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请问在命令行中开启自定义swoole服务器，回调时会切换到异步连接池模式吗？谢谢
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See the following file:
/astro/mwasci/phancock/D0009/queue/logs/asvo_1165125104.e2570960
+ base=/astro/mwasci/phancock/D0009/
+ datadir=/astro/mwasci/phancock/D0009//processing
+ obsnum=11651251…
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According to the documentation, the default for all these scripts is to run on the gpuq (which I understand is where all MWA processes are supposed to be run).
However, when I look at the scripts t…
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Update of vmm-xen-stubdom-linux to v1.0.10 for Qubes r4.0, see comments below for details.
Built from: https://github.com/QubesOS/qubes-vmm-xen-stubdom-linux/commit/e0b91d2574284a830b2effba95d2649141…
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#### Expected behavior
I expected that after winning the round on the queue to receive an upvote from the 1up curation trail I will be upvoted.
#### Actual behavior
After I won the voting round I wa…
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MSI engine uses .NET Framework 4.x to execute the custom actions, which breaks IIS MWA there, which relies on .NET Framework 2.x/3.x.
Also reported as
https://github.com/RonaldCarter/PHPManager/i…
lextm updated
6 years ago
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Simulating an array (in this case, MWA) with three point sources gives blobs of flux density. Things don't quite seem to line up coherently.
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~~FHD/PRISim simulation -> fake gains -> calibrate -> image~~
Real data: MWA hex data - calibrate -> compare with @wenyang-li solutions
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phase_to_time() works differently from phase(). When I try phase_to_time(uvd.time_array[0]), it runs just fine, but then passing the resulting file through FHD simulations leads to waterfall plots lik…
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Maybe this is an issue about astropy rather than pyuvdata. It works well in general, but when I switch to anaconda (4.1.1), if I do uv.read_uvfits('obis.uvfits'), astropy failed to download http://mai…