diff --git a/docs/source/usage/getting_started.rst b/docs/source/usage/getting_started.rst
index f266fa1..61fba7c 100644
--- a/docs/source/usage/getting_started.rst
+++ b/docs/source/usage/getting_started.rst
@@ -9,15 +9,13 @@ Installation
A Python 3 installation is required to run ESBO-ETC. You can get the latest python version
`here `_.
-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 `_ or clone the latest development version from the IRS git server using
.. code-block:: bash
:linenos:
git clone https://egit.irs.uni-stuttgart.de/esbo_ds/ESBO-ETC.git
-or download the code from the `IRS git server `_.
-
Python Virtual Environment
--------------------------
diff --git a/esbo_etc/classes/target/BlackBodyTarget.py b/esbo_etc/classes/target/BlackBodyTarget.py
index 4479d80..0b37db1 100644
--- a/esbo_etc/classes/target/BlackBodyTarget.py
+++ b/esbo_etc/classes/target/BlackBodyTarget.py
@@ -6,6 +6,7 @@ from astropy.constants import c, k_B
from ...lib.logger import logger
from ..Entry import Entry
from typing import Union
+import numpy as np
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
# 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
+ 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:
sfd = bb(wl_bins)
# Initialize super class