Search Publications

Discovery of an inflated hot Jupiter around a slightly evolved star TOI-1789
DOI: 10.1093/mnras/stab2970 Bibcode: 2022MNRAS.509.3339K

Howell, Steve B.; Fridlund, Malcolm; Guenther, Eike W. +11 more

We report here the discovery of a hot Jupiter at an orbital period of 3.208664 ± 0.000015 d around TOI-1789 (TYC 1962-00303-1, TESSmag = 9.1) based on the TESS photometry, ground-based photometry, and high-precision radial velocity (RV) observations. The high-precision RV observations were obtained from the high-resolution spectrographs…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
fBLS - a fast-folding BLS algorithm
DOI: 10.1093/mnras/stac960 Bibcode: 2022MNRAS.513.2732S

Mazeh, T.; Faigler, S.; Shahaf, S. +2 more

We present fBLS - a novel fast-folding technique to search for transiting planets, based on the fast-folding algorithm (FFA), which is extensively used in pulsar astronomy. For a given light curve with N data points, fBLS simultaneously produces all the binned phase-folded light curves for an array of Np trial periods. For each folded l…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
First optical identification of the SRG/eROSITA-detected supernova remnant G 116.6 - 26.1. I. Preliminary results
DOI: 10.1093/mnras/stac1599 Bibcode: 2022MNRAS.515..339P

Palaiologou, E. V.; Leonidaki, I.; Kopsacheili, M.

The supernova remnant (SNR) candidate G 116.6 - 26.1 is one of the few high Galactic latitude (|b| > 15°) remnants detected so far in several wavebands. It was discovered recently in the SRG/eROSITA all-sky X-ray survey and also displays a low-frequency weak radio signature. In this study, we report the first optical detection of G 116.6 - 26.1…

2022 Monthly Notices of the Royal Astronomical Society
AKARI 6
X-ray variability of transitional millisecond pulsars: a faint, stable, and fluctuating disc
DOI: 10.1093/mnras/stac720 Bibcode: 2022MNRAS.512.5269L

Wijnands, Rudy; Linares, Manuel; van der Klis, Michiel +1 more

Transitional millisecond pulsars (tMSPs) have emerged in the last decade as a unique class of neutron stars at the crossroads between accretion- and rotation-powered phenomena. In their (sub-luminous) accretion disc state, with X-ray luminosities of order 1033-1034 erg s-1, they switch rapidly between two distinct …

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 6
Machine learning-based search for cataclysmic variables within Gaia Science Alerts
DOI: 10.1093/mnras/stac2760 Bibcode: 2022MNRAS.517.3362M

Copperwheat, C. M.; Darnley, M. J.; Mistry, D. +1 more

Wide-field time domain facilities detect transient events in large numbers through difference imaging. For example, Zwicky Transient Facility produces alerts for hundreds of thousands of transient events per night, a rate set to be dwarfed by the upcoming Vera C. Rubin Observatory. The automation provided by machine learning (ML) is therefore nece…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6
X-ray response to disc evolution in two γ Cas stars
DOI: 10.1093/mnras/stac314 Bibcode: 2022MNRAS.512.1648N

Nazé, Yaël; Rauw, Gregor; Bohlsen, Terrence +4 more

The Hα emission of a set of southern γ Cas stars was monitored since 2019, with the aim of detecting transition events and examining how their peculiar X-ray emission would react in such cases. Two stars, namely HD 119682 and V767 Cen, were found to display slowly decreasing disc emissions. These decreases were not perfectly monotonic and several …

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 6
Spectral and temporal properties of ultra-luminous X-ray source NGC 55 ULX1
DOI: 10.1093/mnras/stab3307 Bibcode: 2022MNRAS.509.5166J

Jithesh, V.

We investigate the spectral and temporal properties of ultra-luminous X-ray source (ULX) NGC 55 ULX1 using Swift, XMM-Newton and NuSTAR observations conducted during 2013-2021. In these observations, the source flux varies by a factor of ~5-6, and we identify the source mainly in the soft ultraluminous (SUL) state of ULXs. We fit the X-ray spectra…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 6
Galaxy clustering in the VVV near-IR galaxy catalogue
DOI: 10.1093/mnras/stac981 Bibcode: 2022MNRAS.513.2747S

Minniti, Dante; Alonso, M. Victoria; Valotto, Carlos +7 more

Mapping galaxies at low Galactic latitudes and determining their clustering status are fundamental steps in defining the large-scale structure in the nearby Universe. The VISTA Variables in the Vía Láctea (VVV) near-IR galaxy catalogue (VVV NIRGC) allows us to explore this region in great detail. Our goal is to identify galaxy overdensities and ch…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6
Identifying RR Lyrae in the ZTF DR3 data set
DOI: 10.1093/mnras/stab3654 Bibcode: 2022MNRAS.510.3575H

Koposov, Sergey E.; Huang, Kuan-Wei

We present an RR Lyrae (RRL) catalogue based on the combination of the third data release of the Zwicky Transient Facility (ZTF DR3) and Gaia EDR3. We use a multistep classification pipeline relying on the Fourier decomposition fitting to the multiband ZTF light curves and random forest classification. The resulting catalogue contains 71 755 RRLs …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6
An X-ray view of the ambiguous nuclear transient AT2019pev
DOI: 10.1093/mnras/stac2073 Bibcode: 2022MNRAS.515.5198Y

Kochanek, C. S.; Grupe, D.; Mathur, S. +3 more

AT2019pev is a nuclear transient in a narrow-line Seyfert 1 galaxy at z = 0.096. The archival ultraviolet, optical, and infrared data showed features of both tidal disruption events and active galactic nuclei (AGNs), and its nature is not fully understood. We present detailed X-ray observations of AT2019pev taken with Swift, Chandra, and NICER ove…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6