We describe an ongoing search for pulsars and dispersed pulses of radio emission , such as those from rotating radio transients ( RRATs ) and fast radio bursts ( FRBs ) , at 350 MHz using the Green Bank Telescope .
With the Green Bank Ultimate Pulsar Processing Instrument , we record 100 MHz of bandwidth divided into 4,096 channels every 81.92 \mu s .
This survey will cover the entire sky visible to the Green Bank Telescope ( \delta > -40 \arcdeg , or 82 % of the sky ) and outside of the Galactic Plane will be sensitive enough to detect slow pulsars and low dispersion measure ( < 30 \mathrm { pc cm ^ { -3 } } ) millisecond pulsars ( MSPs ) with a 0.08 duty cycle down to 1.1 mJy .
For pulsars with a spectral index of - 1.6 , we will be 2.5 times more sensitive than previous and ongoing surveys over much of our survey region .
Here we describe the survey , the data analysis pipeline , initial discovery parameters for 62 pulsars , and timing solutions for 5 new pulsars .
PSR J0214 + 5222 is an MSP in a long-period ( 512 days ) orbit and has an optical counterpart identified in archival data .
PSR J0636 + 5129 is an MSP in a very short-period ( 96 minutes ) orbit with a very low mass companion ( 8 M _ { \mathrm { J } } ) .
PSR J0645 + 5158 is an isolated MSP with a timing residual RMS of 500 ns and has been added to pulsar timing array experiments .
PSR J1434 + 7257 is an isolated , intermediate-period pulsar that has been partially recycled .
PSR J1816 + 4510 is an eclipsing MSP in a short-period orbit ( 8.7 hours ) and may have recently completed its spin-up phase .