Search Publications

The Star Formation Efficiency during Reionization as Inferred from the Hubble Frontier Fields
DOI: 10.3847/1538-4357/ad06a7 Bibcode: 2024ApJ...961...50S

Lidz, Adam; Sipple, Jackson

A recent ultraviolet luminosity function (UVLF) analysis in the Hubble Frontier Fields, behind foreground lensing clusters, has helped solidify estimates of the faint-end of the z ~ 5-9 UVLF at up to 5 mag fainter than in the field. These measurements provide valuable information regarding the role of low-luminosity galaxies in reionizing the univ…

2024 The Astrophysical Journal
JWST 12
Self-interacting Dark Matter Interpretation of Crater II
DOI: 10.3847/2041-8213/ad50cd Bibcode: 2024ApJ...968L..13Z

Yang, Daneng; Yu, Hai-Bo; Zhang, Xingyu +1 more

The satellite galaxy Crater II of the Milky Way is extremely cold and exceptionally diffuse. These unusual properties are challenging to understand in the standard model of cold dark matter. We use controlled N-body simulations to investigate the formation of Crater II in self-interacting dark matter (SIDM), where dark matter particles can scatter…

2024 The Astrophysical Journal
Gaia 12
The metal-poor atmosphere of a potential sub-Neptune progenitor
DOI: 10.1038/s41550-024-02257-0 Bibcode: 2024NatAs...8..899B

Fortney, Jonathan J.; Désert, Jean-Michel; Petigura, Erik A. +12 more

Young transiting exoplanets offer a unique opportunity to characterize the atmospheres of freshly formed and evolving planets. We present the transmission spectrum of V1298 Tau b, a 23-Myr-old warm Jupiter-sized (0.91 ± 0.05 RJ, where RJ is the radius of Jupiter) planet orbiting a pre-main-sequence star. We detect a mostly cl…

2024 Nature Astronomy
eHST 12
The rate and contribution of mergers to mass assembly from NIRCam observations of galaxy candidates up to 13.3 billion years ago
DOI: 10.1093/mnras/stae2064 Bibcode: 2024MNRAS.533.4472D

Santini, Paola; Calabrò, Antonello; Castellano, Marco +8 more

We present an analysis of the galaxy merger rate in the redshift range $4.0\lt z\lt 9.0$ (i.e. about 1.5 to 0.5 Gyr after the big bang) based on visually identified galaxy mergers from morphological parameter analysis. Our data set is based on high-resolution NIRCam…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 12
A biconical ionised gas outflow and evidence of positive feedback in NGC 7172 uncovered by MIRI/JWST
DOI: 10.1051/0004-6361/202450262 Bibcode: 2024A&A...690A.350H

Rouan, D.; Rigopoulou, D.; Gandhi, P. +35 more

We present observations of the type-2 Seyfert NGC 7172 obtained with the medium-resolution spectrometer (MRS) of the Mid-Infrared Instrument (MIRI) on board the James Webb Space Telescope (JWST). This galaxy hosts one of the lowest ionised gas mass outflow rates (Ṁout ∼ 0.005 M yr‑1) in a sample of six active gala…

2024 Astronomy and Astrophysics
JWST 12
J-PLUS: Toward a homogeneous photometric calibration using Gaia BP/RP low-resolution spectra
DOI: 10.1051/0004-6361/202346012 Bibcode: 2024A&A...683A..29L

Hernández-Monteagudo, C.; Hernán-Caballero, A.; Carrasco, J. M. +21 more


Aims: We present the photometric calibration of the 12 optical passbands for the Javalambre Photometric Local Universe Survey (J-PLUS) third data release (DR3) comprising 1642 pointings of two square degrees each.
Methods: We selected nearly 1.5 million main sequence stars with a signal-to-noise ratio larger than ten in the 12 J-PLUS pas…

2024 Astronomy and Astrophysics
Gaia 12
High Hard X-Ray Polarization in Cygnus X-1 Confined to the Intermediate Hard State: Evidence for a Variable Jet Component
DOI: 10.3847/2041-8213/ad118d Bibcode: 2024ApJ...960L...2C

Rao, A. R.; Bhalerao, Varun; Mithun, N. P. S. +7 more

Cygnus X-1, the well-known accreting black hole system, exhibits several observational features hinting at an intricate interplay between the accretion disk, its atmosphere known as the corona, and the putative relativistic jet. It has been extensively studied using all available observational methods, including using the newly available technique…

2024 The Astrophysical Journal
INTEGRAL 12
The Dynamic, Chimeric Inner Disk of PDS 70
DOI: 10.3847/1538-4357/ad3447 Bibcode: 2024ApJ...966..167G

Banzatti, Andrea; Gaidos, Eric; Shappee, Benjamin J. +4 more

Transition disks, with inner regions depleted in dust and gas, could represent later stages of protoplanetary disk evolution when newly formed planets are emerging. The PDS 70 system has attracted particular interest because of the presence of two giant planets in orbits at tens of astronomical units within the inner disk cavity, at least one of w…

2024 The Astrophysical Journal
AKARI 12
The host dark matter haloes of the first quasars
DOI: 10.1093/mnras/stae1157 Bibcode: 2024MNRAS.531..930C

Costa, Tiago

If z > 6 quasars reside in rare, massive haloes, ΛCDM cosmology predicts they should be surrounded by an anomalously high number of bright companion galaxies. Here, I show that these companion galaxies should also move unusually fast. Using a new suite of cosmological, 'zoom-in' hydrodynamic simulations, I present predictions for the velocity d…

2024 Monthly Notices of the Royal Astronomical Society
JWST 12
DEIMOS spectroscopy of z = 6 protocluster candidate in COSMOS - a massive protocluster embedded in a large-scale structure?
DOI: 10.1093/mnras/stad3409 Bibcode: 2024MNRAS.527.6591B

Casey, Caitlin M.; Zavala, Jorge A.; Brammer, Gabriel +14 more

We present the results of our Keck/DEep Imaging Multi-Object Spectrograph spectroscopic follow-up of candidate galaxies of I-band-dropout protocluster candidate galaxies at z ~ 6 in the COSMOS field. We securely detect Lyman α emission lines in 14 of the 30 objects targeted, 10 of them being at z = 6 with a signal-to-noise ratio of 5-20; the remai…

2024 Monthly Notices of the Royal Astronomical Society
eHST 12