All configuration options¶
Below are all of the possible configuration settings. When being set by a configuration file,
they should be given as described in Setting the configuration, split by [Data]
and [Run]
. When being set
as keyword arguments, this split is not necessary, but each option should be passed
as the correct type.
If you do not set an option, the default value is taken instead. Options with a N/A default value are not optional and must be set by you.
Data options¶
Configuration option | Explanation | Default | Python type |
---|---|---|---|
data_path | Absolute path to the file containing your photometry. | N/A | str |
skip_data_rows | Number of columns to ignore at the top of the data file. | 0 | int |
data_is_csv | Flag of whether data is comma-separated. If
False , the data file is assumed to be whitespace
separated. |
False |
bool |
filter_path | Absolute path to the folder where the files describing your filters are stored. | Filter folder in the included resources. | str |
mag_cols | List of the columns in the data-file where the AB-magnitude of the source in each band is. Indices start at zero. | N/A | list of int |
sigma_cols | List of the columns in the data-file where the error on the AB-magnitude of the source in each band is. Indices start at zero. | N/A | list of int |
spec_z_col | The column in the data-file where the spectroscopic
redshift of the source is. If it’s not present in
the data-file, set to None . Indices start
at zero. |
None |
int or None |
ref_band | Index of the filter band (of the list of filters, not the data file column) that is considered the reference band, the band the priors are conditioned on, and where the soure magnitude is sampled. Indices start at zero. | N/A | int |
filters | List of paths to the filter files, relative to
filter_path , with file extensions. The
included filters are saved in files
without a file extension. |
N/A | list of str |
zero_point_errors | List of errors on the zero point calibration of each filter band. | N/A | list of float |
magnitude_limit | Value of the survey magnitude limit, fixed for
all galaxies. One of magnitude_limit or
magnitude_limit_col must be set. If both
are set. magnitude_limit is ignored. |
N/A | float |
magnitude_limit_col | Value of the survey magnitude limit, set
individually for each
galaxy. One of magnitude_limit or
magnitude_limit_col must be set. If both
are set. magnitude_limit_col
is preferred. |
N/A | int |
no_detect_value | Value of the data when an observation was made but the source was not detected. | 99.0 | float |
no_observe_value | Value of the data when an observation was not made. | -99.0 | float |
angular_resolution | Angular resolution of the data. Sources with a smaller angular separation than this are assumed to be blended (for the correlation function). In units of arcseconds. | N/A | float |
Run options¶
Configuration option | Explanation | Default | Python type |
---|---|---|---|
z_lo | Minimum redshift to sample. | 0 | float |
z_hi | Maximum redshift to sample. | 10 | float |
z_len | Length of redshift grid to calculate functions of redshift on before interpolating. | 1000 | int |
ref_mag_lo | Minimum magnitude to sample (numerically, i.e. the brightest magnitude). | N/A | float |
ref_mag_hi | Fixed maximum magnitude to sample (numerically,
i.e. the dimmest magnitude). One of
ref_mag_hi or ref_mag_hi_sigma must be
set. If both are set, ref_mag_hi is
ignored. |
N/A | float |
ref_mag_hi_sigma | Maximum magnitude to sample (numerically,
i.e. the dimmest magnitude) in terms of
reference band flux error. One of
ref_mag_hi or ref_mag_hi_sigma must be
set. If both are set, ref_mag_hi_sigma is
preferred. |
N/A | float |
template_set_path | Absolute path to the folder containing the template set file, as described in Specifying templates. Templates in the template set file are specified with a path relative to this. | Template folder in the included resources. | str |
template_set | File name of the template set file. | BPZ8 - The set of 8 templates from BPZ |
str |
sort_redshifts | Whether to use redshift sorting to break the
exchangability of blended posteriors. If
False , magnitude sorting is used. |
True |
bool |
omega_mat | Omega-matter cosmological parameter. | 0.3065 | float |
omega_lam | Omega-lambda cosmological parameter. | 0.6935 | float |
omega_k | Omega-k cosmological parameter. | float |
|
hubble | Hubble constant in km/s/Mpc. | 67.9 | float |
r0 | Constant of proportionality in correlation function power law. Units of Mpz/h. | float |
|
gamma | Exponent parameter in correlation function power law. | 1.77 | float |
prior_params | Array of prior parameters used in the
default prior function. Can be set to
None for being set by the prior
calibration described on Prior calibration. |
Parameters from Benitez (2000), plus 0.6 for the additional magnitude prior parameter. | list of float |