We lifted 17 functions out of this paper's own repositories and ran 7 of them in a sandbox. "Ran" means the function executed on a synthesized input and returned a value. It is not a reproduction of the paper's results.
| Repository | Role | Ran |
|---|---|---|
| rmgarnett/gp_dla_detection | canonical | 7 of 13 |
| yishayv/lyacorr | pwc_unofficial | 0 of 4 |
| Function | Status | Where it lives |
|---|---|---|
| Gaussian | Ran | rmgarnett/gp_dla_detection/CDDF_analysis/voigt.py code served (permissive licence) · get_code("a57bc207f6ddcefd") |
| Lorentzian | Ran | rmgarnett/gp_dla_detection/CDDF_analysis/voigt.py code served (permissive licence) · get_code("ea5f29cc0aa083e3") |
| Voigt | Ran | rmgarnett/gp_dla_detection/CDDF_analysis/voigt.py code served (permissive licence) · get_code("8aeede7dbc9a3695") |
| do_MAP_Garnett_comparison | Ran | rmgarnett/gp_dla_detection/CDDF_analysis/make_multi_dla_plots.py code served (permissive licence) · get_code("76072d8283565983") |
| format_latex_num | Ran | rmgarnett/gp_dla_detection/CDDF_analysis/make_tables.py code served (permissive licence) · get_code("ac127482fcea809e") |
| format_latex_two_num | Ran | rmgarnett/gp_dla_detection/CDDF_analysis/make_tables.py code served (permissive licence) · get_code("a4b05b4034087806") |
| search_index_from_another | Ran | rmgarnett/gp_dla_detection/CDDF_analysis/qso_loader.py code served (permissive licence) · get_code("1565258e3ade9752") |
| downsample_spectrum | Not yet run | yishayv/lyacorr/calc_mean_transmittance.py code served (permissive licence) · get_code("51a17680901e801c") |
| find_pixel_noise | Not yet run | rmgarnett/gp_dla_detection/CDDF_analysis/calc_cddf.py code served (permissive licence) · get_code("222bf414dd90e625") |
| find_pixel_snr | Not yet run | rmgarnett/gp_dla_detection/CDDF_analysis/calc_cddf.py code served (permissive licence) · get_code("182da4fc0eea4948") |
| find_snr | Not yet run | rmgarnett/gp_dla_detection/CDDF_analysis/calc_cddf.py code served (permissive licence) · get_code("1c50a1f41e00583e") |
| fit_function | Not yet run | yishayv/lyacorr/continuum_goodness_of_fit.py code served (permissive licence) · get_code("ec69220b26d8f0f7") |
| generate_qsos | Not yet run | rmgarnett/gp_dla_detection/CDDF_analysis/make_multi_dla_plots.py code served (permissive licence) · get_code("a7449f1591071b7d") |
| generate_qsos_lyseries | Not yet run | rmgarnett/gp_dla_detection/CDDF_analysis/make_multi_dla_plots.py code served (permissive licence) · get_code("d30953e8080cd285") |
| load_table | Not yet run | rmgarnett/gp_dla_detection/CDDF_analysis/make_tables.py code served (permissive licence) · get_code("64806c35f9a763ad") |
| max_delta_f_per_snr | Not yet run | yishayv/lyacorr/continuum_goodness_of_fit.py code served (permissive licence) · get_code("45246b62a58b5893") |
| rescale | Not yet run | yishayv/lyacorr/delta_transmittance_remove_mean.py code served (permissive licence) · get_code("8f9d07f118f46224") |
Some links come from the archived Papers with Code dataset (CC BY-SA 4.0): attribution and licence.
We develop an automated technique for detecting damped Lyman-$α$ absorbers (DLAs) along spectroscopic lines of sight to quasi-stellar objects (QSOs or quasars). The detection of DLAs in large-scale spectroscopic surveys such as SDSS-III sheds light on galaxy formation at high redshift, showing the nucleation of galaxies from diffuse gas. We use nearly 50 000 QSO spectra to learn a novel tailored Gaussian process model for quasar emission spectra, which we apply to the DLA detection problem via Bayesian model selection. We propose models for identifying an arbitrary number of DLAs along a given line of sight. We demonstrate our method's effectiveness using a large-scale validation experiment, with excellent performance. We also provide a catalog of our results applied to 162 858 spectra from SDSS-III data release 12.
The same record, over MCP at https://syntology.ai/mcp:
get_harvested_code_for_paper("1605.04460")
get_code_for_paper("1605.04460")
have("1605.04460")
Connect an agent — have() is free.