XMM-Newton Large Programme Details



PROPOSAL OVERVIEW
Proposal Title Measuring the Accretion Rate onto the Edge-on Spiral Galaxy NGC 891
Proposal Category Galaxies, Groups of Galaxies, Clusters of Galaxies and Superclusters
Proposal Type UNDEFINED
Proposal Id 78076
Number of Observations 3
Total exposure time (ks) 319

PI DETAILS
PI Mr Edmund Hodges-Kluck
Institute University of Michigan
Country UNITED STATES

CO-INVESTIGATORS
Name Country
J. Bregman UNITED STATES
M. Miller UNITED STATES
J. Li UNITED STATES

ABSTRACT
The hot halos of spiral galaxies contain material accreted from the intergalactic medium and material expelled from the disk. The mass in each component constrains galaxy formation models, and can be distinguished by the metallicity. However, isolating the hot gas and measuring its metallicity requires a large number of photons, and halos tend to be faint. The best candidate is NGC 891, a nearby, edge-on Milky Way analog with an X-ray bright halo. Existing data indicate an accretion rate of 0.2 Msun/yr, but there are too few photons to rule out several other plausible halo models. We will measure the accretion rate and the hot gas composition up to 8 kpc from the disk.

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 (10 references)
  1. " The Hot, Accreted Halo of NGC 891 "
    Hodges-Kluck, Edmund J.; Bregman, Joel N.; Li, Jiang-tao;
    2018 - The Astrophysical Journal, Volume 866, Issue 2, article id. 126, pp. (2018).
    Number of Citations: 10
    https://ui.adsabs.harvard.edu/search/q=bibcode:2018ApJ...866..126H
    DOI: 10.3847/1538-4357/aae38a

  2. " 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

  3. " Ultraluminous X-ray sources in seven edge-on spiral galaxies "
    Dage, Kristen C.; Vowell, Noah; Thygesen, Erica; Bahramian, Arash; Haggard, Daryl; Kovlakas, Konstantinos; Kundu, Arunav; Maccarone, Thomas J.; Strader, Jay; Urquhart, Ryan; Zepf, Stephen E.;
    2021 - Monthly Notices of the Royal Astronomical Society, Volume 508, Issue 3, pp.4008-4016
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2021MNRAS.508.4008D
    DOI: 10.1093/mnras/stab2850

  4. " A Long-Term Study of Ultraluminous X-ray Sources in NGC 891 "
    Earley, Nicholas M.; Dwarkadas, Vikram V.; Cirillo, Victoria;
    2021 - Universe, vol. 8, issue 1, p. 18
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2021Univ....8...18E
    DOI: 10.3390/universe8010018

  5. " New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints "
    De la Torre Luque, Pedro; Balaji, Shyam; Silk, Joseph;
    2024 - The Astrophysical Journal Letters, Volume 973, Issue 1, id.L6, 10 pp.
    Number of Citations: 2
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024ApJ...973L...6D
    DOI: 10.3847/1538-3881/ad6d60

  6. " 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

  7. " Robust constraints on feebly interacting particles using XMM-Newton "
    Luque, Pedro De la Torre; Balaji, Shyam; Carenza, Pierluca;
    2024 - Physical Review D, Volume 109, Issue 10, article id.L101305
    Number of Citations: 1
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024PhRvD.109j1305L
    DOI: 10.1093/mnras/stae1215

  8. " Multimessenger search for electrophilic feebly interacting particles from supernovae "
    Luque, Pedro De la Torre; Balaji, Shyam; Carenza, Pierluca;
    2024 - Physical Review D, Volume 109, Issue 10, article id.103028
    Number of Citations: 2
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024PhRvD.109j3028L
    DOI: 10.1093/mnrasl/slae038

  9. " Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints "
    De la Torre Luque, Pedro; Balaji, Shyam; Koechler, Jordan;
    2024 - The Astrophysical Journal, Volume 968, Issue 1, id.46, 16 pp.
    Number of Citations: 2
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024ApJ...968...46D
    DOI: 10.3847/1538-4357/ad4494

  10. " Probing ultralight primordial black hole dark matter with XMM telescopes "
    Guo, Jun; Yuan, Qiang; Zhu, Bin;
    2024 - Nuclear Physics, Section B, Volume 1005, id.116601
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024NuPhB100516601G
    DOI: 10.48550/arXiv.2311.07661