 106000 (237) 114300 (455) 119400 (450)