Search Publications

A close quasar pair in a disk-disk galaxy merger at z = 2.17
DOI: 10.1038/s41586-023-05766-6 Bibcode: 2023Natur.616...45C

Shen, Yue; Oguri, Masamune; Chen, Yu-Ching +7 more

Galaxy mergers produce pairs of supermassive black holes (SMBHs), which may be witnessed as dual quasars if both SMBHs are rapidly accreting. The kiloparsec (kpc)-scale separation represents a physical regime sufficiently close for merger-induced effects to be important1 yet wide enough to be directly resolvable with the facilities curr…

2023 Nature
eHST 28
Awesome SOSS: atmospheric characterization of WASP-96 b using the JWST early release observations
DOI: 10.1093/mnras/stad1547 Bibcode: 2023MNRAS.524..817T

MacDonald, Ryan J.; Espinoza, Néstor; Parmentier, Vivien +13 more

The newly operational JWST offers the potential to study the atmospheres of distant worlds with precision that has not been achieved before. One of the first exoplanets observed by JWST in the summer of 2022 was WASP-96 b, a hot Saturn orbiting a G8 star. As a part of the Early Release Observations programme, one transit of WASP-96 b was observed …

2023 Monthly Notices of the Royal Astronomical Society
JWST 28
The Star Formation History of the Milky Way's Nuclear Star Cluster
DOI: 10.3847/1538-4357/aca8ad Bibcode: 2023ApJ...944...79C

Lu, Jessica R.; Morris, Mark R.; Ghez, Andrea M. +6 more

We report the first star formation history study of the Milky Ways nuclear star cluster (NSC), which includes observational constraints from a large sample of stellar metallicity measurements. These metallicity measurements were obtained from recent surveys from Gemini and the Very Large Telescope of 770 late-type stars within the central 1.5 pc. …

2023 The Astrophysical Journal
eHST 28
Binarity and beyond in A stars - I. Survey description and first results of VLTI/GRAVITY observations of VAST targets with high Gaia-Hipparcos accelerations
DOI: 10.1093/mnras/stad872 Bibcode: 2023MNRAS.521.5232W

Katz, Boaz; Waisberg, Idel; Klein, Ygal

The connection between the multiplicity of A stars and that of their white dwarf (WD) descendants is not known and the observational mappings of both multiplicities are far from complete. We are conducting an interferometric survey with VLTI/GRAVITY of 20 out of 108 southern A stars within the VAST sample which show large Gaia-Hipparcos proper mot…

2023 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 28
A Statistical Study of Short-period Decayless Oscillations of Coronal Loops in an Active Region
DOI: 10.3847/1538-4357/acacf4 Bibcode: 2023ApJ...944....8L

Long, David M.; Li, Dong

Coronal loop oscillations are common phenomena in the solar corona, which are often classified as decaying and decayless oscillations. Using the high-resolution observation measured by the Extreme Ultraviolet Imager (EUI) on board the Solar Orbiter, we statistically investigate small-scale transverse oscillations with short periods (<200 s) of …

2023 The Astrophysical Journal
SolarOrbiter 28
Estimating the selection function of Gaia DR3 subsamples
DOI: 10.1051/0004-6361/202346547 Bibcode: 2023A&A...677A..37C

Casey, Andrew R.; Rix, Hans-Walter; Brown, Anthony G. A. +9 more

Context. Understanding the intricacies behind the presence and absence of sources in an astronomical catalogue is crucial for the accurate interpretation of astronomical data. In particular, for the multi-dimensional Gaia data, filters and cuts on different parameters or measurements introduce a selection function that may unintentionally alter sc…

2023 Astronomy and Astrophysics
Gaia 27
Limit on Supernova Emission in the Brightest Gamma-Ray Burst, GRB 221009A
DOI: 10.3847/2041-8213/acbd50 Bibcode: 2023ApJ...946L..25S

Carballo-Bello, Julio A.; Smith, Nathan; Wheeler, J. Craig +30 more

We present photometric and spectroscopic observations of the extraordinary gamma-ray burst (GRB) 221009A in search of an associated supernova. Some past GRBs have shown bumps in the optical light curve that coincide with the emergence of supernova spectral features, but we do not detect any significant light-curve features in GRB 221009A, nor do w…

2023 The Astrophysical Journal
eHST 27
Spatially resolved imaging of the inner Fomalhaut disk using JWST/MIRI
DOI: 10.1038/s41550-023-01962-6 Bibcode: 2023NatAs...7..790G

Rieke, George H.; Gáspár, András; Beichman, Charles +9 more

Planetary debris disks around other stars are analogous to the asteroid and Kuiper belts in the Solar System. Their structure reveals the configuration of small bodies and provides hints for the presence of planets. The nearby star Fomalhaut hosts one of the most prominent debris disks, resolved by the Hubble Space Telescope, Spitzer, Herschel and…

2023 Nature Astronomy
Herschel eHST JWST 27
X-Ray Polarization of BL Lacertae in Outburst
DOI: 10.3847/2041-8213/acd242 Bibcode: 2023ApJ...948L..25P

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +128 more

We report the first >99% confidence detection of X-ray polarization in BL Lacertae. During a recent X-ray/γ-ray outburst, a 287 ks observation (2022 November 27-30) was taken using the Imaging X-ray Polarimetry Explorer (IXPE), together with contemporaneous multiwavelength observations from the Neil Gehrels Swift observatory and XMM-Newton in s…

2023 The Astrophysical Journal
XMM-Newton 27
The Gaia-ESO Survey: Homogenisation of stellar parameters and elemental abundances
DOI: 10.1051/0004-6361/202345910 Bibcode: 2023A&A...676A.129H

Prusti, T.; Gilmore, G.; Montes, D. +59 more

The Gaia-ESO Survey is a public spectroscopic survey that targeted ≳105 stars covering all major components of the Milky Way from the end of 2011 to 2018, delivering its final public release in May 2022. Unlike other spectroscopic surveys, Gaia-ESO is the only survey that observed stars across all spectral types with dedicated, speciali…

2023 Astronomy and Astrophysics
Gaia 27