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| PSR J1810-01 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST09:04:41 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2010MNRAS.409..619K | 19 | D | 1 | 31 | 273 | The High Time Resolution Universe Pulsar Survey - I. System configuration and initial discoveries. | KEITH M.J., JAMESON A., VAN STRATEN W., et al. | ||
2012MNRAS.427.1052B 
|
458 | A | D | S X C F | 10 | 72 | 19 | The High Time Resolution Universe Pulsar Survey - VI. An artificial neural network and timing of 75 pulsars. | BATES S.D., BAILES M., BARSDELL B.R., et al. |
|
2020ApJ...892...76M
|
16 | D | 1 | 516 | 26 | The Green Bank North Celestial Cap pulsar survey. V. Pulsar census and survey sensitivity. | McEWEN A.E., SPIEWAK R., SWIGGUM J.K., et al. | ||
|
2021ApJS..255....5A
|
17 | D | 1 | 977 | ~ | The CHIME pulsar project: system overview. | AMIRI M., BANDURA K.M., BOYLE P.J., et al. | ||
|
2021MNRAS.508.4249P
|
17 | D | 1 | 1181 | 16 | The Thousand-Pulsar-Array programme on MeerKAT - VI. Pulse widths of a large and diverse sample of radio pulsars. | POSSELT B., KARASTERGIOU A., JOHNSTON S., et al. | ||
| 2022MNRAS.511.3304M | 17 | D | 1 | 400 | 6 | An updated glitch rate law inferred from radio pulsars. | MILLHOUSE M., MELATOS A., HOWITT G., et al. | ||
| 2023MNRAS.520.4801J | 17 | D | 1 | 1267 | 4 | The Thousand-Pulsar-Array programme on MeerKAT - XI. Application of the rotating vector model. | JOHNSTON S., KRAMER M., KARASTERGIOU A., et al. | ||
|
2023RAA....23j4002W
|
61 | D | X | 2 | 530 | ~ | FAST Pulsar Database. I. Polarization Profiles of 682 Pulsars. | WANG P.F., HAN J.L., XU J., et al. | |
| 2024MNRAS.532.3893Y | 45 | X | 1 | 209 | ~ | High-priority targets for transient gravitational waves from glitching pulsars. | YIM G., SHAO L. and XU R. |
