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The paper introduces a hypernetwork‑conditioned surrogate model that predicts the mechanical behavior of mycelium‑woodchip composites across varying microstructures, enabling effic…

#multiscale modeling#surrogate modeling#microstructure optimization#mycelium composites

astro-ph.SR2022

Surface brightness-colour relations of dwarf stars from detached eclipsing binaries -- I. Calibrating sample

D. Graczyk, G. PietrzyÅski, C. Galan +19

astro-ph.GA2019

A distance to the Large Magellanic Cloud that is precise to one per cent

G. Pietrzynski, D. Graczyk, A. Gallenne +19

astro-ph.GA2019

4MOST Consortium Survey 3: Milky Way Disc and Bulge Low-Resolution Survey (4MIDABLE-LR)

C. Chiappini, I. Minchev, E. Starkenburg +35

astro-ph2000

Cepheid variables in the LMC cluster NGC 1866. I. New BVRI CCD photometry

W. P. Gieren, M. Gomez, J. Storm +5

Publications (89)

An optimised tiling pattern for multi-object spectroscopic surveys: application to the 4MOST survey

4MOST Scientific Operations

An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent

A pulsational distance to Omega Centauri based on Near-Infrared Period-Luminosity relations of RR Lyrae stars

Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk

The Araucaria Project. The Distance to the Local Group Galaxy WLM from Near-Infrared Photometry of Cepheid Variables

High resolution spectroscopy for Cepheids distance determination. V. Impact of the cross-correlation method on the p-factor and the gamma-velocities

Extremely faint high proper motion objects from SDSS stripe 82 - Optical classification spectroscopy of about 40 new objects

The Araucaria Project. OGLE-LMC-CEP-1718: An exotic eclipsing binary system composed of two classical overtone Cepheids in a 413-day orbit

Reddenings and metallicities in the LMC and SMC from Stroemgren CCD photometry

The Araucaria Project. Near-Infrared Photometry of Cepheid Variables in the Sculptor Galaxy NGC 55

First spectroscopic investigation of Anomalous Cepheid variables

Atmospheric parameters of Cepheids from flux ratios with ATHOS: I. The temperature scale

The distance to the LMC cluster Reticulum from the K-band Period-Luminosity-Metallicity relation of RR Lyrae stars

Direct Distances to Cepheids in the Large Magellanic Cloud: Evidence for a Universal Slope of the Period-Luminosity Relation up to Solar Abundance

On a new Near-Infrared method to estimate the absolute ages of star clusters: NGC3201 as a first test case

Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: VIII: Spectroscopic detection of rare earth dysprosium, erbium, lutetium and thorium in Classical Cepheids

4MOST Consortium Survey 9: One Thousand and One Magellanic Fields (1001MC)

Relative distances of Omega Centauri and 47 Tucanae

New Near-Infrared JHKs​ light-curve templates for RR Lyrae variables

VEGA/CHARA interferometric observations of Cepheids. I. A resolved structure around the prototype classical Cepheid delta Cep in the visible spectral range

The Araucaria Project. Accurate determination of the dynamical mass of the classical Cepheid in the eclipsing system OGLE-LMC-CEP-1812

Cepheid Metallicity in the Leavitt Law (C-MetaLL) Survey. V. New multiband (grizJHKs) Cepheid light curves and period-luminosity relations

Distances to six Cepheids in the LMC cluster NGC1866 from the near-IR surface-brightness method

Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: IX. Metallicity dependence of Period-Wesenheit relations based on a homogeneous spectroscopic sample

Eclipsing binaries in the Magellanic Clouds. uvby CCD light curves and photometric analyses for HV982 (LMC), HV12578 (LMC), HV1433 (SMC), and HV11284 (SMC)

The orbital parameters of the del Cep inner binary system determined using 2019 HARPS-N spectroscopic data

The Araucaria Project: Improving the cosmic distance scale

CORS Baade-Wesselink distance to the LMC NGC 1866 blue populous cluster

On the pulsation parallax of the variable star RR Lyr

A Direct Distance to the LMC Cepheid HV 12198 from the Infrared Surface Brightness Technique

A new calibration of Galactic Cepheid Period-Luminosity relations from B to K bands, and a comparison to LMC PL relations

Distance to Galactic globulars using the near-infrared magnitudes of RR Lyrae stars: IV. The case of M5 (NGC5904)

A new and homogeneous metallicity scale for Galactic classical Cepheids II. The abundance of iron and alpha elements

The Araucaria Project. The Distance to the Sculptor Galaxy NGC 247 from Near-Infrared Photometry of Cepheid Variables

Mixing Data-Driven and Physics-Based Constitutive Models using Uncertainty-Driven Phase Fields

Stromgren photometry of Galactic Globular Clusters. II Metallicity distribution of red giants in Omega Centauri

Physical parameters and the projection factor of the classical Cepheid in the binary system OGLE-LMC-CEP-0227

The effect of metallicity on Cepheid Period-Luminosity relations from a Baade-Wesselink analysis of Cepheids in the Milky Way and Magellanic Clouds

On the Use of Field RR Lyrae as Galactic Probes. V. Optical and radial velocity curve templates

Two very nearby (d ~ 5 pc) ultracool brown dwarfs detected by their large proper motions from WISE, 2MASS, and SDSS data

The Spectral Energy Distribution of the Seyfert galaxy Ton S180

PEPSI: The high-resolution echelle spectrograph and polarimeter for the Large Binocular Telescope

Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: II.High-resolution spectroscopy of the most metal poor Galactic Cepheids

CRIRES high-resolution infrared spectroscopy of the long-period Cepheid l Car

On the anomalous red giant branch of the globular cluster Omega Cen

Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: VI: Radial abundance gradients of 29 chemical species in the Milky Way Disk

ARGOS at the LBT. Binocular laser guided ground layer adaptive optics

Near-Infrared photometry of LMC cluster Reticulum

Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: I. HARPS-N@TNG spectroscopy of 47 Classical Cepheid and 1 BL Her variables

Multiwavelength Time Series Data of the LMC Cluster Reticulum

The Araucaria Project. The Distance to the Sculptor dwarf spheroidal galaxy from infrared photometry of RR Lyrae stars

HARPS-N high spectral resolution observations of Cepheids II. The impact of the surface-brightness color relation on the Baade-Wesselink projection factor of eta Aql

Before the Bar: Kinematic Detection of A Spheroidal Metal-Poor Bulge Component

A pulsational approach to near infrared and visual magnitudes of RR Lyrae stars

The surface brightness - colour relations based on eclipsing binary stars and calibrated with Gaia EDR3

The Araucaria Project: High-precision orbital parallax and masses of eclipsing binaries from infrared interferometry

The Araucaria Project. Near-Infrared Photometry of Cepheid Variables in the Sculptor Galaxy NGC 300

The Araucaria Project. An improved distance to the Sculptor spiral galaxy NGC 300 from its Cepheid variables

Probabilistic fibre-to-target assignment algorithm for multi-object spectroscopic surveys

4MOST Survey Strategy Plan

The Araucaria Project: Distance to the Local Group Galaxy NGC 3109 from Near-Infrared Photometry of Cepheids

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of Î´ Cep revisited

2XMM J083026+524133: The most X-ray luminous cluster at redshift 1

The Araucaria Project. The Distance to the Local Group Galaxy IC 1613 from Near-Infrared Photometry of Cepheid Variables

The angular size of the Cepheid L Car: a comparison of the interferometric and surface brightness techniques

On the Use of Field RR Lyrae as Galactic Probes. III. The I^±-element abundances

Cepheid metallicity in the Leavitt law (C-MetaLL) survey -- III. Simultaneous derivation of the Gaia parallax offset and Period-Luminosity-Metallicity coefficients

On the Use of Field RR Lyrae as Galactic Probes. II. A new I^S calibration to estimate their metallicity

Calibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique I. The p-factor, the Milky Way relations, and a universal K-band relation

Surface brightness-colour relations of Cepheids calibrated by optical interferometry

The RR Lyrae distance scale from near-infrared photometry: current results

The Araucaria Project. Precise physical parameters of the eclipsing binary IO Aqr

RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system

Surface brightness-colour relations of Milky Way and Magellanic Clouds classical Cepheids based on Gaia magnitudes

On a new and homogeneous metallicity scale for Galactic classical Cepheids - I. Physical parameters

On the radial extent of the dwarf irregular galaxy IC10

Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: IV. The metallicity dependence of Cepheid Period-Luminosity relations

Calibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique II. The effect of metallicity, and the distance to the LMC

New Near-Infrared $J H K_{s}$ light-curve templates for RR Lyrae variables

On the Use of Field RR Lyrae as Galactic Probes. III. The $I^\pm$ -element abundances

On the Use of Field RR Lyrae as Galactic Probes. II. A new $I^$ S calibration to estimate their metallicity

Near-Infrared Observations of RR Lyrae Variables in $I ¨ $ Centauri