Difference between revisions of "WormBase Staff Resources"
(→Blog) |
|||
Line 23: | Line 23: | ||
= Contacts = | = Contacts = | ||
− | = | + | = Social Media = |
+ | == Blog == | ||
+ | |||
+ | The official WormBase blog is called "M9": | ||
+ | |||
+ | http://blog.wormbase.org/ | ||
+ | |||
+ | This is our primary vehicle for communication with users. You can subscribe to the blog via email at: | ||
+ | |||
+ | http://feedburner.google.com/fb/a/mailverify?uri=wormbase&loc=en_US | ||
+ | |||
+ | == Twitter == | ||
+ | |||
+ | Our Twitter account is: | ||
+ | |||
+ | http://twitter.com/wormbase | ||
+ | |||
+ | We have a secondary account for source code commits: | ||
+ | |||
+ | http://twitter.com/wormbase-commits | ||
= Issue Tracker = | = Issue Tracker = |
Revision as of 15:32, 10 November 2010
This document describes collaborative tools available to WormBase team members.
Contents
Accounts
To begin, you should request a wormbase.org account [1].
This account will automatically give you access to WormBase documents, discussion groups, calendars, chat, voice, and contact information.
Groups (Mailing Lists)
WormBase uses a number of mailing lists for discussion. You can manage subscriptions yourself, post from the web, etc.
Creating your own discussion group
With your wormbase.org account, you can create your own groups, a perfect way to support new projects. By default discussion within a group is archived, a feature which can be disabled if desired. See the groups main page for details.
Calendar
Documents
Contacts
Social Media
Blog
The official WormBase blog is called "M9":
This is our primary vehicle for communication with users. You can subscribe to the blog via email at:
http://feedburner.google.com/fb/a/mailverify?uri=wormbase&loc=en_US
Our Twitter account is:
We have a secondary account for source code commits:
http://twitter.com/wormbase-commits
Issue Tracker
You can follow and track issues at:
https://bitbucket.org/tharris/wormbase/issues?status=new&status=open
Source Code
Source code is currently maintained in Mercurial (hg):