J/A+A/620/A82 Properties of the SUPER targets (Circosta+, 2018)
SUPER. I. Toward an unbiased study of ionized outflows in z∼2 active galactic
nuclei: survey overview and sample characterization.
Circosta C., Mainieri V., Padovani P., Lanzuisi G., Salvato M.,
Harrison C.M., Kakkad D., Puglisi A., Vietri G., Zamorani G., Cicone C.,
Husemann B., Vignali C., Balmaverde B., Bischetti M., Bongiorno A.,
Brusa M., Carniani S., Civano F., Comastri A., Cresci G., Feruglio C.,
Fiore F., Fotopoulou S., Karim A., Lamastra A., Magnelli B., Mannucci F.,
Marconi A., Merloni A., Netzer H., Perna M., Piconcelli E., Rodighiero G.,
Schinnerer E., Schramm M., Schulze A., Silverman L.Zappacosta J.
<Astron. Astrophys. 620, A82 (2018)>
=2018A&A...620A..82C 2018A&A...620A..82C (SIMBAD/NED BibCode)
ADC_Keywords: Active gal. nuclei ; Galaxies, photometry
Keywords: galaxies: active - galaxies: evolution - quasars: general -
surveys - ISM: jets and outflows
Abstract:
Theoretical models of galaxy formation suggest that the presence of an
active galactic nucleus (AGN) is required to regulate the growth of
its host galaxy through feedback mechanisms, produced by, for example,
AGN-driven outflows. Although many observational studies have revealed
that such outflows are common both at low and high redshift, a
comprehensive picture is still missing. In particular, the peak epoch
of galaxy assembly (1<z<3) has been poorly explored so far, and
current observations in this redshift range are mostly limited to
targets with high chances to be in an outflowing phase. This paper
introduces SUPER (a SINFONI Survey for Unveiling the Physics and
Effect of Radiative feedback), an ongoing ESO's VLT/SINFONI Large
Programme. SUPER will perform the first systematic investigation of
ionized outflows in a sizeable and blindly-selected sample of 39 X-ray
AGN at z∼2, which reaches high spatial resolutions (∼2kpc) thanks to
the adaptive optics-assisted IFS observations. The outflow morphology
and star formation in the host galaxy will be mapped through the broad
component of [OIII]5007 and the narrow component of Hα
emission lines. The main aim of our survey is to infer the impact of
outflows on the on-going star formation and to link the outflow
properties to a number of AGN and host galaxy properties. We describe
here the survey characteristics and goals, as well as the selection of
the target sample. Moreover, we present a full characterization of its
multi-wavelength properties: we measure, via spectral energy
distribution fitting of UV-to-FIR photometry, stellar masses
(4x109-2x1011M☉), star formation rates (25-680M_☉/yr)
and AGN bolometric luminosities (2x1044-8x1047erg/s), along with
obscuring column densities (up to 2x1024cm-2) and luminosities in
the hard 2-10keV band (2x1043-6x1045erg/s) derived through X-ray
spectral analysis. Finally, we classify our AGN as jetted or
non-jetted according to their radio and FIR emission.
Description:
Properties of the 39 targets of the SUPER sample are presented. For
each source, ID, coordinates, redshift, multi-wavelength photometric
data, as well as the results of the SED-fitting and X-ray spectral
analysis are given.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1.dat 64 39 IDs, coordinates and redshifts of the
SUPER targets
table2.dat 141 39 Physical parameters derived through SED-fitting
and X-ray spectral analysis
photom.dat 2658 39 Photometric data of the sample
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Byte-by-byte Description of file: table1.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 9 A9 --- Field Field where the targets are located
11- 20 A10 --- ID Source identification number from the catalogs
corresponding to each field
22- 31 F10.6 deg RAdeg Optical counterpart right ascension (J2000)
33- 45 F13.9 deg DEdeg Optical counterpart declination (J2000)
47- 51 F5.3 --- zspec Spectroscopic redshift
53- 57 F5.2 mag Hmag H magnitude (AB)
59- 64 F6.2 mag Kmag ?=-99 K magnitude (AB)
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Byte-by-byte Description of file: table2.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 10 A10 --- ID ID of each target as given in Table 1
12- 13 A2 --- AGNtype [BL NL] AGN classification into
broad line (BL) and narrow line (NL)
15- 20 F6.2 [Msun] logM* ?=-99 Galaxy stellar mass
22- 27 F6.2 [Msun] e_logM* ?=-99 rms uncertainty on
28 A1 --- l_logLFIR [<] Upper limit flag on logLFIR
29- 34 F6.2 [10-7W] logLFIR ?=-99 FIR luminosity in the 8-1000um
range
36- 43 F8.4 [10-7W] e_logLFIR ? rms uncertainty on logLFIT
44 A1 --- l_SFR [<] Upper limit flag on SFR
45- 49 F5.1 [Msun/yr] SFR ?=-99 SFR from the FIR luminosity
51- 55 F5.1 [Msun/yr] e_SFR ? rms uncertainty on SFR
57- 61 F5.2 [10-7W] logLbol AGN bolometric luminosity, derived from
SED fitting
63- 66 F4.2 [10-7W] e_logLbol rms uncertainty on logLbol
68- 73 F6.1 ct Counts X-ray net counts (i.e., background
subtracted) in the full band
75- 78 F4.1 ct e_Counts rms uncertainty on Counts, computed
assuming a Poisson statistic
80- 84 F5.2 [cm-2] logNH Absorbing hydrogen column density
86- 91 F6.2 [cm-2] e_logNH ?=-99 Error on logNH 90% confidence level
(lower value)
93- 98 F6.2 [cm-2] E_logNH ?=-99 Error on logNH 90% confidence level
(upper value)
100-104 F5.2 [10-7W] logL2-10 Absorption-corrected X-ray luminosity in
the hard band (2-10keV)
106-110 F5.2 [10-7W] e_logL2-10 Error on logL2-10 90% confidence level
(lower value)
112-115 F4.2 [10-7W] E_logL2-10 Error on logL2-10 90% confidence level
(upper value)
117-122 F6.2 [Msun] logMBH ?=-99 Black hole mass
124-128 F5.1 [Msun] e_logMBH ?=-99 rms uncertainty on logMBH
129 A1 --- l_logP1.4GHz [<] Upper limit flag on logP1.4GHz
130-134 F5.2 [W/Hz] logP1.4GHz Radio power at 1.4GHz
136-141 F6.2 [W/Hz] e_logP1.4GHz ? rms uncertainty on logP1.4GHz
--------------------------------------------------------------------------------
Byte-by-byte Description of file: photom.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 10 A10 --- ID ID of each target as given in Table 1
12- 16 F5.3 --- z ?=- Redshift
17 A1 --- l_NUV [<] Upper limit flag on NUV
18- 24 E7.3 mJy NUV ?=- GALEX NUV flux NUV
26- 30 F5.1 mJy e_NUV ?=- rms uncertainty on
32- 52 E21.17 mJy Uctio ?=- CTIO-Blanco/Mosaic-II U-band flux
54- 74 E21.17 mJy e_Uctio ?=- rms uncertainty on Uctio
76- 95 E20.16 mJy Uvimos ?=- VLT/VIMOS U-band flux
97- 116 E20.16 mJy e_Uvimos ?=- rms uncertainty on Uvimos
118- 138 E21.17 mJy umegacam ?=- CFHT/MegaCam u-band flux
140- 160 E21.17 mJy e_umegacam ?=- rms uncertainty on umegacam
162- 174 F13.9 mJy usloan ?=- SDSS u-band flux
176- 187 E12.6 mJy e_usloan ?=- rms uncertainty on usloan
189- 201 F13.9 mJy gsloan ?=- SDSS g-band flux
203- 214 E12.6 mJy e_gsloan ?=- rms uncertainty on gsloan
216- 228 F13.9 mJy rsloan ?=- SDSS r-band flux
230- 241 E12.6 mJy e_rsloan ?=- rms uncertainty on rsloan
243- 255 F13.9 mJy isloan ?=- SDSS i-band flux
257- 268 E12.6 mJy e_isloan ?=- rms uncertainty on isloan
270- 282 F13.9 mJy zsloan ?=- SDSS z-band flux
284- 297 F14.10 mJy e_zsloan ?=- rms uncertainty on zsloan
299- 319 E21.17 mJy Bsubaru ?=- Subaru/Suprime-Cam B flux
321- 341 E21.17 mJy e_Bsubaru ?=- rms uncertainty on Bsubaru
343- 363 E21.17 mJy Vsubaru ?=- Subaru/Suprime-Cam V-band flux
365- 385 E21.17 mJy e_Vsubaru ?=- rms uncertainty on Vsubaru
387- 407 E21.17 mJy rsubaru ?=- Subaru/Suprime-Cam r-band flux
409- 429 E21.17 mJy e_rsubaru ?=- rms uncertainty on rsubaru
431- 451 E21.17 mJy isubaru ?=- Subaru/Suprime-Cam i-band flux
453- 473 E21.17 mJy e_isubaru ?=- rms uncertainty on isubaru
475- 495 E21.17 mJy zsubaru ?=- Subaru/Suprime-Cam z-band flux
497- 517 E21.17 mJy e_zsubaru ?=- rms uncertainty on zsubaru
519- 538 E20.16 mJy WFIU ?=- ESO-MPG/WFI U-band flux
540- 560 E21.17 mJy e_WFIU ?=- rms uncertainty on WFIU
562- 581 E20.16 mJy WFIU38 ?=- ESO-MPG/WFI U38-band flux
583- 602 E20.16 mJy e_WFIU38 ?=- rms uncertainty on WFIU38
604- 624 E21.17 mJy WFIB ?=- ESO-MPG/WFI B-band flux
626- 646 E21.17 mJy e_WFIB ?=- rms uncertainty on WFIB
648- 668 E21.17 mJy WFIV ?=- ESO-MPG/WFI V-band flux
670- 690 E21.17 mJy e_WFIV ?=- rms uncertainty on WFIV
692- 712 E21.17 mJy WFIR ?=- ESO-MPG/WFI R-band flux
714- 734 E21.17 mJy e_WFIR ?=- rms uncertainty on WFIR
736- 756 E21.17 mJy WFII ?=- ESO-MPG/WFI I-band flux
758- 777 E20.16 mJy e_WFII ?=- rms uncertainty on WFII
779- 799 E21.17 mJy acsf435w ?=- HST/ACS F435W-band flux
801- 821 E21.17 mJy e_acsf435w ?=- rms uncertainty on acsf435w
823- 843 E21.17 mJy acsf606w ?=- HST/ACS F606W-band flux
845- 865 E21.17 mJy e_acsf606w ?=- rms uncertainty on acsf606w
867- 886 E20.16 mJy acsf775w ?=- HST/ACS F775W-band flux
888- 908 E21.17 mJy e_acsf775w ?=- rms uncertainty on acsf775w
910- 930 E21.17 mJy acsf814w ?=- HST/ACS F814W-band flux
932- 952 E21.17 mJy e_acsf814w ?=- rms uncertainty on acsf814w
954- 973 E20.19 mJy acsf850lp ?=- HST/ACS F850LP-band flux
975- 995 E21.17 mJy e_acsf850lp ?=- rms uncertainty on acsf850lp
997-1016 E20.19 mJy wfc3098M ?=- HST/WFC3 F098M-band flux
1018-1038 E21.17 mJy e_wfc3098M ?=- rms uncertainty on wfc3098M
1040-1059 E20.16 mJy wfc3Y105W ?=- HST/WFC3 Y105W-band flux
1061-1081 E21.17 mJy e_wfc3Y105W ?=- rms uncertainty on wfc3Y105W
1083-1105 F23.19 mJy wfc3J125W ?=- HST/WFC3 J125W-band flux
1107-1127 E21.17 mJy e_wfc3J125W ?=- rms uncertainty on wfc3J125W
1129-1151 F23.19 mJy wfc3H160W ?=- HST/WFC3 H160W-band flux
1153-1173 E21.17 mJy e_wfc3H160W ?=- rms uncertainty on wfc3H160W
1175-1183 F9.5 mJy ucfhtl ?=- CFHT u-band flux
1185-1191 E7.2 mJy e_ucfhtl ?=- rms uncertainty on ucfhtl
1193-1201 F9.5 mJy gcfhtl ?=- CFHT g-band flux
1203-1209 E7.2 mJy e_gcfhtl ?=- rms uncertainty on gcfhtl
1211-1219 F9.5 mJy rcfhtl ?=- CFHT r-band flux
1221-1227 E7.2 mJy e_rcfhtl ?=- rms uncertainty on rcfhtl
1229-1235 F7.3 mJy icfhtlold ?=- Old CFHT i-band flux
1237-1243 E7.2 mJy e_icfhtlold ?=- rms uncertainty on icfhtlold
1245-1253 F9.5 mJy icfhtlnew ?=- New CFHT i-band flux
1255-1261 E7.2 mJy e_icfhtlnew ?=- rms uncertainty on icfhtlnew
1263-1271 F9.5 mJy zcfhtl ?=- CFHT z-band flux
1273-1279 E7.2 mJy e_zcfhtl ?=- rms uncertainty on zcfhtl
1281-1303 F23.19 mJy Jctio ?=- CTIO-Blanco/ISPI J-band flux
1305-1325 E21.17 mJy e_Jctio ?=- rms uncertainty on Jctio
1327-1348 F22.18 mJy Ksctio ?=- CTIO-Blanco/ISPI Ks-band flux
1350-1370 E21.17 mJy e_Ksctio ?=- rms uncertainty on Ksctio
1372-1392 E21.17 mJy zctio ?=- CTIO-Blanco/Mosaic-II z-band flux
1394-1414 E21.17 mJy e_zctio ?=- rms uncertainty on zctio
1416-1424 F9.5 mJy VISTAZ ?=- VISTA Z-band flux
1426-1432 E7.2 mJy e_VISTAZ ?=- rms uncertainty on VISTAZ
1434-1442 F9.5 mJy VISTAY ?=- VISTA Y-band flux
1444-1450 E7.2 mJy e_VISTAY ?=- rms uncertainty on VISTAY
1452-1464 F13.9 mJy VISTAJ ?=- VISTA J-band flux
1466-1477 E12.7 mJy e_VISTAJ ?=- rms uncertainty on VISTAJ
1479-1491 F13.9 mJy VISTAH ?=- VISTA H-band flux
1493-1504 E12.7 mJy e_VISTAH ?=- rms uncertainty on VISTAH
1506-1518 F13.9 mJy VISTAKs ?=- VISTA Ks-band flux
1520-1531 E12.7 mJy e_VISTAKs ?=- rms uncertainty on VISTAKs
1533-1554 F22.18 mJy Jukidss ?=- UKIDSS J-band flux
1556-1578 F23.19 mJy e_Jukidss ?=- rms uncertainty on Jukidss
1580-1601 F22.18 mJy Hukidss ?=- UKIDSS H-band flux
1603-1625 F23.19 mJy e_Hukidss ?=- rms uncertainty on Hukidss
1627-1648 F22.18 mJy Kukidss ?=- UKIDSS K-band flux
1650-1672 F23.19 mJy e_Kukidss ?=- rms uncertainty on Kukidss
1674-1696 F23.19 mJy Hsofi ?=- NTT/SofI H-band flux
1698-1718 E21.17 mJy e_Hsofi ?=- rms uncertainty on Hsofi
1720-1741 F22.18 mJy isaacKs ?=- VLT/ISAAC Ks-band flux
1743-1762 E20.16 mJy e_isaacKs ?=- rms uncertainty on isaacKs
1764-1786 F23.19 mJy HAWKIKs ?=- VLT/HAWK-I Ks-band
1788-1808 E21.17 mJy e_HAWKIKs ?=- rms uncertainty on HAWKIKs
1810-1830 E21.17 mJy Yuv ?=- VISTA/VIRCAM Y-band flux
1832-1852 E21.17 mJy e_Yuv ?=- rms uncertainty on Yuv
1854-1876 F23.19 mJy Juv ?=- VISTA/VIRCAM J-band flux
1878-1898 E21.17 mJy e_Juv ?=- rms uncertainty on Juv
1900-1922 F23.19 mJy Huv ?=- VISTA/VIRCAM H-band flux
1924-1944 E21.17 mJy e_Huv ?=- rms uncertainty on Huv
1946-1967 F22.18 mJy Kuv ?=- VISTA/VIRCAM K-band flux
1969-1989 E21.17 mJy e_Kuv ?=- rms uncertainty on Kuv
1991-2011 E21.17 mJy Yhsc ?=- Subaru/HSC Y-band flux
2013-2033 E21.17 mJy e_Yhsc ?=- rms uncertainty on Yhsc
2035-2057 F23.19 mJy Hw ?=- CFHT/WIRCam H-band flux
2059-2079 E21.17 mJy e_Hw ?=- rms uncertainty on Hw
2081-2103 F23.19 mJy Kw ?=- CFHT/WIRCam K-band flux
2105-2125 E21.17 mJy e_Kw ?=- rms uncertainty on Kw
2127-2146 F20.16 mJy J2mass ?=- 2MASS J-band flux
2148-2169 F22.18 mJy e_J2mass ?=- rms uncertainty on J2mass
2171-2190 F20.16 mJy H2mass ?=- 2MASS H-band flux
2192-2212 F21.17 mJy e_H2mass ?=- rms uncertainty on H2mass
2214-2233 F20.16 mJy Ks2mass ?=- 2MASS Ks-band flux
2235-2255 F21.17 mJy e_Ks2mass ?=- rms uncertainty on Ks2mass
2257-2269 F13.9 mJy iracch1 ?=- Spitzer/IRAC channel 1 (3.6um)flux
2271-2282 E12.7 mJy e_iracch1 ?=- rms uncertainty on iracch1
2284-2296 F13.9 mJy iracch2 ?=- Spitzer/IRAC channel 2 (4.5um) flux
2298-2309 E12.11 mJy e_iracch2 ?=- rms uncertainty on iracch2
2311-2319 F9.5 mJy iracch3 ?=- Spitzer/IRAC channel 3 (5.8um) flux
2321-2327 E7.2 mJy e_iracch3 ?=- rms uncertainty on iracch3
2328 A1 --- l_iracch4 [<] Upper limit flag on iracch4
2329-2337 F9.5 mJy iracch4 ?=- Spitzer/IRAC channel 4 (8um) flux
2339-2345 E7.2 mJy e_iracch4 ?=- rms uncertainty on iracch4
2347-2359 F13.9 mJy W1 ?=- WISE W1-band (3.4um) flux
2361-2374 F14.10 mJy e_W1 ?=- rms uncertainty on W1
2375 A1 --- l_W2 [<] Upper limit flag on W2
2376-2388 F13.9 mJy W2 ?=- WISE W2-band (4.6um) flux W2
2390-2402 F13.9 mJy e_W2 ?=- rms uncertainty on
2403 A1 --- l_W3 [<] Upper limit flag on W3
2404-2415 F12.8 mJy W3 ?=- WISE W3-band (12um) flux W3
2417-2425 F9.4 mJy e_W3 ?=- rms uncertainty on
2426 A1 --- l_W4 [<] Upper limit flag on W4
2427-2437 F11.7 mJy W4 ?=- WISE W4-band (22um) flux W4
2439-2445 F7.3 mJy e_W4 ?=- rms uncertainty on
2446 A1 --- l_mips24 [<] Upper limit flag on mips24
2447-2453 F7.3 mJy mips24 ?=- Spitzer/MIPS 24um flux
2455-2463 F9.5 mJy e_mips24 ?=- rms uncertainty on mips24
2465-2484 F20.16 mJy pacs70 ?=- Herschel/PACS 70um flux
2486-2506 F21.17 mJy e_pacs70 ?=- rms uncertainty on pacs70
2507 A1 --- l_pacs100 [<] Upper limit flag on pacs100
2508-2514 F7.2 mJy pacs100 ?=- Herschel/PACS 100um flux
2516-2522 F7.3 mJy e_pacs100 ?=- rms uncertainty on pacs100
2523 A1 --- l_pacs160 [<] Upper limit flag on pacs160
2524-2530 F7.2 mJy pacs160 ?=- Herschel/PACS 160um flux
2532-2538 F7.3 mJy e_pacs160 ?=- rms uncertainty on pacs160
2539 A1 --- l_spire250 [<] Upper limit flag on spire250
2540-2546 F7.2 mJy spire250 ?=- Herschel/SPIRE 250um flux
2548-2554 F7.3 mJy e_spire250 ?=- rms uncertainty on spire250
2555 A1 --- l_spire350 [<] Upper limit flag on spire350
2556-2562 F7.2 mJy spire350 ?=- Herschel/SPIRE 350um flux
2564-2570 F7.2 mJy e_spire350 ?=- rms uncertainty on spire350
2571 A1 --- l_spire500 [<] Upper limit flag on spire500
2572-2578 F7.2 mJy spire500 ?=- Herschel/SPIRE 500um flux
2580-2586 F7.2 mJy e_spire500 ?=- rms uncertainty on spire500
2587 A1 --- l_ALMAband7 [<] Upper limit flag on ALMAband7
2588-2609 F22.18 mJy ALMAband7 ?=- ALMA Band 7 (275-373GHz) flux
2611-2631 F21.17 mJy e_ALMAband7 ?=- rms uncertainty on ALMAband7
2632 A1 --- l_ALMAband3 [<] Upper limit flag on ALMAband3
2633-2652 F20.16 mJy ALMAband3 ?=- ALMA Band 3 (84-116GHz) flux
2654-2658 F5.1 mJy e_ALMAband3 ?=- rms uncertainty on ALMAband3
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Acknowledgements:
Chiara Circosta, ccircost(at)eso.org
(End) Patricia Vannier [CDS] 13-Sep-2018