XMM-Newton Large Programme Details



PROPOSAL OVERVIEW
Proposal Title X-raying hyperluminous sub-millimeter galaxies via strong gravitational lenses
Proposal Category Galaxies, Groups of Galaxies, Clusters of Galaxies and Superclusters
Proposal Type LARGE PROGRAM
Proposal Id 088272
Number of Observations 6
Total exposure time (ks) 544

PI DETAILS
PI Prof Q. Daniel Wang
Institute University of Massachusetts
Country UNITED STATES

CO-INVESTIGATORS
Name Country
M. Yun UNITED STATES
K. Harrington CHILE
J. Lowenthal UNITED STATES
P. Kamieneski UNITED STATES
B. Frye UNITED STATES

ABSTRACT
We propose XMM-Newton observations of 3 sub-millimeter bright galaxies (SMGs) spanning z=2.1-3.6. These SMGs are gravitationally lensed by massive foreground galaxies, and each has an apparent luminosity >e14 Lsun, showing no sign for AGN in extensive multi-wavelength analysis. The combination of the sensitivity of XMM- Newton and the lensing magnification, as well as the intrinsic brightness of the SMGs, will enable us to study them individually. We will measure the collective X- ray emission from X-ray binaries and hence its ratio to the star formation rate for the first time and to potentially detect extremely obscured AGN over the rest-frame 2-35 keV range. This study will represent a key step in our multi- wavelength campaign to understand the working of such extreme galaxies.

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. " X-ray detection of the most extreme star-forming galaxies at the cosmic noon via strong lensing "
    Wang, Q. Daniel; Diaz, Carlos Garcia; Kamieneski, Patrick S.; Harrington, Kevin C.; Yun, Min S.; Foo, Nicholas; Frye, Brenda L.; Jimenez-Andrade, Eric F.; Liu, Daizhong; Lowenthal, James D.; Pampliega, Belen Alcalde; Pascale, Massimo; Vishwas, Amit; Gurwell, Mark A.;
    2024 - Monthly Notices of the Royal Astronomical Society, Volume 527, Issue 4, pp.10584-10603
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024MNRAS.52710584W
    DOI: 10.48550/arXiv.2310.04302

  2. " 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

  3. " 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

  4. " 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