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Streams, Substructures, and the Early History of the Milky Way
DOI: 10.1146/annurev-astro-032620-021917 Bibcode: 2020ARA&A..58..205H

Helmi, Amina

The advent of the second data release of the Gaia mission, in combination with data from large spectroscopic surveys, is revolutionizing our understanding of the Galaxy. Thanks to these transformational data sets and the knowledge accumulated thus far, a new, more mature picture of the evolution of the early Milky Way is currently emerging. Two of…

2020 Annual Review of Astronomy and Astrophysics
Gaia 329
The SunPy Project: Open Source Development and Status of the Version 1.0 Core Package
DOI: 10.3847/1538-4357/ab4f7a Bibcode: 2020ApJ...890...68S

Ryan, Daniel F.; Murray, Sophie A.; Ireland, Jack +32 more

The goal of the SunPy project is to facilitate and promote the use and development of community-led, free, and open source data analysis software for solar physics based on the scientific Python environment. The project achieves this goal by developing and maintaining the sunpy core package and supporting an ecosystem of affiliated packages. This …

2020 The Astrophysical Journal
Gaia 320
INTEGRAL Discovery of a Burst with Associated Radio Emission from the Magnetar SGR 1935+2154
DOI: 10.3847/2041-8213/aba2cf Bibcode: 2020ApJ...898L..29M

Tiengo, A.; Sunyaev, R.; Götz, D. +23 more

We report on International Gamma-Ray Astrophysics Laboratory (INTEGRAL) observations of the soft γ-ray repeater SGR 1935+2154 performed between 2020 April 28 and May 3. Several short bursts with fluence of $\sim {10}^{-7}\mbox{--}{10}^{-6}$ erg cm-2 were detected by the Imager on-board INTEGRAL (IBIS) instrument in the 20-200 keV range.…

2020 The Astrophysical Journal
INTEGRAL 320
Pan-STARRS Photometric and Astrometric Calibration
DOI: 10.3847/1538-4365/abb82a Bibcode: 2020ApJS..251....6M

Price, P. A.; Chambers, K. C.; Stubbs, C. W. +20 more

We present the details of the photometric and astrometric calibration of the Pan-STARRS1 3π Survey. The photometric goals were to reduce the systematic effects introduced by the camera and detectors, and to place all of the observations onto a photometric system with consistent zero-points over the entire area surveyed, the ≈30,000 deg2

2020 The Astrophysical Journal Supplement Series
Gaia 312
The third realization of the International Celestial Reference Frame by very long baseline interferometry
DOI: 10.1051/0004-6361/202038368 Bibcode: 2020A&A...644A.159C

Charlot, P.; Lambert, S.; Bourda, G. +17 more

A new realization of the International Celestial Reference Frame (ICRF) is presented based on the work achieved by a working group of the International Astronomical Union (IAU) mandated for this purpose. This new realization follows the initial realization of the ICRF completed in 1997 and its successor, ICRF2, adopted as a replacement in 2009. Th…

2020 Astronomy and Astrophysics
Gaia 307
Unresolved stellar companions with Gaia DR2 astrometry
DOI: 10.1093/mnras/staa1522 Bibcode: 2020MNRAS.496.1922B

Everall, Andrew; Brown, Anthony G. A.; Belokurov, Vasily +9 more

For stars with unresolved companions, motions of the centre of light and that of mass decouple, causing a single-source astrometric model to perform poorly. We show that such stars can be easily detected with the reduced χ2 statistic, or renormalized unit weight error (RUWE), provided as part of Gaia DR2. We convert RUWE into the amplit…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 306
The XMM-Newton serendipitous survey. IX. The fourth XMM-Newton serendipitous source catalogue
DOI: 10.1051/0004-6361/201937353 Bibcode: 2020A&A...641A.136W

Motch, C.; Page, M. J.; Ballet, J. +28 more

Context. Sky surveys produce enormous quantities of data on extensive regions of the sky. The easiest way to access this information is through catalogues of standardised data products. XMM-Newton has been surveying the sky in the X-ray, ultra-violet, and optical bands for 20 years.
Aims: The XMM-Newton Survey Science Centre has been producin…

2020 Astronomy and Astrophysics
AKARI Gaia XMM-Newton 297
The Solar Orbiter EUI instrument: The Extreme Ultraviolet Imager
DOI: 10.1051/0004-6361/201936663 Bibcode: 2020A&A...642A...8R

Vial, J. -C.; Zhang, X.; Peter, H. +146 more

Context. The Extreme Ultraviolet Imager (EUI) is part of the remote sensing instrument package of the ESA/NASA Solar Orbiter mission that will explore the inner heliosphere and observe the Sun from vantage points close to the Sun and out of the ecliptic. Solar Orbiter will advance the "connection science" between solar activity and the heliosphere…

2020 Astronomy and Astrophysics
SolarOrbiter 292
Rapid Reionization by the Oligarchs: The Case for Massive, UV-bright, Star-forming Galaxies with High Escape Fractions
DOI: 10.3847/1538-4357/ab7cc9 Bibcode: 2020ApJ...892..109N

Conroy, Charlie; Tacchella, Sandro; Naidu, Rohan P. +3 more

The protagonists of the last great phase transition of the universe - cosmic reionization - remain elusive. Faint star-forming galaxies are leading candidates because they are found to be numerous and may have significant ionizing photon escape fractions (fesc). Here we update this picture via an empirical model that successfully predic…

2020 The Astrophysical Journal
eHST 279
The milky way total mass profile as inferred from Gaia DR2
DOI: 10.1093/mnras/staa1017 Bibcode: 2020MNRAS.494.4291C

Grand, Robert J. J.; Gómez, Facundo A.; Fattahi, Azadeh +7 more

We determine the Milky Way (MW) mass profile inferred from fitting physically motivated models to the Gaia DR2 Galactic rotation curve and other data. Using various hydrodynamical simulations of MW-mass haloes, we show that the presence of baryons induces a contraction of the dark matter (DM) distribution in the inner regions, r ≲ 20 kpc. We provi…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 275