Search Publications

High-redshift metallicity calibrations for JWST spectra: insights from line emission in cosmological simulations
DOI: 10.1093/mnras/stad2745 Bibcode: 2023MNRAS.526.3504H

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 …

2023 Monthly Notices of the Royal Astronomical Society
JWST 22
JWST NIRSpec Observations of Supernova 1987A-From the Inner Ejecta to the Reverse Shock
DOI: 10.3847/2041-8213/acd555 Bibcode: 2023ApJ...949L..27L

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…

2023 The Astrophysical Journal
JWST 22
Another shipment of six short-period giant planets from TESS
DOI: 10.1093/mnras/stad595 Bibcode: 2023MNRAS.521.2765R

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…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 22
Deep low-frequency radio observations of Abell 2256. II. The ultra-steep spectrum radio halo
DOI: 10.1051/0004-6361/202244925 Bibcode: 2023A&A...669A...1R

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…

2023 Astronomy and Astrophysics
XMM-Newton 22
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
DOI: 10.1051/0004-6361/202245046 Bibcode: 2023A&A...673A..13M

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] 3P13P0 ([CI](1-0)) in 36 local ultra-luminous infrared galaxies (ULIRGs) and 4 additional LIRGs, all of which have pre…

2023 Astronomy and Astrophysics
Herschel 22
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
DOI: 10.3847/1538-4357/acd336 Bibcode: 2023ApJ...951...77T

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…

2023 The Astrophysical Journal
eHST 22
Detection of extended γ-ray emission around the Geminga pulsar with H.E.S.S.
DOI: 10.1051/0004-6361/202245776 Bibcode: 2023A&A...673A.148H

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…

2023 Astronomy and Astrophysics
XMM-Newton 22
The Cool Circumgalactic Medium of Low-redshift Star-forming Galaxies. I. Empirical Model and Mean Properties
DOI: 10.3847/1538-4357/acf217 Bibcode: 2023ApJ...956...92F

Werk, Jessica K.; Faerman, Yakov

We present an analytic model for the cool, T ~ 104 K, circumgalactic medium (CGM), describing the gas distribution, and thermal and ionization states. Our model assumes (total) pressure equilibrium with the ambient warm/hot CGM, photoionization by the metagalactic radiation, and allows for nonthermal pressure support, parameterized by t…

2023 The Astrophysical Journal
eHST 22
Ultracool Dwarfs Observed with the Spitzer Infrared Spectrograph: Equatorial Latitudes in L Dwarf Atmospheres Are Cloudier
DOI: 10.3847/2041-8213/acec4b Bibcode: 2023ApJ...954L...6S

Metchev, Stanimir; Faherty, Jacqueline K.; Vos, Johanna M. +2 more

We report direct observational evidence for a latitudinal dependence of dust cloud opacity in ultracool dwarfs, indicating that equatorial latitudes are cloudier than polar latitudes. These results are based on a strong positive correlation between the viewing geometry and the mid-infrared silicate absorption strength in mid-L dwarfs using mid-inf…

2023 The Astrophysical Journal
JWST 22
JWST Low-resolution MIRI Spectral Observations of SN 2021aefx: High-density Burning in a Type Ia Supernova
DOI: 10.3847/2041-8213/acb8a8 Bibcode: 2023ApJ...945L...2D

Suntzeff, N. B.; Wang, L.; Galbany, L. +38 more

We present a JWST/MIRI low-resolution mid-infrared (MIR) spectroscopic observation of the normal Type Ia supernova (SN Ia) SN 2021aefx at +323 days past rest-frame B-band maximum light. The spectrum ranges from 4 to 14 µm and shows many unique qualities, including a flat-topped [Ar III] 8.991 µm profile, a strongly tilted [Co III] 11.8…

2023 The Astrophysical Journal
JWST 22