This solution is preferred over $\Lambda$CDM at $3. 1\sigma$ for the combination of DESI BAO and CMB data.
Cosmology and Nongalactic Astrophysics
We have built a reliable and robust system that takes as input an astronomical image, and returns as output the pointing, scale, and orientation of that image (the astrometric calibration or WCS information).
Instrumentation and Methods for Astrophysics
Before entering the current long-lasting high state, this object showed three short-lived high states, which might have been precursors to the current state.
Solar and Stellar Astrophysics
We then demonstrate using hydrodynamic simulations that, compared to cold dark matter, these high-$z$ massive FDM solitons with mass $M_s$ can provide additional gravitational potential to accrete gas and boost the Bondi accretion rate of a growing black hole seed with mass $M_{\rm BH}$ by up to two to four orders of magnitude, in the regime of efficient cooling and negligible radiation pressure.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
In this paper, We present the Atmospheric Big Challenge Database (ABC Database), a carefully designed, organised and publicly available database dedicated to the study of the inverse problem in the context of exoplanetary studies.
Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics Data Analysis, Statistics and Probability
In this paper we discuss and implement a wide-band wide-field spectral deconvolution framework (DDFacet) based on image plane faceting, that takes into account generic direction-dependent effects.
Instrumentation and Methods for Astrophysics
We have optimized TLS for both signal detection efficiency (SDE) of small planets and computational speed.
Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics
We release the AllWISE counterparts and Gaia matches to 106, 573 and 17, 665 X-ray sources detected in the ROSAT 2RXS and XMMSL2 surveys with |b|>15.
Astrophysics of Galaxies High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
I describe a method for decorrelating fast and slow parameters so that parameter sampling in the full space becomes almost as efficient as sampling in the slow subspace when the covariance is well known and the distributions are simple.
Cosmology and Nongalactic Astrophysics
We use X-ray observations of quasar microlensing (sensitive to smaller compact objects than in the optical) to study the possible presence of a population of low mass black holes (from $\sim$ $10^{-3}M_{\odot}$ to $10^{-1}M_{\odot}$) in lens galaxies.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
