Search Publications

Ejecta from the DART-produced active asteroid Dimorphos
DOI: 10.1038/s41586-023-05811-4 Bibcode: 2023Natur.616..452L

Granvik, Mikael; Kolokolova, Ludmilla; Weaver, Harold A. +61 more

Some active asteroids have been proposed to be formed as a result of impact events1. Because active asteroids are generally discovered by chance only after their tails have fully formed, the process of how impact ejecta evolve into a tail has, to our knowledge, not been directly observed. The Double Asteroid Redirection Test (DART) miss…

2023 Nature
eHST 76
A structured jet explains the extreme GRB 221009A
DOI: 10.1126/sciadv.adi1405 Bibcode: 2023SciA....9I1405O

Kouveliotou, Chryssa; Buckley, David A. H.; Hammerstein, Erica +29 more

Long-duration gamma-ray bursts (GRBs) are powerful cosmic explosions, signaling the death of massive stars. Among them, GRB 221009A is by far the brightest burst ever observed. Because of its enormous energy ( E iso ≈ 10 55 erg) and proximity ( z ≈ 0.15), GRB 221009A is an exceptionally rare event that pushes the limits of our theories. We present…

2023 Science Advances
XMM-Newton 76
Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems
DOI: 10.1051/0004-6361/202346211 Bibcode: 2023A&A...677A..33B

Vanderburg, A.; Poretti, E.; Sozzetti, A. +31 more

The exoplanet population characterized by relatively short orbital periods (P < 100 d) around solar-type stars is dominated by super-Earths and sub-Neptunes. However, these planets are missing in our Solar System and the reason behind this absence is still unknown. Two theoretical scenarios invoke the role of Jupiter as the possible culprit: Ju…

2023 Astronomy and Astrophysics
Gaia 75
Finding Peas in the Early Universe with JWST
DOI: 10.3847/2041-8213/acaaaf Bibcode: 2023ApJ...942L..14R

Kim, Keunho J.; Malhotra, Sangeeta; Pharo, John +6 more

The Early Release Observations (EROs) of JWST beautifully demonstrate the promise of JWST in characterizing the universe at Cosmic Dawn. We analyze the Near Infrared Spectrograph ERO spectra of three z ~ 8 galaxies to determine their metallicities, gas temperatures, and ionization. These galaxies offer the first opportunity to understand the physi…

2023 The Astrophysical Journal
JWST 75
JADES: Discovery of extremely high equivalent width Lyman-α emission from a faint galaxy within an ionized bubble at z = 7.3
DOI: 10.1051/0004-6361/202346245 Bibcode: 2023A&A...678A..68S

Chevallard, Jacopo; Maseda, Michael V.; Carniani, Stefano +44 more

We report the discovery of a remarkable Lyα emitting galaxy at z = 7.2782, JADES-GS+53.16746−27.7720 (shortened to JADES-GS-z7-LA), with rest-frame equivalent width, EW0(Lyα) = 388.0 ± 88.8 Å and UV magnitude −17.0. The spectroscopic redshift is confirmed via rest-frame optical lines [O II], Hβ and [O III] in its JWST/NIRSpec Micro-Shut…

2023 Astronomy and Astrophysics
JWST 75
Constraints on the Hubble constant from supernova Refsdal's reappearance
DOI: 10.1126/science.abh1322 Bibcode: 2023Sci...380.1322K

Treu, Tommaso; Broadhurst, Tom; Filippenko, Alexei V. +27 more

The gravitationally lensed supernova Refsdal appeared in multiple images produced through gravitational lensing by a massive foreground galaxy cluster. After the supernova appeared in 2014, lens models of the galaxy cluster predicted that an additional image of the supernova would appear in 2015, which was subsequently observed. We use the time de…

2023 Science
eHST 75
The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High-contrast Imaging of the Exoplanet HIP 65426 b from 2 to 16 µm
DOI: 10.3847/2041-8213/acd93e Bibcode: 2023ApJ...951L..20C

Henning, Thomas; Fortney, Jonathan J.; Carter, Aarynn L. +108 more

We present JWST Early Release Science coronagraphic observations of the super-Jupiter exoplanet, HIP 65426b, with the Near-Infrared Camera (NIRCam) from 2 to 5 µm, and with the Mid-Infrared Instrument (MIRI) from 11 to 16 µm. At a separation of ~0.″82 (87 ${}_{-31}^{+108}$ au), HIP 65426b is clearly detected in all seven of our observa…

2023 The Astrophysical Journal
AKARI Gaia JWST 75
A 3D Drizzle Algorithm for JWST and Practical Application to the MIRI Medium Resolution Spectrometer
DOI: 10.3847/1538-3881/acdddc Bibcode: 2023AJ....166...45L

Law, David R.; Vandenbussche, Bart; Patapis, Polychronis +4 more

We describe an algorithm for application of the classic "drizzle" technique to produce 3D spectral cubes using data obtained from the slicer-type integral field unit (IFU) spectrometers on board the James Webb Space Telescope. This algorithm relies upon the computation of overlapping volume elements (composed of two spatial dimensions and one spec…

2023 The Astronomical Journal
JWST 74
Gaia Data Release 3. Specific processing and validation of all sky RR Lyrae and Cepheid stars: The Cepheid sample
DOI: 10.1051/0004-6361/202243990 Bibcode: 2023A&A...674A..17R

Szabados, L.; Audard, M.; Plachy, E. +19 more

Context. Cepheids are pulsating stars that play a crucial role in several astrophysical contexts. Among the different types, the Classical Cepheids are fundamental tools for the calibration of the extragalactic distance ladder. They are also powerful stellar population tracers in the context of Galactic studies. The Gaia Third Data Release (DR3) p…

2023 Astronomy and Astrophysics
Gaia 74
On the ages of bright galaxies 500 Myr after the big bang: insights into star formation activity at z ≳ 15 with JWST
DOI: 10.1093/mnras/stac3535 Bibcode: 2023MNRAS.519..157W

Charlot, Stéphane; Chen, Zuyi; Stark, Daniel P. +3 more

With JWST, new opportunities to study the evolution of galaxies in the early Universe are emerging. Spitzer constraints on rest-optical properties of z ≳ 7 galaxies demonstrated the power of using galaxy stellar masses and star formation histories (SFHs) to indirectly infer the cosmic star formation history. However, only the brightest individual …

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 74