Precise optical timing of PSR J1023+0038, the first millisecond pulsar detected with Aqueye+ in Asiago-Reference-Cited by-同舟云学术

Precise optical timing of PSR J1023+0038, the first millisecond pulsar detected with Aqueye+ in Asiago

Published:2019-03-27 Issue:1 Volume:485 Page:L109-L113
ISSN:1745-3925
Container-title:Monthly Notices of the Royal Astronomical Society: Letters
language:en
Short-container-title:

Author:

Zampieri Luca¹^ORCID,Burtovoi Aleksandr¹²^ORCID,Fiori Michele¹³,Naletto Giampiero¹³^ORCID,Spolon Alessia¹³,Barbieri Cesare¹³,Papitto Alessandro⁴,Ambrosino Filippo⁵

Affiliation:

1. INAF – Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122, Padova, Italy

2. Centre of Studies and Activities for Space (CISAS) ‘G. Colombo’, University of Padova, Via Venezia 15, I-35131 Padova, Italy

3. Department of Physics and Astronomy, University of Padova, Via F. Marzolo 8, I-35131, Padova, Italy

4. INAF – Osservatorio Astronomico di Roma, Via Frascati 33, I-00076, Monteporzio Catone (RM), Italy

5. INAF – Istituto di Astrofisica e Planetologia Spaziali, Via del Fosso del Cavaliere 100, I-00133 Rome, Italy

Funder

Advanced Science Institute

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnrasl/article-pdf/485/1/L109/28246637/slz043.pdf

Reference50 articles.

1. A SEARCH FOR VERY HIGH ENERGY GAMMA RAYS FROM THE MISSING LINK BINARY PULSAR J1023+0038 WITH VERITAS

2. A new class of radio pulsars

3. Optical pulsations from a transitional millisecond pulsar

4. A Radio Pulsar/X-ray Binary Link

5. ACCRETION-POWERED PULSATIONS IN AN APPARENTLY QUIESCENT NEUTRON STAR BINARY

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