We propose non-simultaneous joint Chandra (60 ks), XMM-Newton (60 ks), and HST(1 orbit) observations of the remarkable BAL RLQ PG 1004+130. These, inconjunction with our previous X-ray/UV coverage, will yield (1) one of the mostcomprehensive X-ray spectral monitoring campaigns of a variable BAL quasarundertaken, probing multi-year and multi-month timescales to constrain thenature of the X-ray absorber; (2) the highest S/N X-ray spectra of a BAL RLQcurrently available, enabling modeling of X-ray absorption and the underlyingcontinuum; and (3) the deepest X-ray imaging yet obtained of a disrupting jet ina hybrid morphology radio source, allowing tests for jet flux variability andcharacterization of the morphologies and spectra of the jet and diffuse emission.
Publications
Ultraviolet/X-ray Variability and the Extended X-ray Emission of the Radio-loud Broad Absorption Line Quasar PG 1004+130 |Scott, A. E., Brandt, W. N., et al. | ApJ | 806-210 | 2015 | 2015ApJ...806..210S | http://ui.adsabs.harvard.edu/#abs/2015ApJ...806..210S
Unveiling the X-ray/UV properties of disk winds in active galactic nuclei using broad and mini-broad absorption line quasars |Giustini, M., | AN | 337-459 | 2016 | 2016AN....337..459G | http://ui.adsabs.harvard.edu/#abs/2016AN....337..459G
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies |Ojha, Vineet, Chand, Hum, et al. | ApJ | 896-95 | 2020 | 2020ApJ...896...95O | http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O
Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earth.s Magnetosphere to the Solar Wind Proton Flux |Zhang, Yingjie, Sun, Tianran, et al. | ApJ | 948-69 | 2023 | 2023ApJ...948...69Z | http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z
Robust constraints on feebly interacting particles using XMM-Newton |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-L101305 | 2024 | 2024PhRvD.109j1305L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L
Multimessenger search for electrophilic feebly interacting particles from supernovae |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-103028 | 2024 | 2024PhRvD.109j3028L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L
Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints |De la Torre Luque, Pedro, Balaji, Shyam, | ApJ | 968-46 | 2024 | 2024ApJ...968...46D | http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2013-11-05T05:58:10Z/2013-11-06T00:18:10Z
Version
17.56_20190403_1200
Mission Description
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
European Space Agency, Prof William Brandt, 2014, 'Variable Absorption and Disrupting X-ray Jet of the BAL RLQ PG 1004+130', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-nwqf5so
