Add Pedantic to crate requirements

CHANGELOG.md

@@ -16,6 +16,8 @@ and this project adheres to [Semantic Versioning](https://semver.org/spec/v2.0.0
 
 ### Changed
 
+- Rewrite of NEATM and FRM internal models, remove support for saving files related
+  to thermal and optical models.
 - Throughout the rust code, `Time` is being enforced as inputs for functions instead
   of accepting `f64` in a large number of places.
 

Cargo.toml

@@ -76,12 +76,22 @@ rust.trivial_casts = "deny"
 rust.elided_lifetimes_in_paths = "deny"
 rust.unexpected_cfgs = "deny"
 
-clippy.too_many_arguments = "allow"
-clippy.type_complexity = "allow"
 
 clippy.perf = { level = "deny", priority = 1 }
-# clippy.pedantic = { level = "warn", priority = 1 }
+clippy.pedantic = { level = "deny", priority = 1 }
+
+# Pedantic overrides
+clippy.float_cmp = {level = "allow", priority = 2 }
+clippy.inline_always = {level = "allow", priority = 2 }
+clippy.unreadable-literal = {level = "allow", priority = 2}
+clippy.similar_names = {level = "allow", priority = 2}
+clippy.too_many_lines = {level = "allow", priority = 2}
+clippy.cast_precision_loss = {level = "allow", priority = 2}
+clippy.cast_possible_truncation = {level = "allow", priority = 2}
 
+# General list
+clippy.too_many_arguments = "allow"
+clippy.type_complexity = "allow"
 clippy.allow_attributes_without_reason = "warn"
 clippy.collection_is_never_read = "warn"
 clippy.dbg_macro = "warn"
@@ -102,4 +112,10 @@ clippy.use_self = "warn"
 clippy.cargo_common_metadata = "warn"
 clippy.negative_feature_names = "warn"
 clippy.redundant_feature_names = "warn"
-clippy.wildcard_dependencies = "warn"
+clippy.wildcard_enum_match_arm = "warn"
+clippy.wildcard_dependencies = "warn"
+clippy.fallible_impl_from = "warn"
+clippy.unneeded_field_pattern = "warn"
+clippy.fn_params_excessive_bools = "warn"
+
+clippy.must_use_candidate = "deny"

src/kete/plot.py

@@ -43,8 +43,7 @@ def plot_fits_image(fit, percentiles=(0.1, 99.95), power_stretch=1.0, cmap="gray
         `ZScaleInterval`.
     power_stretch :
         The scaling of the intensity of the plot is a power law, this defines the power
-        of that power law. By default plots are sqrt scaled. If this is set to 1, then
-        this becomes a linear scaling.
+        of that power law. By default plots are linear scaled (`power_stretch=1.0`).
     cmap :
         Color map to use for the plot.
     """

src/kete/rust/fitting.rs

@@ -14,5 +14,5 @@ pub fn ks_test_py(sample_a: Vec<f64>, sample_b: Vec<f64>) -> f64 {
 #[pyo3(name = "fit_chi2")]
 pub fn fit_chi2_py(data: Vec<f64>, sigmas: Vec<f64>) -> f64 {
     assert_eq!(data.len(), sigmas.len());
-    fitting::fit_reduced_chi2(&data, &sigmas)
+    fitting::fit_reduced_chi2(&data, &sigmas).unwrap()
 }

src/kete/rust/flux/common.rs

@@ -1,3 +1,5 @@
+use core::f64;
+
 use crate::{frame::PyFrames, vector::VectorLike};
 use itertools::Itertools;
 use kete_core::constants::{
@@ -232,7 +234,7 @@ pub fn neatm_thermal_py(
     diameter: f64,
     wavelength: f64,
     emissivity: f64,
-) -> f64 {
+) -> PyResult<f64> {
     let sun2obj = sun2obj.into_vector(PyFrames::Ecliptic).into();
     let sun2obs = sun2obs.into_vector(PyFrames::Ecliptic).into();
 
@@ -246,17 +248,13 @@ pub fn neatm_thermal_py(
     )
     .unwrap();
     let params = NeatmParams {
-        obs_bands: ObserverBands::Generic {
-            bands: vec![wavelength; 1],
-            zero_mags: None,
-            solar_correction: vec![1.0],
-        },
-        band_albedos: vec![0.0; 1],
+        obs_bands: vec![BandInfo::new(wavelength, 1.0, f64::NAN, None)],
+        band_albedos: vec![0.0],
         hg_params,
         emissivity,
         beaming,
     };
-    params.apparent_thermal_flux(&sun2obj, &sun2obs).unwrap()[0]
+    Ok(params.apparent_thermal_flux(&sun2obj, &sun2obs).unwrap()[0])
 }
 
 /// Calculate the flux from an object using the FRM thermal model in Jansky.
@@ -300,7 +298,7 @@ pub fn frm_thermal_py(
     diameter: f64,
     wavelength: f64,
     emissivity: f64,
-) -> f64 {
+) -> PyResult<f64> {
     let sun2obj = sun2obj.into_vector(PyFrames::Ecliptic).into();
     let sun2obs = sun2obs.into_vector(PyFrames::Ecliptic).into();
     let hg_params = HGParams::try_new(
@@ -310,20 +308,15 @@ pub fn frm_thermal_py(
         Some(C_V),
         Some(v_albedo),
         Some(diameter),
-    )
-    .unwrap();
+    )?;
 
     let params = FrmParams {
-        obs_bands: ObserverBands::Generic {
-            bands: vec![wavelength; 1],
-            zero_mags: None,
-            solar_correction: vec![1.0],
-        },
-        band_albedos: vec![0.0; 1],
+        obs_bands: vec![BandInfo::new(wavelength, 1.0, f64::NAN, None)],
+        band_albedos: vec![0.0],
         hg_params,
         emissivity,
     };
-    params.apparent_thermal_flux(&sun2obj, &sun2obs).unwrap()[0]
+    Ok(params.apparent_thermal_flux(&sun2obj, &sun2obs).unwrap()[0])
 }
 
 /// Given the M1/K1 and M2/K2 values, compute the apparent Comet visible magnitudes.
@@ -421,7 +414,7 @@ pub fn w4_color_correction_py(temp: f64) -> f64 {
 /// The normal vectors of the fib lattice
 #[pyfunction]
 #[pyo3(name = "fib_lattice_vecs")]
-pub fn fib_lattice_vecs_py(n_facets: usize) -> Vec<[f64; 3]> {
+pub fn fib_lattice_vecs_py(n_facets: u32) -> Vec<[f64; 3]> {
     let facets = ConvexShape::new_fibonacci_lattice(n_facets).facets;
     facets
         .iter()