Search Publications

Identifying Missing Quasars from the DESI Bright Galaxy Survey
DOI: 10.3847/1538-3881/adabc9 Bibcode: 2025AJ....169..157J

Alexander, D. M.; Juneau, S.; Moustakas, J. +59 more

The Dark Energy Spectroscopic Instrument (DESI) cosmology survey includes a Bright Galaxy Survey (BGS), which will yield spectra for over 10 million bright galaxies (r < 20.2 AB mag). The resulting sample will be valuable for both cosmological and astrophysical studies. However, the star/galaxy separation criterion implemented in the nominal BG…

2025 The Astronomical Journal
Gaia 11
VLTI/GRAVITY Observations of AF Lep b: Preference for Circular Orbits, Cloudy Atmospheres, and a Moderately Enhanced Metallicity
DOI: 10.3847/1538-3881/ad9265 Bibcode: 2025AJ....169...30B

Pueyo, Laurent; Henning, Th.; Mollière, Paul +26 more

Direct imaging observations are biased toward wide-separation, massive companions that have degenerate formation histories. Although the majority of exoplanets are expected to form via core accretion, most directly imaged exoplanets have not been convincingly demonstrated to follow this formation pathway. We obtained new interferometric observatio…

2025 The Astronomical Journal
Gaia Hipparcos 7
Predicting Interstellar Object Chemodynamics with Gaia
DOI: 10.3847/1538-3881/ad9eb3 Bibcode: 2025AJ....169...78H

Bannister, Michele T.; Lintott, Chris; Hopkins, Matthew J.

The interstellar object (ISO) population of the Milky Way is a product of its stars. However, what is in fact a complex structure in the solar neighborhood has traditionally in ISO studies been described as smoothly distributed. Using a debiased stellar population derived from the Gaia Data Release 3 stellar sample, we predict that the velocity di…

2025 The Astronomical Journal
Gaia 5
Significant Mutual Inclinations Between the Stellar Spin and the Orbits of Both Planets in the HAT-P-11 System
DOI: 10.3847/1538-3881/ad90b4 Bibcode: 2025AJ....169...22A

Brandt, Timothy D.; Brandt, G. Mirek; Li, Gongjie +2 more

Planet–star obliquity and planet–planet mutual inclination encode a planetary system's dynamical history, but both of their values are hard to measure for misaligned systems with close-in companions. HAT-P-11 is a K4 star with two known planets: a close-in, misaligned super-Neptune with a ≈5 day orbit, and an outer super-Jupiter with a ≈10 yr orbi…

2025 The Astronomical Journal
Gaia 4
Constraining Atmospheric Composition from the Outflow: Helium Observations Reveal the Fundamental Properties of Two Planets Straddling the Radius Gap
DOI: 10.3847/1538-3881/adb490 Bibcode: 2025AJ....169..204Z

Knutson, Heather A.; Horne, Keith; Collins, Karen A. +13 more

TOI-836 is a ∼2–3 Gyr K dwarf with an inner super Earth (R = 1.7 R, P = 3.8 days) and an outer mini-Neptune (R = 2.6 R, P = 8.6 days). JWST/NIRSpec 2.8–5.2 µm transmission spectra are flat for both planets. We present Keck/NIRSPEC observations of escaping helium for super-Earth b, which shows no excess absorption in t…

2025 The Astronomical Journal
XMM-Newton 4
Searching for GEMS: TOI-5688 A b, a Low-density Giant Orbiting a High-metallicity Early M-dwarf
DOI: 10.3847/1538-3881/ada7ea Bibcode: 2025AJ....169..187R

Kobulnicky, Henry A.; Cochran, William D.; Mahadevan, Suvrath +31 more

We present the discovery of a low-density planet orbiting the high-metallicity early M-dwarf TOI-5688 A b. This planet was characterized as part of the search for transiting giant planets (R ≳ 8 R) through the Searching for Giant Exoplanets around M-dwarf Stars (GEMS) survey. The planet was discovered with the Transiting Exoplanet Surv…

2025 The Astronomical Journal
Gaia 3
Gaia-4b and 5b: Radial Velocity Confirmation of Gaia Astrometric Orbital Solutions Reveal a Massive Planet and a Brown Dwarf Orbiting Low-mass Stars
DOI: 10.3847/1538-3881/ada9e1 Bibcode: 2025AJ....169..107S

Callingham, J. R.; Cochran, William D.; Mahadevan, Suvrath +31 more

Gaia astrometry of nearby stars is precise enough to detect the tiny displacements induced by substellar companions, but radial velocity (RV) data are needed for definitive confirmation. Here we present RV follow-up observations of 28 M and K stars with candidate astrometric substellar companions, which led to the confirmation of two systems, Gaia…

2025 The Astronomical Journal
Gaia 3
Sites of Planet Formation in Binary Systems. II. Double the Disks in DF Tau
DOI: 10.3847/1538-3881/ad900a Bibcode: 2025AJ....169...20K

Tang, Shih-Yun; Johns-Krull, Christopher M.; Jensen, Eric L. N. +8 more

This article presents the latest results of our Atacama Large Millimeter/submillimeter Array (ALMA) program to study circumstellar disk characteristics as a function of orbital and stellar properties in a sample of young binary star systems known to host at least one disk. Optical and infrared observations of the eccentric, ∼48 yr period binary DF…

2025 The Astronomical Journal
Gaia 3
The PHANGS-HST-Hα Survey: Warm Ionized Gas Physics at High Angular Resolution in Nearby Galaxies with the Hubble Space Telescope
DOI: 10.3847/1538-3881/adaa80 Bibcode: 2025AJ....169..150C

Leroy, Adam K.; Rosolowsky, Erik; Chevance, Mélanie +38 more

The PHANGS project is assembling a comprehensive, multiwavelength data set of nearby (∼5–20 Mpc), massive star-forming galaxies to enable multiphase, multiscale investigations into the processes that drive star formation and galaxy evolution. To date, large survey programs have provided molecular gas (CO) cubes with the Atacama Large Millimeter/su…

2025 The Astronomical Journal
Gaia 3
Evidence of Truly Young High-α Dwarf Stars
DOI: 10.3847/1538-3881/ada9e0 Bibcode: 2025AJ....169..168L

Angus, Ruth; Bedell, Megan; Claytor, Zachary R. +14 more

The existence of high-α stars with inferred ages <6 Gyr has been confirmed recently with large spectroscopic and photometric surveys. However, stellar mergers or binary interactions can induce properties associated with young ages, such as high mass, rapid rotation, or high activity, even in old populations. Literature studies have confirmed th…

2025 The Astronomical Journal
Gaia 3