XMM-Newton Large Programme Details



PROPOSAL OVERVIEW
Proposal Title Radio-galaxy composition in the LOFAR Two-Metre Sky Survey (LoTSS)
Proposal Category Active Galactic Nuclei, Quasars, BL-Lac Objects and Tidal Disruption Events
Proposal Type LARGE PROGRAM
Proposal Id 86273
Number of Observations 8
Total exposure time (ks) 700

PI DETAILS
PI Dr Judith Croston
Institute Open University
Country UNITED KINGDOM

CO-INVESTIGATORS
Name Country
B. Mingo UNITED KINGDOM
J. Ineson UNITED KINGDOM
M. Hardcastle UNITED KINGDOM

ABSTRACT
Our previous X-ray inverse-Compton and environmental studies of radio galaxies have demonstrated that their composition depends on morphology: edge-brightened, luminous (FRII) radio galaxies are leptonic, while centre-brightened, low luminosity (FRI) radio galaxies are baryonic. Radio morphology is therefore crucial for the inference of jet power and feedback from AGN survey populations. But the traditional FR dichotomy is challenged by our recent discovery of a large population of low luminosity edge-brightened (FRII) sources in the LOFAR Two-Metre Sky Survey (LoTSS). Here we propose to measure lobe inverse-Compton and environmental emission from this new AGN class to determine their particle content and hence enable their environmental impact to be incorporated into feedback models.

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 (4 references)
  1. " The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions "
    Pan, Zeyang; Qu, Zhijie; Bregman, Joel N.; Liu, Jifeng;
    2024 - The Astrophysical Journal Supplement Series, Volume 271, Issue 2, id.62, 18 pp.
    Number of Citations: 1
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024ApJS..271...62P
    DOI: 10.1093/mnras/stad3885

  2. " From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources "
    Rodriguez, Antonio C.;
    2024 - Publications of the Astronomical Society of the Pacific, Volume 136, Issue 5, id.054201, 17 pp.
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024PASP..136e4201R
    DOI: 10.1088/1538-3873/ad357c

  3. " Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE "
    Ma, Xiangyao; Zhang, Yanxia; Zhang, Jingyi; Li, Changhua; Kang, Zihan; Li, Ji;
    2024 - The Astronomical Journal, Volume 168, Issue 5, id.210, 10 pp.
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024AJ....168..210M
    DOI: 10.3847/1538-4357/ad6e81

  4. " Unveiling the origin of XMM-Newton soft proton flares: II. Systematics in the proton spectral analysis "
    Mineo, T.; Fioretti, V.; Lotti, S.; Molendi, S.; Lanzuisi, G.; Cappi, M.; Dadina, M.; Ettori, S.; Gastaldello, F.; Amato, R.;
    2024 - Astronomy & Astrophysics, Volume 691, id.A230, 12 pp.
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024A&A...691A.230M
    DOI: 10.1051/0004-6361/202451697