A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
E-INSPIRE- I. Bridging the gap with the local Universe: stellar population of a statistical sample of ultra-compact massive galaxies at z < 0.3
Tekijät: Mills, John; Spiniello, Chiara; Sergeyev, Alexey; Tortora, Crescenzo; Khramtsov, Vladyslav; D'Ago, Giuseppe; Maksymowicz-Maciata, Michalina; Benedetti, Joao P., V; Ferre-Mateu, Anna; Cappellari, Michele; Davies, Roger; Hartke, Johanna; Rosen, Charles
Kustantaja: OXFORD UNIV PRESS
Kustannuspaikka: OXFORD
Julkaisuvuosi: 2025
Journal: Monthly Notices of the Royal Astronomical Society
Tietokannassa oleva lehden nimi: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Lehden akronyymi: MON NOT R ASTRON SOC
Vuosikerta: 541
Numero: 3
Aloitussivu: 2440
Lopetussivu: 2458
Sivujen määrä: 19
ISSN: 0035-8711
eISSN: 1365-2966
DOI: https://doi.org/10.1093/mnras/staf516
Verkko-osoite: https://doi.org/10.1093/mnras/staf516
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/499401447
This paper presents the first effort to Extend the Investigation of Stellar Populations In RElics (E-INSPIRE). We present a catalogue of 430 spectroscopically confirmed ultra-compact massive galaxies (UCMGs) from the Sloan Digital Sky Survey at redshifts 0.01 < z < 0.3. This increases the original INSPIRE sample eightfold, bridging the gap with the local Universe. For each object, we compute integrated stellar velocity dispersion, age, metallicity, and [Mg/Fe] through spectroscopic stellar population analysis. We infer star formation histories (SFHs), metallicity evolution histories (MEHs) and compute the Degree of Relicness (DoR) of each object. The UCMGs, covering a wide range of DoR from 0.05 to 0.88, can be divided into three groups, according to how extreme their SFH was. The first group consists of 81 extreme relics (DoR greater than or similar to 6) that have formed the totality of their stellar mass by and have super-solar metallicities at all cosmic epochs. The second group (0.3 less than or similar to DoR less than or similar to 0.6) contains 293 objects also characterized by peaked SFHs but with a small percentage of later-formed stars and with a variety of MEHs. The third group (DoR less than or similar to 0.3), has 56 objects that cannot be considered relics since they have extended SFHs and formed a non-negligible fraction (> 25 per cent) of their stellar mass at . We conclude that the most efficient method of finding relics is to select UCMGs with a combination of large velocity dispersion values (as already found by INSPIRE), super-solar metallicities and high [Mg/Fe]
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CS and CT acknowledge funding from the INAF PRIN-INAF 2020 programme 1.05.01.85.11. AFM has received support from RYC2021-031099-I and PID2021-123313NA-I00 of MICIN/AEI/10.13039/501100011033/FEDER,UE, NextGenerationEU/PRT. CT acknowledges the INAF grant 2022 LEMON. GD acknowledges support by UKRI-STFC grants: ST/T003081/1 and ST/X001857/1. JPVB received the support of a fellowship from the ‘la Caixa’ Foundation (ID 100010434). The fellowship code is LCF/BQ/DI23/11990084.
