Search Publications

Formation of Post-CME Blobs Observed by LASCO-C2 and K-Cor on 2017 September 10
DOI: 10.3847/1538-4357/ab799a Bibcode: 2020ApJ...892..129L

Lee, Kyoung-Sun; Jang, Soojeong; Cho, Kyung-Suk +6 more

Understanding the formation of post-CME blobs, we investigate 2 blobs in the outer corona observed by LASCO-C2 and 34 blobs in the inner corona by K-Cor on 2017 September 10 from 17:11 to 18:58 UT. By visual inspection of the structure of a post-CME current sheet (CS) and its associated blobs, we find that the CS is well identified in the K-Cor an…

2020 The Astrophysical Journal
SOHO 20
Measurement of the B-band galaxy Luminosity Function with Approximate Bayesian Computation
DOI: 10.1088/1475-7516/2020/09/048 Bibcode: 2020JCAP...09..048T

Tortorelli, Luca; Herbel, Jörg; Amara, Adam +3 more

The galaxy Luminosity Function (LF) is a key observable for galaxy formation, evolution studies and for cosmology. In this work, we propose a novel technique to forward model wide-field broad-band galaxy surveys using the fast image simulator UFig and measure the LF of galaxies in the B-band. We use Approximate Bayesian Computation (ABC) to constr…

2020 Journal of Cosmology and Astroparticle Physics
Gaia 20
An ALMA/NOEMA study of gas dissipation and dust evolution in the 5 Myr-old HD 141569A hybrid disc
DOI: 10.1051/0004-6361/201732243 Bibcode: 2020A&A...635A..94D

Augereau, J. -C.; Boccaletti, A.; Chapillon, E. +5 more

Context. The study of gas-rich debris discs is fundamental to characterising the transition between protoplanetary discs and debris discs.
Aims: We determine the physical parameters of the brightest gas-rich debris disc orbiting HD 141569A.
Methods: We analyse images from the NOrthern Extended Millimeter Array (NOEMA)1 and the…

2020 Astronomy and Astrophysics
Gaia eHST 20
A charging model for the Rosetta spacecraft
DOI: 10.1051/0004-6361/202038592 Bibcode: 2020A&A...642A..43J

Henri, P.; Eriksson, A. I.; Johansson, F. L. +5 more

Context. The electrostatic potential of a spacecraft, VS, is important for the capabilities of in situ plasma measurements. Rosetta has been found to be negatively charged during most of the comet mission and even more so in denser plasmas.
Aims: Our goal is to investigate how the negative VS correlates with electron den…

2020 Astronomy and Astrophysics
Rosetta 20
Optical polarization properties of AGNs with significant VLBI-Gaia offsets
DOI: 10.1093/mnrasl/slaa008 Bibcode: 2020MNRAS.493L..54K

Blinov, D.; Kovalev, Y. Y.; Zobnina, D. I. +1 more

Significant positional offsets of the value from 1 mas to more than 10 mas were found previously between radio (VLBI) and optical (Gaia) positions of active galactic nuclei (AGNs). They happen preferentially parallel to the parsec-scale jet direction. AGNs with VLBI-to-Gaia offsets pointed downstream the jet are found to have favourably higher opt…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20
The MASSIVE Survey XIV—Stellar Velocity Profiles and Kinematic Misalignments from 200 pc to 20 kpc in Massive Early-type Galaxies
DOI: 10.3847/1538-4357/ab7016 Bibcode: 2020ApJ...891...65E

Ma, Chung-Pei; Greene, Jenny E.; Blakeslee, John P. +3 more

We use high spatial resolution stellar velocity maps from the Gemini integral-field spectrograph (IFS) and wide-field velocity maps from the McDonald Mitchell IFS to study the stellar velocity profiles and kinematic misalignments from ∼200 pc to ∼20 kpc in 20 early-type galaxies (ETGs) with stellar mass M* > 1011.7M⊙<…

2020 The Astrophysical Journal
eHST 20
Truth or Delusion? A Possible Gravitational Lensing Interpretation of the Ultraluminous Quasar SDSS J010013.02+280225.8 at z = 6.30
DOI: 10.3847/1538-4357/ab718c Bibcode: 2020ApJ...891...64F

Ouchi, Masami; Fujimoto, Seiji; Oguri, Masamune +2 more

Gravitational lensing sometimes dominates the observed properties of apparently very bright objects. We present morphological properties in the high-resolution (FWHM ∼ 0"15) Atacama Large Millimeter/submillimeter Array (ALMA) 1 mm map for an ultraluminous quasar at z = 6.30, SDSS J010013.02+280225.8 (hereafter J0100+2802), whose black hole (BH) ma…

2020 The Astrophysical Journal
Gaia eHST 20
Longitudinal filament oscillations enhanced by two C-class flares
DOI: 10.1051/0004-6361/201937291 Bibcode: 2020A&A...635A.132Z

Guo, J. H.; Zhang, Q. M.; Xu, A. A. +1 more

Context. Large-amplitude, longitudinal filament oscillations triggered by solar flares have been well established in the literature. However, filament oscillations enhanced by flares have never been reported.
Aims: In this paper we report the multiwavelength observations of a very long filament in active region (AR) 11112 on 2010 October 18. …

2020 Astronomy and Astrophysics
SOHO 20
FOXSI-2 Solar Microflares. I. Multi-instrument Differential Emission Measure Analysis and Thermal Energies
DOI: 10.3847/1538-4357/ab7200 Bibcode: 2020ApJ...891...78A

Krucker, Säm; Narukage, Noriyuki; Musset, Sophie +8 more

In this paper we present the differential emission measures (DEMs) of two sub-A class microflares observed in hard X-rays (HXRs) by the FOXSI-2 sounding rocket experiment, on 2014 December 11. The second Focusing Optics X-ray Solar Imager (FOXSI) flight was coordinated with instruments X-ray Telescope (Hinode/XRT) and Solar Dynamics Observatory/At…

2020 The Astrophysical Journal
Hinode 20
Ultra-luminous quasars at redshift z > 4.5 from SkyMapper
DOI: 10.1093/mnras/stz2955 Bibcode: 2020MNRAS.491.1970W

Wolf, Christian; Schmidt, Brian P.; Bian, Fuyan +6 more

The most luminous quasars at high-redshift harbour the fastest growing and most massive black holes in the early Universe. They are exceedingly rare and hard to find. Here, we present our search for the most luminous quasars in the redshift range from z = 4.5 to 5 using data from SkyMapper, Gaia, and WISE. We use colours to select likely high-reds…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20