How to use is_not_nan method in assertpy

Best Python code snippet using assertpy_python

lsst_single_exp_cat_match_aper_corr.py

Source:lsst_single_exp_cat_match_aper_corr.py Github

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1from astropy.io import ascii2import numpy as np3import matplotlib4matplotlib.use("TkAgg")5import matplotlib.pyplot as plt6import matplotlib.colors7from astropy.coordinates import SkyCoord8from astropy import coordinates as coords9import astropy.units as u10from astropy.io import fits11from astropy import wcs12from astropy.table import Table, vstack13sex_dir=("/Users/duhokim/work/abell/sex/cat/")14plot_dir=("/Users/duhokim/work/abell/plot/")15cat_dir=("/Users/duhokim/work/abell/cat/")16work_dir=("/Users/duhokim/work/abell/")17# lsst_dir=("/Users/duhokim/lsst_stack/demo_data_newinstall_decam/DATA/rerun/coaddForcedPhot/deepCoadd-results/")18# sav_dir=("/Users/duhokim/lsst_stack/demo_data_newinstall_decam/")19lsst_dir=("/Users/duhokim/lsst_stack/demo_data_orig_20_intersect/DATA/rerun/coaddForcedPhot/deepCoadd-results/")20sav_dir=("/Users/duhokim/lsst_stack/demo_data_orig_20_intersect/")21visit_nums = ['0350110', '0350835']22'''23patches = [24 ['0,2', '0,3', '0,4', '1,3', '1,4', '1,5', '2,2', '3,1', '3,3', '4,1', '4,2', '4,3',25 '4,5', '5,1', '5,2', '5,3', '5,5', '6,2', '6,3'],26 ['0,2', '0,3', '0,4', '1,3', '1,4', '1,5', '2,1', '2,2', '2,6', '3,0', '3,1', '3,3', '4,0', '4,1', '4,2', '4,3',27 '4,5', '5,2', '5,3', '5,5', '6,2', '6,3']28 ]29patches_all = ['0,2', '0,3', '0,4', '1,3', '1,4', '1,5', '2,2', '3,1', '3,3', '4,1', '4,2', '4,3', '4,5', '5,2', '5,3',30 '5,5', '6,2', '6,3']31'''32patches = [33 ['0,2', '0,3', '1,2', '2,2', '2,3', '3,2', '4,2', '5,2', '6,2'],34 ['0,2', '0,3', '1,1', '1,2', '2,0', '3,0', '3,1', '3,2', '4,0', '4,1', '4,2', '5,1', '5,2']35 ]36patches_all = ['0,2', '0,3', '1,2', '3,2', '4,2', '5,2']37ver = 'v1.1'38sdss_mag_sys = 'petroMag_'39sex_mag_sys = 'MAG_PETRO'40class_star_lim = 0.941mag_lim = [99, 99, 99] # limit magnitude for analysis42mag_ran = [25, 13]43clusters = ['A2670']44bands = ['g', 'r']45fn = ['60_0420', '300_0351']46single_dqm_fn = ['A2670_gd_60_0420_21aug.fits', 'A2670_rd_300_0351_19aug.fits']47exp = [60, 300]48seeing = ['1.28', '0.92']49X = [1.26, 1.41]50a = [0.179, 0.567]51b = [-0.036, -0.136]52# gal_ext = [ [0.159, 0.124, 0.086], # irsa.ipac.caltech.edu, S and F (2011)53# [0.188, 0.146, 0.101],54# [0.157, 0.122, 0.085]]55gal_ext = [0, 0]56max_sep = 1.057ccd_x = 204658ccd_y = 409459fig, axs = plt.subplots(2, 2, tight_layout = True, figsize = (10, 10))60sex_cat = ascii.read(sex_dir + 'DECam_19_21_aug_2014_single_best_exposure_SEx_cat_A2670_match_rad_1as_'61 'Gal_ext_corrected_' + ver + '.txt')62sex_coords = SkyCoord(sex_cat['ALPHA_J2000'], sex_cat['DELTA_J2000'], unit='deg')63for j in range(0, len(bands)):64 for i in range(0, len(patches[j])):65 rMags = np.load(sav_dir+bands[j]+'mag'+patches[j][i][0]+patches[j][i][2]+'.npy')66 lsst_all = Table.read(lsst_dir + bands[j] + '/0/' + patches[j][i] + '/forcedSrc-'+bands[j]+'-0-'+67 patches[j][i]+'.fits')68 is_not_nan = [(not np.isnan(rMags[x][0])) & (not np.isnan(rMags[x][1])) & (rMags[x][1] < 0.1) for x in range(0, len(rMags))]69 rMags = rMags[is_not_nan]70 lsst_all = lsst_all[is_not_nan]71 lsst_coords = SkyCoord(lsst_all['coord_ra'], lsst_all['coord_dec'], unit=(u.rad, u.rad))72 idx, d2d, d3d = sex_coords.match_to_catalog_sky(lsst_coords)73 sep_constraint = d2d.arcsec < max_sep74 sex_matches = sex_cat[sep_constraint]75 lsst_matches = rMags[idx[sep_constraint]]76 axs[0, j].scatter(sex_matches['MAG_AUTO_'+bands[j]],77 lsst_matches[:, 0],78 alpha=0.2, s=1)79 axs[0, j].scatter(sex_matches['MAG_AUTO_'+bands[j]],80 lsst_matches[:, 0],81 alpha=0.2, s=1)82for i in range(0, len(patches_all)):83 gMags = np.load(sav_dir+'gmag'+patches_all[i][0]+patches_all[i][2]+'.npy')84 rMags = np.load(sav_dir+'rmag'+patches_all[i][0]+patches_all[i][2]+'.npy')85 is_not_nan = [(not np.isnan(gMags[x][0])) & (not np.isnan(gMags[x][1])) & (not np.isnan(rMags[x][0])) &86 (not np.isnan(rMags[x][1])) & (gMags[x][1] < 0.1) & (rMags[x][1] < 0.1) for x in range(0, len(rMags))]87 if i == 0:88 lsst_g = gMags[is_not_nan, 0]89 lsst_r = rMags[is_not_nan, 0]90 else:91 lsst_g = np.append(lsst_g, gMags[is_not_nan, 0], axis=0)92 lsst_r = np.append(lsst_r, rMags[is_not_nan, 0], axis=0)93axs[1, 0].scatter(sex_cat['MAG_AUTO_'+bands[1]],94 sex_cat['MAG_AUTO_'+bands[0]] - sex_cat['MAG_AUTO_'+bands[1]],95 alpha=0.2, s=1, label='SEx (CLASS_STAR < 0.9 & DQM_cen = 0,128)')96axs[1, 1].scatter(lsst_r,97 lsst_g - lsst_r,98 alpha=0.2, s=1, label='LSST (merr < 0.1)')99axs[0, 0].plot(mag_ran, mag_ran, linestyle=':', alpha=0.5)100axs[0, 1].plot(mag_ran, mag_ran, linestyle=':', alpha=0.5)101axs[0, 0].text(27.5, 13, 'A2670', fontsize=24)102axs[0, 0].text(27.5, 13, 'A2670', fontsize=24)103axs[0, 0].set_title('g band (60s exposure)')104axs[0, 1].set_title('r band (300s exposure)')105axs[0, 0].set_xlabel('SEx (MAG_AUTO)')106axs[0, 1].set_xlabel('SEx (MAG_AUTO)')107axs[0, 0].set_ylabel('LSST (base_PsfFlux) (merr < 0.1)')108axs[0, 1].set_ylabel('LSST (base_PsfFlux) (merr < 0.1)')109axs[0, 0].set_xlim(mag_ran)110axs[0, 1].set_xlim(mag_ran)111axs[0, 0].set_ylim(mag_ran)112axs[0, 1].set_ylim(mag_ran)113axs[1, 0].set_xlabel('r')114axs[1, 0].set_ylabel('g-r')115axs[1, 0].set_xlim(mag_ran)116axs[1, 0].set_ylim([-3, 5])117axs[1, 0].legend()118axs[1, 1].set_xlabel('r')119axs[1, 1].set_ylabel('g-r')120axs[1, 1].set_xlim(mag_ran)121axs[1, 1].set_ylim([-3, 5])122axs[1, 1].legend()...

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lidar2d.py

Source:lidar2d.py Github

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1import numpy as np2from math import cos, sin3class LiDAR2D:4 def __init__(self, robot_ptr):5 # specification: default values from SICK TiM571 datasheet6 self.range_min = 0.05 # meter7 self.range_max = 8 # meter (actually this is the range typical of the sensor)8 # self.range_max = 25 #9 self.fov = 360 # in degree10 self.resolution = 2 # per degree11 self.angle_min_radian = lambda: - self.fov / 2 * np.pi / 180.12 self.angle_max_radian = lambda: + self.fov / 2 * np.pi / 180.13 self.angle_increment_radian = lambda: (1 / self.resolution) * np.pi / 18014 self.num_pts = lambda: self.fov * self.resolution15 self.scanning_freq = 15. # Hz16 self.time_increment = lambda: 1. / self.scanning_freq17 self.systematic_error_abs = 0.060 # m18 self.statistical_error = 0.020 # m19 self.data_type = np.float3220 self.robot_ptr = robot_ptr21 # scan results22 class Data:23 def __init__(self):24 self.last_rotated_rays = []25 self.last_points = []26 self.last_range_data = []27 self.last_intensities = []28 self.last_occupancy_gridmap = []29 self.occlusion_hist = dict((ii, []) for ii in range(10))30 self.data = Data()31 def scan(self, world):32 angles = np.deg2rad(np.arange(-self.fov / 2, self.fov / 2, 1 / self.resolution))33 rays_end = (np.array([np.cos(angles), np.sin(angles)]) * self.range_max).T34 rays_origin = np.zeros_like(rays_end)35 rays = np.stack([rays_origin, rays_end], axis=1)36 self.data.last_rotated_rays = rays37 # Rotate (to robot face)38 rot_matrix = np.array([[cos(self.robot_ptr.orien), -sin(self.robot_ptr.orien)],39 [sin(self.robot_ptr.orien), cos(self.robot_ptr.orien)]])40 self.data.last_rotated_rays[:, 1, :] = np.matmul(rot_matrix, self.data.last_rotated_rays[:, 1, :].transpose()).transpose()41 # Translate (to robot position)42 self.data.last_rotated_rays[:, 0, :] = self.data.last_rotated_rays[:, 0, :] + self.robot_ptr.pos43 self.data.last_rotated_rays[:, 1, :] = self.data.last_rotated_rays[:, 1, :] + self.robot_ptr.pos44 # scan the obstacles45 all_intersects = [self.data.last_rotated_rays[:, 1]]46 for obs in world.obstacles:47 results, intersect_pts_ = obs.intersect_many(self.data.last_rotated_rays)48 is_not_nan = 1 - np.any(np.isnan(intersect_pts_), axis=1)49 results = np.bitwise_and(results, is_not_nan)50 intersect_pts = np.stack([res * intersect_pts_[ii] + (1-res) * (self.range_max/np.sqrt(2) + self.robot_ptr.pos)51 for ii, res in enumerate(results)])52 all_intersects.append(intersect_pts)53 # scan the pedestrians54 for kk, ped in enumerate(world.crowds):55 dist = np.linalg.norm(ped.pos - self.robot_ptr.pos) - ped.radius56 # ignore the objects that are farther than max_range of the lidar from the robot57 if dist > self.range_max:58 continue59 ped_geometry = ped.geometry()60 results, intersect_pts_ = ped_geometry.intersect_many(self.data.last_rotated_rays)61 is_not_nan = 1 - np.any(np.isnan(intersect_pts_), axis=1)62 results = np.bitwise_and(results, is_not_nan)63 intersect_pts = np.stack([res * intersect_pts_[ii] + (1-res) * (self.range_max/np.sqrt(2) + self.robot_ptr.pos)64 for ii, res in enumerate(results)])65 all_intersects.append(intersect_pts)66 # combine the intersection points67 all_intersects = np.stack(all_intersects)68 dists = all_intersects - self.data.last_rotated_rays[0, 0]69 dists = np.linalg.norm(dists, axis=2)70 min_dist_idx = np.argmin(dists, axis=0)71 self.data.last_points = np.stack([all_intersects[ind, ii] for ii, ind in enumerate(min_dist_idx)])72 # Todo: add gaussian noise73 # which agents are occluded74 min_dist = np.min(dists, axis=0)75 for ii in range(len(world.obstacles), len(dists)):76 rays_might_have_hit_i = dists[ii] < (self.range_max - 1E-3)77 rays_have_hit_i = np.bitwise_and((dists[ii] - 1E-3) < min_dist, rays_might_have_hit_i)78 if np.sum(rays_might_have_hit_i) != 0:79 occ_i = 1 - np.sum(rays_have_hit_i) / (np.sum(rays_might_have_hit_i) + 1E-9)80 bin_idx = int(min(dists[ii]))81 else: # put it in the bin, out of lidar range (>8.0m)82 occ_i = 183 bin_idx = int(round(self.range_max))84 self.data.occlusion_hist[bin_idx].append(int(round(occ_i * 100)))85 self.data.last_range_data = np.sqrt(np.power(self.data.last_points[:, 0] - self.robot_ptr.pos[0], 2) +86 np.power(self.data.last_points[:, 1] - self.robot_ptr.pos[1], 2))87 # Todo: set lidar intensities...

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outlier_detection.py

Source:outlier_detection.py Github

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1import numpy as np2import fbprophet as fbp3import statsmodels.api as sm4def find_outliers_prophet(data):5 """Iteratively find outliers, excluding new outliers and refitting.6 Outlier: point lying outside interval_width of fitted model.7 :param data: Data.8 """9 df = data.get_df()10 outlier = np.zeros(len(df), dtype=bool)11 for i in range(data.n_iterations):12 m = fbp.Prophet(**{"interval_width": 0.99, **data.method_kws})13 m.fit(df)14 df_pred = m.predict(df)15 new_outlier = ((df_pred.yhat_lower > df.y) | (df_pred.yhat_upper < df.y)).values16 if new_outlier.sum() == 0:17 break18 df.loc[outlier, "y"] = np.nan19 outlier |= new_outlier20 df_pred["outlier"] = outlier21 return m, df_pred22def find_outliers_lowess(data):23 """Iteratively find outliers, excluding new outliers and refitting.24 Outlier: Point which has large residual compared to nearby (=rolling window) points.25 :param data: Data.26 """27 frac = data.method_kws.get("frac", 1 / 5)28 outlier_n_std = data.method_kws.get("outlier_n_std", 2.5)29 rolling_window_size = data.method_kws.get("rolling_window_size")30 rolling_window_min_periods = data.method_kws.get("rolling_window_min_periods", 4)31 # Minimum requirements for window32 rolling_window_size = rolling_window_size or max(int(frac * len(data.y)), 2)33 rolling_window_min_periods = min(rolling_window_min_periods, rolling_window_size)34 df = data.get_df()35 df["y_orig"] = df.y36 outlier = np.zeros(len(df), dtype=bool)37 for i in range(data.n_iterations):38 y_lowess = sm.nonparametric.lowess(df.y, df.ds, frac=frac, return_sorted=False)39 df["res"] = (df.y_orig - y_lowess).abs()40 # Use rolling window to allow for changes in noise level over "time"41 rolling = df.res.rolling(rolling_window_size, min_periods=rolling_window_min_periods, center=True)42 df["res_ma"] = rolling.mean().bfill().ffill()43 df["res_mstd"] = rolling.std().bfill().ffill()44 # Classify datapoints far from rolling mean as outliers45 new_outlier = (df.res - df.res_ma).abs() > outlier_n_std * df.res_mstd46 if new_outlier.sum() == 0:47 break48 outlier |= new_outlier49 df["y"] = df.y_orig50 df.loc[outlier, "y"] = np.nan51 df["yhat"] = y_lowess52 df["yhat_upper"] = df.yhat + outlier_n_std * np.abs(df.res_mstd)53 df["yhat_lower"] = (df.yhat - outlier_n_std * np.abs(df.res_mstd))54 # Interpolation for outliers55 is_nan, is_not_nan = np.isnan(y_lowess), ~np.isnan(y_lowess)56 x = np.arange(len(df))57 for col in ("yhat", "yhat_upper", "yhat_lower"):58 df[col] = np.interp(x, x[is_not_nan], df[col][is_not_nan])59 # Cleanup60 df.drop(columns=["y_orig", "res", "res_ma", "res_mstd"], inplace=True)61 df["outlier"] = outlier62 return None, df63def find_outliers(data):64 if data.method == "prophet":65 m, df_pred = find_outliers_prophet(data)66 elif data.method == "lowess":67 m, df_pred = find_outliers_lowess(data)68 else:69 raise ValueError("Invalid method (%s)!" % data.method)...

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