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| PSR J1627+3219 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST15:05:44 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2023ApJ...958..191S | 17 | D | 2 | 502 | ~ | The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars. | SMITH D.A., ABDOLLAHI S., AJELLO M., et al. | ||
| 2024ApJ...966..161B | 18 | D | 2 | 76 | ~ | A 350 MHz Green Bank Telescope Survey of Unassociated Fermi LAT Sources: Discovery and Timing of 10 Millisecond Pulsars. | BANGALE P., BHATTACHARYYA B., CAMILO F., et al. | ||
| 2024A&A...692A.187G | 179 | A | D | X | 5 | 75 | ~ | Millisecond pulsars phenomenology under the light of graph theory. | GARCIA C.R., ILLIANO G., TORRES D.F., et al. |
| 2025ApJ...979..143K | 19 | D | 1 | 123 | ~ | Unveiling Low-frequency Eclipses in Spider Millisecond Pulsars Using Wideband GMRT Observations. | KUMARI S., BHATTACHARYYA B., KANSABANIK D., et al. | ||
| 2025ApJ...985...58A | 19 | D | 1 | 297 | ~ | Prediction of Radio-quiet Gamma-Ray Pulsar Distances Using the Fundamental Plane Relation. | ANGUNER E.O. | ||
| 2025MNRAS.541..806I | 112 | D | F | 2 | 230 | ~ | Synchro-curvature description of γ-ray light curves and spectra of pulsars: concurrent fitting. | INIGUEZ-PASCUAL D., TORRES D.F. and VIGANO D. | |
| 2025A&A...702A.256B | 1866 | T A | D | S X C | 38 | 7 | ~ |
Studying the black widow pulsars PSR J0312-0921 and PSR J1627+3219 in the optical and X-rays. |
BOBAKOV A.V., KIRICHENKO A., ZHARIKOV S.V., et al. |
|
2025ApJ...994....8K |
19 | D | 3 | 126 | ~ | SpiderCat: A Catalog of Compact Binary Millisecond Pulsars. | KOLJONEN K.I.I. and LINARES M. | ||
| 2026ApJ...998...94S | 20 | D | 2 | 50 | ~ | Gamma-Ray Orbital Modulation in Spider Pulsars: Three Discoveries and a Universal Modulated Fraction. | SATYBALDIEV M., LINARES M. and VECCHIOTTI V. | ||
| 2026A&A...706A.259R | 50 | X | 1 | 48 | ~ | Pulsars identified in the LOFAR Two-metre Sky Survey at 144 MHz. | RIJKERS G.A.C., BASSA C.G., CALLINGHAM J.R., et al. |