Search Publications

Mineralogical and Morphological Investigation of Butterfly-Shaped Unnamed Crater Using Datasets from Recent Lunar Missions
Bibcode: 2022LPICo2678.1330N

Pathak, S.; Bhattacharya, S.; Naik, S. S. +3 more

Mineralogical and morphological analyses of an unnamed-butterfly-shaped crater have been studied using Chandrayaan-2 IIRS and other data sets.

2022 53rd Lunar and Planetary Science Conference
Chandrayaan-1 0
Terrestrial Martian analogues from the Indian subcontinent: Implications for hydrological activity on Mars
DOI: 10.1016/j.icarus.2022.115118 Bibcode: 2022Icar..38515118C

Chavan, Anil; Bhandari, Subhash; Bhore, Vivek

Martian geology and surface geomorphic features are grouped under Noachian, Hesperian, and Amazonian eras, based on the crater retention ages and resurfacing ages by crater densities. Comparing the similarities and differences between Martian landforms and their terrestrial analogues promotes an understanding of how surface processes operated on b…

2022 Icarus
MEx 0
Possibilities of velocity field analysis from Hinode SOT/SP data
DOI: 10.1515/astro-2021-0026 Bibcode: 2022OAst...30..203M

Mozharovsky, Sergei G.

The possibility of analyzing the line of sight (LOS) velocity and its gradient at each point of the Hinode SOT/SP maps using bisector analysis is revealed. A technique for obtaining such gradient is described. To estimate the velocity gradient, it is necessary to know both the velocity value and the layer height to which the bisector point is resp…

2022 Open Astronomy
Hinode 0
Análisis cinemático de una eyección coronal de masa de 10 a 46 radios solares
Bibcode: 2022BAAA...63...24D

Cremades, H.; Balmaceda, L. A.; Di Lorenzo, L.

In this work we perform the three-dimensional reconstruction (3D) of the morphology of a coronal mass ejection (CME), in the range of heliocentric distances of approximately 10 to 46 solar radii. The event occurs on 2 April 2019, and we use observations made by LASCO-C3 aboard the Solar and Heliospheric Observatory (SOHO), SECCHI-COR2 and HI-1 abo…

2022 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
SOHO 0
Constraining the shape of Milky Way satellites with distance gradients
DOI: 10.1093/mnras/stac308 Bibcode: 2022MNRAS.511.4316A

Koposov, Sergey E.; An, Zhaozhou

We combine the Dark Energy Camera Legacy Survey DR8 photometry with Gaia photometry to study the 3D structure of Bootes I, Draco, Ursa Minor, Sextans, and Sculptor dwarf galaxies using blue horizontal branch (BHB) stars as distance indicators. We construct a new colour-absolute magnitude of BHB stars that we use to measure the distance gradients w…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 0
Numerical modeling of mapping of Martian epithermal neutron emission: Applications to FREND investigation onboard ESA's Trace Gas Orbiter
DOI: 10.1016/j.nima.2022.166997 Bibcode: 2022NIMPA103966997M

Mitrofanov, I. G.; Golovin, D. V.; Litvak, M. L. +2 more

Neutron telescope FREND is operating onboard ESA TGO mission from May 2018 till present. The instrument measures epithermal neutron flux from the Martian surface. Measured variations of the neutron flux may be used to determine hydrogen abundance in the soil usually interpreted as a water/water ice. The unique design of the instrument provides mea…

2022 Nuclear Instruments and Methods in Physics Research A
ExoMars-16 0
Martian Atmospheric Spectral End-Members Retrieval From ExoMars Thermal Infrared (TIRVIM) Data
DOI: 10.1029/2022JE007429 Bibcode: 2022JGRE..12707429A

Grigoriev, A.; Korablev, O.; Arnold, G. +7 more

Key knowledge about planetary composition can be recovered from the study of thermal infrared spectral range datasets. This range has a huge diagnostic potential because it contains diagnostic absorptions from a planetary surface and atmosphere. The main goal of this study is to process and interpret the dataset from the Thermal Infrared channel (…

2022 Journal of Geophysical Research (Planets)
ExoMars-16 MEx 0
X-ray absorption and reprocessing in the z 2.5 lensed quasar 2MASS J1042+1641
DOI: 10.1093/mnras/stac2554 Bibcode: 2022MNRAS.516.5997W

Stern, D.; Brightman, M.; Walton, D. J. +2 more

We present new broad-band X-ray observations of the z ~ 2.5 lensed quasar 2MASS J1042+1641, combining XMM-Newton, Chandra, and NuSTAR to provide coverage of the X-ray spectrum over the 0.3-40 keV bandpass in the observed frame, corresponding to the ~1-140 keV band in the rest frame of 2MASS J1042+1641. The X-ray data show clear evidence for strong…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
Gaia EDR3 Data For Three Young Stellar Objects
DOI: 10.52526/25792776-22.69.1-77 Bibcode: 2022CoBAO..69...77G

Gigoyan, K. K.; Gigoyan, K. S.; Azatyan, N. M.

We present Gaia Early Data Release 3 (GaiaEDR3) high accurate astrometric and photometric data and also Catalina Sky Survey (CSS) phase-dependent light curves for three Young Stellar Objects (YSO). They are LRL245, 2MASSJ04300424+3533238, and CVSO592. These tree YSOs are presented as periodic variables in the Catalina Surveys Data Release-1 (CSDR1…

2022 Communications of the Byurakan Astrophysical Observatory
Gaia 0
Five New faint cataclysmic variables from the Zwicky Transient Facility
DOI: 10.5817/OEJV2022-0228 Bibcode: 2022OEJV..228....1L

Bernhard, K.; Lloyd, Ch.

A search of faint, large-amplitude variables in the Zwicky Transient Facility datahas led to the identification of five new CVs. Four of the stars, ZTFJ010013.34+610809.8, ZTFJ051913.86+293006.0, ZTFJ210441.02+394052.7 and ZTFJ210705.14+394617.7 are probably SS Cyg-type systems, while ZTFJ173854.93+175136.3 is a likely SU UMa system.

2022 Open European Journal on Variable Stars
Gaia 0