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abhijeetmanhas commented Feb 18, 2020

I ran test for test_fido file and this warning pops up:

_ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ 

self = <[AttributeError("'Time' object has no attribute 'start'",) raised in repr()] Time object at 0x7f7eff4ebf98>
args = ('2011-06-07 06:33', '2011-06-07 06:33:08'), kwargs = {}, name = 'Time'

    def __init__(
yanyuechuixue commented Feb 22, 2020

my config is

name = dynesty
nlive = 1200
dlogz = 0.001
checkpoint-interval = 5000

However, the sampler stop too early. There is no enough points.

I have tried to decrease dlogz in [sampler] config, but it does not work.
In the output on the screen, it always says ... | dlogz: 10.085 > 1.209 no matter what dlogz is (no matter what dlogz is, the last n

perrygreenfield commented Feb 19, 2020

Peter Teuben points out that the example on readthedocs (which comes from the README.rst) of the following:

sequence = np.array([x for x in range(100)])
squares = np.array([x**2 for x in range(100)])

is better expressed as

sequence = np.arange(100)
squares  = sequence**2

It is hard to argue with that.

kelle commented Dec 9, 2019
"This elementary review covers the basics of working with astronomical data, notably with images, spectra and higher-level (catalog) data. The basic concepts and tools are presented using both application software (DS9 and TOPCAT) and Python. The level of presentation is suitable for undergraduate students, but should also be accessible to advanced high school stu

jmeyers314 commented Dec 2, 2019

In the redder bands of LSST, and presumably other cameras too, the best focus occurs when the geometric focus of the optics is located in the bulk of the silicon rather than at the surface.

I think simulating this can be achieved via a focus_depth kwarg to SiliconSensor and some small changes around I guess

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