English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We introduce our new code MYOSOTIS (Make Your Own Synthetic ObservaTIonS)which is designed to produce synthetic observations from simulated clusters.The code can synthesise observations from both ground- and spaced-basedobservatories, for a range of different filters, observational conditions andangular/spectral resolution. In this paper, we highlight some of the featuresof MYOSOTIS, creating synthetic observations from young massive star clusters.Our model clusters are simulated using nbody6 code and have different totalmasses, half-mass radii, and binary fractions. The synthetic observations aremade at the age of 2 Myr with Solar metallicity and under different extinctionconditions. For each cluster, we create synthetic images of the Hubble SpaceTelescope (HST) in the visible (WFPC2/F555W) as well as Very Large Telescopes(VLT) in the nearIR (SPHERE/IRDIS/Ks). We show how MYOSOTIS can be used to lookat mass function (MF) determinations. For this aim we re-estimate stellarmasses using a photometric analysis on the synthetic images. The synthetic MFslopes are compared to their actual values. Our photometric analysisdemonstrate that depending on the adopted filter, extinction, angularresolution and pixel sampling of the instruments, the power-law index of theunderlying MFs can be shallower than the observed ones by at least 0.25 dexwhich is in agreement with the observed discrepancies reported in theliterature, specially for young star clusters.

A Code to Make Your Own Synthetic ObservaTIonS (MYOSOTIS)