The full table of disturbance levels for 608 individual host galaxies of SNe. We define for all 608 hosts their level of morphological disturbance with the possible presence of signs of interactions and mergers. (1 data file)

Adibekyan, V. Z.

Aramyan, L. S.

Bertin, E.

de Lapparent, V.

Gomes, J. M.

Hakobyan, A. A.

Kunth, D.

Mamon, G. A.

Nazaryan, T. A.

Petrosian, A. R.

TURATTO, Massimo

OA@INAF - Istituto Nazionale di Astrofisica

2015Publication Year2020-04-14T19:26:19ZAcceptance in OA@INAFVizieR Online Data Catalog: Disturbance levels of SNe host galaxies (Hakobyan+, 2014)TitleHakobyan, A. A.; Nazaryan, T. A.; Adibekyan, V. Z.; Petrosian, A. R.; Aramyan, L. S.; et al.Authorshttp://hdl.handle.net/20.500.12386/24029HandleVizieR Online Data CatalogJournal07/04/2020 J/MNRAS/444/2428https://cdsarc.unistra.fr/viz-bin/ReadMe/J/MNRAS/444/2428?format=html&tex=true 1/2J/MNRAS/444/2428    Disturbance levels of SNe host galaxies  (Hakobyan+, 2014) Supernovae and their host galaxies. II. The relative frequencies of supernovae types in spirals.     Hakobyan A.A., Nazaryan T.A., Adibekyan V.Z., Petrosian A.R., Aramyan L.S.,     Kunth D., Mamon G.A., de Lapparent V., Bertin E., Gomes J.M., Turatto M.    <Mon. Not. R. Astron. Soc., 444, 2428-2441 (2014)>    =2014MNRAS.444.2428HADC_Keywords: Supernovae ; Galaxies, optical ; Galaxies, peculiar Keywords: supernovae: general - galaxies: active - galaxies: interactions -           galaxies: spiral - galaxies: stellar content Abstract:     We present an analysis of the relative frequencies of different     supernova (SN) types in spirals with various morphologies and in     barred or unbarred galaxies. We use a well-defined and homogeneous     sample of spiral host galaxies of 692 SNe from the Sloan Digital Sky     Survey in different stages of galaxy-galaxy interaction and activity     classes of nucleus. We propose that the underlying mechanisms shaping     the number ratios of SNe types can be interpreted within the framework     of interaction-induced star formation, in addition to the known     relations between morphologies and stellar populations. We find a     strong trend in behaviour of the NIa/NCC ratio depending     on host morphology, such that early spirals include more Type Ia SNe.     The NIbc/NII ratio is higher in a broad bin of early-type     hosts. The NIa/NCC ratio is nearly constant when changing     from normal, perturbed to interacting galaxies, then declines in     merging galaxies, whereas it jumps to the highest value in     post-merging/remnant galaxies. In contrast, the NIbc/NII     ratio jumps to the highest value in merging galaxies and slightly     declines in post-merging/remnant subsample. The interpretation is that     the star formation rates and morphologies of galaxies, which are     strongly affected in the final stages of interaction, have an impact     on the number ratios of SNe types. The NIa/NCC (NIbc/NII)     ratio increases (decreases) from star-forming to active galactic     nuclei (AGN) classes of galaxies. These variations are consistent with     the scenario of an interaction-triggered starburst evolving into AGN     during the later stages of interaction, accompanied with the change of     star formation and transformation of the galaxy morphology into an     earlier type. Description:     The full table of disturbance levels for 608 individual host galaxies     of SNe. We define for all 608 hosts their level of morphological     disturbance with the possible presence of signs of interactions and     mergers. File Summary:        FileName      Lrecl  Records   Explanations ReadMe            80        .   This file table1.dat        32      608   Disturbance levels of 608 individual host galaxies See also:            B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)  J/PASP/117/773 : Classifications of SN host galaxies. III (van den Bergh+ 2005)  J/A+A/544/A81  : Supernovae and their hosts in the SDSS DR8 (Hakobyan+, 2012)  http://www.sdss.org : SDSS Home Page Byte-by-byte Description of file: table1.dat   Bytes Format Units   Label     Explanations    1- 19  A19   ---     Hgal      SN host galaxy identification (1)   21- 32  A12   ---     Dlev      Disturbance level of SN host galaxy (2)Note (1): JHHMMSS.ss+DDMMSS.s for SDSS JHHMMSS.ss+DDMMSS.s Note (2): We define four categories of SN host disturbances as:        normal = hosts without any visible disturbance in their morphological                 structure     perturbed = hosts with visible morphological disturbance, but without long                 tidal arms, bridges, or destruction of spiral patterns   interacting = hosts with obvious signs of galaxy-galaxy interaction      merging  = hosts with evidence of an ongoing merging process;                 see e.g. Lambas et al., 2012A&A...539A..45L  p-merg./rem. = post-merging/remnant, single galaxies that exhibit signs of a Portal Simbad VizieR Aladin X-Match HelpOther07/04/2020 J/MNRAS/444/2428https://cdsarc.unistra.fr/viz-bin/ReadMe/J/MNRAS/444/2428?format=html&tex=true 2/2       • Contact© Université de Strasbourg/CNRS                past interaction, with a strong or already relaxed                 disturbance, see e.g. Ellison et al., 2013MNRAS.435.3627E and                 Lotz et al., 2008MNRAS.391.1137L, respectively Acknowledgements:    Artur Hakobyan, hakobyan(at)bao.sci.am References:    Hakobyan et al., Paper I   2012A&A...544A..81H, Cat. J/A+A/544/A81(End)     Artur Hakobyan [BAO], Patricia Vannier [CDS]               23-Apr-2015 The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files intoarrays or line by line

VizieR Online Data Catalog: Disturbance levels of SNe host galaxies (Hakobyan+, 2014)

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VizieR Online Data Catalog: Disturbance levels of SNe host galaxies (Hakobyan+, 2014)

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