Search Publications

Lyα emission in galaxies at z ≃ 5-6: new insight from JWST into the statistical distributions of Lyα properties at the end of reionization
DOI: 10.1093/mnras/stae1338 Bibcode: 2024MNRAS.531.2701T

Charlot, Stéphane; Chevallard, Jacopo; Maseda, Michael V. +22 more

JWST has recently sparked a new era of Lyα spectroscopy, delivering the first measurements of the Lyα escape fraction and velocity profile in typical galaxies at z ≃ 6-10. These observations offer new prospects for insight into the earliest stages of reionization. But to realize this potential, we need robust models of Lyα properties in galaxies a…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 27
JWST Photometric Time-delay and Magnification Measurements for the Triply Imaged Type Ia "SN H0pe" at z = 1.78
DOI: 10.3847/1538-4357/ad3c43 Bibcode: 2024ApJ...967...50P

Pérez-Fournon, I.; Fox, O. D.; Ryan, R. E. +60 more

Supernova (SN) SN H0pe is a gravitationally lensed, triply imaged, Type Ia SN (SN Ia) discovered in James Webb Space Telescope imaging of the PLCK G165.7+67.0 cluster of galaxies. Well-observed multiply imaged SNe provide a rare opportunity to constrain the Hubble constant (H 0), by measuring the relative time delay between the images a…

2024 The Astrophysical Journal
JWST 27
JWST Transmission Spectroscopy of HD 209458b: A Supersolar Metallicity, a Very Low C/O, and No Evidence of CH4, HCN, or C2H2
DOI: 10.3847/2041-8213/ad2682 Bibcode: 2024ApJ...963L...5X

Bean, Jacob L.; Zhang, Michael; Welbanks, Luis +3 more

We present the transmission spectrum of the original transiting hot Jupiter HD 209458b from 2.3 to 5.1 µm as observed with the NIRCam instrument on the James Webb Space Telescope (JWST). Previous studies of HD 209458b's atmosphere have given conflicting results on the abundance of H2O and the presence of carbon- and nitrogen-beari…

2024 The Astrophysical Journal
JWST 27
A Combined Ground-based and JWST Atmospheric Retrieval Analysis: Both IGRINS and NIRSpec Agree that the Atmosphere of WASP-77A b Is Metal-poor
DOI: 10.3847/1538-3881/ad17bf Bibcode: 2024AJ....167..110S

Brogi, Matteo; Kempton, Eliza; Line, Michael R. +12 more

Ground-based high-resolution and space-based low-resolution spectroscopy are the two main avenues through which transiting exoplanet atmospheres are studied. Both methods provide unique strengths and shortcomings, and combining the two can be a powerful probe into an exoplanet's atmosphere. Within a joint atmospheric retrieval framework, we combin…

2024 The Astronomical Journal
JWST 27
Near-infrared transmission spectroscopy of HAT-P-18 b with NIRISS: Disentangling planetary and stellar features in the era of JWST
DOI: 10.1093/mnras/stad3813 Bibcode: 2024MNRAS.528.3354F

MacDonald, Ryan J.; Johnstone, Doug; Dang, Lisa +24 more

The JWST Early Release Observations (ERO) included a NIRISS/SOSS (0.6-2.8 µm) transit of the ~ 850 K Saturn-mass exoplanet HAT-P-18 b. Initial analysis of these data reported detections of water, escaping helium and haze. However, active K dwarfs like HAT-P-18 possess surface heterogeneities - star-spots and faculae - that can complicate the…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 26
Identification of High-redshift Galaxy Overdensities in GOODS-N and GOODS-S
DOI: 10.3847/1538-4357/ad6867 Bibcode: 2024ApJ...974...41H

Bunker, Andrew J.; Maiolino, Roberto; Willott, Chris +18 more

We conduct a systematic search for high-redshift galaxy overdensities at 4.9 < z spec < 8.9 in both the Great Observatories Origins Deep Survey (GOODS)-N and GOODS-S fields using James Webb Space Telescope/Near-Infrared Camera (JWST/NIRCam) imaging from the JWST Advanced Deep Extragalactic Survey and JWST Extragalactic Medium-band…

2024 The Astrophysical Journal
Gaia eHST JWST 26
Probing orbits of stellar mass objects deep in galactic nuclei with quasiperiodic eruptions
DOI: 10.1103/PhysRevD.109.103031 Bibcode: 2024PhRvD.109j3031Z

Pan, Zhen; Zhou, Cong; Huang, Lei +2 more

Quasiperiodic eruptions (QPEs) are intense, repeating, soft x-ray bursts with recurrence times of about a few to ten hours from nearby galactic nuclei. The origin of QPEs is still unclear. In this work, we investigate the extreme mass ratio inspiral (EMRI) + accretion disk model, where the disk is formed from a previous tidal disruption event (TDE…

2024 Physical Review D
XMM-Newton 26
Magnetic field properties inside the jet of Mrk 421. Multiwavelength polarimetry, including the Imaging X-ray Polarimetry Explorer
DOI: 10.1051/0004-6361/202347408 Bibcode: 2024A&A...681A..12K

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +133 more


Aims: We aim to probe the magnetic field geometry and particle acceleration mechanism in the relativistic jets of supermassive black holes.
Methods: We conducted a polarimetry campaign from radio to X-ray wavelengths of the high-synchrotron-peak (HSP) blazar Mrk 421, including Imaging X-ray Polarimetry Explorer (IXPE) measurements from 2…

2024 Astronomy and Astrophysics
XMM-Newton 26
Project Dinos I: A joint lensing-dynamics constraint on the deviation from the power law in the mass profile of massive ellipticals
DOI: 10.1093/mnras/stae884 Bibcode: 2024MNRAS.530.1474T

Treu, Tommaso; Sonnenfeld, Alessandro; Birrer, Simon +7 more

The mass distribution in massive elliptical galaxies encodes their evolutionary history, thus providing an avenue to constrain the baryonic astrophysics in their evolution. The power-law assumption for the radial mass profile in ellipticals has been sufficient to describe several observables to the noise level, including strong lensing and stellar…

2024 Monthly Notices of the Royal Astronomical Society
eHST 26
A magnetar giant flare in the nearby starburst galaxy M82
DOI: 10.1038/s41586-024-07285-4 Bibcode: 2024Natur.629...58M

Thuillot, William; Mereghetti, Sandro; Esposito, Paolo +32 more

Magnetar giant flares are rare explosive events releasing up to 1047 erg in gamma rays in less than 1 second from young neutron stars with magnetic fields up to 1015−16 G (refs. 1,2). Only three such flares have been seen from magnetars in our Galaxy3,4 and in the Large Magellanic Cloud5 in ro…

2024 Nature
INTEGRAL XMM-Newton 26