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Mass of the Asteroid (7348) 1993FJ22 as Determined by the Dynamic Method
DOI: 10.1134/S1990341322010072 Bibcode: 2022AstBu..77..112K

Kuznetsov, V. B.; Chernetenko, Yu. A.

—The mass of the asteroid ($$7348$$) is determined by the dynamic method based on the analysis of gravitational perturbations in the motion of the asteroid (7562) Kagiroino–Oka caused by asteroid (7348). The choice of these asteroids is due to the fact that on March

2022 Astrophysical Bulletin
Gaia 0
Refining the Masses and Radii of the Star Kepler-33 and its Five Transiting Planets
DOI: 10.3847/1538-3881/ac98c4 Bibcode: 2022AJ....164..242S

Lissauer, Jack J.; Jontof-Hutter, Daniel; Sikora, James +1 more

Kepler-33 hosts five validated transiting planets ranging in period from 5 to 41 days. The planets are in nearly coplanar orbits and exhibit remarkably similar (appropriately scaled) transit durations indicative of similar impact parameters. The outer three planets have a radius of 3.5 ≲ R p/R ≲ 4.7 and are closely packed d…

2022 The Astronomical Journal
Gaia 0
Indian Planetary Missions and Science
Bibcode: 2022cosp...44..960B

Bhardwaj, Anil

The planetary exploration program in India started in the new millennium with the launch of Chandrayaan-1 orbiter mission to the Moon in 2008, which was a highly successful mission since it discovered water on the Moon. The next Indian planetary mission was to Mars: the Mars Orbiter Mission (MOM), launched in November 2013 and arriving on Mars in …

2022 44th COSPAR Scientific Assembly. Held 16-24 July
Chandrayaan-1 0
Red giant branch bump brightness in 7 metal-poor globular clusters obtained with GAIA DR2
DOI: 10.1007/s10509-022-04058-1 Bibcode: 2022Ap&SS.367...32S

Nie, Jundan; Wu, Tao; Pietrinferni, Adriano +10 more

The identification of the red giant branch bump brightness in metal-poor globular clusters is important for low-mass stellar evolution. The release of Gaia DR2 prompted us to revisit the red giant branch bump (RGBB) in galactic globular clusters. We apply a popular nonparametric density estimation approach, kernel density estimation (KDE), to expl…

2022 Astrophysics and Space Science
Gaia 0
New late-type stars found in the BAO Plate Archive
DOI: 10.52526/25792776-22.69.2-343 Bibcode: 2022CoBAO..69..343K

Kostandyan, G. R.; Abrahamyan, H. V.; Paronyan, G. M. +1 more

The BAO Plate Archive low-resolution spectral plate centered \alpha = +04h; \delta = +240 is analyzed to find new late-type stars. 25 new late-type stars have been detected. We have performed cross-correlations with GAIA DR3, USNO-B1.0, 2MASS, AllWISE, IRAS PSC/FSC, AKARI and SDSS. For new detected objects, we present luminosity classes estimated …

2022 Communications of the Byurakan Astrophysical Observatory
Gaia 0
Retrieval of Lunar Surface Temperature and Spectral Emissivity in 3-5 µm Range from Chandrayaan-2 IIRS Observations
Bibcode: 2022LPICo2678.1201O

Bhattacharya, S.; Ojha, S. P.; Vikram, K. V. N. G.

Algorithm for the retrieval of lunar surface temperature and emissivity is presented in this study.

2022 53rd Lunar and Planetary Science Conference
Chandrayaan-1 0
Description and Application of the Surfing Effect
DOI: 10.3390/universe8120620 Bibcode: 2022Univ....8..620M

Nucita, Achille A.; De Paolis, Francesco; Maiorano, Michele

The standard technique for very low-frequency gravitational wave detection is mainly based on searching for a specific spatial correlation in the variation of the times of arrival of the radio pulses emitted by millisecond pulsars with respect to a timing model. This spatial correlation, which in the case of the gravitational wave background must …

2022 Universe
Gaia 0
Joint Cluster/Ground-Based Studies in the First 20 Years of the Cluster Mission
DOI: 10.1029/2021JA029928 Bibcode: 2022JGRA..12729928F

Fear, R. C.

Ground-based facilities make an important contribution to our understanding of the magnetospheric system. Coordination with ground-based facilities has been embedded within the Cluster mission since before launch, and this has given rise to a large number of studies which have exploited data from both Cluster and one or more of the diverse range o…

2022 Journal of Geophysical Research (Space Physics)
Cluster 0
The Extragalactic Population of Accreting Neutron Stars and the Ultraluminous X-ray Sources Paradigm: from ULTraS to PULSULTraS
DOI: 10.36116/MEMSAIT_93N2_3.2022.4 Bibcode: 2022MmSAI..93b..34I

Salvaterra, R.; Tiengo, A.; de Luca, A. +11 more

The unambiguous identification of the nature of a neutron star in X-rays is achieved through the detection of coherent signals reflecting the spin period of the compact object. The search for coherent signals in the whole XMM-Newton source catalog was one of the main aims of the EU/FP7-funded project EXTraS (active in 2014-2016). The ULTraS and PU…

2022 Memorie della Societa Astronomica Italiana
XMM-Newton 0
Spectral Unmixing and Abundance Estimation of Different Pyroxene Species Using IIRS Chandrayaan-2 Hyperspectral Imagery
Bibcode: 2022LPICo2678.1070A

Bhattacharya, S.; Kumar, A.; Misra, A. +6 more

Chandrayaan-2 IIRS was used to determine lunar minerals and their abundance near Taurus-Littrow valley consisting of Gardner Crater using linear mixing model.

2022 53rd Lunar and Planetary Science Conference
Chandrayaan-1 0