Search Publications

Detection of 2460 double-lined spectroscopic binary candidates in the LAMOST-MRS using projected rotational velocities and a binary spectral model
DOI: 10.1093/mnras/stac2513 Bibcode: 2022MNRAS.517..356K

Han, Zhanwen; Kovalev, Mikhail; Chen, Xuefei

We present a new method for the detection of double-lined spectroscopic binaries (SB2s) using Vsin i values from spectral fits. The method is tested on synthetic and real spectra from the Large Sky Area Multi-Object fiber Spectroscopic Telescope Medium Resolution Survey. It can reliably detect SB2 candidates for double-lined binaries with $V \sin …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
An INTEGRAL/SPI view of reticulum II: particle dark matter and primordial black holes limits in the MeV range
DOI: 10.1093/mnras/stac008 Bibcode: 2022MNRAS.511..914S

Calore, Francesca; Vincent, Aaron C.; Diehl, Roland +4 more

Reticulum II (Ret II) is a satellite galaxy of the Milky Way (MW) and presents a prime target to investigate the nature of dark matter (DM) because of its high mass-to-light ratio. We evaluate a dedicated INTEGRAL observation campaign data set to obtain γ-ray fluxes from Ret II and compare those with expectations from DM. Ret II is not detected in…

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL 22
The XMM Cluster Survey analysis of the SDSS DR8 redMaPPer catalogue: implications for scatter, selection bias, and isotropy in cluster scaling relations
DOI: 10.1093/mnras/stac2414 Bibcode: 2022MNRAS.516.3878G

Nichol, R. C.; Miller, C. J.; Romer, A. K. +21 more

In this paper, we present the X-ray analysis of Sloan Digital Sky Survey DR8 redMaPPer (SDSSRM) clusters using data products from the XMM Cluster Survey (XCS). In total, 1189 SDSSRM clusters fall within the XMM-Newton footprint. This has yielded 456 confirmed detections accompanied by X-ray luminosity (LX) measurements. Of these cluster…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 22
Five young δ Scuti stars in the Pleiades seen with Kepler/K2
DOI: 10.1093/mnras/stac240 Bibcode: 2022MNRAS.511.5718M

Li, Yaguang; Bedding, Timothy R.; White, Timothy R. +4 more

We perform mode identification for five δ Scuti stars in the Pleiades star cluster, using custom light curves from K2 photometry. By creating échelle diagrams, we identify radial and dipole mode ridges, comprising a total of 28 radial and 16 dipole modes across the five stars. We also suggest possible identities for those modes that lie offset fro…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
Stellar and black hole assembly in z < 0.3 infrared-luminous mergers: intermittent starbursts versus super-Eddington accretion
DOI: 10.1093/mnras/stac980 Bibcode: 2022MNRAS.513.4770F

Lebouteiller, Vianney; Pearson, Chris; Clements, David L. +20 more

We study stellar and black hole mass assembly in a sample of 42 infrared-luminous galaxy mergers at z < 0.3 by combining results from radiative transfer modelling with archival measures of molecular gas and black hole mass. The ratios of stellar mass, molecular gas mass, and black hole mass to each other are consistent with those of massive gas…

2022 Monthly Notices of the Royal Astronomical Society
Herschel 22
Improving blazar redshift constraints with the edge of the Ly α forest: 1ES 1553+113 and implications for observations of the WHIM
DOI: 10.1093/mnras/stab3331 Bibcode: 2022MNRAS.509.4330D

Narayanan, A.; Sameer; Charlton, J. +6 more

Blazars are some of the brightest ultraviolet (UV) and X-ray sources in the sky and are valuable probes of the elusive warm-hot intergalactic medium (WHIM; T ≃ 105-107 K). However, many of the brightest blazars - called BL Lac objects such as 1ES 1553+113 - have quasi-featureless spectra and poorly constrained redshifts. Here…

2022 Monthly Notices of the Royal Astronomical Society
eHST 22
The value-added catalogue of ASAS-SN eclipsing binaries: parameters of 30 000 detached systems
DOI: 10.1093/mnras/stac2520 Bibcode: 2022MNRAS.517.2190R

Kochanek, C. S.; Stanek, K. Z.; Thompson, Todd A. +6 more

Detached eclipsing binaries are a fundamental tool for measuring the physical parameters of stars that are effectively evolving in isolation. Starting from more than 40 000 eclipsing binary candidates identified by the All-Sky Automated Survey for Supernovae (ASAS-SN), we use PHOEBE to determine the sum of the fractional radii, the ratio of effect…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
Chromosome maps of globular clusters from wide-field ground-based photometry
DOI: 10.1093/mnras/stac3086 Bibcode: 2022MNRAS.517.5687J

Milone, A. P.; Cordoni, G.; Marino, A. F. +10 more

Hubble Space Telescope (HST) photometry is providing an extensive analysis of globular clusters (GCs). In particular, the pseudo-two-colour diagram dubbed 'chromosome map (ChM)' allowed to detect and characterize their multiple populations with unprecedented detail. The main limitation of these studies is the small field of view of HST, which make…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
The white dwarf binary pathways survey - VIII. A post-common envelope binary with a massive white dwarf and an active G-type secondary star
DOI: 10.1093/mnras/stac2837 Bibcode: 2022MNRAS.517.2867H

Gänsicke, B. T.; Rebassa-Mansergas, A.; Raddi, R. +6 more

The white dwarf binary pathways survey is dedicated to studying the origin and evolution of binaries containing a white dwarf and an intermediate-mass secondary star of the spectral type A, F, G, or K (WD + AFGK). Here, we present CPD-65 264, a new post-common envelope binary with an orbital period of 1.37 d that contains a massive white dwarf ($0…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 22
Eclipsing white dwarf binaries in Gaia and the Zwicky Transient Facility
DOI: 10.1093/mnras/stab3293 Bibcode: 2022MNRAS.509.4171K

Belokurov, Vasily; Breedt, Elmé; Hodgkin, Simon +4 more

Gaia provided the largest ever catalogue of white dwarf stars. We use this catalogue, along with the third public data release of the Zwicky Transient Facility (ZTF), to identify new eclipsing white dwarf binaries. Our method exploits light-curve statistics and the box least-squares algorithm to detect periodic light-curve variability. The search …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22