In order to enable an iCal export link, your account needs to have an API key created. This key enables other applications to access data from within Indico even when you are neither using nor logged into the Indico system yourself with the link provided. Once created, you can manage your key at any time by going to 'My Profile' and looking under the tab entitled 'HTTP API'. Further information about HTTP API keys can be found in the Indico documentation.
Additionally to having an API key associated with your account, exporting private event information requires the usage of a persistent signature. This enables API URLs which do not expire after a few minutes so while the setting is active, anyone in possession of the link provided can access the information. Due to this, it is extremely important that you keep these links private and for your use only. If you think someone else may have acquired access to a link using this key in the future, you must immediately create a new key pair on the 'My Profile' page under the 'HTTP API' and update the iCalendar links afterwards.
Permanent link for public information only:
Permanent link for all public and protected information:
(Institute of Astronomy, National Tsing Hua University, Taiwan)
The evolutionary and formation of millisecond pulsars (MSPs) has long
been a subject of inquiry, and one widely accepted version is that an
old neutron star has been spun up to a spin period on the order of
millisecond via accretion from a late-type companion which transferred
mass and angular momentum to the pulsar. Once the accretion has
stopped, the relativistic, strongly magnetized pulsar wind will
possibly carry away the pulsar rotational energy and angular momentum, meanwhile ablate and eventually evaporate its companion. It is generally believed that radio MSPs can only be turned on when the mass transfer from the companion star is extremely low. However, the
observational evidence of such transition has not been found until
recently. In this talk, I will review recent discoveries of "transformer" MSPs that switch between low-mass X-ray binaries and radio MSPs. I will also discuss how multi-wavelength observations reveal a new population of black widow/redback MSPs that provides new
insight into MSP's emission mechanisms and the physics of compact