Search Publications

Consistency testing for invariance of the speed of light at different redshifts: the newest results from strong lensing and Type Ia supernovae observations
DOI: 10.1093/mnras/stab1868 Bibcode: 2021MNRAS.506.2181L

Liu, Yuting; Cao, Shuo; Biesiada, Marek +3 more

The invariance of the speed of light in the distant Universe has profound significance for fundamental physics. In this paper, we propose a new model-independent method to test the invariance of the speed of light c at different redshifts by combining the strong gravitational lensing (SGL) systems and the observations of Type Ia supernovae (SNe Ia…

2021 Monthly Notices of the Royal Astronomical Society
eHST 18
Classical Novae Masquerading as Dwarf Novae? Outburst Properties of Cataclysmic Variables with ASAS-SN
DOI: 10.3847/1538-4357/abe53d Bibcode: 2021ApJ...910..120K

Mukai, K.; Kochanek, C. S.; Stanek, K. Z. +12 more

The unprecedented sky coverage and observing cadence of the All-Sky Automated Survey for SuperNovae (ASAS-SN) has resulted in the discovery and continued monitoring of a large sample of Galactic transients. The vast majority of these are accretion-powered dwarf nova outbursts in cataclysmic variable systems, but a small subset are thermonuclear-po…

2021 The Astrophysical Journal
Gaia 18
Quasi-periodic Oscillations in the TESS Light Curve of TX Col, a Diskless Intermediate Polar on the Precipice of Forming an Accretion Disk
DOI: 10.3847/1538-3881/ac062b Bibcode: 2021AJ....162...49L

Garnavich, Peter; Littlefield, Colin; Szkody, Paula +4 more

One of the fundamental properties of an intermediate polar is the dynamical nature of the accretion flow as it encounters the white dwarf's (WD's) magnetosphere. Many works have presumed a dichotomy between disk-fed accretion, in which the WD accretes from a Keplerian disk, and stream-fed accretion, in which the matter stream from the donor star d…

2021 The Astronomical Journal
Gaia 18
Chandra and Magellan/FIRE follow-up observations of PSO167-13: An X-ray weak QSO at z = 6.515
DOI: 10.1051/0004-6361/202140399 Bibcode: 2021A&A...649A.133V

Bauer, F. E.; Brandt, W. N.; Vignali, C. +19 more

Context. The discovery of hundreds of quasi-stellar objects (QSOs) in the first gigayear of the Universe powered by already grown supermassive black holes (SMBHs) challenges our knowledge of SMBH formation. In particular, investigations of z > 6 QSOs that present notable properties can provide unique information on the physics of fast SMBH grow…

2021 Astronomy and Astrophysics
Gaia 18
CAPOS: The bulge Cluster APOgee Survey. II. The intriguing "Sequoia" globular cluster FSR 1758
DOI: 10.1051/0004-6361/202141294 Bibcode: 2021A&A...652A.158R

Cohen, Roger E.; Beers, Timothy C.; Minniti, Dante +16 more

We present results from a study of 15 red giant members of the intermediate-metallicity globular cluster (GC) FSR 1758 using high-resolution, near-infrared spectra collected with the Apache Point Observatory Galactic Evolution Experiment II survey (APOGEE-2) that were obtained as part of CAPOS (the bulge Cluster APOgee Survey). Since its very rece…

2021 Astronomy and Astrophysics
Gaia 18
Long-term stellar activity variations and their effect on radial-velocity measurements
DOI: 10.1093/mnras/stab1183 Bibcode: 2021MNRAS.505..830C

Günther, Maximilian N.; Jenkins, James S.; Watson, Christopher A. +8 more

Long-term stellar activity variations can affect the detectability of long-period and Earth-analogue extrasolar planets. We have, for 54 stars, analysed the long-term trend of five activity indicators: log $R^{\prime }_\mathrm{{HK}}$, the cross-correlation function (CCF) bisector span, CCF full-width-at-half-maximum, CCF contrast, and the area of …

2021 Monthly Notices of the Royal Astronomical Society
Gaia 18
Long-term Coherent Timing of the Accreting Millisecond Pulsar IGR J17062-6143
DOI: 10.3847/1538-4357/abf13f Bibcode: 2021ApJ...912..120B

Bult, Peter; Malacaria, Christian; Ng, Mason +2 more

We report on a coherent timing analysis of the 163 Hz accreting millisecond X-ray pulsar IGR J17062-6143. Using data collected with the Neutron Star Interior Composition Explorer and XMM-Newton, we investigated the pulsar evolution over a time span of four years. We obtained a unique phase-coherent timing solution for the stellar spin, finding the…

2021 The Astrophysical Journal
XMM-Newton 18
Reproducing the UVJ Color Distribution of Star-forming Galaxies at 0.5 < z < 2.5 with a Geometric Model of Dust Attenuation
DOI: 10.3847/2041-8213/ac3831 Bibcode: 2021ApJ...922L..32Z

Belli, Sirio; Tacchella, Sandro; Leja, Joel +1 more

We analyze the distribution of rest-frame U - V and V - J colors for star-forming galaxies at 0.5 < z < 2.5. Using stellar population synthesis, stochastic star formation histories, and a simple prescription for the dust attenuation that accounts for the shape and inclination of galaxies, we construct a model for the distribution of galaxy c…

2021 The Astrophysical Journal
Herschel 18
Estimates of the change rate of solar mass and gravitational constant based on the dynamics of the Solar System
DOI: 10.1051/0004-6361/202039893 Bibcode: 2021A&A...647A.141P

Pitjeva, E. V.; Pitjev, N. P.; Pavlov, D. A. +1 more

The estimate of the change rate of the solar gravitational parameter d(GM)∕dt is obtained from processing modern positional observations of planets and spacecraft. Observations were processed and parameters were determined basing on the numerical planetary ephemeris EPM2019. The obtained annual decrease in solar mass M acco…

2021 Astronomy and Astrophysics
Ulysses 18
The Composition of the South Polar Cap of Mars Derived From Orbital Data
DOI: 10.1029/2020JE006730 Bibcode: 2021JGRE..12606730B

Wieczorek, M. A.; Broquet, A.; Fa, W.

The flexure of the lithosphere under stresses imposed by the geologically young south polar cap is one of the few clues we have regarding the south polar cap composition and the present-day thermal state of Mars. Here, we combine radar, gravity, and topography data with a flexural loading model to estimate the bulk density (ρ) and average real die…

2021 Journal of Geophysical Research (Planets)
MEx 18