Search Publications

Improvement of Pan-STARRS Photometric Calibration with LAMOST and Gaia
DOI: 10.3847/1538-4365/acee73 Bibcode: 2023ApJS..268...53X

Huang, Bowen; Yuan, Haibo; Xiao, Kai +3 more

In this work, we perform the recalibration of Pan-STARRS1 (PS1) photometry by correcting for position-dependent systematic errors using the spectroscopy-based stellar color regression (SCR) method, the photometry-based SCR method, and the Gaia BP/RP synthetic photometry method. We confirm the significant large-scale and small-scale spatial variati…

2023 The Astrophysical Journal Supplement Series
Gaia 13
Linear Mode Decomposition in Magnetohydrodynamics Revisited
DOI: 10.3847/1538-4365/acdf5d Bibcode: 2023ApJS..268...18Z

Zank, G. P.; Zhao, L. -L.; Telloni, D. +4 more

Small-amplitude fluctuations in the magnetized solar wind are measured typically by a single spacecraft. In the magnetohydrodynamics (MHD) description, fluctuations are typically expressed in terms of the fundamental modes admitted by the system. An important question is how to resolve an observed set of fluctuations, typically plasma moments such…

2023 The Astrophysical Journal Supplement Series
SolarOrbiter 13
A Single Ejection Model of the DART/Dimorphos Debris Trail
DOI: 10.3847/2041-8213/acfd1d Bibcode: 2023ApJ...956L..26K

Jewitt, David; Kim, Yoonyoung

The collision of the NASA DART spacecraft with asteroid Dimorphos resulted in the formation of a distinctive and long-lived debris trail, formed by the action of solar radiation pressure on ejected particles. This trail briefly displayed a double appearance, which has been interpreted as the result of a double ejection. We present a model that can…

2023 The Astrophysical Journal
eHST 13
Volatile exposures on the 67P/Churyumov-Gerasimenko nucleus
DOI: 10.1051/0004-6361/202245614 Bibcode: 2023A&A...672A.136F

Fulle, M.; Fornasier, S.; Ciarniello, M. +2 more


Aims: We present the most extensive catalog of exposures of volatiles on the 67P/Churyumov-Gerasimenko nucleus generated from observations acquired with the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) on board the Rosetta mission. We investigate the volatile exposure distribution across the nucleus, their size distribu…

2023 Astronomy and Astrophysics
Rosetta 13
The MUSCLES Extension for Atmospheric Transmission Spectroscopy: UV and X-Ray Host-star Observations for JWST ERS & GTO Targets
DOI: 10.3847/1538-3881/acdb70 Bibcode: 2023AJ....166...35B

Brown, Alexander; France, Kevin; Youngblood, Allison +8 more

X-ray through infrared spectral energy distributions (SEDs) are essential for understanding a star's effect on exoplanet atmospheric composition and evolution. We present a catalog of panchromatic SEDs, hosted on the Barbara A. Mikulski Archive for Space Telescopes, for 11 exoplanet-hosting stars that have guaranteed JWST observation time as part …

2023 The Astronomical Journal
Gaia XMM-Newton eHST 13
The edge-on protoplanetary disk HH 48 NE. I. Modeling the geometry and stellar parameters
DOI: 10.1051/0004-6361/202346052 Bibcode: 2023A&A...677A..17S

Rocha, W. R. M.; Dartois, E.; McClure, M. K. +11 more

Context. Observations of edge-on disks are an important tool for constraining general protoplanetary disk properties that cannot be determined in any other way. However, most radiative transfer models cannot simultaneously reproduce the spectral energy distributions (SEDs) and resolved scattered light and submillimeter observations of these system…

2023 Astronomy and Astrophysics
eHST JWST 13
The Eclipsing Binaries from the LAMOST Medium-resolution Survey. III. A High-precision Empirical Stellar Mass Library
DOI: 10.3847/1538-3881/aca288 Bibcode: 2023AJ....165...30X

Li, Jiadong; Xiong, Jianping; Liu, Chao +6 more

High-precision stellar masses and radii measured directly from binaries can effectively calibrate stellar models. However, such a database containing full spectral types and a large range of metallicity is still not fully established. A continuous effort of data collection and analysis is requested to complete the database. In this work, we provid…

2023 The Astronomical Journal
Gaia 13
Late-time HST UV and optical observations of AT 2018cow: extracting a cow from its background
DOI: 10.1093/mnras/stad2531 Bibcode: 2023MNRAS.525.4042I

Jonker, Peter G.; Perley, Daniel A.; Mummery, Andrew +4 more

The bright, blue, rapidly evolving AT 2018cow is a well-studied peculiar extragalactic transient. Despite an abundance of multiwavelength data, there still is no consensus on the nature of the event. We present our analysis of three epochs of Hubble Space Telescope (HST) observations spanning the period from 713 to 1474 d post-burst, paying partic…

2023 Monthly Notices of the Royal Astronomical Society
eHST 13
IXPE and XMM-Newton Observations of the Soft Gamma Repeater SGR 1806-20
DOI: 10.3847/1538-4357/aced05 Bibcode: 2023ApJ...954...88T

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +96 more

Recent observations with the Imaging X-ray Polarimetry Explorer (IXPE) of two anomalous X-ray pulsars provided evidence that X-ray emission from magnetar sources is strongly polarized. Here we report on the joint IXPE and XMM-Newton observations of the soft γ-repeater SGR 1806-20. The spectral and timing properties of SGR 1806-20 derived from XMM-…

2023 The Astrophysical Journal
XMM-Newton 13
Absence of nuclear polycyclic aromatic hydrocarbon emission from a compact starburst: The case of the type-2 quasar Mrk 477
DOI: 10.1051/0004-6361/202245409 Bibcode: 2023A&A...669L...5R

Rigopoulou, D.; Tadhunter, C. N.; Acosta-Pulido, J. A. +11 more

Mrk 477 is the closest type-2 quasar, at a distance of 163 Mpc. This makes it an ideal laboratory for studying the interplay between nuclear activity and star formation with a great level of detail and signal-to-noise. In this Letter we present new mid-infrared (mid-IR) imaging and spectroscopic data with an angular resolution of 0.4″ (∼300 pc) ob…

2023 Astronomy and Astrophysics
eHST 13