XMM-Newton Large Programme Details



PROPOSAL OVERVIEW
Proposal Title Long Term X-ray Monitoring of the Double Pulsar PSR J0737-3039
Proposal Category Supernovae, Supernova Remnants, Diffuse (galactic) Emission and Isolated Neutron Stars
Proposal Type LARGE PROGRAM
Proposal Id 067081
Number of Observations 3
Total exposure time (ks) 299

PI DETAILS
PI Dr Alberto Pellizzoni
Institute INAF-Oss.Astron.di Cagliari
Country ITALY

CO-INVESTIGATORS
Name Country
A. Possenti ITALY
P. Esposito ITALY
M. Burgay ITALY
M. Kramer GERMANY
A. Tiengo ITALY
N. D'Amico ITALY

ABSTRACT
Clear evidences of orbital phase-dependent interactions between the two pulsars of the relativistic double neutron star binary PSR J0737-3039 are seen both in radio and X-rays observations. In particular, XMM recently discovered the X-ray brightening of PSR B via energy transfer from PSR A, a process probably correlated with the strong radio intensity fluctuations of PSR B seen along the orbit. No other X-ray observatory of the current generation (or foreseen within the next decade) will be able to yield better information, and considering the disappearance of PSR B (March 2008) in the radio band, XMM offers the exclusive opportuinity to monitor this evolving pulsar and its related neutron star surface thermodynamics.

PAPERS
Authors marked in red are (co-)investigators in the proposal

Classification of papers are:
- CLASS 1:   papers that present specific XMM-Newton observations
- CLASS 2: papers that refer to published XMM-Newton results with complementary observations, follow-up analysis, or theoretical analysis
- CLASS 3: further deliveries which resulted from the program and which are made available to the community (e.g. source catalogues, processed images or spectra in public data base)
- CLASS 4: comments and suggestions from PI

CLASS 1 (5 references)
  1. " Long-term X-ray timing of the double pulsar PSR J0737-3039 "
    Iacolina , M. N.; Pellizzoni, A.; Egron, E.;
    2014 - Astronomische Nachrichten, Vol.335, Issue 3, p.324-328
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2014AN....335..324I
    DOI: 10.1002/asna.201312040

  2. " Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift "
    Yershov, V. N.;
    2014 - Astrophysics and Space Science, Volume 354, Issue 1, pp.97-101
    Number of Citations: 3
    https://ui.adsabs.harvard.edu/search/q=bibcode:2014Ap&SS.354...97Y
    DOI: 10.1007/s10509-014-1944-5

  3. " Long-term Study of the Double Pulsar J0737-3039 with XMM-Newton: Pulsar Timing "
    Iacolina, M. N.; Pellizzoni, A.; Egron, E.; Possenti, A.; Breton, R.; Lyutikov, M.; Kramer, M.; Burgay, M.; Motta, S. E.; De Luca, A.; Tiengo, A.;
    2016 - The Astrophysical Journal, Volume 824, Issue 2, article id. 87, pp. (2016).
    Number of Citations: 3
    https://ui.adsabs.harvard.edu/search/q=bibcode:2016ApJ...824...87I
    DOI: 10.3847/0004-637X/824/2/87

  4. " Long-term Study of the Double Pulsar J0737-3039 with XMM-Newton: Spectral Analysis "
    Egron, E.; Pellizzoni, A.; Pollock, A.; Iacolina, M. N.; Ikhsanov, N. R.; Possenti, A.; Marongiu, M.;
    2017 - The Astrophysical Journal, Volume 838, Issue 2, article id. 120, pp. (2017).
    Number of Citations: 1
    https://ui.adsabs.harvard.edu/search/q=bibcode:2017ApJ...838..120E
    DOI: 10.3847/1538-4357/aa6189

  5. " Classification of 4XMM-DR9 sources by machine learning "
    Zhang, Yanxia; Zhao, Yongheng; Wu, Xue-Bing;
    2021 - Monthly Notices of the Royal Astronomical Society, Volume 503, Issue 4, pp.5263-5273
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2021MNRAS.503.5263Z
    DOI: 10.1093/mnras/stab744