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Discovery of OH Absorption from a Galaxy at z ∼ 0.05: Implications for Large Surveys with SKA Pathfinders

  • Authors: N. Gupta, E. Momjian, R. Srianand, P. Petitjean, P. Noterdaeme, D. Gyanchandani, R. Sharma, and S. Kulkarni

2018 The Astrophysical Journal Letters 860 L22.

  • Provider: AAS Journals

Caption: Figure 2.

Left: OHM detected in G0248+430. The zero of the velocity scale (z = 0.05192) is centered at the peak of the 1667 MHz line. Right: H I 21 cm and OH main-line absorption spectra toward Q0248+430. The zero of the velocity scale (z = 0.05151) is centered at the peak of H I 21 cm absorption line. In both panels, individual Gaussian components (see Table 2), the resulting fits to the stokes-I spectrum are plotted as dotted and continuous lines, respectively. The residuals, on an offset arbitrarily shifted for clarity, are also shown.

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