Search Publications

Observations of Titan's Stratosphere during Northern Summer: Temperatures, CH3CN and CH3D Abundances
DOI: 10.3847/PSJ/ad47bd Bibcode: 2024PSJ.....5..125T

Butler, Bryan; Vinatier, Sandrine; Lellouch, Emmanuel +11 more

Titan's atmospheric composition and dynamical state have previously been studied over numerous epochs by both ground- and space-based facilities. However, stratospheric measurements remain sparse during Titan's northern summer and fall. The lack of seasonal symmetry in observations of Titan's temperature field and chemical abundances raises questi…

2024 The Planetary Science Journal
ISO 1
Scientific Highlights of the AGILE Gamma-ray Mission
DOI: 10.3390/universe10040153 Bibcode: 2024Univ...10..153V

Tavani, Marco; Pittori, Carlotta; Vercellone, Stefano

The γ-ray sky above a few tens of megaelectronvolts (MeV) reveals some of the most powerful and energetic phenomena of our Universe. The Astrorivelatore Gamma ad Immagini LEggero (AGILE) Gamma-ray Mission was launched in 2007 with the aim…

2024 Universe
XMM-Newton 1
Updated absolute parameters and kinematics of IS CMa
DOI: 10.1002/asna.20240038 Bibcode: 2024AN....34540038E

Alan, Neslihan; Canbay, Remziye; Evcil, Serkan +2 more

Eclipsing binary systems are significant objects for astrophysics in that direct observations can determine the fundamental parameters of stars. In this study, we precisely determined the fundamental parameters of the binary component stars obtained by simultaneous analysis of radial velocities and the TESS light curve using the Wilson and Devinne…

2024 Astronomische Nachrichten
Gaia 1
Sp1149. II. Spectroscopy of H II Regions near the Critical Curve of MACS J1149 and Cluster Lens Models
DOI: 10.3847/1538-4357/ad4354 Bibcode: 2024ApJ...967...92W

Filippenko, Alexei V.; Oguri, Masamune; Diego, Jose M. +3 more

Galaxy-cluster gravitational lenses enable the study of faint galaxies even at large lookback times, and, recently, time-delay constraints on the Hubble constant. There have been few tests, however, of lens model predictions adjacent to the critical curve (≲8″) where the magnification is greatest. In a companion paper, we use the GLAFIC lens model…

2024 The Astrophysical Journal
eHST 1
Chandra/HETG Doppler velocity measurements in stellar coronal sources
DOI: 10.1093/mnras/stae275 Bibcode: 2024MNRAS.528.4591B

de Plaa, J.; Costantini, E.; Paltani, S. +4 more

Stellar coronal sources have been observed in the past not only for their astrophysical interest in the field of binary system evolution and interaction but also for their invaluable roles as benchmarks for plasma spectral models and as calibration sources for high resolution spectroscopic X-ray instruments. These include the gratings on-board Cha…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
Rotation in stellar evolution: Probing the influence on population synthesis in high-redshift galaxies
DOI: 10.1051/0004-6361/202348693 Bibcode: 2024A&A...685A..40S

Sun, Weijia

Stellar population synthesis (SPS) is essential for understanding galaxy formation and evolution. However, the recent discovery of rotation-driven phenomena in star clusters warrants a review of uncertainties in SPS models caused by overlooked factors, including stellar rotation. In this study, we investigated the impact of rotation on SPS specifi…

2024 Astronomy and Astrophysics
JWST 1
Recurrently Propagating Intensity Disturbances along Polar Plumes Observed in White Light and Extreme Ultraviolet
DOI: 10.3847/1538-4357/ad11d2 Bibcode: 2024ApJ...961..128C

Moon, Yong-Jae; Lee, Harim; Cho, Kyung-Suk +5 more

We study properties of intensity disturbances along polar coronal rays that are associated with plumes below. For this, we draw azimuth–time images of extreme ultraviolet (EUV) emission of 171 Å band observed by the SDO/AIA and white light (WL) observed by the SOHO/LASCO C2 in 2020 July. From the azimuth–time image, we define two tracks in which t…

2024 The Astrophysical Journal
SOHO 1
New Yarkovsky drift detections using astrometric observations of NEAs
DOI: 10.1007/s10686-024-09925-z Bibcode: 2024ExA....57....4L

Lisa, Bedini; Giacomo, Tommei

The Yarkovsky drift represents the semi-major axis variation of a celestial body due to the Yarkovsky effect. This thermodynamic effect acts more significantly on bodies with a diameter between ≈10 m and ≈30 km . Therefore, the orbits of many minor bodies of the solar system are affected: knowing the value of the Yarkovsky drift can be crucial to …

2024 Experimental Astronomy
Gaia 1
Searching for Neutral Hydrogen Escape from the 120 Myr Old Sub-Neptune HIP94235b using HST
DOI: 10.3847/1538-3881/ad6a53 Bibcode: 2024AJ....168..141M

Mayorga, L. C.; Zhou, George; Wittenmyer, Robert A. +9 more

HIP94235 b, a 120 Myr old sub-Neptune, provides us the unique opportunity to study mass loss at a pivotal stage of the system's evolution: the end of a 100 Myr old phase of intense XUV irradiation. We present two observations of HIP94235 b using the Hubble Space Telescope's Space Telescope Imaging Spectrograph in the Lyα wavelength region. We do n…

2024 The Astronomical Journal
eHST 1
Optimal Fitting and Debiasing for Detectors Read Out Up-the-Ramp
DOI: 10.1088/1538-3873/ad38d9 Bibcode: 2024PASP..136d5004B

Brandt, Timothy D.

This paper derives the optimal fit to a pixel's count rate in the case of an ideal detector read out nondestructively in the presence of both read and photon noise. The approach is general for any readout scheme, provides closed-form expressions for all quantities, and has a computational cost that is linear in the number of resultants (groups of …

2024 Publications of the Astronomical Society of the Pacific
JWST 1