Loading README +10 −8 Original line number Diff line number Diff line Loading @@ -2,10 +2,11 @@ Reproduction pipeline for Section 4 of "The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection", Bacon et al. (2017), A&A 608, A1. The purpose of this reproduction pipline is to show the calibration of pseudo-broad-band images created from MUSE data cubes with HST's broad-band images. For any issues with the pipeline, please contact Mohammad Akhlaghi at `mohammad@akhlaghi.org'. The purpose of this reproduction pipline is to show the photometric and astrometric calibration of pseudo-broad-band images created from the MUSE data cubes described in the paper with HST's broad-band images of the same field. For any issues with the pipeline, please contact Mohammad Akhlaghi at `mohammad@akhlaghi.org'. Loading Loading @@ -70,10 +71,11 @@ difference. Gnuastro is a large collection of programs for astronomical data analysis on the command-line. This is an intermediate version of Gnuastro (the tarball is not officially released on the Gnuastro webpage). But for convenience, this tarball is available in the webpage). However, this pipeline will ONLY work with this version of Gnuastro. But for convenience, this tarball is available in the following link: https://doi.org/10.5281/zenodo.1163746 https://zenodo.org/record/1163746/files/gnuastro-0.2.51-bc56.tar.gz To uncompress, build and install the Gnuastro tarball, follow the instructions here: Loading @@ -89,8 +91,8 @@ difference. $ git checkout bc565a5 Afterwords, you need to bootstrap Gnuastro as described in the following link. Afterwards, you can configure and build it as in the link above. following link and configure and build it as described in the link above. https://www.gnu.org/software/gnuastro/manual/html_node/Bootstrapping.html Loading Loading
README +10 −8 Original line number Diff line number Diff line Loading @@ -2,10 +2,11 @@ Reproduction pipeline for Section 4 of "The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection", Bacon et al. (2017), A&A 608, A1. The purpose of this reproduction pipline is to show the calibration of pseudo-broad-band images created from MUSE data cubes with HST's broad-band images. For any issues with the pipeline, please contact Mohammad Akhlaghi at `mohammad@akhlaghi.org'. The purpose of this reproduction pipline is to show the photometric and astrometric calibration of pseudo-broad-band images created from the MUSE data cubes described in the paper with HST's broad-band images of the same field. For any issues with the pipeline, please contact Mohammad Akhlaghi at `mohammad@akhlaghi.org'. Loading Loading @@ -70,10 +71,11 @@ difference. Gnuastro is a large collection of programs for astronomical data analysis on the command-line. This is an intermediate version of Gnuastro (the tarball is not officially released on the Gnuastro webpage). But for convenience, this tarball is available in the webpage). However, this pipeline will ONLY work with this version of Gnuastro. But for convenience, this tarball is available in the following link: https://doi.org/10.5281/zenodo.1163746 https://zenodo.org/record/1163746/files/gnuastro-0.2.51-bc56.tar.gz To uncompress, build and install the Gnuastro tarball, follow the instructions here: Loading @@ -89,8 +91,8 @@ difference. $ git checkout bc565a5 Afterwords, you need to bootstrap Gnuastro as described in the following link. Afterwards, you can configure and build it as in the link above. following link and configure and build it as described in the link above. https://www.gnu.org/software/gnuastro/manual/html_node/Bootstrapping.html Loading