Search Publications

An interferometric SETI observation of Kepler-111 b
DOI: 10.1093/mnras/stad1151 Bibcode: 2023MNRAS.522.3784W

Gajjar, Vishal; Garrett, Michael A.; Wandia, Kelvin +8 more

The application of very long baseline interferometry (VLBI) to the search for extraterrestrial intelligence (SETI) has been limited to date, despite the technique offering many advantages over traditional single-dish SETI observations. In order to further develop interferometry for SETI, we used the European VLBI network (EVN) at 21 cm to observe …

2023 Monthly Notices of the Royal Astronomical Society
Gaia 2
New photometric solutions of contact binaries HX UMa and FP Boo
DOI: 10.1016/j.newast.2022.101946 Bibcode: 2023NewA...9901946Y

Yıldırım, M. F.

By using different databases (TESS, SuperWASP, KWS and ASAS-SN), light curve analyzes of HX UMa and FP Boo systems were performed, and the changes in the orbital period of the systems were also examined. The light curve analyzes of the systems were conducted simultaneously with the radial velocities using the Wilson and Devinney (WD) code. As a re…

2023 New Astronomy
Gaia 2
Dark halos around solar active regions. I. Emission properties of the dark halo around NOAA 12706
DOI: 10.1051/0004-6361/202347414 Bibcode: 2023A&A...680A..61L

Andretta, V.; Del Zanna, G.; Murabito, M. +1 more

Context. Dark areas around active regions (ARs) were first observed in chromospheric lines more than a century ago and are now associated with the Hα fibril vortex around ARs. Nowadays, large areas surrounding ARs with reduced emission relative to the quiet Sun (QS) are also observed in spectral lines emitted in the transition region (TR) and the …

2023 Astronomy and Astrophysics
IRIS 2
NGC 4117: A New Compton-thick AGN Revealed by Broadband X-Ray Spectral Analysis
DOI: 10.1088/1674-4527/acc151 Bibcode: 2023RAA....23e5002M

Mohanadas, Pavithra; Annuar, Adlyka

In this paper, we present the broadband (0.5-195 keV) X-ray spectral analysis for one of the newly detected AGNs in the Swift-BAT 105 month Hard X-ray Survey Catalog, NGC 4117. According to our ongoing research on low luminosity AGNs from the Swift-BAT 105 month catalog, we examine whether they are indeed low luminosity or heavily obscured AGNs. O…

2023 Research in Astronomy and Astrophysics
XMM-Newton 2
An astrometric approach to measuring the colour of an object
DOI: 10.1093/mnras/stad2619 Bibcode: 2023MNRAS.525.4999G

Lin, F. R.; Peng, Q. Y.; Guo, B. F. +1 more

The colour of a star is a critical feature to reflect its physical property such as the temperature. The colour index is usually obtained via absolute photometry, which is demanding for weather conditions and instruments. In this work, we present an astrometric method to measure the catalogue-matched colour index of an object based on the effect o…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 2
Photometric calibration in u-band using blue halo stars
DOI: 10.1093/mnras/stac3671 Bibcode: 2023MNRAS.519.2281L

von der Linden, Anja; Liang, Shuang

We develop a method to calibrate u-band photometry based on the observed colour of blue Galactic halo stars. The Galactic halo stars belong to an old stellar population of the Milky Way and have relatively low metallicity. The 'blue tip' of the halo population - the main sequence turn-off (MSTO) stars - is known to have a relatively uniform intrin…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 2
G 68-34: A Double-lined M-dwarf Eclipsing Binary in a Hierarchical Triple System
DOI: 10.3847/1538-4357/accadf Bibcode: 2023ApJ...949...37P

Charbonneau, David; Pass, Emily K.

Using high-resolution spectra from the Tillinghast Reflector Echelle Spectrograph and photometry from sector 56 of the Transiting Exoplanet Survey Satellite, we report that the nearby M dwarf G 68-34 is a double-lined eclipsing binary. The pair is spin-orbit synchronized with a period of 0.655 days. The light curve shows significant spot modulatio…

2023 The Astrophysical Journal
Gaia 2
A Catalog of Collected Debris Disks: Properties, Classifications and Correlations between Disks and Stars/Planets
DOI: 10.1088/1674-4527/acd591 Bibcode: 2023RAA....23h5002C

Liu, Qiong; Liao, Neng-Hui; Cao, Peng-Cheng +2 more

We have collected a catalog of 1095 debris disks with properties and classification (resolved, planet, gas) information. From the catalog, we defined a less biased sample with 612 objects and presented the distributions of their stellar and disk properties to search for correlations between disks and stars. We found debris disks were widely distri…

2023 Research in Astronomy and Astrophysics
Gaia 2
A possible mechanism for the formation of an eastward moving auroral spiral
DOI: 10.3389/fspas.2023.1240081 Bibcode: 2023FrASS..1040081M

Grigorenko, Elena E.; Kronberg, Elena A.; Partamies, Noora +1 more

The generation process of auroral spirals is described by different theories varying for their morphology and surrounding conditions. Here, a possible mechanism is proposed for an eastward moving auroral spiral, which was observed in Tromsø, Norway, during the expansion phase of a substorm on 18 September 2013. Measurements from the THEMIS-A and C…

2023 Frontiers in Astronomy and Space Sciences
Cluster 2
Spectral Clustering of CRISM Datasets in Jezero Crater Using UMAP and k-Means
DOI: 10.3390/rs15040939 Bibcode: 2023RemS...15..939P

Thomas, Nicolas; Rossi, Angelo Pio; Fernandes, Michael +2 more

In this paper, we expand upon our previous research on unsupervised learning algorithms to map the spectral parameters of the Martian surface. Previously, we focused on the VIS-NIR range of hyperspectral data from the CRISM imaging spectrometer instrument onboard NASA's Mars Reconnaissance Orbiter to relate to other correspondent imager data sourc…

2023 Remote Sensing
MEx 2