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Constraining cold accretion on to supermassive black holes: molecular gas in the cores of eight brightest cluster galaxies revealed by joint CO and CN absorption

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Figure

Table 1. For the 18 sources observed in our survey, the above table highlights the lines for which observations have been carried out and detections of emission and absorption lines have been made
Table 2. A summary of the ALMA observations presented in this paper, all of which were taken using ALMA band 3 and have a frequency resolution of 977 kHz
Figure 1. Our observations show detections of two CN lines, labelled as CN-A and CN-B throughout the paper
Table 4. Stellar redshifts and their corresponding velocities used as zero-points for the spectra shown in Fig
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