esbo_ds/ESBO-ETC
esbo_ds
/
ESBO-ETC
11
0
Fork 1
Code Issues 1 Pull Requests Releases 1 Wiki Activity

Instruction to download release added

This commit is contained in:
Lukas Klass 2020-10-23 14:50:31 +02:00
parent 59439964c6
commit 68b37f763e
2 changed files with 6 additions and 3 deletions
Show Stats Download Patch File Download Diff File Expand all files Collapse all files

4
docs/source/usage/getting_started.rst
View File

@ -9,15 +9,13 @@ Installation
A Python 3 installation is required to run ESBO-ETC. You can get the latest python version A Python 3 installation is required to run ESBO-ETC. You can get the latest python version
`here <https://www.python.org/downloads/>`_. `here <https://www.python.org/downloads/>`_.
In order to get ESBO-ETC, clone the code from the IRS git server using In order to get ESBO-ETC, download the latest release from the `IRS git server <https://egit.irs.uni-stuttgart.de/esbo_ds/ESBO-ETC/releases>`_ or clone the latest development version from the IRS git server using
.. code-block:: bash .. code-block:: bash
:linenos: :linenos:
git clone https://egit.irs.uni-stuttgart.de/esbo_ds/ESBO-ETC.git git clone https://egit.irs.uni-stuttgart.de/esbo_ds/ESBO-ETC.git
or download the code from the `IRS git server <https://egit.irs.uni-stuttgart.de/esbo_ds/ESBO-ETC>`_.
Python Virtual Environment Python Virtual Environment
-------------------------- --------------------------

5
esbo_etc/classes/target/BlackBodyTarget.py
View File

@ -6,6 +6,7 @@ from astropy.constants import c, k_B
from ...lib.logger import logger from ...lib.logger import logger
from ..Entry import Entry from ..Entry import Entry
from typing import Union from typing import Union
import numpy as np
class BlackBodyTarget(ATarget): class BlackBodyTarget(ATarget):
@ -71,6 +72,10 @@ class BlackBodyTarget(ATarget):
factor = self._band[band.upper()]["sfd"] / (bb(self._band[band.upper()]["wl"]) * u.sr) * u.sr factor = self._band[band.upper()]["sfd"] / (bb(self._band[band.upper()]["wl"]) * u.sr) * u.sr
# Calculate spectral flux density for the given wavelengths and scale it for a star of the given magnitude # Calculate spectral flux density for the given wavelengths and scale it for a star of the given magnitude
sfd = bb(wl_bins) * factor * 10 ** (- 2 / 5 * mag / u.mag) # / 1.195 * 1.16 # scaling for AETC validation sfd = bb(wl_bins) * factor * 10 ** (- 2 / 5 * mag / u.mag) # / 1.195 * 1.16 # scaling for AETC validation
wl_bins_2 = np.arange(15.71, 23.71, 0.01) << u.um
sfd_2 = bb(wl_bins_2) * factor * 10 ** (- 2 / 5 * mag / u.mag)
sqty_2 = SpectralQty(wl_bins_2, sfd_2).integrate()
print((sqty_2 / (8 * u.um)).to(u.W / (u.m ** 2 * u.um)))
else: else:
sfd = bb(wl_bins) sfd = bb(wl_bins)
# Initialize super class # Initialize super class