Table 2.
OHM detected in our GMRT observations.
| AGC name | OH position | Major | Minor | PA | Vpeak | Fpeak | FWHM | rmsimage | rmsline | ∫SdV | OH luminosity |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (J2000) | (″) | (″) | (°) | (km s−1) | (mJy) | (km s−1) | (mJy) | (mJy) | (Jy km s−1) | (log L⊙) | |
| 115713 | 014135.19+165730.73 | < 1.3 | < 0.7 | – | 51 065.2 | 14.39 | 186.7 | 1.03 | 1.70 | 1.66 | 3.15 |
| 249507 | 140340.34+295456.39 | 1.24 ± 0.23 | 0.55 ± 0.39 | 6.5 | 53 421.4 | 8.26 | 203.4 | 0.79 | 0.92 | 1.35 | 3.06 |
Notes. Columns 2–5: the Gaussian fitted peak position and component size of the OH emission from the image plane. Columns 6–8: The fitted parameters of the line profile. Columns 9–10: the noise level from the image plane with a frequency width of about 24 kHz (∼6 km s−1) and the noise level from our extracted line as shown in Fig. 2. Columns 11–12: the integrated line flux densities and luminosities. We have used the identical redshift for calculating the luminosity, as detailed in Table 1.
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