To send content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about sending content to .
To send content items to your Kindle, first ensure email@example.com
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about sending to your Kindle.
Note you can select to send to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
Phased Array Feed (PAF) technology is the next major advancement in radio astronomy in terms of combining high sensitivity and large field of view. The Focal L-band Array for the Green Bank Telescope (FLAG) is one of the most sensitive PAFs developed so far. It consists of 19 dual-polarization elements mounted on a prime focus dewar resulting in seven beams on the sky. Its unprecedented system temperature of ~17 K will lead to a 3 fold increase in pulsar survey speeds as compared to contemporary single pixel feeds. Early science observations were conducted in a recently concluded commissioning phase of the FLAG where we clearly demonstrated its science capabilities. We observed a selection of normal and millisecond pulsars and detected giant pulses from PSR B1937+21.
The Parkes pulsar data archive currently provides access to 144044 data files obtained from observations carried out at the Parkes observatory since the year 1991. Around 105 files are from surveys of the sky, the remainder are observations of 775 individual pulsars and their corresponding calibration signals. Survey observations are included from the Parkes 70 cm and the Swinburne Intermediate Latitude surveys. Individual pulsar observations are included from young pulsar timing projects, the Parkes Pulsar Timing Array and from the PULSE@Parkes outreach program. The data files and access methods are compatible with Virtual Observatory protocols. This paper describes the data currently stored in the archive and presents ways in which these data can be searched and downloaded.
In a note on Aesch. Ag. 1243 f. in C.R. lxxv (1961) 187-8, I had occasion to cite a number of examples of adverbial transference. Whether they were or were not (cf. C.R. lxxvii , 127) adequate to establish the point I was seeking to make I leave to the judgement of others, but the idiom possesses interest of its own, and it seems worth while to quote some further instances of it that I have noted since my article appeared. I will divide them according as they occur with verbs of hearing or with other verbs.
In C.Q. xliii (1949), p. 126, Messrs. Klos and Minio-Paluello write: ‘Burnet's and Robin's collations of W… differ for the text of the Phaedo in about 130 readings of a more than orthographical interest. A new inspection of the manuscript has shown that Robin very often corrected Burnet, but added some twenty mistakes.’ As this may give a false impression of Burnet as a collator, it will be well to recall Burnet's own statement in C.Q. xiv (1920), p. 132: ‘He [Wilamowitz] says (p. 333, n. 1) that my collations of W are inadequate, and have been shown to be so by Schoene for the Symposium, and by Hensel for the Theaetetus and Politicus. As he refers his readers to my Prefaces (p. 332, n. 3), he has presumably read them, and ought to have known that I never collated W at all or even saw it.’