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| PSR J1529-3828 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST06:13:19 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2013MNRAS.434.1387L | 92 | D | F | 3 | 55 | 31 | The high time resolution universe pulsar survey -VIII. The galactic millisecond pulsar population. | LEVIN L., BAILES M., BARSDELL B.R., et al. | |
| 2014MNRAS.439.1865N | 480 | D | X C F | 11 | 23 | 37 | The High Time Resolution Universe pulsar survey - X. Discovery of four millisecond pulsars and updated timing solutions of a further 12. | NG C., BAILES M., BATES S.D., et al. | |
| 2015MNRAS.446.4019B | 16 | D | 1 | 39 | 19 | The High Time Resolution Universe survey - XI. Discovery of five recycled pulsars and the optical detectability of survey white dwarf companions. | BATES S.D., THORNTON D., BAILES M., et al. | ||
|
2015BaltA..24..395M |
16 | D | 1 | 619 | 2 | Binary star DataBase: binaries discovered in non-optical bands. | MALKOV O.Y., TESSEMA S.B. and KNIAZEV A.Y. | ||
| 2017ApJ...834..137L | 16 | D | 1 | 75 | 11 | Timing of 29 pulsars discovered in the PALFA survey. | LYNE A.G., STAPPERS B.W., BOGDANOV S., et al. | ||
| 2018ApJ...864...30H | 16 | D | 1 | 89 | 2 | On the orbital properties of millisecond pulsar binaries. | HUI C.Y., WU K., HAN Q., 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. | ||
| 2022MNRAS.510.6011W | 17 | D | 1 | 53 | 15 | Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white dwarfs. | WANG B., LIU D. and CHEN H. | ||
| 2024MNRAS.532.2196W | 18 | D | 1 | 49 | ~ | Formation of millisecond pulsars with wide orbits. | WANG B., LIU D., GUO Y., et al. | ||
| 2025ApJ...992..116M | 19 | D | 1 | 181 | ~ | Irradiated Pulsar Planets and Companions as 511 keV Positron Annihilation Line Sources. | METZLER Z. and WADIASINGH Z. |