From a4442a04e62a3ce74ee65402f15205ef97667736 Mon Sep 17 00:00:00 2001 From: Adam Carnall Date: Sun, 14 May 2017 21:36:29 +0100 Subject: [PATCH 1/4] Update README.md --- README.md | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/README.md b/README.md index cf23d0b..1519e82 100644 --- a/README.md +++ b/README.md @@ -8,7 +8,7 @@ An article explaining the method the code employs will be published at www.ArXiv ## Installation -The code is essentially pretty simple and so is currently formatted as a single Python function. If you want the function to be available to your other Python scripts, either copy the _spectres.py_ file into the directory containing the scripts, or you can add the directory you clone the repository into to your **PYTHONPATH** variable. +The code is currently formatted as a single Python function. If you want the function to be available to your other Python scripts, either copy the _spectres.py_ file into the directory containing the scripts, or you can add the directory you clone the repository into to your **PYTHONPATH** variable. ## Using The Code From dfa8eeff4ca68669bf49b09ca05ac53e14c145a4 Mon Sep 17 00:00:00 2001 From: Adam Carnall Date: Sun, 14 May 2017 21:37:53 +0100 Subject: [PATCH 2/4] Update README.md --- README.md | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/README.md b/README.md index 1519e82..fb9773c 100644 --- a/README.md +++ b/README.md @@ -8,7 +8,7 @@ An article explaining the method the code employs will be published at www.ArXiv ## Installation -The code is currently formatted as a single Python function. If you want the function to be available to your other Python scripts, either copy the _spectres.py_ file into the directory containing the scripts, or you can add the directory you clone the repository into to your **PYTHONPATH** variable. +The code is currently formatted as a single Python function. If you want the function to be available to your other Python scripts, either copy the _spectres.py_ file into the directory containing the scripts, or you can add the directory containing it to your **PYTHONPATH** variable. ## Using The Code From bf611b4949c9111d9216d96bd3e40109be5d930e Mon Sep 17 00:00:00 2001 From: Adam Carnall Date: Tue, 16 May 2017 11:26:47 +0100 Subject: [PATCH 3/4] Update README.md --- README.md | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/README.md b/README.md index fb9773c..1ef1039 100644 --- a/README.md +++ b/README.md @@ -4,7 +4,7 @@ SpectRes is a Python function which efficiently resamples spectra and their asso This may be of use for binning data to increase the signal to noise ratio, obtaining synthetic photometry, or resampling model spectra to match the sampling of observed data for spectral energy distribution fitting. -An article explaining the method the code employs will be published at www.ArXiv.org in the coming days. If you make use of the code in your research, please cite this article in any publications. +An article explaining the method the code uses is available at https://arxiv.org/abs/1705.05165. If you make use of the code in your research, please cite this article in any publications. ## Installation From 5027c60cb4601e3cc930c6ef95e12baab71574ad Mon Sep 17 00:00:00 2001 From: Adam Carnall Date: Tue, 23 May 2017 14:03:07 +0100 Subject: [PATCH 4/4] Update README.md --- README.md | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/README.md b/README.md index 1ef1039..9d6ef5c 100644 --- a/README.md +++ b/README.md @@ -18,4 +18,4 @@ The function returns an array, _**resampled**_ containing the resampled spectrum ## Example Files -Two examples are provided, the first resamples the spectrum of a high redshift quasar from Carnall et al. (2015) onto a coarser wavelength grid (bins the data) in order to improve the signal to noise ratio. The second resamples a whole grid of BC03 models (available at http://www.bruzual.org/bc03) onto a new wavelength grid. +Two examples are provided, the first rebins the spectrum of a high redshift quasar from Carnall et al. (2015) onto a coarser wavelength grid (bins the data) in order to improve the signal to noise ratio. The second resamples a whole grid of BC03 models (available at http://www.bruzual.org/bc03) onto a new wavelength grid.