Search Publications

A Statistical Comparison of EUV Brightenings Observed by SO/EUI with Simulated Brightenings in Nonpotential Simulations
DOI: 10.1007/s11207-022-02074-6 Bibcode: 2022SoPh..297..141B

Harra, Louise K.; Barczynski, Krzysztof; Berghmans, David +3 more

The High Resolution Imager (HRIEUV) telescope of the Extreme Ultraviolet Imager (EUI) instrument onboard Solar Orbiter has observed EUV brightenings, so-called campfires, as fine-scale structures at coronal temperatures. The goal of this paper is to compare the basic geometrical (size, orientation) and physical (intensity, lifetime) pro…

2022 Solar Physics
SolarOrbiter 4
A deeper solution to the actual geometry of CCD mosaic chips
DOI: 10.1051/0004-6361/202141725 Bibcode: 2022A&A...661A..75Z

Vienne, A.; Lin, F. R.; Peng, Q. Y. +2 more

Context. For charge-coupled device (CCD) mosaic chips in the focal plane of a large telescope, the unification for all the measurements of each chip is vital to some scientific projects, such as deep astrometric standards or construction for deeper images that can also seamlessly cover a larger area of the sky. A key part of the reduction involves…

2022 Astronomy and Astrophysics
Gaia 4
Cloud motion and magnetic fields: Four clouds in the Cepheus Flare region
DOI: 10.1051/0004-6361/202140495 Bibcode: 2022A&A...658A..55S

Maheswar, G.; Dib, S.; Sharma, E.

Context. The Cepheus Flare region consists of a group of dark cloud complexes that are currently active in star formation.
Aims: The aim of this work is to estimate the motions of four clouds, namely L1147/1158, L1172/1174, L1228, and L1251, located at relatively high Galactic latitude (b > 14°) in the Cepheus Flare region. We study the re…

2022 Astronomy and Astrophysics
Gaia Herschel 4
Infrared Properties of OGLE4 Mira Variables in Our Galaxy
DOI: 10.5303/JKAS.2022.55.6.195 Bibcode: 2022JKAS...55..195S

Suh, Kyung-Won

We investigate infrared properties of OGLE4 Mira variables in our Galaxy. For each object, we cross-identify the AllWISE, 2MASS, Gaia, and IRAS counterparts. We present various IR two-color diagrams (2CDs) and period-magnitude and period-color relations for the Mira variables. Generally, the Mira variables with longer periods are brighter in the I…

2022 Journal of Korean Astronomical Society
AKARI Gaia 4
Interplanetarymedium monitoring with LISA: Lessons from LISA Pathfinder
DOI: 10.1051/swsc/2022031 Bibcode: 2022JSWSC..12...36C

Cesarini, A.; Grimani, C.; Telloni, D. +4 more

The Laser Interferometer Space Antenna (LISA) of the European Space Agency (ESA) will be the first low-frequency gravitational-wave observatory orbiting the Sun at 1 AU. The LISA Pathfinder (LPF) mission, aiming at testing the instruments to be located on board the LISA spacecraft (S/C), hosted, among the others, fluxgate magnetometers and a parti…

2022 Journal of Space Weather and Space Climate
LISAPathfinder 4
Dust extinction map of the Galactic plane based on the VVV survey data
DOI: 10.1093/mnras/stac3012 Bibcode: 2022MNRAS.517.5180Z

Zhang, M.; Kainulainen, J.

Dust extinction is one of the most reliable tracers of the gas distribution in the Milky Way. The near-infrared (NIR) Vista Variables in the Vía Láctea (VVV) survey enables extinction mapping based on stellar photometry over a large area in the Galactic plane. We devise a novel extinction mapping approach, XPNICER, by bringing together VVV photome…

2022 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 4
Clay sediments derived from fluvial activity in and around Ladon basin, Mars
DOI: 10.1016/j.icarus.2022.115090 Bibcode: 2022Icar..38415090W

Weitz, Catherine M.; Wilson, Sharon A.; Grant, John A. +5 more

The morphology and mineralogy of light-toned layered sedimentary deposits were investigated using multiple orbital datasets across the Ladon basin region, including within northern Ladon Valles, southern Ladon basin, and the southwestern highlands of Ladon basin. Light-toned layered deposits are particularly widespread in Ladon Valles and Ladon ba…

2022 Icarus
MEx 4
Insights into the Evolution of Five Isolated Galaxies
DOI: 10.3847/1538-4357/ac4808 Bibcode: 2022ApJ...927..124M

Wolter, A.; Uslenghi, M.; Marino, A. +3 more

Galaxy evolution is believed to be conditioned by the environment. Isolated galaxies or galaxies in poor groups are an excellent laboratory to study evolutionary mechanisms where effects of the environment are minimal. We present new Swift-UVOT data in six filters, three in the ultraviolet (UV), of five isolated galaxies aiming at shedding light i…

2022 The Astrophysical Journal
AKARI 4
Completing the protostellar luminosity function in Cygnus-X with SOFIA/FORCAST imaging
DOI: 10.1093/mnras/stac436 Bibcode: 2022MNRAS.512..960C

Gutermuth, Robert A.; Pokhrel, Riwaj; Heyer, Mark +4 more

We present a new SOFIA/FORCAST mid-infrared survey of luminous protostars and crowded star-forming environments in Cygnus X, the nearest million-solar mass molecular cloud complex. We derive bolometric luminosities for over 1000 sources in the region with these new data in combination with extant Spitzer and UKIDSS photometry, with 63 new luminous…

2022 Monthly Notices of the Royal Astronomical Society
Herschel 4
The strongly irradiated planets in Praesepe
DOI: 10.1093/mnras/stac437 Bibcode: 2022MNRAS.512...41K

Wheatley, Peter J.; Agüeros, Marcel A.; King, George W. +3 more

We present an analysis of XMM-Newton observations of four stars in the young (670 Myr) open cluster Praesepe. The planets hosted by these stars all lie close in radius-period space to the radius-period valley and/or the Neptunian desert, two features that photoevaporation by X-ray and extreme ultraviolet (EUV) photons could be driving. Although th…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 4