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| PSR J1714-1054 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST22:55:02 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2005AJ....129.1993M 
|
11 | 68 | 2431 | The Australia telescope national facility pulsar catalogue. | MANCHESTER R.N., HOBBS G.B., TEOH A., et al. | ||||
|
2008MNRAS.391.1210W
|
15 | D | 355 | 115 | Profile and polarization characteristics of energetic pulsars. | WELTEVREDE P. and JOHNSTON S. | |||
| 2009ApJ...699.2009J | 15 | D | 2 | 101 | 27 | A large-area survey for radio pulsars at high Galactic latitudes. | JACOBY B.A., BAILES M., ORD S.M., et al. | ||
|
2011ARep...55..878M
|
15 | D | 1 | 319 | 8 | The geometry of radio pulsar magnetospheres. | MALOV I.F. and NIKITINA E.B. | ||
|
2017ARep...61..591N
|
376 | 2 | Magnetic fields of radio pulsars. | NIKITINA E.B. and MALOV I.F. | |||||
|
2018MNRAS.474.4629J
|
16 | D | 1 | 596 | 85 | Polarimetry of 600 pulsars from observations at 1.4 GHz with the Parkes radio telescope. | JOHNSTON S. and KERR M. | ||
| 2019MNRAS.483.3673M | 17 | D | 1 | 37 | 31 | The High Time Resolution Universe survey - XIV. Discovery of 23 pulsars through GPU-accelerated reprocessing. | MORELLO V., BARR E.D., COOPER S., et al. | ||
| 2021MNRAS.508.4249P | 87 | C | 1 | 22 | 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. | ||
| 2023MNRAS.520.4562S | 19 | D | 1 | 42 | 3 | The Thousand-Pulsar-Array programme on MeerKAT - VIII. The subpulse modulation of 1198 pulsars. | SONG X., WELTEVREDE P., SZARY A., et al. | ||
| 2023MNRAS.520.4801J | 19 | 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. |
