Table 2.
Open in new tab

Power-law indices (α) for the pulse energy distributions presented in Fig. 6. The power-law regime is obeyed for pulse energies ≳2 Jy |$\mu$|s, below which the distribution is flattened. The IGP distribution is well-described by a single power law, while the MGP and all-GP distributions are better-described by a broken power law, with indices listed here as ‘low’ and ‘high’.

Data setPulse energy (Jy |$\mu$|s)α
IGP≳2−3.99 ± 0.04
MGPlow∼2–7−3.26 ± 0.03
MGPhigh≳7−1.81 ± 0.06
GPlow∼2–7−3.48 ± 0.04
GPhigh≳7−2.10 ± 0.09
Data setPulse energy (Jy |$\mu$|s)α
IGP≳2−3.99 ± 0.04
MGPlow∼2–7−3.26 ± 0.03
MGPhigh≳7−1.81 ± 0.06
GPlow∼2–7−3.48 ± 0.04
GPhigh≳7−2.10 ± 0.09
Table 2.
Open in new tab

Power-law indices (α) for the pulse energy distributions presented in Fig. 6. The power-law regime is obeyed for pulse energies ≳2 Jy |$\mu$|s, below which the distribution is flattened. The IGP distribution is well-described by a single power law, while the MGP and all-GP distributions are better-described by a broken power law, with indices listed here as ‘low’ and ‘high’.

Data setPulse energy (Jy |$\mu$|s)α
IGP≳2−3.99 ± 0.04
MGPlow∼2–7−3.26 ± 0.03
MGPhigh≳7−1.81 ± 0.06
GPlow∼2–7−3.48 ± 0.04
GPhigh≳7−2.10 ± 0.09
Data setPulse energy (Jy |$\mu$|s)α
IGP≳2−3.99 ± 0.04
MGPlow∼2–7−3.26 ± 0.03
MGPhigh≳7−1.81 ± 0.06
GPlow∼2–7−3.48 ± 0.04
GPhigh≳7−2.10 ± 0.09
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close