Katarzyna Ewa Małek

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professor

National Centre for Nuclear Research

Poland

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About

Dr. Katarzyna Ewa Małek is a professor at the National Centre for Nuclear Research in Poland. Her research focuses on the astrophysical properties of galaxies, including the structural characterization of extended-UV galaxies, quasar continuum estimation using neural networks, and the effects of galaxy environments on merger fractions. She has contributed to the understanding of low-surface-brightness galaxies and their spectral energy distributions through advanced modeling techniques.

Recent Grants

Grant: Close

ASTROdust: wyczerpujący opis atenuacji pyłu w galaktykach na podstawie miliona galaktyk obserwowanych przez satelitę Herschel

Open Date: 2019-04-25

Close Date: 2023-04-24

Grant: Close

Klasyfikacja galaktyk o przesunięciu ku czerwieni ~ 1

Open Date: 2014-05-05

Close Date: 2017-05-04

Grant: Close

大光度赤外銀河のダスト放射の起源の研究

Open Date: 2011-01-01

Close Date: 2013-12-31

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2021

Collaborators (9)

Agnieszka Pollo

National Centre for Nuclear Research

POLAND

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Reinout van Weeren

Assistant Professor

Leiden University

NETHERLANDS

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Fangyou Gao

University of Groningen

NETHERLANDS

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Matthew Smith

Lecturer

Cardiff University

UNITED KINGDOM

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Masafumi Yagi

助教/Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

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Miguel Figueira

National Centre for Nuclear Research

POLAND

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Nicholas Seymour

Curtin University

AUSTRALIA

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Hyunjin Shim

Kyungpook National University

SOUTH KOREA

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Raphael Shirley

Max Planck Institute for Extraterrestrial Physics

GERMANY

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Katarzyna Ewa Małek

Research Interests

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About

Recent Grants

Articles (19)

DES to HSC: Detecting low-surface-brightness galaxies in the Abell 194 cluster using transfer learning

Characterizing the outer disk of extended-UV galaxies in the optical domain with deep surveys

Spatially resolved spectrophotometric SED modeling of NGC 253’s central molecular zone

Automated quasar continuum estimation using neural networks

The host galaxies of radio AGN: New views from combining LoTSS and MaNGA observations

Effects of galaxy environment on merger fraction

Radio-only and Radio-to-far-ultraviolet Spectral Energy Distribution Modeling of 14 ULIRGs: Insights into the Global Properties of Infrared Bright Galaxies

Attenuation proxy hidden in surface brightness – colour diagrams

Shedding light on low-surface-brightness galaxies in dark energy surveys with transformer models

Variation in optical and infrared properties of galaxies in relation to their surface brightness

Piercing the dusty veil of hyper-luminous infrared galaxies: Sub-arcsecond 144 MHz ILT observations of HLIRGs in the Lockman Hole

The fundamental metallicity relation from SDSS (z ∼ 0) to VIPERS (z ∼ 0.7)

Low-frequency Radio Continuum Imaging and SED Modeling of 11 LIRGs: Radio-only and FUV to Radio Bands

Fitting AGN/Galaxy X-Ray-to-radio SEDs with CIGALE and Improvement of the Code

Environmental effects on AGN activity via extinction-free mid-infrared census

Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS

A hyperluminous obscured quasar at a redshift of z ≈ 4.3

HELP: The Herschel Extragalactic Legacy Project

Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z∼2

Collaborators (9)

Agnieszka Pollo

Reinout van Weeren

Fangyou Gao

Matthew Smith

Masafumi Yagi

Miguel Figueira

Nicholas Seymour

Hyunjin Shim

Raphael Shirley

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