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J/ApJ/796/7     NIR spectral analysis of star-forming galaxies   (Genzel+, 2014)

Evidence for wide-spread active galactic nucleus-driven outflows in the most massive z ∼ 1-2 star-forming galaxies. Genzel R., Forster Schreiber N.M., Rosario D., Lang P., Lutz D., Wisnioski E., Wuyts E., Wuyts S., Bandara K., Bender R., Berta S., Kurk J., Mendel J.T., Tacconi L.J., Wilman D., Beifiori A., Brammer G., Burkert A., Buschkamp P., Chan J., Carollo C.M., Davies R., Eisenhauer F., Fabricius M., Fossati M., Kriek M., Kulkarni S., Lilly S.J., Mancini C., Momcheva I., Naab T., Nelson E.J., Renzini A., Saglia R., Sharples R.M., Sternberg A., Tacchella S., Van Dokkum P. <Astrophys. J., 796, 7 (2014)> =2014ApJ...796....7G (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, IR - Redshifts - Spectra, infrared Keywords: galaxies: evolution; galaxies: high-redshift galaxies: kinematics and dynamics; infrared: galaxies Abstract: In this paper, we follow up on our previous detection of nuclear ionized outflows in the most massive (log(M*/M)≥10.9) z∼1-3 star-forming galaxies (SFGs) by increasing the sample size by a factor of six (to 44 galaxies above log(M*/M)≥10.9) from a combination of the SINS/zC-SINF, LUCI, GNIRS, and KMOS3D spectroscopic surveys. Description: For the analysis in this paper, we included a total of 110 SFGs at z∼1-3 with near-IR integral field or slit spectroscopy covering the Hα+[NII] line emission from surveys carried out with SINFONI, KMOS, LUCI, and GNIRS. The targets for these surveys were originally drawn from rest-frame optical, UV, and near-IR selected samples in broadband imaging surveys with optical spectroscopic redshifts, and from stellar mass-selected samples with near-IR or optical spectroscopic redshifts. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 114 110 Star-forming galaxy (SFG) Sample table4.dat 103 20 Outflow parameters
See also: J/AJ/126/539 : The Chandra Deep Fields North and South (Alexander+, 2003) J/ApJS/161/21 : Extended Chandra Deep Field-South survey (Lehmer+, 2005) J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006) J/MNRAS/372/741 : SXDF 100µJy catalogue (Simpson+, 2006) J/MNRAS/375/989 : Quasar variability (Wold+, 2007) J/A+A/488/73 : Variability-selected AGN in Chandra DFS (Trevese+, 2008) J/ApJ/682/985 : FIREWORKS photometry of GOODS CDF-S (Wuyts+, 2008) J/ApJS/177/431 : Mid-IR sources in EGS (Barmby+, 2008) J/ApJS/179/124 : Subaru/XMM-Newton deep survey (SXDS) III. (Ueda+, 2008) J/A+A/507/1277 : Multiwavelength photometry of CDFS X-ray sources (Brusa+, 2009) J/ApJ/706/1364 : SINS survey of high-z galaxies (Forster Schreiber+, 2009) J/ApJS/180/102 : AEGIS-X: Chandra deep survey (Laird+, 2009) J/ApJS/188/178 : VLA 1.4GHz observations of GOODS-N field (Morrison+, 2010) J/ApJS/188/384 : The VLA-COSMOS survey. IV. (Schinnerer+, 2010) J/ApJ/723/737 : Catalog of variability selected AGNs in GOODS (Villforth+, 2010) J/ApJ/720/368 : Color-magnitude relations of galaxies in CDFs (Xue+, 2010) J/ApJ/742/61 : Photometric redshift of AGNs from XMM- and C-COSMOS (Salvato+ 2011) J/ApJS/195/10 : The CDF-S survey: 4Ms source catalogs (Xue+, 2011) J/ApJ/748/124 : AGN X-ray variability in the 4Ms catalog (Young+, 2012) J/ApJ/768/74 : PHIBSS: CO observations of star-forming galaxies (Tacconi+, 2013) J/ApJ/771/85 : Dynamical masses of z∼2 quiescent galaxies (van de Sande+, 2013) J/ApJS/205/13 : VLA 1.4GHz survey of ECDF-S (DR2) (Miller+, 2013) J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 22 A22 --- Source Source 24- 36 A13 --- Survey Survey 38- 50 A13 --- kin Kinematic classification (1) 52- 55 A4 --- Mode Observing mode (2) 57- 60 F4.1 h Tint [1.7/23] Total on-source integration time of the observations 61 A1 --- f_S/N [w] Indicates a weak signal-to-noise ratio 62- 65 F4.1 --- S/N [1/50]? Signal-to-noise ratio 67- 69 F3.1 --- Broad [0.5/2]? Broad nuclear emission component (3) 71- 74 F4.2 --- z [0.79/2.61] Spectroscopic redshift 76- 80 F5.2 [Msun] logM* [9.36/11.68] Log of the stellar mass 82- 86 F5.3 --- sSFR [0.003/6.975] Normalized specific star formation rate, sSFR/sSFRms (4) 87 A1 --- f_[NII]/Ha [Obn] Flag on [NII]/Ha (5) 88- 91 F4.2 --- [NII]/Ha [0.05/1.5]? [NII]/Hα line ratio 93- 96 F4.1 kpc R1/2 [0.2/32]? Radius 99-102 A4 --- AGN AGN ("cand": 14 occurrences, "det": 18 occurrences) 104 A1 --- l_logLAGN [<] Limit flag on logLAGN 105-108 F4.1 10-7W logLAGN [44.4/46.3]? Bolometric AGN luminosity (erg/s) (6) 110-114 F5.2 --- Lsfr/Lagn [0.08/29]? L(SFR)/L(AGN)
Note (1): Kinematic classification of galaxy from Hα data, defined as follows: disk = rotation, disp = dispersion dominated kinematics, merger = perturbed motions in a major merger system, BLR = a compact AGN broad line region component. Note (2): Observing mode for the data used in this work, defined as follows: AO = adaptive-optics-assisted observations with FWHM resolution of 0.2"-0.3", s = seeing-limited observations with FWHM resolution of 0.5"-0.7", ss = seeing-limited observations with FWHM resolution of 0.5"-0.7", objects for which the kinematics are well resolved. Note (3): Identification of a broad nuclear emission component, defined as follows: 2.0 = a strong nuclear broad component, 1.0 = a clear nuclear broad component, 0.5 = a candidate nuclear broad component. Note (4): Specific SFR normalized to that of the main sequence of SFGs at the redshift and stellar mass of each object using the parameterization of Whitaker et al. (2012ApJ...754L..29W), applicable for log(M*/M)>10. Note (5): Flag on [NII]/Ha, defined as follows: n = no b = broad O = OH Note (6): The bolometric AGN luminosity is estimated either from the absorption corrected X-ray luminosity (as in Rosario et al. 2012A&A...545A..45R), or from the rest-frame 8µm luminosity of power-law mid-IR SEDs extrapolated to the total blue bump luminosity with AGN SEDs (Richards et al. 2006, Cat. J/ApJS/166/470), or an average. If only a mid-IR estimate is available, we consider this luminosity an upper limit to the AGN luminosity.
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 22 A22 --- Source Source 24- 27 F4.2 --- z [0.88/2.53] Spectroscopic redshift 29- 33 F5.2 [Msun] logM* [10.81/11.5] Log of the stellar mass 35- 39 F5.3 --- sSFR [0.033/5.052] Normalized specific star formation rate, sSFR/sSFR(ms) 41- 45 F5.1 Msun/yr SFRnuc [2.1/200] Star formation rate (Nucleus) 47- 49 F3.1 kpc Rad [1.3] Half-width at half maximum radius 51- 55 F5.2 --- Fb/FnHa [0.2/10] Broad to narrow Hα flux ratio, F(Hαbroad)/F(Hαnarrow) 57- 64 E8.2 10-7W LHa [1e+40/1e+44] Extinction-corrected, optically thin Hα luminosity (in erg/s) 66- 69 I4 km/s Vout [214/1300] Outflow velocity 71- 72 I2 cm-3 n(e) [80] Electron density, n(e)broad 74- 81 E8.2 Msun Mass [1.5e+07/4.2e+09] Mass in HII and He, Mbroad(HII+He) 83- 86 I4 Msun/yr dM/dt [8/1743] Mass loss rate, dMout/dt 88- 91 F4.1 --- eta [0.1/87.8] dMout/dt/SFR Ionized gas 93- 95 I3 --- O/R [1/564] Momentum ratio Outflow/Radiation 97-103 E7.1 --- dE/dt/L [0.00038/1.2] Energy ratio
History: From electronic version of the journal
(End) Marianne Brouty [CDS] 24-Feb-2017
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

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