The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass-size relation up to z = 2

DOI: 
10.1051/0004-6361/202037861
Publication date: 
24/03/2021
Main author: 
Nadolny, Jakub
IAA authors: 
Pović, Mirjana;Alfaro, Emilio;Ignacio González-Serrano, J.
Authors: 
Nadolny, Jakub;Bongiovanni, Ángel;Cepa, Jordi;Cerviño, Miguel;Pérez García, Ana María;Pović, Mirjana;Pérez Martínez, Ricardo;Sánchez-Portal, Miguel;de Diego, José A.;Pintos-Castro, Irene;Alfaro, Emilio;Castañeda, Héctor O.;Gallego, Jesús;Jesús González, J.;Ignacio González-Serrano, J.;Lara-López, Maritza A.;Padilla Torres, Carmen P.
Journal: 
Astronomy and Astrophysics
Publication type: 
Article
Volume: 
647
Pages: 
A89
Abstract: 
Context. The morphology of galaxies provide us with a unique tool for relating and understanding other physical properties and their changes over the course of cosmic time. It is only recently that we have been afforded access to a wealth of data for an unprecedented number galaxies thanks to large and deep surveys. <BR /> Aims: We present the morphological catalogue of the OTELO survey galaxies detected with the Hubble Space Telescope (HST)-ACS F814W images. We explore various methods applied in previous works to separate early-type (ET) and late-type (LT) galaxies classified via spectral energy distribution (SED) fittings using galaxy templates. Together with this article, we are releasing a catalogue containing the main morphological parameters in the F606W and F814W bands derived for more than 8000 sources. <BR /> Methods: The morphological analysis is based on the single-Sérsic profile fit. We used the GALAPAGOS2 software to provide multi-wavelength morphological parameters fitted simultaneously in two HST-ACS bands. The GALAPAGOS2 software detects, prepares guess values for GALFIT-M, and provides the best-fitting single-Sérsic model in both bands for each source. Stellar masses were estimated using synthetic rest-frame magnitudes recovered from SED fittings of galaxy templates. The morphological catalogue is complemented with concentration indexes from a separate SExtractor dual, high dynamical range mode. <BR /> Results: A total of 8812 sources were successfully fitted with single-Sérsic profiles. The analysis of a carefully selected sample of ∼3000 sources up to z<SUB>phot</SUB> = 2 is presented in this work, of which 873 sources were not detected in previous studies. We found no statistical evidence for the evolution of the low-mass end of mass-size relation for ET and LT since z = 2. Furthermore, we found a good agreement for the median size evolution for ET and LT galaxies, for a given stellar mass, with the data from the literature. Compared to previous works on faint field galaxies, we found similarities regarding their rest-frame colours as well as the Sérsic and concentration indices. <P />The catalogue are only available at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr/">cdsarc.u-strasbg.fr</A> (ftp://130.79.128.5) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/647/A89">http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/647/A89</A>
Database: 
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/2021A&A...647A..89N/abstract
ADS Bibcode: 
2021A&A...647A..89N
Keywords: 
catalogs;galaxies: evolution;galaxies: fundamental parameters;galaxies: structure;Astrophysics - Astrophysics of Galaxies