Trending Research
YOLO-CIANNA: Galaxy detection with deep learning in radio data. I. A new YOLO-inspired source detection method applied to the SKAO SDC1
deyht/cianna
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YOLO-CIANNA achieves state-of-the-art detection and characterization results on the simulated SDC1 dataset.
Instrumentation and Methods for Astrophysics Astrophysics of Galaxies
Did the Universe Reheat After Recombination?
Here, we consider cosmological models with post-recombination reheating (PRR), in which the CMB monopole temperature abruptly increases due to energy injection after last scattering.
Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology
The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
Disc instabilities and their associated starbursts dominate for intermediate-mass spheroids ($10^{8. 5}<M_\mathrm{*, sph}<10^{11}$ M$_\odot$) at $z=0$.
Astrophysics of Galaxies
Caustic and hydrostatic mass bias: Implications for modified gravity
We propose and perform a joint analysis of the two different mass estimates of galaxy clusters, namely the hydrostatic and caustic techniques.
Cosmology and Nongalactic Astrophysics
PeTar: a high-performance N-body code for modeling massive collisional stellar systems
Until now, only a few realistic million-body simulations of GCs with a small fraction of binaries (5%) have been performed by using the NBODY6++GPU code.
Instrumentation and Methods for Astrophysics Astrophysics of Galaxies
NLTE Spectra of Kilonovae
We suggest the Rb I $\rm{5p^{1}}$- $\rm{5s^{1}}$ 7900 angstrom transition as a candidate for the $\lambda_0 \sim$ 7500--7900 angstrom P-Cygni feature in AT2017gfo.
High Energy Astrophysical Phenomena
Temperature inhomogeneities in Mrk71 can not be discarded
In a very recent work, [1] claim that the scenario of temperature inhomogeneities proposed by [2] ($t2$ > 0) is not able to explain the O$^{2+}$/H$^{+}$ abundance discrepancy observed between the calculations based on the optical [OIII] collisional excited lines (CELs) and the OII recombination lines (RLs) in the star forming galaxy Mrk71.
Astrophysics of Galaxies
Rainbow: a colorful approach on multi-passband light curve estimation
We evaluate the quality of the estimated light curves according to three different tests: goodness of fit, time of peak prediction and ability to transfer information to machine learning (ML) based classifiers.
Instrumentation and Methods for Astrophysics Data Analysis, Statistics and Probability
The cosmological simulation code $\scriptstyle{\rm CO}N{\rm CEPT}\, 1.0$
We present version 1. 0 of the cosmological simulation code $\scriptstyle{\rm CO}N{\rm CEPT}$, designed for simulations of large-scale structure formation.
Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics
AutoProf -- I. An automated non-parametric light profile pipeline for modern galaxy surveys
It is established that elliptical isophote fitting, and in particular AutoProf, is ideally suited for a broad range of automated isophotal analysis tasks.
Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
