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The assembly, calibration, and predicted performance of the SISTINE-2 sounding rocket payload
DOI: 10.1117/12.2594393 Bibcode: 2021SPIE11821E..0HC

Kruczek, Nicholas; France, Kevin; Fleming, Brian +4 more

The Suborbital Imaging Spectrograph for Transition-region Irradiance from Nearby Exoplanet host stars (SIS- TINE) sounding rocket payload is an f /30 imaging spectrograph designed to measure the far ultraviolet (1000 - 1275 and 1300 - 1565 Å) output of exoplanet host stars. The instrument is composed of an f /14 Cassegrain telescope with a 500 mm …

2021 UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII
eHST 2
Comprehensive in-orbit performance evaluation of the BepiColombo Laser Altimeter (BELA)
DOI: 10.1016/j.pss.2020.105088 Bibcode: 2021P&SS..19505088H

Thomas, Nicolas; Hussmann, Hauke; Pommerol, Antoine +7 more

The BepiColombo Laser Altimeter (BELA) is on its way to Mercury on board the Mercury Planetary Orbiter (MPO), one of the two spacecraft of the BepiColombo mission. It will arrive at Mercury in December 2025 and start measurements of Mercury's surface and environment. The goal of this study is to analyze the performance of BELA by using a comprehen…

2021 Planetary and Space Science
BepiColombo 2
Comet 21P/Giacobini-Zinner: Water production activity over 20 years with SOHO/SWAN
DOI: 10.1016/j.icarus.2020.114242 Bibcode: 2021Icar..35714242C

Bertaux, J. -L.; Combi, M. R.; Quémerais, E. +3 more

In 1985 Comet 21P/Giacobini-Zinner was the first comet visited by a spacecraft, the International Cometary Explorer (ICE) satellite, several months before the armada of Halley spacecraft had their encounters in 1986. ICE was originally the ISEE-3 satellite, designed for magnetospheric measurements near the Earth, and was diverted via a lunar gravi…

2021 Icarus
SOHO 2
Flare stars in nearby Galactic open clusters based on TESS data
DOI: 10.31577/caosp.2021.51.1.78 Bibcode: 2021CoSka..51...78M

Baratella, M.; Vida, K.; Maryeva, O. +3 more

The study is devoted to search for flare stars among confirmed members of Galactic open clusters using high-cadence photometry from TESS mission. We analyzed 957 high-cadence light curves of members from 136 open clusters. As a result, 56 flare stars were found, among them 8 hot B-A type objects. Of all flares, 63 % were detected in sample of cool…

2021 Contributions of the Astronomical Observatory Skalnate Pleso
Gaia 2
UBVI CCD photometry of Berkeley 55 open cluster
DOI: 10.1007/s12036-021-09757-9 Bibcode: 2021JApA...42...60A

Akkaya Oralhan, İnci

Fundamental astrophysical parameters have been derived for Berkeley 55 (Be 55) open cluster based on the UBVI charge-coupled device (CCD) photometric data observed using a AZT-22 1.5 m telescope at Maidanak Astronomical Observatory (MAO) in Uzbekistan. The mean reddening is obtained as E

2021 Journal of Astrophysics and Astronomy
Gaia 2
Detection of Strongly Turbulent Regions in the Supercorona with the Venus Express and Mars Express Satellites
DOI: 10.1134/S001679322103004X Bibcode: 2021Ge&Ae..61..293E

Bird, M. K.; Efimov, A. I.; Lukanina, L. A. +3 more

Experiments involving the radio sounding of solar plasma with signals from the Venus Express and Mars Express spacecraft, which were carried out from October 6 to December 6, 2006, provided data on frequency fluctuations of the radio signals for the western and eastern coronal limbs. The processing of this data provided information on the intensit…

2021 Geomagnetism and Aeronomy
MEx VenusExpress 2
Mass Segregation as a New Indicator of Binary, IMBH, and Stellar-mass Black Hole Systems in Globular Clusters
DOI: 10.3847/1538-4357/abd6b8 Bibcode: 2021ApJ...908..224W

Zhao, Gang; Wu, Wenbo

This study presents the mass segregation of 35 Galactic globular clusters (GCs) through the radial profile of the mean mass of main-sequence stars. Most of them are found to be mass segregated due to two-body relaxation effects. The GCs with a larger core to half-mass-radius ratio tend to be less mass segregated. Recent simulations show that energ…

2021 The Astrophysical Journal
eHST 2
Observations of bright stars with AstroSat soft X-ray telescope
DOI: 10.1007/s12036-020-09677-0 Bibcode: 2021JApA...42...77S

Singh, K. P.; Dewangan, G. C.; Bhattacharyya, S. +5 more

We present observations of four bright stars observed with the AstroSat Soft X-ray Telescope (SXT). Visible light from bright stars like these can leak through the very thin filter in front of the CCD in the focal plane CCD camera of the SXT and thus making the extraction of X-ray events difficult. Here, we show how to extract the X-ray events wit…

2021 Journal of Astrophysics and Astronomy
Gaia Hipparcos 2
Role of host galaxy in the formation of multiple stellar populations: analysis of NGC 1786 and NGC 1898
DOI: 10.1093/mnras/stab2094 Bibcode: 2021MNRAS.507..282V

Goudfrooij, Paul; Niederhofer, Florian; Vanaraj, Viswajith

Even after decades of research, the origin of multiple stellar populations in globular clusters (GCs) remains enigmatic. The question as to whether the galaxy environment plays a role in their formation remains unanswered. To that extent, we analysed two classical (>10 Gyr old) Large Magellanic Cloud GCs, NGC 1786 and NGC 1898, using imaging da…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 2
Sizes of the smallest particles at Saturn's ring edges
DOI: 10.1016/j.icarus.2020.114224 Bibcode: 2021Icar..35714224E

Colwell, Joshua E.; Esposito, Larry W.; Becker, Tracy M. +1 more

The Ultraviolet Imaging Spectrograph (UVIS) on the Cassini spacecraft observed 275 ring stellar occultations from July 2004 until August 2017. We use stellar occultation data from the UVIS High Speed Photometer (HSP) to characterize the smallest particles at ring edges by modeling observed diffraction signatures. We identify these signatures as sp…

2021 Icarus
Cassini 2