Results 151 to 160 of about 2,843 (308)
What Is the Nature of Little Red Dots and what Is Not, MIRI SMILES Edition
We study 31 little red dots (LRD) detected by JADES/NIRCam and covered by the SMILES/MIRI survey, of which ∼70% are detected in the two bluest MIRI bands and 40% in redder MIRI filters.
Pablo G. Pérez-González +22 more
doaj +1 more source
PanGraphRNA is an easy‐to‐use platform that improves RNA‐seq analysis by using graph pangenomes instead of a single reference genome. It increases read alignment accuracy, detects important genes missed by traditional methods, and works across major crops, helping researchers obtain more reliable transcriptome results for diverse plant research and ...
Yifan Bu +10 more
wiley +1 more source
The ASTRID Simulation at z = 0: From Massive Black Holes to Large-scale Structure
We present the z = 0 results for the cosmological simulation ASTRID . Hosting 2 × 5500 ^3 ≈ 0.33 trillion particles in a box of 370 Mpc per side, ASTRID is one of the largest cosmological hydrodynamic simulations evolved to z = 0. ASTRID features a large
Yihao Zhou +9 more
doaj +1 more source
The stellar content and distance to the nearby blue compact dwarf galaxy NGC 6789
In this paper we present the results of a detailed B, V, R, I, and Hα study of the isolated nearby blue compact dwarf (BCD) galaxy NGC 6789. The observed galaxy has not yet been resolved into stars up to now.
I. Drozdovsky, N. Tikhonov
core +1 more source
Modular training resources for bioimage analysis
Abstract Modern microscopy enables us to measure structural and dynamical properties of many biological processes and is therefore an indispensable research tool. However, the amount and complexity of the produced imaging data is steadily increasing.
Christian Tischer +17 more
wiley +1 more source
We present new JWST/NIRCam observations of the interacting dwarf galaxy system NGC 4485–NGC 4490 (aka Arp 269), obtained as part of the Cycle 1 Feedback in Emerging Extragalactic Star Clusters (FEAST) program. NGC 4485 and NGC 4490 form the closest known
Giacomo Bortolini +25 more
doaj +1 more source
Systematic uncertainties in stellar mass estimation for distinct galaxy populations
We show that different stellar mass estimation methods yield overall mass scales that disagree by factors up to ∼2 for the z = 0 galaxy population and, more importantly, relative mass scales that sometimes disagree by factors ≳3 between distinct classes ...
Kannappan, S.J., Gawiser, E.
core +1 more source
ABSTRACT Aim To summarize the current evidence on reducing loneliness among informal caregivers of people with dementia, such as family members or friends. Design A systematic review. Methods The methodological quality was evaluated using the revised Cochrane risk‐of‐bias tool for randomized controlled trials and the revised JBI critical appraisal ...
Tianxue Hou +5 more
wiley +1 more source
The spectrum of a galaxy is a complicated convolution of many properties of the galaxy, such as the star formation history (SFH), initial mass function, and metallicity.
Yanzhe Zhang +3 more
doaj +1 more source
Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
Aims. We present an investigation of the evolutionary pathways of green valley (GV) galaxies, defined as galaxies with a distance to the star-forming main sequence in the range −1.3
Zhou S. +4 more
doaj +1 more source

