Search Publications

The velocity dispersion function of early-type galaxies and its redshift evolution: the newest results from lens redshift test
DOI: 10.1093/mnras/stab519 Bibcode: 2021MNRAS.503.1319G

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

The redshift distribution of galactic-scale lensing systems provides a laboratory to probe the velocity dispersion function (VDF) of early-type galaxies (ETGs) and measure the evolution of ETGs at redshift z ~ 1. Through the statistical analysis of the currently largest sample of ETG gravitational lenses, we conclude that the VDF inferred solely f…

2021 Monthly Notices of the Royal Astronomical Society
eHST 24
Black hole mass measurement using ALMA observations of [CI] and CO emissions in the Seyfert 1 galaxy NGC 7469
DOI: 10.1093/mnras/stab1002 Bibcode: 2021MNRAS.504.4123N

Baba, Shunsuke; Meier, David S.; Turner, Jean L. +11 more

We present a supermassive black hole (SMBH) mass measurement in the Seyfert 1 galaxy NGC 7469 using Atacama Large Millimeter/submillimeter Array (ALMA) observations of the atomic-[CI](1-0) and molecular-12CO(1-0) emission lines at the spatial resolution of ≈0${_{.}^{\prime\prime}}$3 (or ≈100 pc). These emissions reveal that NGC 7469 hos…

2021 Monthly Notices of the Royal Astronomical Society
eHST 24
The Cosmic Ultraviolet Baryon Survey (CUBS) - IV. The complex multiphase circumgalactic medium as revealed by partial Lyman limit systems
DOI: 10.1093/mnras/stab2869 Bibcode: 2021MNRAS.508.4359C

Faucher-Giguère, Claude-André; Johnson, Sean D.; Petitjean, Patrick +18 more

We present a detailed study of two partial Lyman limit systems (pLLSs) of neutral hydrogen column density $N_\mathrm{H\, I}\approx (1-3)\times 10^{16}\, \mathrm{cm}^{-2}$ discovered at $z$ = 0.5 in the Cosmic Ultraviolet Baryon Survey (CUBS). Available far-ultraviolet spectra from the Hubble Space Telescope Cosmic Origins Spectrograph and optical …

2021 Monthly Notices of the Royal Astronomical Society
eHST 24
High-resolution ALMA and HST images of q1 Eri: an asymmetric debris disc with an eccentric Jupiter
DOI: 10.1093/mnras/stab1678 Bibcode: 2021MNRAS.506.1978L

Krist, J.; Stapelfeldt, K.; Kral, Q. +10 more

We present Atacama Large Millimetre/sub-Millimetre Array (ALMA) 1.3 and 0.86 mm observations of the nearby (17.34 pc) F9V star q1 Eri (HD 10647, HR 506). This system, with age ~1.4 Gyr, hosts a ~2 au radial velocity planet and a debris disc with the highest fractional luminosity of the closest 300 FGK type stars. The ALMA images, with resolution ~…

2021 Monthly Notices of the Royal Astronomical Society
AKARI Gaia eHST 24
Tidal tails in the disintegrating open cluster NGC 752
DOI: 10.1093/mnras/stab1404 Bibcode: 2021MNRAS.505.1607B

Vaidya, Kaushar; Rao, Khushboo K.; Agarwal, Manan +1 more

We utilize the robust membership determination algorithm, ML-MOC, on the precise astrometric and deep photometric data from Gaia Early Data Release 3 within a region of radius 5° around the centre of the intermediate-age Galactic open cluster NGC 752 to identify its member stars. We report the discovery of the tidal tails of NGC 752, extending out…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 24
WISDOM project - VII. Molecular gas measurement of the supermassive black hole mass in the elliptical galaxy NGC 7052
DOI: 10.1093/mnras/stab791 Bibcode: 2021MNRAS.503.5984S

Williams, Thomas G.; Sarzi, Marc; Cappellari, Michele +7 more

Supermassive black hole (SMBH) masses can be measured by resolving the dynamical influences of the SMBHs on tracers of the central potentials. Modern long-baseline interferometers have enabled the use of molecular gas as such a tracer. We present here Atacama Large Millimeter/submillimeter Array observations of the elliptical galaxy NGC 7052 at 0.…

2021 Monthly Notices of the Royal Astronomical Society
eHST 24
A method for finding anomalous astronomical light curves and their analogues
DOI: 10.1093/mnras/stab2588 Bibcode: 2021MNRAS.508.5734M

Graham, Matthew J.; Giles, Daniel; Mahabal, Ashish A. +4 more

Our understanding of the Universe has profited from deliberate targeted studies of known phenomena, as well as from serendipitous unexpected discoveries, such as the discovery of a complex variability pattern in the direction of KIC 8462852 (Boyajian's star). Upcoming surveys such as the Vera C. Rubin Observatory Legacy Survey of Space and Time wi…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 23
The centres of M83 and the Milky Way: opposite extremes of a common star formation cycle
DOI: 10.1093/mnras/stab1527 Bibcode: 2021MNRAS.505.4310C

Henshaw, Jonathan D.; Kruijssen, J. M. Diederik; Longmore, Steven N. +8 more

In the centres of the Milky Way and M83, the global environmental properties thought to control star formation are very similar. However, M83's nuclear star formation rate (SFR), as estimated by synchrotron and H α emission, is an order of magnitude higher than the Milky Way's. To understand the origin of this difference we use ALMA observations o…

2021 Monthly Notices of the Royal Astronomical Society
eHST 23
Locating the gamma-ray emission region in the brightest Fermi-LAT flat-spectrum radio quasars
DOI: 10.1093/mnras/staa3483 Bibcode: 2021MNRAS.500.5297A

Brown, Anthony M.; Acharyya, Atreya; Chadwick, Paula M.

We present a temporal and spectral analysis of the gamma-ray flux from nine of the brightest flat-spectrum radio quasars (FSRQs) detected with the Fermi Large Area Telescope during its first 8 yr of operation, with the aim of constraining the location of the emission region. Using the increased photon statistics obtained from the two brightest fla…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 23
Gauging the effect of supermassive black holes feedback on quasar host galaxies
DOI: 10.1093/mnras/stab1067 Bibcode: 2021MNRAS.504.3890D

Kraemer, S. B.; Crenshaw, D. M.; Storchi-Bergmann, T. +6 more

In order to gauge the role that active galactic nuclei play in the evolution of galaxies via the effect of kinetic feedback in nearby QSO 2's (z ~ 0.3), we observed eight such objects with bolometric luminosities $L_{bol} \sim 10^{46}\rm {erg\, s^{-1}}$ using Gemini Multi-Object Spectrograph-integral field units. The emission lines were fitted wit…

2021 Monthly Notices of the Royal Astronomical Society
eHST 23