From 9f8bde082c1fa54e6fab40c9534514b7d7f1e813 Mon Sep 17 00:00:00 2001
From: Jan David Mol <mol@astron.nl>
Date: Thu, 9 Dec 2021 09:16:47 +0100
Subject: [PATCH] L2SS-499: Update our Jupyter documentation to use import of
tangostationcontrol
---
docs/source/devices/sst-xst.rst | 4 ++--
1 file changed, 2 insertions(+), 2 deletions(-)
diff --git a/docs/source/devices/sst-xst.rst b/docs/source/devices/sst-xst.rst
index cdb689e45..092bdda83 100644
--- a/docs/source/devices/sst-xst.rst
+++ b/docs/source/devices/sst-xst.rst
@@ -63,7 +63,7 @@ Typically, ``N_ant == 192``, and ``N_blocks == 136``.
The metadata refers to the *blocks*, which are emitted by the FPGAs to represent the XSTs between 12 x 12 consecutive antennas. The following code converts block numbers to the indices of the first antenna pair in a block::
- from common.baselines import baseline_from_index
+ from tangostationcontrol.common.baselines import baseline_from_index
def first_antenna_pair(block_nr: int) -> int:
coarse_a, coarse_b = baseline_from_index(block_nr)
@@ -71,7 +71,7 @@ The metadata refers to the *blocks*, which are emitted by the FPGAs to represent
Conversely, to calculate the block index for an antenna pair ``(a,b)``, use::
- from common.baselines import baseline_index
+ from tangostationcontrol.common.baselines import baseline_index
def block_nr(a: int, b: int) -> int:
return baseline_index(a // 12, b // 12)
--
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