Search Publications

The X-Ray Luminosity Function Evolution of Quasars and the Correlation between the X-Ray and Ultraviolet Luminosities
DOI: 10.3847/1538-4357/ac6f06 Bibcode: 2022ApJ...932..111S

Singal, J.; Mutchnick, S.; Petrosian, V.

We explore the evolution of the X-ray luminosity function of quasars and the intrinsic correlation between the X-ray and 2500 Å ultraviolet luminosities, utilizing techniques verified in previous works and a sample of over 4000 quasars detected with Chandra and XMM-Newton in the range 0 < z < 5. We find that quasars have undergone significan…

2022 The Astrophysical Journal
XMM-Newton 13
A New X-Ray Tidal Disruption Event Candidate with Fast Variability
DOI: 10.1088/1674-4527/ac5800 Bibcode: 2022RAA....22e5004H

Greiner, J.; Komossa, S.; Erben, T. +3 more

During a close encounter between a star and a supermassive black hole, the star can get disrupted by the black hole's tidal forces, resulting in a tidal disruption event (TDE). The accretion of the star's material onto the black hole produces strong emission in different wavelength regimes. Here we report the discovery with the Roentgen Satellite …

2022 Research in Astronomy and Astrophysics
XMM-Newton 13
Weak gravitational lensing shear measurement with FPFS: analytical mitigation of noise bias and selection bias
DOI: 10.1093/mnras/stac342 Bibcode: 2022MNRAS.511.4850L

Massey, Richard; Li, Xiangchong; Li, Yin

Dedicated 'Stage IV' observatories will soon observe the entire extragalactic sky, to measure the 'cosmic shear' distortion of galaxy shapes by weak gravitational lensing. To measure the apparent shapes of those galaxies, we present an improved version of the Fourier Power Function Shapelets (FPFS) shear measurement method. This now includes analy…

2022 Monthly Notices of the Royal Astronomical Society
eHST 13
The merging galaxy cluster Abell 3266 at low radio frequencies
DOI: 10.1093/mnras/stac335 Bibcode: 2022MNRAS.511.3525D

Bartalucci, I.; Riseley, C. J.; Johnston-Hollitt, M. +2 more

We present new low-frequency (ν = 88-216 MHz) observations of the complex merging galaxy cluster Abell 3266. These new observations are taken with the Murchison Widefield Array (MWA) in its Phase II 'extended', long-baseline configuration, offering the highest resolution low-frequency view of the cluster to date. We report on the detection of four…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 13
Orion Bar as a window to the evolution of PAHs
DOI: 10.1093/mnras/stab3061 Bibcode: 2022MNRAS.509..800M

Kirsanova, Maria S.; Boley, Paul A.; Murga, Maria S. +1 more

We investigate the mid-infrared (IR) emission in the Orion Bar photodissociation region (PDR), using archival photometric and spectroscopic observations from the United Kingdom Infrared Telescope (UKIRT), Spitzer, Infrared Space Observatory(ISO), and Stratospheric Observatory for Infrared Astronomy (SOFIA) telescopes. Specifically, we consider flu…

2022 Monthly Notices of the Royal Astronomical Society
ISO 13
Physics of ULIRGs with MUSE and ALMA: The PUMA project. III. Incidence and properties of ionised gas disks in ULIRGs, associated velocity dispersion, and its dependence on starburstiness
DOI: 10.1051/0004-6361/202142659 Bibcode: 2022A&A...662A..94P

Maiolino, R.; Colina, L.; Perna, M. +11 more

Context. A classical scenario suggests that ultra-luminous infrared galaxies (ULIRGs) transform colliding spiral galaxies into a spheroid-dominated early-type galaxy. Recent high-resolution simulations have instead shown that, under some circumstances, rotation disks can be preserved during the merging process or rapidly regrown after coalescence.…

2022 Astronomy and Astrophysics
Gaia eHST 13
The Basal Detectability of an Ice-Covered Mars by MARSIS
DOI: 10.1029/2021GL096518 Bibcode: 2022GeoRL..4996518G

Mouginot, J.; Kofman, W.; Hérique, A. +2 more

The detection of anomalously strong relative basal reflectivity beneath the Martian South Polar Layered Deposits (SPLD) from the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) has led to hypotheses suggesting the presence of basal materials such as liquid water. Here, we propose a forward approach to assess whether such a high…

2022 Geophysical Research Letters
MEx 13
Probing the physicochemical properties of the Leo Ring and the Leo I group
DOI: 10.1093/mnras/stac052 Bibcode: 2022MNRAS.510.5796S

Richter, Philipp; Charlton, Jane C.; Kacprzak, Glenn G. +6 more

We present an absorption line study of the physical and chemical properties of the Leo H I Ring and the Leo I Group as traced by 11 quasar sightlines spread over a ≈600 × 800 kpc2 region. Using HST/COS G130/G160 archival observations as constraints, we couple cloud-by-cloud, multiphase, Bayesian ionization modelling with galaxy property…

2022 Monthly Notices of the Royal Astronomical Society
eHST 13
An Open-source Bayesian Atmospheric Radiative Transfer (BART) Code. III. Initialization, Atmospheric Profile Generator, Post-processing Routines
DOI: 10.3847/PSJ/ac3515 Bibcode: 2022PSJ.....3...82B

Cubillos, Patricio E.; Blecic, Jasmina; Challener, Ryan C. +12 more

This and companion papers by Harrington et al. and Cubillos et al. describe an open-source retrieval framework, Bayesian Atmospheric Radiative Transfer (BART), available to the community under the reproducible-research license via https://github.com/exosports/BART. BART is a radiative transfer code (transit; https://github.com/exosports/transit; R…

2022 The Planetary Science Journal
eHST 13
Deep XMM-Newton Observations of an X-ray Weak Broad Absorption Line Quasar at z = 6.5
DOI: 10.3847/2041-8213/ac45f2 Bibcode: 2022ApJ...924L..25Y

Fan, Xiaohui; Keeton, Charles R.; Walter, Fabian +14 more

We report X-ray observations of the most distant known gravitationally lensed quasar, J0439+1634 at z = 6.52, which is also a broad absorption line (BAL) quasar, using the XMM-Newton Observatory. With a 130 ks exposure, the quasar is significantly detected as a point source at the optical position with a total of ${358}_{-19}^{+19}$ net counts usi…

2022 The Astrophysical Journal
XMM-Newton 13