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| PSR J0709+0458 , the SIMBAD biblio (17 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST21:15:30 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 2019ApJ...881..166M | 674 | K A | S X C | 15 | 21 | ~ | The discovery of six recycled pulsars from the Arecibo 327 MHz Drift-Scan Pulsar Survey. | MARTINEZ J.G., GENTILE P., FREIRE P.C.C., et al. | |
|
2021ApJ...916..100R |
17 | D | 1 | 422 | 2 | Analyzing the Galactic pulsar distribution with machine learning. | RONCHI M., GRABER V., GARCIA-GARCIA A., et al. | ||
| 2021ApJ...923...85A | 476 | D | X | 12 | 8 | ~ | New searches for continuous gravitational waves from seven fast pulsars. | ASHOK A., BEHESHTIPOUR B., PAPA M.A., et al. | |
| 2023ApJ...951L...9A | 192 | D | X C | 4 | 68 | 35 | The NANOGrav 15 yr Data Set: Observations and Timing of 68 Millisecond Pulsars. | AGAZIE G., ALAM M.F., ANUMARLAPUDI A., et al. | |
| 2023ApJ...951L..10A | 87 | C | 1 | 72 | 14 | The NANOGrav 15 yr Data Set: Detector Characterization and Noise Budget. | AGAZIE G., ANUMARLAPUDI A., ARCHIBALD A.M., et al. | ||
| 2023ApJ...951L..50A | 17 | D | 1 | 72 | 13 | The NANOGrav 15 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries. | AGAZIE G., ANUMARLAPUDI A., ARCHIBALD A.M., et al. | ||
| 2023A&A...679A..17P | 17 | D | 1 | 140 | ~ | Improving the spin-down limits of the continuous gravitational waves emitted from rotating triaxial pulsars. | PATHAK D. and CHATTERJEE D. | ||
|
2023RAA....23j4002W |
17 | D | 1 | 530 | ~ | FAST Pulsar Database. I. Polarization Profiles of 682 Pulsars. | WANG P.F., HAN J.L., XU J., et al. | ||
|
2024ApJS..271...23D |
18 | D | 1 | 203 | ~ | The AO327 Drift Survey Catalog and Data Release of Pulsar Detections. | DENEVA J.S., McLAUGHLIN M., OLSZANSKI T.E.E., et al. | ||
| 2024MNRAS.532.3893Y | 18 | D | 1 | 209 | ~ | High-priority targets for transient gravitational waves from glitching pulsars. | YIM G., SHAO L. and XU R. | ||
| 2024MNRAS.534.3400L | 18 | D | 1 | 47 | ~ | Ultraluminous X-ray sources with He star companions. | LI L., WANG B., LIU D., et al. | ||
| 2024A&A...690A.253C | 134 | X C | 2 | 16 | ~ | PSR J1227-6208 and its massive white dwarf companion: Pulsar emission analysis, timing update, and mass measurements. | COLOM I BERNADICH M., VENKATRAMAN KRISHNAN V., CHAMPION D.J., et al. | ||
| 2024ApJ...975..217C | 18 | D | 1 | 134 | ~ | Determining the Magnetic Field in the Galactic Plane from New Arecibo Pulsar Faraday Rotation Measurements. | CURTIN A.P., WEISBERG J.M. and RANKIN J.M. | ||
| 2024ApJ...976..212S | 18 | D | 1 | 67 | ~ | Characterizing the Nanohertz Gravitational Wave Background Using a t-process Power Spectral Density. | SARDESAI S.C., SIMON J. and VIGELAND S.J. | ||
| 2025ApJ...978..168A | 93 | F | 6 | 65 | ~ | The NANOGrav 15 Yr Data Set: Removing Pulsars One by One from the Pulsar Timing Array. | AGAZIE G., ANUMARLAPUDI A., ARCHIBALD A.M., et al. | ||
| 2026ApJ...997..116D | 20 | D | 3 | 71 | ~ | The NANOGrav 15 yr Dataset: Search for Gravitational Scattering of Pulsars by Free-floating Objects in Interstellar Space. | DEY L., JENNINGS R.J., TAYLOR J.D., et al. | ||
| 2026ApJ...999..226A | 50 | X | 1 | 2 | ~ | Graph-based Summary Statistics for Revealing the Stochastic Gravitational-wave Background in Pulsar Timing Arrays. | ALAKHRAS M. and MOVAHED S.M.S. |