ReadPaper-Pulsar Survey
1. The Giant Metrewave Radio Telescope (GMRT)
1, The GMRT High Resolution Southern Sky Survey for Pulsars and Transients. I. Survey Description and Initial Discoveries
https://ui.adsabs.harvard.edu/abs/2016ApJ...817..130B/abstract
2, The GMRT High-resolution Southern Sky Survey for Pulsars and Transients. II. New Discoveries, Timing, and Polarization Properties
https://ui.adsabs.harvard.edu/abs/2019ApJ...881...59B/abstract
3, The GMRT High Resolution Southern Sky Survey for Pulsars and Transients. III. Searching for Long-period Pulsars
https://ui.adsabs.harvard.edu/abs/2022ApJ...934..138S/abstract
4, The GMRT High Resolution Southern Sky Survey for Pulsars and Transients. IV. Discovery of Four New Pulsars with an FFA Search
https://ui.adsabs.harvard.edu/abs/2023ApJ...944...54S/abstract
5, The GMRT High Resolution Southern Sky Survey for Pulsars and Transients. V. Localization of Two Millisecond Pulsars
https://ui.adsabs.harvard.edu/abs/2023ApJ...947...88S/abstract
6, The GMRT High Resolution Southern Sky Survey for pulsars and transients -- VI: Discovery of nulling, localisation and timing of PSR J1244-4708
https://ui.adsabs.harvard.edu/abs/2023arXiv230701477S/abstract
2. The Parkes
1, The Parkes multi-beam pulsar survey - I. Observing and data analysis systems, discovery and timing of 100 pulsars
https://ui.adsabs.harvard.edu/abs/2001MNRAS.328...17M/abstract
2, The Parkes Multibeam Pulsar Survey - II. Discovery and timing of 120 pulsars
https://ui.adsabs.harvard.edu/abs/2002MNRAS.335..275M/abstract
3, The Parkes Multibeam Pulsar Survey - III. Young pulsars and the discovery and timing of 200 pulsars
https://ui.adsabs.harvard.edu/abs/2003MNRAS.342.1299K/abstract
4, The Parkes multibeam pulsar survey - IV. Discovery of 180 pulsars and parameters for 281 previously known pulsars
https://ui.adsabs.harvard.edu/abs/2004MNRAS.352.1439H/abstract
5, The Parkes Multibeam Pulsar Survey - V. Finding binary and millisecond pulsars
https://ui.adsabs.harvard.edu/abs/2004MNRAS.355..147F/abstract
6, The Parkes Multibeam Pulsar Survey - VI. Discovery and timing of 142 pulsars and a Galactic population analysis
https://ui.adsabs.harvard.edu/abs/2006MNRAS.372..777L/abstract
3. The Arecibo
1, Arecibo Pulsar Survey Using ALFA. I. Survey Strategy and First Discoveries
https://ui.adsabs.harvard.edu/abs/2006ApJ...637..446C/abstract
2, Arecibo Pulsar Survey Using ALFA. II. The Young, Highly Relativistic Binary Pulsar J1906+0746
https://ui.adsabs.harvard.edu/abs/2006ApJ...640..428L/abstract
3, Arecibo Pulsar Survey Using ALFA. III. Precursor Survey and Population Synthesis
https://ui.adsabs.harvard.edu/abs/2014ApJ...787..137S/abstract
4, Arecibo Pulsar Survey Using ALFA. IV. Mock Spectrometer Data Analysis, Survey Sensitivity, and the Discovery of 40 Pulsars
https://ui.adsabs.harvard.edu/abs/2015ApJ...812...81L/abstract
5, Arecibo Pulsar Survey Using ALFA: Probing Radio Pulsar Intermittency And Transients
https://ui.adsabs.harvard.edu/abs/2009ApJ...703.2259D/abstract
4. The Green Bank Telescope
1. The Green Bank Telescope 350 MHz Drift-scan Survey
1, The Green Bank Telescope 350 MHz Drift-scan survey. I. Survey Observations and the Discovery of 13 Pulsars
https://ui.adsabs.harvard.edu/abs/2013ApJ...763...80B/abstract
A total of 1191 hr of "drift-scan" pulsar search observations with GBT at a radio frequency of 350 HMz was obtained. The survey setup, search procedure, the discovery and follow-up timing of 13 pulsars was described in here.
Since the discovery of the first pulsar in 1967, many fascinating sources and experiments have been associated with pulsars. These include, but are not limited to, tests of general relativity, studies of binary evolution, probes of electron density models of the interstellar medium, constraints on the neutron star equation of state and the use in a pulsar timing array for gravitational wave detection.
Lower frequency observations (< 500 HMz) are better used to locate weak sources away from the Galactic plane where the effects of scattering, higher sky temperature, and dispersion broadening are minimized.
One TOA per observation for each isolated pulsar and three per observation for each binary pulsar for better determination of binary parameters. As is a common practice in pulsar timing, the TOA uncertainties are scaled by a constant factor, EFAC, to bring the reduced χ2 of each timing model to unity.
Fluxes were measured using PSRCHIVE, and on- and off-source scans of the extragalactic radio source 3C190 were used for flux calibration. Before each observation, a 1 minute calibration scan was taken with a 25 Hz noise diode at the receiver.
PRESTO prepfold plot (the right bottom): a χ2 intensity plot of P-Pdot space.
The rotation measures (RM) were calculated for pulsars with enough linearly polarized flux.
Figure 5. Profiles at 820 MHz for nine newly discovered pulsars created from multi-epoch data using the GUPPI backend. Spin periods are listed.
A new survey named the Green Bank North Celestial Cap (GBNCC) survey is underway due to the success of this survey.
2, The Green Bank Telescope 350 MHz Drift-scan Survey II: Data Analysis and the Timing of 10 New Pulsars, Including a Relativistic Binary
https://ui.adsabs.harvard.edu/abs/2013ApJ...763...81L/abstract
3, The GBT 350-MHz Drift Scan Pulsar Survey - III. Detection of a magnetic field in the eclipsing material of PSR J2256-1024
https://ui.adsabs.harvard.edu/abs/2020MNRAS.495.3052C/abstract
2. The Green Bank North Celestial Cap Pulsar Survey
1, The Green Bank Northern Celestial Cap Pulsar Survey. I. Survey Description, Data Analysis, and Initial Results
https://ui.adsabs.harvard.edu/abs/2014ApJ...791...67S/abstract
2, The Green Bank Northern Celestial Cap Pulsar Survey. II. The Discovery and Timing of 10 Pulsars
https://ui.adsabs.harvard.edu/abs/2018ApJ...857..131K/abstract
3, The Green Bank North Celestial Cap Pulsar Survey. III. 45 New Pulsar Timing Solutions
https://ui.adsabs.harvard.edu/abs/2018ApJ...859...93L/abstract
4, The Green Bank North Celestial Cap Pulsar Survey. IV. Four New Timing Solutions
https://ui.adsabs.harvard.edu/abs/2019ApJ...875...19A/abstract
5, The Green Bank North Celestial Cap Pulsar Survey. V. Pulsar Census and Survey Sensitivity
https://ui.adsabs.harvard.edu/abs/2020ApJ...892...76M/abstract
6, The Green Bank Northern Celestial Cap Pulsar Survey. VI. Discovery and Timing of PSR J1759+5036: A Double Neutron Star Binary Pulsar
https://ui.adsabs.harvard.edu/abs/2021ApJ...922...35A/abstract
7, The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions
https://ui.adsabs.harvard.edu/abs/2023ApJ...944..154S/abstract
8, The Green Bank North Celestial Cap Survey. VIII. 21 New Pulsar Timing Solutions
https://ui.adsabs.harvard.edu/abs/2023arXiv230513624F/abstract
Other:
The Green Bank North Celestial Cap Pulsar Survey: Status and Future
https://ui.adsabs.harvard.edu/abs/2018IAUS..337...13L/abstract
The Green Bank North Celestial Cap Pulsar Survey: New Pulsars and Future Prospects
https://ui.adsabs.harvard.edu/abs/2018AAS...23124313L/abstract
The Green Bank North Celestial Cap Pulsar Survey: A Decade of Discovery
https://ui.adsabs.harvard.edu/abs/2021AAS...23734501L/abstract
5, The Five-hundred-meter Aperture Spherical radio Telescope (FAST)
1, The FAST Galactic Plane Pulsar Snapshot survey: I. Project design and pulsar discoveries
https://ui.adsabs.harvard.edu/abs/2021RAA....21..107H/abstract
2, The FAST Galactic Plane Pulsar Snapshot Survey: II. Discovery of 76 Galactic rotating radio transients and their enigma
https://ui.adsabs.harvard.edu/abs/2023arXiv230317279Z/abstract
3,
4, The FAST Galactic Plane Pulsar Snapshot Survey: IV. Timing results of 30 FAST-GPPS discovered pulsars
https://ui.adsabs.harvard.edu/abs/2023arXiv230516754S/abstract
6, The Southern-sky MWA Rapid Two-metre (SMART)
1, The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey—I. Survey design and processing pipeline
https://ui.adsabs.harvard.edu/abs/2023PASA...40...21B/abstract
2, The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey—II. Survey status, pulsar census, and first pulsar discoveries
https://ui.adsabs.harvard.edu/abs/2023PASA...40...20B/abstract
