J/ApJS/261/4 BASS. XXIV. DR2 spectral line measurements of AGNs (Oh+, 2022)
BASS. XXIV. The BASS DR2 spectroscopic line measurements and AGN demographics.
Oh K., Koss M.J., Ueda Y., Stern D., Ricci C., Trakhtenbrot B., Powell M.C.,
den Brok J.S., Lamperti I., Mushotzky R., Ricci F., Bar R.E., Rojas A.F.,
Ichikawa K., Riffel R., Treister E., Harrison F., Urry C.M., Bauer F.E.,
Schawinski K.
<Astrophys. J. Suppl. Ser., 261, 4 (2022)>
=2022ApJS..261....4O 2022ApJS..261....4O
ADC_Keywords: Active gal. nuclei; Spectra, optical; Galaxies, Seyfert; QSOs
Keywords: Supermassive black holes ; Active galactic nuclei ;
X-ray active galactic nuclei ; AGN host galaxies ; Quasars
Abstract:
We present the second catalog and data release of optical spectral
line measurements and active galactic nucleus (AGN) demographics of
the BAT AGN Spectroscopic Survey, which focuses on the Swift-BAT hard
X-ray detected AGNs. We use spectra from dedicated campaigns and
publicly available archives to investigate spectral properties of most
of the AGNs listed in the 70 month Swift-BAT all-sky catalog;
specifically, 743 of the 746 unbeamed and unlensed AGNs (99.6%). We
find a good correspondence between the optical emission line widths
and the hydrogen column density distributions using the X-ray spectra,
with a clear dichotomy of AGN types for NH=1022cm-2. Based on
optical emission-line diagnostics, we show that 48%-75% of BAT AGNs
are classified as Seyfert, depending on the choice of emission lines
used in the diagnostics. The fraction of objects with upper limits on
line emission varies from 6% to 20%. Roughly 4% of the BAT AGNs have
lines too weak to be placed on the most commonly used diagnostic
diagram, [OIII]λ5007/Hβ versus [NII]λ6584/Hα,
despite the high signal-to-noise ratio of their spectra. This value
increases to 35% in the [OIII]λ5007/[OII]λ3727 diagram,
owing to difficulties in line detection. Compared to optically
selected narrow-line AGNs in the Sloan Digital Sky Survey, the BAT
narrow-line AGNs have a higher rate of reddening/extinction, with
Hα/Hβ>5 (∼36%), indicating that hard X-ray selection more
effectively detects obscured AGNs from the underlying AGN population.
Finally, we present a subpopulation of AGNs that feature complex broad
lines (34%, 250/743) or double-peaked narrow emission lines (2%,
17/743).
Description:
Following BASS DR1 (Paper I.; Koss+ 2017, J/ApJ/850/74), we limit our
sample of interest to nonbeamed and nonlensed AGNs by crossmatching
the 858 BAT AGNs from BASS DR2 (Papers XXI & XXII;
Koss+ 2022ApJS..261....1K 2022ApJS..261....1K and J/ApJS/262/2) with the Roma Blazar
Catalog (BZCAT; Massaro+ 2009, J/A+A/495/691) and the follow-up work
by Paliya+ (2019, J/ApJ/881/154).
In this study, we present 743 optical spectra from the DR2 cat. (see
Koss+ 2022, J/ApJS/262/2).
The largest number of optical spectra was obtained from the
spectroscopic programs using the Palomar Double Spectrograph (DBSP),
which is attached to the Hale 200 inch telescope (N=271, 36.4% of our
AGNs). These spectra were obtained as part of a dedicated Yale program
on BAT AGN (led by C. M. Urry and M. Powell) or from observations of
NuSTAR programs (led by F. Harrison and D. Stern). Most of the
observations were performed between 2012 October and 2020 November.
Another large portion of the spectra (N=169, 22.7%) was obtained
using the X-Shooter spectrograph, mounted on the European Southern
Observatory's Very Large Telescope (ESO-VLT). The service-mode
X-Shooter observations took place between 2016 December and 2019
October, under the ESO run IDs 98.A-0635, 99.A-0403, 100.B-0672,
101.A-0765, 102.A-0433, 103.A-0521, and 104.A-0353 (led by K. Oh and
B. Trakhtenbrot). We also included available archival X-shooter spectra.
We also utilized observations (led by C. Ricci) with the Boller and
Chivens (B and C) spectrograph mounted on the 2.5m Irenee du Pont
telescope at the Las Campanas Observatory for 41 sources in 2016 March
and September.
Additionally, we used observations from the Goodman spectrograph
on the Southern Astrophysical Research (SOAR) telescope for 32 sources
between 2017 and 2020 (led by C. Ricci).
Finally, five spectra were obtained with the low-resolution imaging
spectrometer (LRIS) on the Keck telescope (led by D. Stern and
F. Harrison).
The largest number of archival optical spectra (118 sources, 15.9%;
see Figure 1) is from SDSS Data Release 15 (Aguado+ 2019ApJS..240...23A 2019ApJS..240...23A).
The second largest portion of the spectra (N=36, 4.8%) is drawn from
the 6dF Galaxy Survey (6dFGS; Jones et al. 2009, VII/259).
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table2.dat 127 743 Optical spectra
table4.dat 89 743 Emission line classification
table5.dat 168 17 Double-peaked narrow emission-line BAT AGNs
table6.dat 114 155 Wing components
table7.dat 178 743 Emission-line Measurements from HeIIλ3203
to Hγλ4340
table8.dat 207 743 Emission-line Measurements -
from [OIII]λ4363 to HeIλ5875
table9.dat 178 743 Emission-line Measurements -
from [OI]λ6300 to [OII]λ7330
table10.dat 154 743 Emission-line Measurements -
from [SXII]λ7611 to Pa13λ8665
table11.dat 180 743 Emission-line measurements -
from Pa12λ8750 to [SVIII]λ9913
--------------------------------------------------------------------------------
See also:
VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009)
V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)
J/ApJS/121/473 : A diagnostic diagram for Seyfert 2 Galaxies (Bassani+, 1999)
J/A+A/378/30 : ROSAT-BSC galaxy identifications (Zimmermann+, 2001)
J/ApJ/633/L77 : SWIFT/BAT detections of AGN (Markwardt+, 2005)
J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)
J/ApJ/681/113 : Swift BAT survey of AGNs (Tueller+, 2008)
J/MNRAS/398/1165 : AGN in nearby galaxies (Goulding+, 2009)
J/A+A/495/691 : Multifreq. catalogue of blazars, Roma-BZCAT (Massaro+, 2009)
J/ApJ/705/L76 : AGNs with double-peaked [OIII] lines (Wang+, 2009)
J/ApJ/708/427 : Type 2 AGNs with double-peaked [OIII] lines (Liu+, 2010)
J/ApJS/186/378 : Hard X-ray survey from Swift-BAT 2004-2006 (Tueller+, 2010)
J/MNRAS/421/1043 : Emission-line galaxies from SDSS DR7 (Shirazi+, 2012)
J/ApJS/207/19 : Hard X-ray survey from Swift-BAT (Baumgartner+, 2013)
J/A+A/565/A117 : X-Shooter Spectral Library (XSL). DR1 (Chen+, 2014)
J/A+A/561/A67 : Spectra of 75 Swift/BAT optical counterparts (Parisi, 2014)
J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)
J/ApJS/219/1 : Catalog of Type-1 AGNs from SDSS-DR7 (Oh+, 2015)
J/ApJ/815/L13 : AGNs from the 70-month Swift/BAT cat. (Ricci+, 2015)
J/ApJ/815/129 : X-ray AGNs with Subaru/FMOS NIR observations (Suh+, 2015)
J/A+A/588/A103 : 2nd ROSAT all-sky survey (2RXS) source cat. (Boller+, 2016)
J/MNRAS/463/24 : AGNs with double-peaked narrow emission lines (Lyu+, 2016)
J/ApJ/850/74 : Swift/BAT AGN Spectroscopic Survey. I. (Koss+, 2017)
J/ApJ/836/99 : NuSTAR serendipitous survey: 40-month cat. (Lansbury+, 2017)
J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray (Ricci+, 2017)
J/ApJS/235/4 : 105-month Swift-BAT all-sky hard X-ray survey (Oh+, 2018)
J/ApJ/881/154 : BAT AGN spectroscopic survey. XVI. Blazars (Paliya+, 2019)
J/ApJS/261/2 : BASS. XXII. Swift/BAT AGN Sp. Survey DR2 cat. (Koss+, 2022)
http://swift.gsfc.nasa.gov/results/bs70mon/ : Swift-BAT 70-months
http://www.bass-survey.com/ : The BAT AGN Spectroscopic Survey home page
Byte-by-byte Description of file: table2.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- ID [1/1210] Swift-BAT 70-month hard X-ray survey
identification number (G1)
5 A1 --- m_ID [AB] Component ID on BAT number
7- 11 A5 --- --- [SWIFT]
12- 24 A13 --- SWIFT Swift/BAT position-based identifier
(JHHMM.m+DDMMA)
26- 53 A28 --- CName Counterpart source name
55- 62 F8.4 deg RAdeg Right Ascension (J2000) (1)
64- 71 F8.4 deg DEdeg [-86.64/86] Declination (J2000) (1)
73- 87 A15 --- Tel Source of optical spectrum
89- 95 F7.4 --- z[OIII] [-0.0001/0.6] Input redshift used
from [OIII]λ5007 (2)
97-106 A10 "Y/M/D" Date Date taken optical spectra
108-121 A14 s Exp Exposure time (3)
123-127 A5 --- Type ? AGN classification (4)
--------------------------------------------------------------------------------
Note (1): J2000 coordinates based on WISE positions (Koss+ 2022, J/ApJS/262/2).
Note (2): Input redshift used from [OIII]λ5007. A full list of BASS DR2
redshifts estimated from single fits to [OIII]λ5007, is provided in
(Koss+ 2022, J/ApJS/262/2).
Note (3): The notation for the case of ESO-VLT (X-Shooter) indicates
UVB/VIS/NIR.
Note (4): AGN classification following Winkler (1992MNRAS.257..677W 1992MNRAS.257..677W)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table4.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- ID [1/1210] Swift-BAT 70-month hard X-ray
survey identification number (G1)
5 A1 --- m_ID [AB] Component ID on BAT number
7- 34 A28 --- CName Counterpart source name
36- 45 A10 --- [NII]/Ha The [NII]λ6584/Hα diagnostic
classification (5)
47- 56 A10 --- [SII]/Ha The [SII]λ6717,
λ6731/Hα diagnostic
classification (5)
58- 67 A10 --- [OI]/Ha The [OI]λ6300/Hα diagnostic
classification (5)
69- 78 A10 --- HeII The HeIIλ4686 diagnostic
classification (5)
80- 89 A10 --- [OIII]/[OII] The [OIII]λ5007/[OII]λ3727
diagnostic classification (5)
--------------------------------------------------------------------------------
Note (5): Classification includes:
Weak lines = objects lacking sufficiently strong emission-line strengths
with A/N<3 to be placed on the diagnostic diagrams;
AGN Limit = objects classified as either Seyfert or LINER having a
3σ upper limit in the used emission lines.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table5.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- ID [37/1186] Swift-BAT 70-month hard
X-ray survey ID (G1)
6- 8 I3 km/s dV [114/347] Average velocity
offset (1)
10- 14 F5.2 0.1nm lambda-Hb-b [-6/0]? Emission line center,
Hβ, Angstroms, blue component
16- 20 F5.2 0.1nm lambda-Hb-r [-0.6/5]? Emission line center,
Hβ, Angstroms, red component
22 A1 --- l_Flux-Hb-b Limit flag on Flux-Hb-b
24- 29 F6.1 10-17mW/m2 Flux-Hb-b [19/1126]? Emission line flux,
H{beta, rblueed component}, 10-17
erg/s/cm2
31- 34 F4.1 10-17mW/m2 e_Flux-Hb-b [3/34]? Uncertainty in Flux-Hb-b
36 A1 --- l_Flux-Hb-r Limit flag on Flux-Hb-r
38- 42 F5.1 10-17mW/m2 Flux-Hb-r [19/858]? Emission line flux,
Hβ, red component, 10-17
erg/s/cm2
44- 47 F4.1 10-17mW/m2 e_Flux-Hb-r [4/36]? Uncertainty in Flux-Hb-r
49- 53 F5.2 0.1nm lambda-OIII-b [-6/0.5]? Emission line center,
Hβ, Angstroms, blue component
55- 59 F5.2 0.1nm lambda-OIII-r [-0.6/3.8]? Emission line center,
Hβ, Angstroms, red component
61- 66 F6.1 10-17mW/m2 Flux-OIII-b [169/6922]? Emission line flux,
[OIII], blue component, 10-17
erg/s/cm2
68- 72 F5.1 10-17mW/m2 e_Flux-OIII-b [9/241]? Uncertainty in Flux-OIII-b
74- 79 F6.1 10-17mW/m2 Flux-OIII-r [208/3319]? Emission line flux,
[OIII], red component, 10-17
erg/s/cm2
81- 85 F5.1 10-17mW/m2 e_Flux-OIII-r [6/189]? Uncertainty in Flux-OIII-r
87- 89 I3 km/s FWHM-F [30/246]? FWHM, forbidden lines, [N
II]λ6584
91- 95 F5.2 0.1nm lambda-Ha-b [-7/1.5]? Emission line center,
Hα, Angstroms, blue component
97- 101 F5.2 0.1nm lambda-Ha-r [-0.6/5.5]? Emission line center,
Hα, Angstroms, red component
103- 108 F6.1 10-17mW/m2 Flux-Ha-b [50/5828]? Emission line flux,
Hα, blue component, 10-17
erg/s/cm2
110- 113 F4.1 10-17mW/m2 e_Flux-Ha-b [11/98]? Uncertainty in Flux-Ha-b
115- 120 F6.1 10-17mW/m2 Flux-Ha-r [85/7194]? Emission line flux,
Hα, red component, 10-17
erg/s/cm2
122- 126 F5.1 10-17mW/m2 e_Flux-Ha-r [12/283]? Uncertainty in Flux-Ha-r
128- 132 F5.2 0.1nm lambda-NII-b [-7/1.7]? Emission line center,
[NII], Angstroms, blue component
134- 138 F5.2 0.1nm lambda-NII-r [-0.6/5]? Emission line center,
[NII], Angstroms, red component
140- 145 F6.1 10-17mW/m2 Flux-NII-b [63/4979]? Emission line flux,
[NII], blue component, 10-17
erg/s/cm2
147- 151 F5.1 10-17mW/m2 e_Flux-NII-b [8/126]? Uncertainty in Flux-NII-b
153- 158 F6.1 10-17mW/m2 Flux-NII-r [65/3752]? Emission line flux,
[NII], red component, 10-17
erg/s/cm2
160- 164 F5.1 10-17mW/m2 e_Flux-NII-r [8/111]? Uncertainty in Flux-NII-r
166- 168 I3 km/s FWHM-B [37/282]? FWHM, Balmer lines
measured from Hα
--------------------------------------------------------------------------------
Note (1): Average velocity offset in units of km/s between double-peaked narrow
emission-lines measured from [NII]λ6584 and Hα.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table6.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- ID [1/1203] Swift-BAT 70-month hard X-ray
survey identification number (G1)
5 A1 --- m_ID [AB] Component ID on BAT number
7- 12 F6.1 0.1nm lambda-Hb [4855.4/4874.7]? Emission line
center, Hβ Angstroms
14- 16 I3 km/s FWHM-Hb [94/864]? Full width at half max,
km/s, Hβ
18 A1 --- l_Flux-Hb Limit flag on Flux-Hb
20- 26 F7.1 10-17mW/m2 Flux-Hb [43.1/45604.1]? Emission line flux,
Hβ, 10-17 erg/s/cm2
28- 31 F4.1 10-17mW/m2 e_Flux-Hb [0.2/50.2]? Uncertainty in Flux-Hb
33- 38 F6.1 0.1nm lambda-OIII [4994.7/5021.8]? Emission line
center, [OIII] Angstroms
40- 43 I4 km/s FWHM-OIII [94/1696]? Full width at half max,
km/s, [OIII]
45 A1 --- l_Flux-OIII Limit flag on Flux-OIII
47- 54 F8.1 10-17mW/m2 Flux-OIII [31.9/438096]? Emission line flux,
[OIII], 10-17 erg/s/cm2
56- 60 F5.1 10-17mW/m2 e_Flux-OIII [0/736]? Uncertainty in Flux-OIII
62- 67 F6.1 0.1nm lambda-Ha [6556.3/6573.7]? Emission line
center, Hα Angstroms
69- 72 I4 km/s FWHM-Ha [94/1177]? Full width at half max,
km/s, Hα
74- 81 F8.1 10-17mW/m2 Flux-Ha [210/125945]? Emission line flux,
Hα, 10-17 erg/s/cm2
83- 87 F5.1 10-17mW/m2 e_Flux-Ha [0.4/224]? Uncertainty in Flux-Ha
89- 94 F6.1 0.1nm lambda-NII [6576.8/6591.3]? Emission line
center, [NII] Angstroms
96- 98 I3 km/s FWHM-NII [117/851]? Full width at half max,
km/s, [NII]
100 A1 --- l_Flux-NII Limit flag on Flux-NII
102- 108 F7.1 10-17mW/m2 Flux-NII [39.5/87686]? Emission line flux,
[NII], 10-17 erg/s/cm2
110- 114 F5.1 10-17mW/m2 e_Flux-NII [0.2/244]? Uncertainty in Flux-NII
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table7.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- ID [1/1210] Swift-BAT 70-month hard X-ray
survey identification number (G1)
5 A1 --- m_ID [AB] Component on sequential number
7 A1 --- l_FHeII3203 Limit flag for FHeII3203, 3σ
upper limit (G2)
9- 14 F6.1 10-17mW/m2 FHeII3203 [12.6/7168]? Emission line flux,
HeIIλ3203 (G2)
16- 19 F4.1 10-17mW/m2 e_FHeII3203 [0/32]? Uncertainty for FHeII3203 (G2)
21 A1 --- l_FNeV3345 Limit flag for FNeV3345, 3σ
upper limit (G2)
23- 28 F6.1 10-17mW/m2 FNeV3345 [10.6/8794]? Emission line flux,
[NeV]λ3345 (G2)
30- 33 F4.1 10-17mW/m2 e_FNeV3345 [0/70]? Uncertainty for FNeV3345 (G2)
35 A1 --- l_FNeV3425 Limit flag for FNeV3425, 3σ
upper limit (G2)
37- 43 F7.1 10-17mW/m2 FNeV3425 [26/30623]? Emission line flux,
[NeV]λ3425 (G2)
45- 49 F5.1 10-17mW/m2 e_FNeV3425 [0/590]? Uncertainty for FNeV3425 (G2)
51 A1 --- l_FOII3727 Limit flag for FOII3727, 3σ
upper limit (G2)
53- 60 F8.1 10-17mW/m2 FOII3727 [33/101595]? Emission line flux,
[OII]λ3727 (G2)
62- 67 F6.1 10-17mW/m2 e_FOII3727 [0/6636]? Uncertainty for FOII3727 (G2)
69 A1 --- l_FNeIII3868 Limit flag for FNeIII3868, 3σ
upper limit (G2)
71- 78 F8.1 10-17mW/m2 FNeIII3868 [19.6/104594]? Emission line flux,
[NeIII]λ3868 (G2)
80- 85 F6.1 10-17mW/m2 e_FNeIII3868 [0/2017]? Uncertainty for FNeIII3868
(G2)
87 A1 --- l_FNeIII3967 Limit flag for FNeIII3967, 3σ
upper limit (G2)
89- 95 F7.1 10-17mW/m2 FNeIII3967 [7.5/32397]? Emission line flux,
[NeIII]λ3967 (G2)
97- 102 F6.1 10-17mW/m2 e_FNeIII3967 [0/2242]? Uncertainty for FNeIII3967
(G2)
104 A1 --- l_FHz Limit flag for FHz, 3σ upper
limit (G2)
106- 112 F7.1 10-17mW/m2 FHz [3.9/18723]? Emission line flux,
Hζλ3889 (G2)
114- 117 F4.1 10-17mW/m2 e_FHz [0/13]? Uncertainty for FHz (G2)
119 A1 --- l_FHeps Limit flag for FHeps, 3σ upper
limit (G2)
121- 127 F7.1 10-17mW/m2 FHeps [6.5/21609]? Emission line flux,
Hελ3970 (G2)
129- 132 F4.1 10-17mW/m2 e_FHeps [0/19]? Uncertainty for FHeps (G2)
134 A1 --- l_FHd Limit flag for FHd, 3σ upper
limit (G2)
136- 142 F7.1 10-17mW/m2 FHd [5.6/19747]? Emission line flux,
Hδλ4101 (G2)
144- 149 F6.1 10-17mW/m2 e_FHd [0/31]? Uncertainty for FHd (G2)
151 A1 --- l_FHg Limit flag for FHg, 3σ upper
limit (G2)
153- 160 F8.1 10-17mW/m2 FHg [4/147007]? Emission line flux,
Hγλ4340 (G2)
162- 168 F7.1 10-17mW/m2 e_FHg [0/1375]? Uncertainty for FHg (G2)
170- 173 I4 km/s FWHM-N2 [22/4968]? FWHM, forbidden lines,
[NII]λ6584 (G2)
175- 176 I2 km/s e_FWHM-N2 [0/42]? Uncertainty in FWHM-N2 (G2)
178 A1 --- Flag7 Flag for emission line measurements
from HeIIλ3203 to
Hγλ4340 (G3)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table8.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- ID [1/1210] Swift-BAT 70-month hard X-ray
survey ID (G1)
5 A1 --- m_ID [AB] Component on sequential number
7 A1 --- l_FOIII4363 Limit flag for FOIII4363, 3σ
upper limit (G2)
9- 16 F8.1 10-17mW/m2 FOIII4363 [0/187391]? Emission line flux,
[OIII]λ4363 (G2)
18- 22 F5.1 10-17mW/m2 e_FOIII4363 [0/287]? Uncertainty for FOIII4363 (G2)
24 A1 --- l_FHeII4685 Limit flag for FHeII4685, 3σ
upper limit (G2)
26- 33 F8.1 10-17mW/m2 FHeII4685 [9.6/436892]? Emission line flux,
HeIIλ4685 (G2)
35- 40 F6.1 10-17mW/m2 e_FHeII4685 [0/1082]? Uncertainty for FHeII4685 (G2)
42 A1 --- l_FArIV4711 Limit flag for FArIV4711, 3σ
upper limit (G2)
44- 51 F8.1 10-17mW/m2 FArIV4711 [5.3/202343]? Emission line flux,
[ArIV]λ4711 (G2)
53- 57 F5.1 10-17mW/m2 e_FArIV4711 [0/605]? Uncertainty for FArIV4711 (G2)
59 A1 --- l_FArIV4740 Limit flag for FArIV4740, 3σ
upper limit (G2)
61- 67 F7.1 10-17mW/m2 FArIV4740 [6.3/39998]? Emission line flux,
[ArIV]λ4740 (G2)
69- 73 F5.1 10-17mW/m2 e_FArIV4740 [0/561]? Uncertainty for FArIV4740 (G2)
75 A1 --- l_FHb Limit flag for FHb, 3σ upper
limit (G2)
77- 84 F8.1 10-17mW/m2 FHb [7/980571]? Emission line flux,
Hβλ4861 (G2)
86- 92 F7.1 10-17mW/m2 e_FHb [0/2933]? Uncertainty for FHb (G2)
94 A1 --- l_FOIII4958 Limit flag for FOIII4958, 3σ
upper limit (G2)
96- 104 F9.1 10-17mW/m2 FOIII4958 [15.8/1401943]? Emission line flux,
[OIII]λ4958 (G2)
106- 112 F7.1 10-17mW/m2 e_FOIII4958 [0/5497]? Uncertainty for FOIII4958 (G2)
114 A1 --- l_FOIII5007 Limit flag for FOIII5007, 3σ
upper limit (G2)
116- 124 F9.1 10-17mW/m2 FOIII5007 [27.7/4005550]? Emission line flux,
[OIII]λ5007 (G2)
126- 132 F7.1 10-17mW/m2 e_FOIII5007 [0/15704]? Uncertainty for FOIII5007
(G2)
134 A1 --- l_FNI5197 Limit flag for FNI5197, 3σ upper
limit (G2)
136- 143 F8.1 10-17mW/m2 FNI5197 [5.8/223242]? Emission line flux,
[NI]λ5197 (G2)
145- 149 F5.1 10-17mW/m2 e_FNI5197 [0/487]? Uncertainty for FNI5197 (G2)
151 A1 --- l_FNI5200 Limit flag for FNI5200, 3σ upper
limit (G2)
153- 159 F7.1 10-17mW/m2 FNI5200 [6.6/12041]? Emission line flux,
[NIλ5200 (G2)
161- 167 F7.1 10-17mW/m2 e_FNI5200 [0/20929]? Uncertainty for FNI5200 (G2)
169 A1 --- l_FHeI5875 Limit flag for FHeI5875, 3σ upper
limit (G2)
171- 178 F8.1 10-17mW/m2 FHeI5875 [11.6/146759]? Emission line flux,
HeIλ5875 (G2)
180- 186 F7.1 10-17mW/m2 e_FHeI5875 [0/59423]? Uncertainty for FHeI5875 (G2)
188- 191 I4 km/s FWHMHa [16/1292]? FWHM, Balmer lines measured
from Hα (G2)
193- 194 I2 km/s e_FWHMHa [0/35]? Uncertainty in FWHMHa (G2)
196 A1 --- Flag8 Flag for emission line measurements from
[OIII]λ4363 to
HeIλ5875 (G3)
198- 201 F4.2 --- Corr [1/7.8]? Correction factor (1)
203- 207 F5.2 --- Ha/Hb [2.8/32.5]? Ratio, Hα/Hβ
emission line flux
--------------------------------------------------------------------------------
Note (1): Correction factor, where [OIII]intr.=C*[OIII]obs. We use the
Cardelli et al. (1989ApJ...345..245C 1989ApJ...345..245C) reddening curve assuming an
intrinsic ratio of RV=3.1 to correct for dust extinction.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table9.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- ID [1/1210] Swift-BAT 70-month hard X-ray
survey ID (G1)
5 A1 --- m_ID [AB] Component on sequential number
7 A1 --- l_FOI6300 Limit flag for FOI6300, 3σ upper
limit (G2)
9- 15 F7.1 10-17mW/m2 FOI6300 [13.8/57614]? Emission line flux,
[OI]λ6300 (G2)
17- 22 F6.1 10-17mW/m2 e_FOI6300 [0/1926]? Uncertainty for FOI6300 (G2)
24 A1 --- l_FOI6363 Limit flag for FOI6363, 3σ upper
limit (G2)
26- 32 F7.1 10-17mW/m2 FOI6363 [4.7/21523]? Emission line flux,
[OI]λ6363 (G2)
34- 40 F7.1 10-17mW/m2 e_FOI6363 [0/642]? Uncertainty for FOI6363 (G2)
42 A1 --- l_FNII654 Limit flag for FNII654, 3σ upper
limit (G2)
44- 51 F8.1 10-17mW/m2 FNII654 [17.5/197348]? Emission line flux,
[NII]λ6548 (G2)
53- 59 F7.1 10-17mW/m2 e_FNII654 [0/1797]? Uncertainty for FNII654 (G2)
61 A1 --- l_FHa Limit flag for FHa, 3σ upper
limit (G2)
63- 71 F9.1 10-17mW/m2 FHa [14.4/2801632]? Emission line flux,
Hαλ6562 (G2)
73- 79 F7.1 10-17mW/m2 e_FHa [0/8380]? Uncertainty for FHa (G2)
81 A1 --- l_FNII6583 Limit flag for FNII6583, 3σ
upper limit (G2)
83- 90 F8.1 10-17mW/m2 FNII6583 [29.4/414516]? Emission line flux,
[NII]λ6583 (G2)
92- 97 F6.1 10-17mW/m2 e_FNII6583 [0/5283]? Uncertainty for FNII6583 (G2)
99 A1 --- l_FSII6716 Limit flag for FSII6716, 3σ
upper limit (G2)
101- 107 F7.1 10-17mW/m2 FSII6716 [19.5/92443]? Emission line flux,
[SII]λ6716 (G2)
109- 113 F5.1 10-17mW/m2 e_FSII6716 [0/983]? Uncertainty for FSII6716 (G2)
115 A1 --- l_FSII6730 Limit flag for FSII6730, 3σ
upper limit (G2)
117- 123 F7.1 10-17mW/m2 FSII6730 [20.6/94253]? Emission line flux,
[SII]λ6730 (G2)
125- 130 F6.1 10-17mW/m2 e_FSII6730 [0/1328]? Uncertainty for FSII6730 (G2)
132 A1 --- l_FArIII7135 Limit flag for FArIII7135, 3σ
upper limit (G2)
134- 140 F7.1 10-17mW/m2 FArIII7135 [4.4/20080]? Emission line flux,
[ArIII]λ7135 (G2)
142- 146 F5.1 10-17mW/m2 e_FArIII7135 [0/616]? Uncertainty for
FArIII7135 (G2)
148 A1 --- l_FOII7310 Limit flag for FOII7310, 3σ
upper limit (G2)
150- 156 F7.1 10-17mW/m2 FOII7310 [6/13775]? Emission line flux,
[OII]λ7310 (G2)
158- 161 F4.1 10-17mW/m2 e_FOII7310 [0/31]? Uncertainty for FOII7310 (G2)
163 A1 --- l_FOII7330 Limit flag for FOII7330, 3σ
upper limit (G2)
165- 171 F7.1 10-17mW/m2 FOII7330 [6/11969]? Emission line flux,
[OII]λ7330 (G2)
173- 176 F4.1 10-17mW/m2 e_FOII7330 [0/21]? Uncertainty for FOII7330 (G2)
178 A1 --- Flag9 Flag for emission line measurements
from [OI]λ6300
to [OII]λ7330 (G3)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table10.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- ID [1/1210] Swift-BAT 70-month hard X-ray
survey ID (G1)
5 A1 --- m_ID [AB] Component on sequential number
7 A1 --- l_FSXII7611 Limit flag for FSXII7611, 3σ
upper limit (G2)
9- 13 F5.1 10-17mW/m2 FSXII7611 [8.7/340]? Emission line flux,
[SXII]λ7611 (G2)
15- 17 F3.1 10-17mW/m2 e_FSXII7611 [0.1/5]? Uncertainty for FSXII7611 (G2)
19 A1 --- l_FArIII7751 Limit flag for FArIII7751, 3σ
upper limit (G2)
21- 26 F6.1 10-17mW/m2 FArIII7751 [4.6/9294]? Emission line flux,
[ArIII]λ7751 (G2)
28- 31 F4.1 10-17mW/m2 e_FArIII7751 [0/15]? Uncertainty for FArIII7751 (G2)
33 A1 --- l_FHeI7816 Limit flag for FHeI7816, 3σ
upper limit (G2)
35- 39 F5.1 10-17mW/m2 FHeI7816 [6.8/410]? Emission line flux,
HeIλ7816 (G2)
41- 44 F4.1 10-17mW/m2 e_FHeI7816 [0.1/18]? Uncertainty for FHeI7816 (G2)
46 A1 --- l_FArI7868 Limit flag for FArI7868, 3σ
upper limit (G2)
48- 52 F5.1 10-17mW/m2 FArI7868 [6.4/891]? Emission line flux,
[ArI]λ7868 (G2)
54- 57 F4.1 10-17mW/m2 e_FArI7868 [0.1/24]? Uncertainty for FArI7868 (G2)
59 A1 --- l_FFeXI7891 Limit flag for FFeXI7891, 3σ
upper limit (G2)
61- 65 F5.1 10-17mW/m2 FFeXI7891 [6.1/894]? Emission line flux,
[FeXI]λ7891 (G2)
67- 70 F4.1 10-17mW/m2 e_FFeXI7891 [0/28]? Uncertainty for FFeXI7891 (G2)
72 A1 --- l_FHeII8236 Limit flag for FHeII8236, 3σ
upper limit (G2)
74- 79 F6.1 10-17mW/m2 FHeII8236 [6.7/1914]? Emission line flux,
HeIIλ8236 (G2)
81- 84 F4.1 10-17mW/m2 e_FHeII8236 [0/23]? Uncertainty for FHeII8236 (G2)
86 A1 --- l_FOI8446 Limit flag for FOI8446, 3σ upper
limit (G2)
88- 93 F6.1 10-17mW/m2 FOI8446 [6.9/9317]? Emission line flux,
[OI]λ8446 (G2)
95- 98 F4.1 10-17mW/m2 e_FOI8446 [0/22]? Uncertainty for FOI8446 (G2)
100 A1 --- l_FPa16 Limit flag for FPa16, 3σ upper
limit (G2)
102- 107 F6.1 10-17mW/m2 FPa16 [6.9/7582]? Emission line flux, Pa16
λ8502 (G2)
109- 112 F4.1 10-17mW/m2 e_FPa16 [0/22]? Uncertainty for FPa16 (G2)
114 A1 --- l_FPa15 Limit flag for FPa15, 3σ upper
limit (G2)
116- 121 F6.1 10-17mW/m2 FPa15 [10.5/5262]? Emission line flux, Pa15
λ8545 (G2)
123- 126 F4.1 10-17mW/m2 e_FPa15 [0/18]? Uncertainty for FPa15 (G2)
128 A1 --- l_FPa14 Limit flag for FPa14, 3σ upper
limit (G2)
130- 135 F6.1 10-17mW/m2 FPa14 [7/4909]? Emission line flux, Pa14
λ8598 (G2)
137- 140 F4.1 10-17mW/m2 e_FPa14 [0.1/19]? Uncertainty for FPa14 (G2)
142 A1 --- l_FPa13 Limit flag for FPa13, 3σ upper
limit (G2)
144- 149 F6.1 10-17mW/m2 FPa13 [7/3226]? Emission line flux, Pa13
λ8665 (G2)
151- 154 F4.1 10-17mW/m2 e_FPa13 [0/21]? Uncertainty for FPa13 (G2)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table11.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- ID [1/1210] Swift-BAT 70-month hard X-ray
survey identifier (G1)
5 A1 --- m_ID [AB] Component on sequential number
7 A1 --- l_FPa12 Limit flag for FPa12, 3σ upper
limit (G2)
9- 14 F6.1 10-17mW/m2 FPa12 [10.8/5291]? Emission line flux, Pa12
λ8750 (G2)
16- 19 F4.1 10-17mW/m2 e_FPa12 [0.1/11]? Uncertainty for FPa12 (G2)
21 A1 --- l_FSIII8829 Limit flag for FSIII8829, 3σ
upper limit (G2)
23- 29 F7.1 10-17mW/m2 FSIII8829 [10.9/12598]? Emission line flux,
[SIII]λ8829 (G2)
31- 34 F4.1 10-17mW/m2 e_FSIII8829 [0/17]? Uncertainty for FSIII8829 (G2)
36 A1 --- l_FPa11 Limit flag for FPa11, 3σ upper
limit (G2)
38- 44 F7.1 10-17mW/m2 FPa11 [7/16497]? Emission line flux, Pa11
λ8862 (G2)
46- 49 F4.1 10-17mW/m2 e_FPa11 [0.1/24]? Uncertainty for FPa11 (G2)
51 A1 --- l_FFeIII8891 Limit flag for FFeIII8891, 3σ
upper limit (G2)
53- 59 F7.1 10-17mW/m2 FFeIII8891 [11/17669]? Emission line flux,
[FeIII]λ8891 (G2)
61- 64 F4.1 10-17mW/m2 e_FFeIII8891 [0.1/17]? Uncertainty for FFeIII8891
(G2)
66 A1 --- l_FPa10 Limit flag for FPa10, 3σ upper
limit (G2)
68- 74 F7.1 10-17mW/m2 FPa10 [10.9/17885]? Emission line flux, Pa10
λ9014 (G2)
76- 79 F4.1 10-17mW/m2 e_FPa10 [0.1/19]? Uncertainty for FPa10 (G2)
81 A1 --- l_FSIII9068 Limit flag for FSIII9068, 3σ
upper limit (G2)
83- 89 F7.1 10-17mW/m2 FSIII9068 [23.5/38973]? Emission line flux,
[SIII]λ9068 (G2)
91- 94 F4.1 10-17mW/m2 e_FSIII9068 [0.1/58]? Uncertainty for
FSIII9068 (G2)
96 A1 --- l_FPa9 Limit flag for FPa9, 3σ upper
limit (G2)
98- 103 F6.1 10-17mW/m2 FPa9 [13.4/7513]? Emission line flux, Pa9
λ9229 (G2)
105- 108 F4.1 10-17mW/m2 e_FPa9 [0.1/43]? Uncertainty for FPa9 (G2)
110 A1 --- l_FSIII9531 Limit flag for FSIII9531, 3σ
upper limit (G2)
112- 119 F8.1 10-17mW/m2 FSIII9531 [22/103562]? Emission line flux,
[SIII]λ9531 (G2)
121- 125 F5.1 10-17mW/m2 e_FSIII9531 [0.1/131]? Uncertainty for FSIII9531
(G2)
127 A1 --- l_FPaeps Limit flag for FPaeps, 3σ upper
limit (G2)
129- 135 F7.1 10-17mW/m2 FPaeps [8.6/14104]? Emission line flux,
Paε λ9545 (G2)
137- 140 F4.1 10-17mW/m2 e_FPaeps [0.1/33]? Uncertainty for FPaeps (G2)
142 A1 -- l_FCI9824 Limit flag for FCI9824, 3σ upper
limit (G2)
144- 148 F5.1 10-17mW/m2 FCI9824 [28/261]? Emission line flux,
[CI]λ9824 (G2)
150- 153 F4.1 10-17mW/m2 e_FCI9824 [4/37]? Uncertainty for FCI9824 (G2)
155 A1 -- l_FCI9850 Limit flag for FCI9850, 3σ upper
limit (G2)
157- 161 F5.1 10-17mW/m2 FCI9850 [28/733]? Emission line flux,
[CI]λ9850 (G2)
163- 167 F5.1 10-17mW/m2 e_FCI9850 [4/112]? Uncertainty for FCI9850 (G2)
169 A1 --- l_FSVIII9913 Limit flag for FSIV9913, 3σ
upper limit (G2)
171- 175 F5.1 10-17mW/m2 FSVIII9913 [31/723]? Emission line flux,
[SVIII]λ9913 (G2)
177- 180 F4.1 10-17mW/m2 e_FSVIII9913 [4/23]? Uncertainty for FSIV9913 (G2)
--------------------------------------------------------------------------------
Global notes:
Note (G1): BAT 70-month survey catalog identifier
(http://swift.gsfc.nasa.gov/results/bs70mon/).
See also BASS DR2 (Koss+, 2022, J/ApJS/261/2)
Note (G2): Null (blank) values indicate a lack of spectral coverage,
while sources without uncertainties and have l_ flags = "<" are
3σ upper limits.
Note (G3): Flag indicating the use of broad Balmer components (Hδ,
Hγ, Hβ, and Hα) in spectral line fitting.
--------------------------------------------------------------------------------
History:
From electronic version of the journal
References:
Koss et al. Paper I. 2017ApJ...850...74K 2017ApJ...850...74K Cat. J/ApJ/850/74
Berney et al. Paper II. 2015MNRAS.454.3622B 2015MNRAS.454.3622B
Oh et al. Paper III. 2017MNRAS.464.1466O 2017MNRAS.464.1466O
Lamperti et al. Paper IV. 2017MNRAS.467..540L 2017MNRAS.467..540L Cat. J/MNRAS/467/540
Ricci et al. Paper V. 2017ApJS..233...17R 2017ApJS..233...17R Cat. J/ApJS/233/17
Trakhtenbrot et al. Paper VI. 2017MNRAS.470..800T 2017MNRAS.470..800T
Ricci et al. Paper VII. 2017Natur.549..488R 2017Natur.549..488R
Shimizu et al. Paper VIII. 2018ApJ...856..154S 2018ApJ...856..154S
Powell et al. Paper IX. 2018ApJ...858..110P 2018ApJ...858..110P
Oh et al. Paper X. 2018ApJS..235....4O 2018ApJS..235....4O Cat. J/ApJS/235/4
Ichikawa et al. Paper XI. 2019ApJ...870...31I 2019ApJ...870...31I Cat. J/ApJ/870/31
Ricci et al. Paper XII. 2018MNRAS.480.1819R 2018MNRAS.480.1819R
Bar et al. Paper XIII. 2019MNRAS.489.3073B 2019MNRAS.489.3073B
Koss et al. Paper XIV. 2018Natur.563..214K 2018Natur.563..214K
Smith et al. Paper XV. 2020MNRAS.492.4216S 2020MNRAS.492.4216S
Paliya et al. Paper XVI. 2019ApJ...881..154P 2019ApJ...881..154P Cat. J/ApJ/881/154
Baek et al. Paper XVII. 2019MNRAS.488.4317B 2019MNRAS.488.4317B
Liu et al. Paper XVIII. 2020ApJ...896..122L 2020ApJ...896..122L
Rojas et al. Paper XIX. 2020MNRAS.491.5867R 2020MNRAS.491.5867R
Koss et al. Paper XX. 2021ApJS..252...29K 2021ApJS..252...29K Cat. J/ApJS/252/29
Koss et al. Paper XXI. 2022ApJS..261....1K 2022ApJS..261....1K
Koss et al. Paper XXII. 2022ApJS..261....2K 2022ApJS..261....2K Cat. J/ApJS/261/2
Pfeifle et al. Paper XXIII. 2022ApJS..261....3P 2022ApJS..261....3P
Oh et al. Paper XXIV. 2022ApJS..261....4O 2022ApJS..261....4O This catalog
Mejia-Restrepo et al. Paper XXV. 2022ApJS..261....5M 2022ApJS..261....5M Cat. J/ApJS/261/5
Koss et al. Paper XXVI. 2022ApJS..261....6K 2022ApJS..261....6K Cat. J/ApJS/261/6
Gupta et al. Paper XXVII. 2021MNRAS.504..428G 2021MNRAS.504..428G
den Brok et al. Paper XXVIII. 2022ApJS..261....7D 2022ApJS..261....7D Cat. J/ApJS/261/7
Ricci et al. Paper XXIX. 2022ApJS..261....8R 2022ApJS..261....8R Cat. J/ApJS/261/8
Ananna et al. Paper XXX. 2022ApJS..261....9A 2022ApJS..261....9A
Kakkad et al. Paper XXXI. 2022MNRAS.511.2105K 2022MNRAS.511.2105K
Kawamuro et al. Paper XXXII. 2022ApJ...938...87K 2022ApJ...938...87K
Marcotulli et al. Paper XXXIII. 2022ApJ...940...77M 2022ApJ...940...77M Cat. J/ApJ/940/77
Kawamuro et al. Paper XXXIV. 2023ApJS..269...24K 2023ApJS..269...24K Cat. J/ApJS/269/24
Caglar et al. Paper XXXV. 2023ApJ...956...60C 2023ApJ...956...60C
Powell et al. Paper XXXVI. 2022ApJ...938...77P 2022ApJ...938...77P
Ricci et al. Paper XXXVII. 2022ApJ...938...67R 2022ApJ...938...67R
Ananna et al. Paper XXXVIII. 2022ApJ...939L..13A 2022ApJ...939L..13A
Temple et al. Paper XXXIX. 2023MNRAS.518.2938T 2023MNRAS.518.2938T
Tortosa et al. Paper XL. 2023MNRAS.526.1687T 2023MNRAS.526.1687T
Ricci et al. Paper XLII. 2023ApJ...959...27R 2023ApJ...959...27R
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 31-Aug-2022