cmpute

/* 
 * OJ中加速IO常用的代码片段
 * Author Jacob C
 * THU_ID 2014010812
 */

//OJ中常用的头文件和预编译指令
#ifndef _OJ_
#define DEBUG
#endif

cmpute

import os
import os.path as op

# Paths can be user-defined
pcl_dir = os.environ["PCL_ROOT"]
pcl_ver = pcl_dir.split(' ')[-1]
vctool_ver = list(filter(lambda part: part.startswith('vc'),
    os.listdir(op.join(pcl_dir, '3rdParty', 'Boost', 'lib'))[0].split('-')))[0] #vc140
openni_dir = op.sep.join(os.environ['OPENNI2_LIB64'].split(op.sep)[:-2])

cmpute

'''
Interface for caltrans data repo
'''

import os
import os.path as osp

_default_data_root = 'E:\\Data\\Caltrans_2010-2012'

class _DirIndexer():

cmpute

# This script only works when Google Drive is mounted at G:\
# Change the encoding to UTF-8-BOM before executing this script
# To run this file: powershell -noprofile -executionpolicy bypass -file ./PinGoogleDriveFS.ps1 [add/remove]

# Settings
$ErrorActionPreference = "Stop"
$clsid     = "{81539FE6-33C7-4CE7-90C7-1C7B8F2F2D41}" # CLSID for personal drive namespace
$clsid_i   = "{0E5AAE11-A475-4c5b-AB00-C66DE400274E}" # CLSID for personal drive instance
$clsid_g   = "{FB9411E2-c3F8-4004-BA95-47D459C219D1}" # CLSID for shared drive namespace
$clsid_g_i = "{1A223FF4-D08D-4B38-A051-5D2391FE655C}" # CLSID for shared drive instance

cmpute

import filecmp
import os.path as osp

dir_a = "E:/"
dir_b = "F:/"

def print_diff_files(dcur, dcmp):
     for name in dcmp.diff_files:
         print("[diff_file @ %s ] %s" % (dcur, name))
     for name in dcmp.left_only:

cmpute

This script is a tool to manual calibrate image and lidar point cloud.

Requirements:

numpy, scipy>=1.2.0, cv2 (opencv),

Input/Output

The input is specified by the variable image_in and cloud_in, the value of these two variables have to be either a path to the file, or a path to the folder containing the data. Point cloud should be stored in txt format with points value starting from the second row. (This could be modified in the code) The output contains three translation parameters (x,y,z) and three rotation parameters (roll,pitch,yaw). The calibration output will be printed when the calibration process finishes.

Usage

cmpute

import os, sys
import os.path as osp
import cv2
from cv_bridge import CvBridge
import rosbag
import sensor_msgs
import sensor_msgs.point_cloud2 as pc
import zipfile
import tqdm

cmpute

'''
Before running the scripts, please set page loading order to descending by post date (instead of reply date)
'''

import browsercookie
import sqlalchemy
import tqdm
from random import uniform
from itertools import count as icount
from time import sleep

cmpute

#!/usr/bin/env /usr/bin/python3

import argparse
import os
import signal
import tarfile
import time
import zipfile
from itertools import count
from multiprocessing import Pool, Manager

cmpute

Delete all remote branches

git branch -r | grep <remote> | cut -c 10- | xargs -n 10 git push <remote> --delete

Useful for clean forked repository. 10 in cut -c 10- here represents the length of string <remote>\ 10 in xargs -n 10 represents how many branch to delete at a time, sometimes detele will report error, so less branches a time can reduces number of branched to be deleted manually