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This page contains a list of the major events for the PPTA project. These include changes to the instrumentation of software that affect the observations in blue , major publications and other useful dates. Timing properties not predicted to be different.

Data from 1st Jan until this date will therefore be affected. Limited configs and still instrumental problems. Attenuator settings moved to digstats table. Gal l,b, PA, FA, parang, tel coords added to subint table. For and chan, no correction was applied. The actual delays fluctuate around these values by ns or so. Occasional instances of alt-mode TCS giving incorrect sign of bw e. Spectrum remains inverted despite bw sign. The actual d2 delays see 16 March above are halved.

For MHz, chan the actual delay is 4. Input power increased by about 10db to compensate, bringing rms levels back to RMS levels multiplied by sqrt 8 to restore to correct value. Previously middle of 1st subint, now original value. Most recent firmware with PTU on-board. Largely fixed by JR inserting 8m cable in 5 MHz line. Amplifier bypassed since approx unity gain overall.

Another 8m cable added by JR. Reset bug introduced so that folding period not updated leading to phase drift during observation. Also intermittent phase jumps introduced due to sync problem in PTU firmware. V4 MJD Data are OK. Uses Ver 4. Start of good APSR data. Clock lost lock at MJD Reset to Only pulsars with DM1 entries in par file were affected. J added to ppta. Snake cables on MB receiver replaced.

Problems at cable-connector interface, causing intermittent bad connections. Data from MJD GH gave talk via skype. Effective RF MHz. Reinstalled 3 July. Organised by PPTA collaboration members.

Highlight of school was Pulse Parkes timing masterclass. Also changes to BAT wiring after clock; effect should be 20ns or less. Among other things, clock maser failed. Reset by Brett P. Fixes problems with search mode: spurious blocks at EoF for 1-bit mode, first sample zero, channel offset for first block. Dick Manchester attended Friday.

Mike Keith presented a talk via proxy GH. This required updates to psrcat, tempo2 and T2psrcoeff. The various catalogue files were all moved to a new location and the most up to date versions of tempo2 etc. Should be CAL mode so atten not reset. Schedule fixed. New version is labelled "current". Previous version "latest" now labelled "previous".

Clock reset about 3 us off, but still drifting slowly. Search mode and spectral-line modes continue to function. Linqing Wen also attended.

They were many years out of date. Delay changes expected. Bandpass observed to be different before and after move. Receiver position optimized for 45 degrees elevation. Move took place on Check electronic log for details of corrupted observations.


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This page contains a list of the major events for the PPTA project. These include changes to the instrumentation of software that affect the observations in blue , major publications and other useful dates. Timing properties not predicted to be different. Data from 1st Jan until this date will therefore be affected. Limited configs and still instrumental problems. Attenuator settings moved to digstats table. Gal l,b, PA, FA, parang, tel coords added to subint table. For and chan, no correction was applied. The actual delays fluctuate around these values by ns or so. Occasional instances of alt-mode TCS giving incorrect sign of bw e.

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Gravitational waves are disturbances in the curvature of spacetime , generated by accelerated masses, that propagate as waves outward from their source at the speed of light. The first indirect evidence for the existence of gravitational waves came from the observed orbital decay of the Hulse—Taylor binary pulsar , which matched the decay predicted by general relativity as energy is lost to gravitational radiation. In , Russell A. Hulse and Joseph Hooton Taylor Jr. The first direct observation of gravitational waves was not made until , when a signal generated by the merger of two black holes was received by the LIGO gravitational wave detectors in Livingston and in Hanford.

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Ideally, a differential amplifier takes the voltages V + and V − on its two Op-Amp Basics High input impedance Low output impedance Made using.

Timeline for the PPTA project

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In order to support our access to knowledge about party policies that impact upon our people we have decided to find as many policies as we can over the next weeks and include into a series of blogs. The issues that are currently topical in terms of the dirtypolitics are highlighting more clearly the insidious nature of politics in this country and the depths that some will sink to in order to control and determine our futures. We must challenge those ways of being. They do not align to the fundamental values of our tupuna.

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Gravitational wave

PPTA Te Wehengarua is here to support you in your introduction to teaching and throughout your teaching career. It is with great pleasure that we introduce you to the Beginning Teachers Handbook. This handbook provides you with the vital information you require in starting your teaching career and the reasons why you should join your colleagues and become a member of your union and professional association. The information contained in this publication is a quick reference only. More detailed information about all of the issues contained in this book are available from the PPTA branch at your workplace, the PPTA website or you can contact the PPTA office in your area see directory at the back of this publication. We extend to you our best wishes for your teaching career.

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