From 996bfb4ad21c4bb816785812335a27e3aca4eae0 Mon Sep 17 00:00:00 2001 From: Matt Craig Date: Mon, 11 Dec 2023 09:36:53 -0600 Subject: [PATCH] Escape an item in photometry docstring --- stellarphot/photometry/photometry.py | 5 ++--- 1 file changed, 2 insertions(+), 3 deletions(-) diff --git a/stellarphot/photometry/photometry.py b/stellarphot/photometry/photometry.py index b41df53e..4beb4e18 100644 --- a/stellarphot/photometry/photometry.py +++ b/stellarphot/photometry/photometry.py @@ -609,7 +609,7 @@ def multi_image_photometry(directory_with_images, reject_unmatched : bool, optional (Default: True) If ``True``, any sources that are not detected on all the images are rejected. If you are interested in a source that can intermittently - fall below your detection limits, we suggest setting this to ``False`` + fall below your detection limits, we suggest setting this to ``False`` so that all sources detected on each image are reported. include_dig_noise : bool, optional (Default: True) @@ -973,7 +973,7 @@ def calculate_noise(camera=None, counts=0.0, sky_per_pix=0.0, \\sigma = \\sqrt{G \\cdot N_C + A \\cdot \\left(1 + \\frac{A}{B}\\right)\\cdot \\left[ G\\cdot S + D \\cdot t + R^2 + (0.289 G)^2\\right]} - where :math:`\sigma` is the noise, :math:`G` is the gain, + where :math:`\\sigma` is the noise, :math:`G` is the gain, :math:`N_C` is the source counts (which is photon/electron counts divided by gain), :math:`A` is the aperture area in pixels, :math:`B` is the annulus area in pixels, @@ -1053,4 +1053,3 @@ def calculate_noise(camera=None, counts=0.0, sky_per_pix=0.0, digitization = area_ratio * (gain * 0.289) ** 2 return np.sqrt(poisson_source + sky + dark + rn_error + digitization) -