Table 1.
Characteristics of the dust continuum and the H2O and HF emission lines in BR 1202-0725.
QSO (SE) | SMG (NW) | |
---|---|---|
Continuum | ||
RA | 12:05:23.134 ± 0.001 | 12:05:22.980 ± 0.001 |
Dec | −07:42:32.76 ± 0.01 | −07:42:29.680 ± 0.01 |
S216 GHz (mJy) | 4.9 ± 0.2 | 5.1 ± 0.2 |
H2O(220–211) | ||
z | 4.6948 ± 0.0001 | (4.6915) ( † ) |
Speak (mJy) | 2.2 ± 0.1 | 1.0 ± 0.1 |
FWHM (km s−1) | 340 ± 15 | 1020 ± 50 |
SΔv (Jy beam−1 km s−1) | 0.80 ± 0.03 | 1.1 ± 0.2 |
HF | ||
Speak (mJy) | 1.0 ± 0.1 | − |
FWHM (km s−1) | 285 ± 45 | − |
SΔv (Jy beam−1 km s−1) | 0.25 ± 0.03 | – |
Notes. ( † )Because part of the H2O line profile lies outside our frequency coverage, we constrained this to the [CII] redshift (Carilli et al. 2013). The rest-frame frequencies of HF J = 1–0 and H2O (220–211) are 1232.476 and 1228.789 GHz respectively.
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