J/AJ/151/120 z<1 3CR radio galaxies and quasars star formation (Westhues+, 2016)
Star formation in 3CR radio galaxies and quasars at z<1.
Westhues C., Haas M., Barthel P., Wilkes B.J., Willner S.P.,
Kuraszkiewicz J., Podigachoski P., Leipski C., Meisenheimer K.,
Siebenmorgen R., Chini R.
<Astron. J., 151, 120-120 (2016)>
=2016AJ....151..120W 2016AJ....151..120W (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, radio ; QSOs ; Active gal. nuclei ; Spectroscopy ;
Photometry, infrared ; Energy distributions ; Abundances ;
Stars, ages ; Stars, masses
Keywords: galaxies: active - infrared: galaxies - radio continuum: galaxies
Abstract:
Using the Herschel Space Observatory we have observed a representative
sample of 87 powerful 3CR sources at redshift z<1. The far-infrared
(FIR, 70-500 µm) photometry is combined with mid-infrared (MIR)
photometry from the Wide-Field Infrared Survey Explorer and cataloged
data to analyze the complete spectral energy distributions (SEDs) of
each object from optical to radio wavelength. To disentangle the
contributions of different components, the SEDs are fitted with a set
of templates to derive the luminosities of host galaxy starlight, dust
torus emission powered by active galactic nuclei (AGNs), and cool dust
heated by stars. The level of emission from relativistic jets is also
estimated to isolate the thermal host galaxy contribution. The new
data are in line with the orientation-based unification of
high-excitation radio-loud AGN, in that the dust torus becomes
optically thin longwards of 30 µm. The low-excitation radio
galaxies and the MIR-weak sources represent an MIR- and FIR-faint AGN
population that is different from the high-excitation MIR-bright
objects; it remains an open question whether they are at a later
evolutionary state or an intrinsically different population. The
derived luminosities for host starlight and dust heated by star
formation are converted to stellar masses and star-formation rates
(SFR). The host-normalized SFR of the bulk of the 3CR sources is low
when compared to other galaxy populations at the same epoch. Estimates
of the dust mass yield a 1-100 times lower dust/stellar mass ratio
than for the Milky Way, which indicates that these 3CR hosts have very
low levels of interstellar matter and explains the low level of star
formation. Less than 10% of the 3CR sources show levels of star
formation above those of the main sequence of star-forming galaxies.
Description:
This work studies a sample of 87 sources from the 3CR catalog (Edge et al.
1959, Cat. VIII/1; Bennett 1962MNRAS.125...75B 1962MNRAS.125...75B; Laing et al. 1983,
J/MNRAS/204/151; Spinrad et al. 1985, J/PASP/97/932). With the
Herschel Space Observatory (Pilbratt et al. 2010A&A...518L...1P 2010A&A...518L...1P) we
measured the FIR/submm spectral energy distributions (SEDs) of the 3CR
sources in two complementary proposals: one at redshift 1<z<3 (PI:
Barthel, Barthel et al. 2012ApJ...757L..26B 2012ApJ...757L..26B; Podigachoski et al. 2015,
J/A+A/575/A80 and 2015ApJ...806L..11P 2015ApJ...806L..11P) and one at medium (0.5<z<1) and low
(z<0.5) redshift (PI: Haas).
We here present sensitive Herschel Photoconducter Array Camera and
Spectrometer (PACS)/Spectral and Photometric Imaging Receiver (SPIRE)
70-500 µm photometry of the representative 3CR sample at low and
medium redshift. We here analyze the full optical to radio SEDs, also
combined with Wide-Field Infrared Survey Explorer (WISE) 3-22 µm
photometry. The purpose is to explore dust emission in the FIR for the
most powerful radio-loud AGN, provide constraints on the star-forming
activity, and investigate the evolutionary status of their host galaxies.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1.dat 107 40 3CR Sources 0.5<z<1 Observed with Herschel
table2.dat 107 51 3CR Sources z<0.5 Observed with Herschel
table4.dat 58 39 3CR Sources 0.5<z<1 PACS and SPIRE Flux
Densities
table5.dat 58 48 3CR Sources z<0.5 PACS and SPIRE Flux Densities
table6.dat 76 40 Median Spectral Templates for Different Galaxy
Types Separated for Low- (z<0.5) and
Medium-redshift (0.5<z<1)
table10.dat 106 39 Host Fit Parameters for the 3Cs at 0.5<z<1.0
table11.dat 109 48 Host Fit Parameters for the 3Cs at z<0.5
table12.dat 78 39 AGN Fit Parameters for the 3Cs at 0.5<z<1.0
table13.dat 84 48 AGN Fit Parameters for the 3Cs at z<0.5
table14.dat 92 39 FIR Fit Parameters for the 3Cs at 0.5<z<1.0
table15.dat 94 48 FIR Fit Parameters for the 3Cs at z<0.5
table16.dat 67 39 Monochromatic Luminosities for the 3Cs
at 0.5<z<1.0
table17.dat 67 48 Monochromatic Luminosities for the 3Cs at z<0.5
--------------------------------------------------------------------------------
See also:
VIII/1 : The 3C and 3CR Catalogues (Edge+ 1959-1962)
VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)
J/MNRAS/204/151 : Bright radio sources at 178 MHz (3CRR) (Laing+ 1983)
J/PASP/97/932 : 3CR Source Identifications (Spinrad+, 1985)
J/A+A/575/A80 : FIR photometry of 3CR galaxies (Podigachoski+, 2015)
Byte-by-byte Description of file: table1.dat table2.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- --- [3C]
3- 7 F5.1 --- 3C [006.1/459] 3CR source name (3CNNN.N)
9- 10 I2 h RAh Hour of Right Ascension (J2000)
12- 13 I2 min RAm Minute of Right Ascension (J2000)
15- 18 F4.1 s RAs Second of Right Ascension (J2000)
20 A1 --- DE- Sign of the Declination (J2000)
21- 22 I2 deg DEd Degree of Declination (J2000)
24- 25 I2 arcmin DEm Arcminute of Declination (J2000)
27- 28 I2 arcsec DEs Arcsecond of Declination (J2000)
29 A1 --- n_DEs [c] Note on DEs (1)
31- 36 F6.4 --- z [0.0169/0.996] Redshift
38- 41 I4 Mpc DL [66/6426] Luminosity distance
43- 46 A4 --- Type Type of galaxy (2)
48- 50 A3 --- n_Type [b,c d] Note(s) on Type (1)
52 I1 --- PID [1/6] Proposal identifier (3)
54- 63 I10 --- PObsID1 ? Herschel/PACS first ObsID
65- 74 I10 --- PObsID2 ? Herschel/PACS second ObsID
76- 85 I10 --- PObsID3 ? Herschel/PACS third ObsID
87- 96 I10 --- PObsID4 ? Herschel/PACS fourth ObsID
98-107 I10 --- SPObsID [1342229105/1342268340]? Herschel/SPIRE ObsID
--------------------------------------------------------------------------------
Note (1): Note as follows:
b = Compact steep-spectrum (CSS) source;
c = Coordinates/classifiaction revised;
d = Fanaroff-Riley class I (FR I) source.
Note (2): Type as follows:
BLRG = Broad-line radio galaxy;
HERG = High-excitation radio galaxy;
LENS = Gravitational lens;
LERG = Low-excitation radio galaxy;
QSR = Quasar.
Note (3): Proposal ID as follows:
1 = OT1mhaas2;
2 = OT1jstevens1;
3 = OT1pogle011;
4 = OT1rmushotz1;
5 = OT1lho1;
6 = OT1dfarrah1.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table4.dat table5.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- --- [3C]
3- 7 F5.1 --- 3C [006.1/459] 3CR source name (3CNNN.N)
9- 10 I2 --- Fig [1/15] Figure number in the paper
12 A1 --- l_F70 [<] Limit flag on F70
13- 15 I3 mJy F70 [6/783]?=- Herschel/PACS 70 µm flux density
17 I1 mJy e_F70 [2/8]? 1σ uncertainty in F70
19 A1 --- l_F100 [<] Limit flag on F100
20- 22 I3 mJy F100 [6/867]?=- Herschel/PACS 100 µm flux density
24 I1 mJy e_F100 [1/6]? 1σ uncertainty in F100
26 A1 --- l_F160 [<] Limit flag on F160
27- 30 I4 mJy F160 [13/1347]?=- Herschel/PACS 160 µm flux density
32- 33 I2 mJy e_F160 [3/24]? 1σ uncertainty in F160
35 A1 --- l_F250 [<] Limit flag on F250
36- 38 I3 mJy F250 [22/955]?=- Herschel/SPIRE 250 µm flux density
40- 41 I2 mJy e_F250 [8/27]? 1σ uncertainty in F250
43 A1 --- l_F350 [<] Limit flag on F350
44- 46 I3 mJy F350 [20/741]?=- Herschel/SPIRE 350 µm flux density
48- 49 I2 mJy e_F350 [8/26]? 1σ uncertainty in F350
51 A1 --- l_F500 [<] Limit flag on F500
52- 55 I4 mJy F500 [23/1062]?=- Herschel/SPIRE 500µm flux density
57- 58 I2 mJy e_F500 [7/31]? 1σ uncertainty in F500
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table6.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 F4.1 [um] log(lrest) [-0.4/6.6] Log of rest wavelength
λRest
6- 9 F4.1 [Lsun] log(nuLnu)Hl [8.7/11.1] Log of rest frame luminosity
νLν for high-excitation radio
low-z galaxy type
11- 13 F3.1 [Lsun] e_log(nuLnu)Hl [0.1/1] Uncertainty in log(nuLnu)Hl
15- 18 F4.1 [Lsun] log(nuLnu)Hm [10/11.5] Log of rest frame luminosity
νLν for high-excitation radio
medium-z galaxy type
20- 22 F3.1 [Lsun] e_log(nuLnu)Hm [0.1/0.7] Uncertainty in log(nuLnu)Hm
24- 27 F4.1 [Lsun] log(nuLnu)L [8.7/11.2]?=- Log of rest frame luminosity
νLν for low-excitation radio
galaxy type
29- 31 F3.1 [Lsun] e_log(nuLnu)L [0.1/1.3]? Uncertainty in log(nuLnu)L
33- 36 F4.1 [Lsun] log(nuLnu)B [9.1/11.5]?=- Log of rest frame luminosity
νLν for broad-line radio galaxy
type
38- 40 F3.1 [Lsun] e_log(nuLnu)B [0.1/0.9]? Uncertainty in log(nuLnu)B
42- 45 F4.1 [Lsun] log(nuLnu)Fl [8.4/11]?=- Log of rest frame luminosity
νLν for flat-spectrum low-z
quasar type
47- 49 F3.1 [Lsun] e_log(nuLnu)Fl [0.3/0.8]? Uncertainty in log(nuLnu)Fl
51- 54 F4.1 [Lsun] log(nuLnu)Fm [10.2/12.1]?=- Log of rest frame
luminosity νLν for flat-spectrum
medium-z quasar type
56- 58 F3.1 [Lsun] e_log(nuLnu)Fm [0.2/0.3]? Uncertainty in log(nuLnu)Fm
60- 63 F4.1 [Lsun] log(nuLnu)Sl [10.2/12.2]?=- Log of rest frame
luminosity νLν for steep-spectrum
low-z quasar type
65- 67 F3.1 [Lsun] e_log(nuLnu)Sl [0.2/1.6]? Uncertainty in log(nuLnu)Sl
69- 72 F4.1 [Lsun] log(nuLnu)Sm [10.3/12.5] Log of rest frame luminosity
νLν for steep-spectrum
medium-z quasar type
74- 76 F3.1 [Lsun] e_log(nuLnu)Sm [0.1/0.8]Uncertainty in log(nuLnu)Sm
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table10.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- --- [3C]
3- 7 F5.1 --- 3C [6.1/455] 3CR source name (3CNNN.N)
9- 14 F6.2 [W/m2] logAHost [-15.72/-14.42] Log of the host galaxy
flux
16- 19 F4.2 [W/m2] e_logAHost [0.03/0.23] Lower limit uncertainty
in logAHost
21- 24 F4.2 [W/m2] E_logAHost [0.03/0.27] Upper limit uncertainty
in logAHost
26- 30 F5.3 --- Z [0.004/0.05] Metallicity
32- 35 F4.1 [yr] upsilon [6.9/10] Timescale υ
37- 39 F3.1 [yr] e_upsilon [0.3/2] Lower limit uncertainty
in upsilon
41- 43 F3.1 [yr] E_upsilon [0.3/2.2] Upper limit uncertainty
in upsilon
45- 49 F5.2 [yr] logAge [9.1/10] Log of the age of the
stellar population
51- 54 F4.2 [yr] e_logAge [0.04/0.3] Lower limit uncertainty
in logAge
56- 59 F4.2 [yr] E_logAge [0.03/0.3] Upper limit uncertainty
in logAge
61- 64 F4.1 10+11Msun M* [0.3/19] Stellar mass
66- 69 F4.1 10+11Msun e_M* [0.1/7.2] Lower limit uncertainty in M*
71- 74 F4.1 10+11Msun E_M* [0.1/19] Upper limit uncertainty in M*
76- 79 F4.1 10+11Lsun LHost [0.9/28] Luminosity of the host galaxy
81- 83 F3.1 10+11Lsun e_LHost [0.2/8.5] Lower limit uncertainty
in LHost
85- 87 F3.1 10+11Lsun E_LHost [0.2/8.4] Upper limit uncertainty
in LHost
89- 93 F5.1 10+7Msun MBH [3.8/428.7] Black hole mass
95- 99 F5.1 10+7Msun e_MBH [1.9/256.5] Lower limit uncertainty
in MBH
101-106 F6.1 10+7Msun E_MBH [2.6/1030.6] Upper limit uncertainty
in MBH
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table11.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- --- [3C]
3- 7 F5.1 --- 3C [20/459] 3CR source name (3CNNN.N)
9- 14 F6.2 [W/m2] logAHost [-15.14/-12.21] Log of the host galaxy
flux
16- 19 F4.2 [W/m2] e_logAHost [0.01/0.24] Lower limit uncertainty
in logAHost
21- 24 F4.2 [W/m2] E_logAHost [0.01/0.17] Upper limit uncertainty
in logAHost
26- 30 F5.3 --- Z [0.004/0.05] Metallicity
32- 35 F4.1 [yr] upsilon [6.6/11] Timescale υ
37- 39 F3.1 [yr] e_upsilon [0.1/1.6] Lower limit uncertainty
in upsilon
41- 43 F3.1 [yr] E_upsilon [0.2/2.1] Upper limit uncertainty
in upsilon
45- 49 F5.2 [yr] logAge [9.1/10] Log of the age of the
stellar population
51- 54 F4.2 [yr] e_logAge [0.02/0.24] Lower limit uncertainty
in logAge
56- 59 F4.2 [yr] E_logAge [0.01/0.3] Upper limit uncertainty
in logAge
61- 65 F5.1 10+10Msun M* [0.4/210] Log of stellar mass
67- 70 F4.1 10+10Msun e_M* [0.2/65] Lower limit uncertainty in M*
72- 75 F4.1 10+10Msun E_M* [0.1/70] Upper limit uncertainty in M*
77- 81 F5.1 10+10Lsun LHost [0.5/170] Luminosity of the host galaxy
83- 86 F4.1 10+10Lsun e_LHost [0.1/44] Lower limit uncertainty
in LHost
88- 91 F4.1 10+10Lsun E_LHost [0.1/59] Upper limit uncertainty
in LHost
93- 97 F5.1 10+7Msun MBH [0.4/479.6] Black hole mass
99-103 F5.1 10+7Msun e_MBH [0.2/265.3] Lower limit uncertainty
in MBH
105-109 F5.1 10+7Msun E_MBH [0.2/538.2] Upper limit uncertainty
in MBH
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table12.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- --- [3C]
3- 7 F5.1 --- 3C [6.1/455] 3CR source name (3CNNN.N)
9- 14 F6.2 [W/m2] logAagn [-15.6/-14.11] Log of the AGN-heated
warm dust flux
16- 19 F4.2 [W/m2] e_logAagn [0.02/0.22] Lower limit uncertainty
in logAagn
21- 24 F4.2 [W/m2] E_logAagn [0.01/0.12] Upper limit uncertainty
in logAagn
26- 27 I2 deg Inc [0/75] Inclination angle to the observer
29- 32 F4.1 --- NCloud [2.5/10] Number of clouds along
the equatorial line of sight
34- 38 F5.2 --- a [-2/0] Index of the power law for radial
dust-cloud distribution
40- 41 I2 deg theta [5/60] Half opening angle θ
43- 44 I2 --- tau [30/80] Optical depth τ
46- 49 F4.1 10+11Lsun LAGN [0.9/56] AGN luminosity
51- 53 F3.1 10+11Lsun e_LAGN [0.1/7.7] Lower limit uncertainty
in LAGN
55- 57 F3.1 10+11Lsun E_LAGN [0.1/8.7] Upper limit uncertainty
in LAGN
59- 64 F6.4 --- LAGN/LEdd [0.0044/0.508] Ratio of AGN luminosity
in the MIR and Eddington luminosity
(G1)
66- 71 F6.4 --- e_LAGN/LEdd [0.0021/0.2891] Lower limit uncertainty
in LAGN/LEdd
73- 78 F6.4 --- E_LAGN/LEdd [0.0045/0.7034] Upper limit uncertainty
in LAGN/LEdd
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table13.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- --- [3C]
3- 7 F5.1 --- 3C [20/459] 3CR source name (3CNNN.N)
9- 14 F6.2 [W/m2] logAagn [-16.23/-12.89] Log of the AGN-heated
warm dust flux
16- 19 F4.2 [W/m2] e_logAagn [0.01/0.27] Lower limit uncertainty
in logAagn
21- 24 F4.2 [W/m2] E_logAagn [0.01/0.23] Upper limit uncertainty
in logAagn
26- 27 I2 deg Inc [0/75] Inclination angle to the observer
29- 32 F4.1 --- NCloud [2.5/10] Number of clouds along
the equatorial line of sight
34- 38 F5.2 --- a [-2/0] Index of the power law for radial
dust-cloud distribution
40- 41 I2 deg theta [5/60] Half opening angle θ
43- 44 I2 --- tau [30/80] Optical depth τ
46- 51 F6.1 10+9Lsun LAGN [0.1/3900] AGN luminosity
53- 57 F5.1 10+9Lsun e_LAGN [0.1/890] Lower limit uncertainty in LAGN
59- 63 F5.1 10+9Lsun E_LAGN [0.1/580] Upper limit uncertainty in LAGN
65- 70 F6.4 --- LAGN/LEdd [0.0001/0.6886] Ratio of AGN luminosity
in the MIR and Eddington luminosity (G1)
72- 77 F6.4 --- e_LAGN/LEdd [0.0001/0.3371] Lower limit uncertainty
in LAGN/LEdd
79- 84 F6.4 --- E_LAGN/LEdd [0.0001/1.184] Upper limit uncertainty
in LAGN/LEdd
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table14.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- --- [3C]
3- 7 F5.1 --- 3C [6.1/455] 3CR source name (3CNNN.N)
9- 14 F6.2 [W/m2] logAFIR [-15.59/-14.21] Log of the SF-heated
cool dust flux
16- 19 F4.2 [W/m2] e_logAFIR [0.03/0.23] Lower limit uncertainty
in logAFIR
21- 24 F4.2 [W/m2] E_logAFIR [0.02/0.15] Upper limit uncertainty
in logAFIR
26- 29 F4.1 K TFIR [20/47] FIR dust temperature
31- 33 F3.1 K e_TFIR [0.2/3.1] Lower limit uncertainty
in TFIR
35- 37 F3.1 K E_TFIR [0.2/3.1] Upper limit uncertainty
in TFIR
39- 43 F5.1 Msun/yr SFR [16.8/555.8] Star formation rate
45- 48 F4.1 Msun/yr e_SFR [1.4/83.4] Lower limit uncertainty
in SFR
50- 53 F4.1 Msun/yr E_SFR [1.6/69.5] Upper limit uncertainty
in SFR
55- 58 F4.1 10+11Lsun LFIR [1/32] Luminosity of cool
FIR emitting dust
60- 62 F3.1 10+11Lsun e_LFIR [0.1/4.8] Lower limit uncertainty
in LFIR
64- 66 F3.1 10+11Lsun E_LFIR [0.1/4] Upper limit uncertainty in LFIR
68- 73 F6.2 10+7Msun MDust [1.85/264.41] Dust mass
75- 80 F6.2 10+7Msun e_MDust [0.13/125.32] Lower limit
uncertainty in MDust
82- 86 F5.2 10+7Msun E_MDust [0.09/57.8] Upper limit uncertainty
in MDust
88- 92 F5.3 --- MDust/M* [0.017/8.814] Dust-to-stellar mass
ratio in per mille units
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table15.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- --- [3C]
3- 7 F5.1 --- 3C [20/459] 3CR source name (3CNNN.N)
9- 14 F6.2 [W/m2] logAFIR [-15.7/-13.39] Log of the SF-heated
cool dust flux
16- 19 F4.2 [W/m2] e_logAFIR [0.03/0.31] Lower limit uncertainty
in logAFIR
21- 24 F4.2 [W/m2] E_logAFIR [0.02/0.2] Upper limit uncertainty
in logAFIR
26- 29 F4.1 K TFIR [21/66] FIR dust temperature
31- 33 F3.1 K e_TFIR [0.2/2.5] Lower limit uncertainty
in TFIR
35- 37 F3.1 K E_TFIR [0.2/2.5] Upper limit uncertainty
in TFIR
39- 43 F5.1 Msun/yr SFR [0.1/573.2] Star formation rate
45- 48 F4.1 Msun/yr e_SFR [0/55.6] Lower limit uncertainty in SFR
50- 53 F4.1 Msun/yr E_SFR [0/52.1] Upper limit uncertainty in SFR
55- 60 F6.1 10+9Lsun LFIR [0.3/3300] Luminosity of cool
FIR emitting dust
62- 66 F5.1 10+9Lsun e_LFIR [0.1/320] Lower limit uncertainty
in LFIR
68- 72 F5.1 10+9Lsun E_LFIR [0.2/300] Upper limit uncertainty
in LFIR
74- 78 F5.2 10+7Msun MDust [0.02/27.37] Dust mass
80- 83 F4.2 10+7Msun e_MDust [0/6.37] Lower limit uncertainty
in MDust
85- 88 F4.2 10+7Msun E_MDust [0/4.26] Upper limit uncertainty
in MDust
90- 94 F5.3 --- MDust/M* [0.004/5.474] Dust-to-stellar mass
ratio in per mille units
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table16.dat table17.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- --- [3C]
3- 7 F5.1 --- 3C [6.1/459] 3CR source name (3CNNN.N)
9- 13 F5.2 [Lsun] log(nuLnu)30GHz [7.21/11.6] Log of rest frame 30 GHz
monochromatic luminosity
νLν30GHz
15- 19 F5.3 [Lsun] e_log(nuLnu)30GHz [0.005/0.08] Uncertainty
in log(nuLnu)30GHz
21- 25 F5.2 [Lsun] log(nuLnu)178MHz [6.58/10.97] Log of rest frame 178 MHz
monochromatic luminosity
νLν178MHz
27- 31 F5.3 [Lsun] e_log(nuLnu)178MHz [0.001/0.065] Uncertainty
in log(nuLnu)178MHz
33- 37 F5.2 [Lsun] log(nuLnu)30um [7.98/12.34] Log of rest frame
30 µm monochromatic luminosity
νLν30µm
39- 43 F5.3 [Lsun] e_log(nuLnu)30um [0.002/0.239] Uncertainty
in log(nuLnu)30um
45- 49 F5.2 [Lsun] log(nuLnu)60um [8.19/12.45] Log of rest frame
60 µm monochromatic luminosity
νLν60µm
51- 55 F5.3 [Lsun] e_log(nuLnu)60um [0.001/0.137] Uncertainty
in log(nuLnu)60um
57- 61 F5.2 [Lsun] log(nuLnu)100um [8.44/12.31] Log of rest frame
100 µm monochromatic luminosity
νLν100µm
63- 67 F5.3 [Lsun] e_log(nuLnu)100um [0.001/0.283] Uncertainty
in log(nuLnu)100um
--------------------------------------------------------------------------------
Global notes:
Note (G1): LEdd∼3.2x104(MBH/M☉)L☉.
--------------------------------------------------------------------------------
History:
From electronic version of the journal
(End) Tiphaine Pouvreau [CDS] 26-Mar-2018