jpstroop

# (Paste into your bash .profile or whatever you use)
#
#   $ asdf which python
#   /Users/jstroop/.asdf/installs/python/3.8.5/bin/python # version in .tool-versions
#   $ asdf which python 3.7.6
#   /Users/jstroop/.asdf/installs/python/3.7.6/bin/python # version from 3rd arg
#
# NOTE: Python < 3.11-dev does not compile on Apple silicon.
#       See: https://bugs.python.org/issue43878. 
#       Use Rosetta if necessary.

jpstroop

Setting up Network UPS Tools (NUT) at Home

Note that these instructions use offensive master/slave terminology because they are still necessary keywords in the NUT configuration files. There is work in progress to change this. I am going to use server and client whenever I can, but you can't avoid master/slave in upsd.users or upsmon.conf.

Given two UPS's:

• CyberPower CP850PFCLCD
• CyberPower CP1000PFCLCD

And a Raspberry Pi, I'm setting up my home network and critical hardware to shutdown gracefully when the power fails.

jpstroop

#!/bin/bash

# Script takes a single argument, which is a path in an image file.
# NOTE: this file will be replaced with the version that this script deems to be 'correct'
file=$1

TMP="/tmp/pulfa/img_harvester/rotation-calc"
# Clean up if there are files from the last run
# (leaving them around is handy for debugging)
if [ -d $TMP ]; then

jpstroop

#!/bin/bash
for md_file in $(find . -name "*.md"); do
  gsed -r -i -e 's/([A-z])\.\s{2,3}([A-Z])/\1. \2/g' $md_file
done

jpstroop

{
  "@context": "http://iiif.io/api/presentation/2/context.json",
  "id": "https://plum.princeton.edu/concern/scanned_resources/pt722jw092/manifest",
  "type": "sc:Manifest",
  "label": [
    "Reports of the Princeton University expeditions to Patagonia, 1896-1899 : J. B. Hatcher in charge"
  ],
  "viewingHint": "paged",
  "viewingDirection": "left-to-right",
  "rendering": {

jpstroop

#!/usr/bin/env python
#
# Unwatch from all Github repositories. Note that it will only work with up to
# 100 repos at a time (pagination is not implemented), so you may need to run
# more than once.
#
# Depends:
#  requests : http://docs.python-requests.org/en/master/
#
# Output (to stdout):

jpstroop

Deprecated. Moved here: https://docs.google.com/document/d/1GY9_CfvFb5WCFOoSQ54DwzoMKPXmh5UrBgBuN5QXjUg/edit#

Proposed Flow

0. Talk to RBSC cat.
1. Enhace EAD w/ item level data from TEI. Including pudl0123 IDs temporarily
2. Use TEI to EAD mapping to reorg. images to match new EAD (item level) components
3. Remove temporary pudl0123 IDs from new EAD components
4. Generate new PULFA METS and load EAD
5. Migration New PULFA METS to Plum - Make sure EAD component ID is in dc:replaces
6. Map Plum manifest URIs back to TEI

jpstroop

IIIF Aggregation, Discovery, and Import

Introduction

Audience and Scope

• Carefully acknowledge somehow that this extends the scope of IIIF, but is at least controlled mission creep (i.e. similar to a controlled burn :-))

• Use cases:

  • thematic registries and portals

• ad-hoc reuse/remixing/mashups

jpstroop

from PIL import Image
from PIL.ExifTags import GPSTAGS
from PIL.ExifTags import TAGS

# Keys are listed here:
# https://github.com/python-pillow/Pillow/blob/master/PIL/ExifTags.py

def _map_key(k):
    try:
        return TAGS[k]

jpstroop

$ kdu_expand -quiet -i 0001.jp2 -o 0001.bmp -reduce 0; identify 0001.bmp
0001.bmp BMP3 5906x7200 5906x7200+0+0 8-bit sRGB 127.6MB 0.120u 0:00.129
$ opj_decompress -i 0001.jp2 -o 0001.bmp -r 0; identify 0001.bmp
0001.bmp BMP3 5906x7200 5906x7200+0+0 8-bit sRGB 127.6MB 0.120u 0:00.129

$ kdu_expand -quiet -i 0001.jp2 -o 0001.bmp -reduce 1; identify 0001.bmp
0001.bmp BMP3 2953x3600 2953x3600+0+0 8-bit sRGB 31.9MB 0.030u 0:00.040
$ opj_decompress -i 0001.jp2 -o 0001.bmp -r 1; identify 0001.bmp
0001.bmp BMP3 2953x3600 2953x3600+0+0 8-bit sRGB 31.9MB 0.030u 0:00.040