tokens: velocity, which was mostly determined by the NH 3 line observations (Table 1). Figure 5.50. 3775 The detected 22 GHz H 2 O maser spectra of the sources detected only at 22 GHz. Red and Black colors represent the first and second epochs, respectively. The source name is given in the top-left corner of the upper panel and “M” is attached for the source associated with 6.7 GHz CH 3 OH maser emission (see Section 3.1). The observing dates are shown in the top-right corner. The vertical dotted line indicates the systemic velocity, which was mostly determined by the NH 3 line observations (Table 1). Figure 5.51. 3816 The detected 22 GHz H 2 O maser spectra of the sources detected only at 22 GHz. Red and Black colors represent the first and second epochs, respectively. The source name is given in the top-left corner of the upper panel and “M” is attached for the source associated with 6.7 GHz CH 3 OH maser emission (see Section 3.1). The observing dates are shown in the top-right corner. The vertical dotted line indicates the systemic velocity, which was mostly determined by the NH 3 line observations (Table 1). Figure 5.52. 3866 The detected 22 GHz H 2 O maser spectra of the sources detected only at 22 GHz. Red and Black colors represent the first and second epochs, respectively. The source name is given in the top-left corner of the upper panel and “M” is attached for the source associated with 6.7 GHz CH 3 OH maser emission (see Section 3.1). The observing dates are shown in the top-right corner. The vertical dotted line indicates the systemic velocity, which was mostly determined by the NH 3 line observations (Table 1). Figure 5.53. 3878 The detected 22 GHz H 2 O maser spectra of the sources detected only at 22 GHz. Red and Black colors represent the first and second epochs, respectively. The source name is given in the top-left corner of the upper panel and “M” is attached for the source associated with 6.7 GHz CH 3 OH maser emission (see Section 3.1). The observing dates are shown in the top-right corner. The vertical dotted line indicates the systemic velocity, which was mostly determined by the NH 3 line observations (Table 1). Figure 5.54. 3880 The detected 22 GHz H 2 O maser spectra of the sources detected only at 22 GHz. Red and Black colors represent the first and second epochs, respectively. The source name is given in the top-left corner of the upper panel and “M” is attached for the source associated with 6.7 GHz CH 3 OH maser emission (see Section 3.1). The observing dates are shown in the top-right corner. The vertical dotted line indicates the systemic velocity, which was mostly determined by the NH 3 line observations (Table 1). Figure 5.55. 3914 The detected 22 GHz H 2 O maser spectra of the sources detected only at 22 GHz. Red and Black colors represent the first and second epochs, respectively. The source name is given in the top-left corner of the upper panel and “M” is attached for the source associated with 6.7 GHz CH 3 OH
ner_tags: O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O B-Wavelength I-Wavelength O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Wavelength I-Wavelength O O O