Search Publications
CLASSY. VI. The Density, Structure, and Size of Absorption-line Outflows in Starburst Galaxies
Martin, Crystal L.; Scarlata, Claudia; Henry, Alaina +12 more
Galaxy formation and evolution are regulated by the feedback from galactic winds. Absorption lines provide the most widely available probe of winds. However, since most data only provide information integrated along the line of sight, they do not directly constrain the radial structure of the outflows. In this paper, we present a method to directl…
Carbon-enhanced metal-poor star candidates from BP/RP spectra in Gaia DR3
Ting, Yuan-Sen; Yoon, Jinmi; Beers, Timothy C. +6 more
Carbon-enhanced metal-poor (CEMP) stars comprise almost a third of stars with [Fe/H] < -2, although their origins are still poorly understood. It is highly likely that one sub-class (CEMP-s stars) is tied to mass-transfer events in binary stars, while another sub-class (CEMP-no stars) are enriched by the nucleosynthetic yields of the first gene…
Detection of the Low-stellar-mass Host Galaxy of a z 6.25 Quasar with JWST
Lyu, Jianwei; Rieke, George H.; Alberts, Stacey +1 more
We characterize the stellar mass of J2239+0207, a z ~ 6.25 sub-Eddington quasar (M 1450 = -24.6), using dedicated JWST/NIRCam medium-band observations of a nearby point-spread function star to remove the central point source and reveal the underlying galaxy emission. We detect the host galaxy in two bands longward of the Balmer break, o…
High-redshift metallicity calibrations for JWST spectra: insights from line emission in cosmological simulations
Somerville, Rachel S.; Charlot, Stephane; Hirschmann, Michaela
Optical emission-line ratios are traditionally used to estimate gas metallicities from observed galaxy spectra. While such estimators have been calibrated primarily at low redshift, they are commonly used to interpret observations of high-redshift galaxies, where their applicability may be questioned. We use comprehensive emission-line catalogues …
JWST NIRSpec Observations of Supernova 1987A-From the Inner Ejecta to the Reverse Shock
Fox, O. D.; Blommaert, J. A. D. L.; Larsson, J. +23 more
We present initial results from JWST NIRSpec integral field unit observations of the nearby supernova SN 1987A. The observations provide the first spatially resolved spectroscopy of the ejecta and equatorial ring (ER) over the 1-5 µm range. We construct 3D emissivity maps of the [Fe I] 1.443 µm line from the inner ejecta and the He I 1…
Another shipment of six short-period giant planets from TESS
Henning, Thomas; Vanderburg, Andrew; Hellier, Coel +130 more
We present the discovery and characterization of six short-period, transiting giant planets from NASA's Transiting Exoplanet Survey Satellite (TESS) -- TOI-1811 (TIC 376524552), TOI-2025 (TIC 394050135), TOI-2145 (TIC 88992642), TOI-2152 (TIC 395393265), TOI-2154 (TIC 428787891), and TOI-2497 (TIC 97568467). All six planets orbit bright host stars…
Deep low-frequency radio observations of Abell 2256. II. The ultra-steep spectrum radio halo
Brunetti, G.; Rossetti, M.; Dallacasa, D. +17 more
We present the first detailed analysis of the radio halo in the merging galaxy cluster Abell 2256 using the LOw Frequency ARray, the upgraded Giant Metrewave Radio Telescope, and the Karl G. Jansky Very Large Array. Radio observations (120 MHz-2 GHz) combined with archival Chandra and XMM-Newton X-ray data allowed us to study the central radio hal…
A sensitive APEX and ALMA CO(1-0), CO(2-1), CO(3-2), and [CI](1-0) spectral survey of 40 local (ultra-)luminous infrared galaxies
Weiss, A.; Aravena, M.; Severgnini, P. +8 more
We present a high sensitivity, ground-based spectral line survey of low-J carbon monoxide (CO(Jup → Jup − 1) with Jup = 1, 2, 3) and neutral carbon [CI] 3P1−3P0 ([CI](1-0)) in 36 local ultra-luminous infrared galaxies (ULIRGs) and 4 additional LIRGs, all of which have pre…
The Next Generation Virgo Cluster Survey (NGVS). XXXV. First Kinematical Clues of Overly Massive Dark Matter Halos in Several Ultradiffuse Galaxies in the Virgo Cluster
Côté, Patrick; Peng, Eric W.; Ferrarese, Laura +8 more
We present Keck/DEIMOS spectroscopy of the first complete sample of ultradiffuse galaxies (UDGs) in the Virgo cluster. We select all UDGs in Virgo that contain at least 10 globular cluster (GC) candidates and are more than 2.5σ outliers in scaling relations of size, surface brightness, and luminosity (a total of 10 UDGs). We use the radial velocit…
Detection of extended γ-ray emission around the Geminga pulsar with H.E.S.S.
Santangelo, A.; Quirrenbach, A.; Funk, S. +164 more
Geminga is an enigmatic radio-quiet γ-ray pulsar located at a mere 250 pc distance from Earth. Extended very-high-energy γ-ray emission around the pulsar was discovered by Milagro and later confirmed by HAWC, which are both water Cherenkov detector-based experiments. However, evidence for the Geminga pulsar wind nebula in gamma rays has long evade…