J/MNRAS/475/5133    3DHST CANDELS redshift compilation       (Rodrigues+, 2018)

Testing the hierarchical assembly of massive galaxies using accurate merger rates out to z ∼ 1.5. Rodrigues M., Puech M., Flores H., Hammer F., Pirzkal N. <Mon. Not. R. Astron. Soc., 475, 5133-5143 (2018)> =2018MNRAS.475.5133R 2018MNRAS.475.5133R (SIMBAD/NED BibCode)
ADC_Keywords: Galaxy catalogs ; Redshifts Keywords: galaxies: evolution - galaxies: formation - galaxies: high-redshift - galaxies: interactions Abstract: We established an accurate comparison between observationally and theoretically estimated major merger rates over a large range of mass (logMbar/M=9.9-11.4) and redshift (z=0.7-1.6). For this, we combined a new estimate of the merger rate from an exhaustive count of pairs within the virial radius of massive galaxies at z∼1.265 and cross-validated with their morphology, with estimates from the morpho-kinematic analysis of two other samples. Theoretical predictions were estimated using semi-empirical models with inputs matching the properties of the observed samples, while specific visibility time-scales scaled to the observed samples were used. Both theory and observations are found to agree within 30 per cent of the observed value, which provides strong support to the hierarchical assembly of galaxies over the probed ranges of mass and redshift. Here, we find that ∼60 per cent of population of local massive (Mstellar=1010.3-11.6M) galaxies would have undergone a wet major merger since z=1.5, consistently with previous studies. Such recent mergers are expected to result in the (re-)formation of a significant fraction of local disc galaxies. Description: We collected all zspec measurements available in GOODS-S and constructed an updated catalogue of the most accurate redshift measurements for 3D-HST sources in this field. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 56 13984 3DHST CANDELS redshift compilation -------------------------------------------------------------------------------- See also: J/ApJS/225/27 : 3D-HST Survey: grism spectra master catalog (Momcheva+ 2016) J/MNRAS/475/5133 : 3D-HST CANDELS redshift compilation (Rodrigues+, 2018) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- ID [1/50502] Identification number, [SWM2014] GOODS-S NN in Simbad 7- 17 F11.8 deg RAdeg Right ascension (J2000) 19- 30 F12.8 deg DEdeg declination (J2000) 32- 38 F7.4 mag Jmag ?=- J magnitude 40- 46 F7.4 --- z ?=-1 Spectroscopic or photometric redshift 51 I1 --- q_z [0/3] Redshift quality flag (1) 55- 56 I2 --- Flag [-1/4] Flag type (2) -------------------------------------------------------------------------------- Note (1): Redshift quality flag as follows: 3 = secure (99% sure) 2 = likely (95% sure, including spectrum with a single line) 1 = insecure Note (2): Flag type as follows: 1 = single zspec match 2 = multiple zspec matches for a single photometric source. If all zspec measurements agreed within 0.001, the zspec with higher spectroscopic QF was considered and we then set QF=3. If the disagreement between the different zspec was larger than 0.001, all spectra were checked visually to determine the final zspec and associated QF. 3 = multiple zspec matches for multiple photometric sources within the cross-correlation radius of 0.5 arcsec. All spectra and astrometry were checked to determine the final zspec and associated QF for all sources 4 = no zspec match. The zgrism estimate from Momcheva et al. (2016, Cat. J/ApJS/225/27) was adopted. -1 = neither zspec nor zgrism match. The zphot estimate from Momcheva et al. (2016, Cat. J/ApJS/225/27) was adopted. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 08-Apr-2021
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 into arrays or line by line