Details

Autor(en) / Beteiligte

• Swiggum, J. K.
• Pleunis, Z.
• Parent, E.
• Kaplan, D. L.
• McLaughlin, M. A.
• Stairs, I. H.
• Spiewak, R.
• Agazie, G. Y.
• Chawla, P.
• DeCesar, M. E.
• Dolch, T.
• Fiore, W.
• Fonseca, E.
• Istrate, A. G.
• Kaspi, V. M.
• Kondratiev, V. I.
• van Leeuwen, J.
• Levin, L.
• Lewis, E. F.
• Lynch, R. S.
• McEwen, A. E.
• Al Noori, H.
• Ransom, S. M.
• Siemens, X.
• Surnis, M.

Titel

The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions

Ist Teil von

• The Astrophysical journal, 2023-02, Vol.944 (2), p.154

Ort / Verlag

Philadelphia: The American Astronomical Society

Erscheinungsjahr

2023

Quelle

Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals

Beschreibungen/Notizen

• Abstract We present timing solutions for 12 pulsars discovered in the Green Bank North Celestial Cap 350 MHz pulsar survey, including six millisecond pulsars (MSPs), a double neutron star (DNS) system, and a pulsar orbiting a massive white dwarf companion. Timing solutions presented here include 350 and 820 MHz Green Bank Telescope data from initial confirmation and follow-up, as well as a dedicated timing campaign spanning 1 ryr PSR J1122−3546 is an isolated MSP, PSRs J1221−0633 and J1317−0157 are MSPs in black widow systems and regularly exhibit eclipses, and PSRs J2022+2534 and J2039−3616 are MSPs that can be timed with high precision and have been included in pulsar timing array experiments seeking to detect low-frequency gravitational waves. PSRs J1221−0633 and J2039−3616 have Fermi Large Area Telescope gamma-ray counterparts and also exhibit significant gamma-ray pulsations. We measure proper motions for three of the MSPs in this sample and estimate their space velocities, which are typical compared to those of other MSPs. We have detected the advance of periastron for PSR J1018−1523 and therefore measure the total mass of the DNS system, m tot = 2.3 ± 0.3 M ⊙ . Long-term pulsar timing with data spanning more than 1 yr is critical for classifying recycled pulsars, carrying out detailed astrometry studies, and shedding light on the wealth of information in these systems post-discovery.