Results 1 to 10 of about 1,014 (183)

JWST Photometry of Globular Cluster Populations in MACS0417.5−1154

open access: yesThe Astrophysical Journal
Deep JWST imaging of the massive galaxy cluster MACS0417.5−1154, at redshift z = 0.443, reveals a huge population of globular clusters (GCs) and ultracompact dwarfs (UCDs) primarily distributed around its single central giant brightest cluster galaxy ...
William E. Harris   +10 more
doaj   +1 more source

Deep photometry of the Draco dwarf spheroidal galaxy [PDF]

open access: yesThe Astronomical Journal, 1986
We report the results of deep CCD photometry of two overlapping fields in the Draco dwarf spheroidal galaxy. We find (B-V)o,g = m0.69, indicating a mean [Fe/H] = −2.0. The width of the giant branch below the horizontal branch is somewhat wider than our observational errors permit, from which we infer there is a spread in metallicities amongst the Draco
Bruce W. Carney, P. Seitzer
openaire   +1 more source

Photo-z Estimation with Normalizing Flow

open access: yesThe Astrophysical Journal
Accurate photometric redshift (photo- z ) estimation is a key challenge in cosmology, as uncertainties in photo- z directly limit the scientific return of large-scale structure and weak lensing studies, especially in upcoming Stage IV surveys.
Yiming Ren   +8 more
doaj   +1 more source

PEARLS: Near-infrared Photometry in the JWST North Ecliptic Pole Time Domain Field

open access: yesThe Astrophysical Journal Supplement Series, 2023
We present near-infrared (NIR) ground-based Y , J , H , and K imaging obtained in the James Webb Space Telescope (JWST) North Ecliptic Pole Time Domain Field (NEP TDF) using the MMT-Magellan Infrared Imager and Spectrometer on the MMT.
Christopher N. A. Willmer   +25 more
doaj   +1 more source

The Structure of Galaxies I: Surface Photometry Techniques [PDF]

open access: yesPublications of the Astronomical Society of Australia, 2012
AbstractThis project uses the 2MASS all-sky image database to study the structure of galaxies over a range of luminosities, sizes and morphological types. This first paper in this series will outline the techniques, reliability and data products to our surface photometry program.
Schombert, James, Smith, Anna K.
openaire   +2 more sources

pop-cosmos: A Comprehensive Picture of the Galaxy Population from COSMOS Data

open access: yesThe Astrophysical Journal Supplement Series
We present pop-cosmos : a comprehensive model characterizing the galaxy population, calibrated to 140,938 ( r < 25 selected) galaxies from the Cosmic Evolution Survey (COSMOS) with photometry in 26 bands from the ultraviolet to the infrared. We construct
Justin Alsing   +6 more
doaj   +1 more source

Surface Photometry of Spiral Galaxy NGC 5005 and Elliptical Galaxy NGC 4278

open access: yesمجلة بغداد للعلوم, 2018
Two galaxies have been chosen, spiral galaxy NGC 5005 and elliptical galaxy NGC 4278 to study their photometric properties by using surface photometric techniques with griz-Filters. Observations are obtained from the Sloan Digital Sky Survey (SDSS).
Baghdad Science Journal
doaj   +1 more source

The JWST Resolved Stellar Populations Early Release Science Program. V. DOLPHOT Stellar Photometry for NIRCam and NIRISS

open access: yesThe Astrophysical Journal Supplement Series
We present NIRCam and NIRISS modules for DOLPHOT, a widely used crowded-field stellar photometry package. We describe details of the modules including pixel masking, astrometric alignment, star finding, photometry, catalog creation, and artificial star ...
Daniel R. Weisz   +40 more
doaj   +1 more source

Machine Learning versus Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation

open access: yesThe Astrophysical Journal
Traditional spectral energy distribution (SED)–fitting methods for stellar mass estimation face persistent challenges including systematic biases and computational constraints.
Vahid Asadi   +2 more
doaj   +1 more source

3D-Herschel: Constraining Dust Emission with Panchromatic Modeling of 3D-HST Galaxies

open access: yesThe Astrophysical Journal
We present 3D-Herschel, a new publicly released 0.3–350 μ m photometric catalog that combines deblended Herschel far-infrared (FIR) imaging with the CANDELS/3D-HST legacy fields to probe the dust-obscured Universe. Using the 17-parameter Bayesian fitting
Seamus McNulty   +11 more
doaj   +1 more source

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