Search Publications

Investigating Mercury's Environment with the Two-Spacecraft BepiColombo Mission
DOI: 10.1007/s11214-020-00712-8 Bibcode: 2020SSRv..216...93M

André, N.; Kallio, E.; Barabash, S. +76 more

The ESA-JAXA BepiColombo mission will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric dynamics at Mercury as well as their interactions with the solar wind, radiation, and interplanetary dust. Many scientific instruments onboard the two spacecraft will be com…

2020 Space Science Reviews
BepiColombo 78
Binary deviations from single object astrometry
DOI: 10.1093/mnras/staa1148 Bibcode: 2020MNRAS.495..321P

Koposov, S. E.; Belokurov, Vasily; Penoyre, Zephyr +2 more

Most binaries are undetected. Astrometric reductions of a system using the assumption that the object moves like a single point mass can be biased by unresolved binary stars. The discrepancy between the centre of mass of the system (which moves like a point mass) and the centre of light (which is what we observe) introduces additional motion. We e…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 78
A heatwave of accretion energy traced by masers in the G358-MM1 high-mass protostar
DOI: 10.1038/s41550-019-0989-3 Bibcode: 2020NatAs...4..506B

Eislöffel, J.; Stecklum, B.; Kim, Kee-Tae +20 more

High-mass stars are thought to accumulate much of their mass via short, infrequent bursts of disk-aided accretion1,2. Such accretion events are rare and difficult to observe directly but are known to drive enhanced maser emission3-6. In this Letter we report high-resolution, multi-epoch methanol maser observations toward G358…

2020 Nature Astronomy
Gaia 78
Structural Evolution in Massive Galaxies at z ∼ 2
DOI: 10.3847/1538-4357/abaf4a Bibcode: 2020ApJ...901...74T

Übler, Hannah; Mowla, Lamiya; Kohno, Kotaro +18 more

We present 0"2 resolution Atacama Large Millimeter/submillimeter Array (ALMA) observations at 870 µm in a stellar mass-selected sample of 85 massive ( ${M}_{\star }\gt {10}^{11}\,{M}_{\odot }$ ) star-forming galaxies (SFGs) at $z=1.9\mbox{--}2.6$ in the CANDELS/3D-Hubble Space Telescope fields of UDS and GOODS-S. We measure the effective rad…

2020 The Astrophysical Journal
eHST 78
A Low-mass Stellar-debris Stream Associated with a Globular Cluster Pair in the Halo
DOI: 10.3847/2041-8213/aba49f Bibcode: 2020ApJ...898L..37Y

Huang, Yang; Beers, Timothy C.; Chang, Jiang +1 more

There are expected to be physical relationships between the globular clusters (GCs) and stellar substructures in the Milky Way, not all of which have yet been found. We search for such substructures from a combined halo sample of SDSS blue horizontal-branch and SDSS+LAMOST RR Lyrae stars, cross-matched with astrometric information from Gaia DR2. T…

2020 The Astrophysical Journal
Gaia 78
Modelling the He I triplet absorption at 10 830 Å in the atmosphere of HD 209458 b
DOI: 10.1051/0004-6361/201937175 Bibcode: 2020A&A...636A..13L

Alonso-Floriano, F. J.; Sánchez-López, A.; López-Puertas, M. +16 more

Context. HD 209458 b is an exoplanet with an upper atmosphere undergoing blow-off escape that has mainly been studied using measurements of the Lyα absorption. Recently, high-resolution measurements of absorption in the He I triplet line at 10 830 Å of several exoplanets (including HD 209458 b) have been reported, creating a new opportunity to pro…

2020 Astronomy and Astrophysics
eHST 77
Palomar Gattini-IR: Survey Overview, Data Processing System, On-sky Performance and First Results
DOI: 10.1088/1538-3873/ab6069 Bibcode: 2020PASP..132b5001D

Soria, Roberto; Burdge, Kevin B.; De, Kishalay +24 more

Palomar Gattini-IR is a new wide-field, near-infrared (NIR) robotic time domain survey operating at Palomar Observatory. Using a 30 cm telescope mounted with a H2RG detector, Gattini-IR achieves a field of view (FOV) of 25 sq. deg. with a pixel scale of 8.″7 in J-band. Here, we describe the system design, survey operations, data processing system …

2020 Publications of the Astronomical Society of the Pacific
Gaia 77
A Probabilistic Approach to Kepler Completeness and Reliability for Exoplanet Occurrence Rates
DOI: 10.3847/1538-3881/ab8a30 Bibcode: 2020AJ....159..279B

Huber, D.; Mullally, S. E.; Berger, T. +5 more

Exoplanet catalogs produced by surveys suffer from a lack of completeness (not every planet is detected) and less than perfect reliability (not every planet in the catalog is a true planet), particularly near the survey's detection limit. Exoplanet occurrence rate studies based on such a catalog must be corrected for completeness and reliability. …

2020 The Astronomical Journal
Gaia 77
X-ray detected AGN in SDSS dwarf galaxies
DOI: 10.1093/mnras/staa040 Bibcode: 2020MNRAS.492.2268B

Birchall, Keir L.; Watson, M. G.; Aird, J.

In this work we present a robust quantification of X-ray selected AGN in local (z ≤ 0.25) dwarf galaxies (M_* ≤ 3 × 10^9 M_⊙ ). We define a parent sample of 4331 dwarf galaxies found within the footprint of both the MPA-JHU galaxy catalogue (based on SDSS DR8) and 3XMM DR7, performed a careful review of the data to remove misidentifications and pr…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 77
Stellar rotation periods from K2 Campaigns 0-18. Evidence for rotation period bimodality and simultaneous variability decrease
DOI: 10.1051/0004-6361/201936887 Bibcode: 2020A&A...635A..43R

Reinhold, Timo; Hekker, Saskia

Context. Rotation period measurements of stars observed with the Kepler mission have revealed a lack of stars at intermediate rotation periods, accompanied by a decrease of photometric variability. Whether this so-called dearth region is a peculiarity of stars in the Kepler field, or reflects a general manifestation of stellar magnetic activity, i…

2020 Astronomy and Astrophysics
Gaia 77