<=== observer ===> "HSMITH",\ "Smith, Howard A.",\ "Laboratory for Astrophysics",\ "National Air and Space Museum",\ "Smithsonian Institution",\ "",\ "",\ "Washington DC 20560",\ "United States",\ "1 202 3574932",\ "1 202 6338174",\ "howard@wright.nasm.edu" <=== proposal ===> "AGN",1,4,\ {"active galactic nuclei"},\ {"LWS consortium", "Ceccarelli", "Fischer", "Greenhouse",\ "Liseau", "Lorenzetti", "Malkan", "McDowell", "McMahon", "Nisini",\ "Omont", "Puget", "Rieu", "Spinoglio"} <=== title ===> ISO Spectroscopy of Active Galactic Nuclei <=== abstract ===> SCIENTIFIC ABSTRACT We propose spectroscopic survey observations and individual line observations using LWS, SWS, and ISOPHOT designed to provide the first complete spectral characterization of AGN in the 3-200 micron region. The major goals of the program are to: a) distinguish between non-stellar engine and starburst origins of the luminosity in galactic nuclei (emission line ratios sensitive to density and excitation will identify all of the current classes of nuclear activity, discriminating between thermal and nonthermal models), b) measure the distribution and kinematics of nuclear gas and probe the dynamical geography of the nucleus via line profile shape analysis, c) study the nature and the origin of the coronal line emission region of AGN, d) measure heavy element abundances in AGN, e) determine accurately how dust obscures the intrinsic AGN spectra, f) search for the postulated hidden BLR in ``narrow-line'' AGNs, g) search for molecules in thick tori (Seyfert 2) and outer regions of accretion disks and study their kinematics at high spectral resolution, h) determine the importance of thermal and nonthermal emission for the continua of all classes of AGNs and the shape of the far infrared continuum turnover, and i) measure the detailed continuum energy distribution of AGN, with emphasis on high z QSOs for which we will address questions about the formation of heavy elements at very large z, the formation of galaxies and its relation with QSOs, the structure and the energetics of host galaxies of QSOs. OBSERVATION SUMMARY This program includes observation of roughly 50 AGN and QSOs. The majority of AGN will be spectroscopically surveyed using LWS, SWS, and ISOPHOT grating spectra; distant QSOs will use PHOT22. All of the survey spectra will cover the full wavelength range at the full resolving power afforded by the grating subsystem of each instrument. Full SWS scans on NGC 1068 and NGC 4151 are omitted to avoid duplication with the SWS team Guaranteed time proposal "Infrared Spectroscopy of Bright Galactic Nuclei and the Connection between Starformation and AGN's". Similarly, PHT spectroscopy on a number of our program objects (I Zw 1, Mkn 551, and Mkn 463) are omitted to avoid duplication with the SWS team proposal.) The SWS and PHT observation times (including SWS01, SWS02, and SWS06 AOTs) are designed to achieve a signal to noise ratio of twenty to several hundred on the continuum of each object. The lowest signal to noise occurs in SWS01 scans shortward of 7 microns. The survey AOTs utilized are LWS01, SWS01, and PHT40. Specific line observations utilize SWS02 and SWS06. In all cases, SWS01 observations will be made in full R mode, and LWS01 observations will be Nyquist sampled over 45-180 microns. Depending on the wavelength range, a signal to noise ratio of twenty to several hundred on the continuum will be obtained for each object. For most of the targets these correspond to 10-sigma detections of emission lines with fluxes of 5.0e-17 Watts/meter2 in the most sensitive wavelength regions (around 100um). In the least sensitive detector bands (at the shortest wavelengths), lines of this flux would typically be detected at only the 2-sigma level. Higher signal-to-noise ratios will be obtained for the two brightest archetypical AGNs, the Seyfert 1 NGC 4151, and the Seyfert 2 NGC 1068, allowing detection of even fainter lines in these two special cases. In addition to these survey observations, high quality line profiles will be obtained on lines listed in Table 1a and 1b below. These lines are chosen to included all ISO observable ionization states of neon. Transitions of several other intermediate mass elements are included to yield abundances and to produce a data set that spans a wide range of transition critical densities to probe AGN dynamical structure. All SWS02 observations in the program pertain to Table 1. Observations of Mkn 3, I Zw 1, NGC 3783, Mkn 573, and Mkn 463 with SWS02 will observe lines listed in Table 1b to avoid duplication with the SWS team proposal. The remainder of our SWS02 and SWS06 observations will observe lines listed in Table 1a. Observations with SWS02 or SWS06 will also be made on lines listed in Table 2 during follow up time only, and where no duplication with the SWS team observations exist. Observations made with SWS06 cover a 2000 km/s spectral baseline centered on the line. We propose to obtain high-resolution Fabry-Perot scans for the profiles of two emission lines expected to be strong in the Seyfert 2 nucleus of NGC 1068: [O I] 63um and the CO (J=57-->56) line at 46um. While this is a top sientific priority, we have listed it as priority 3 because the priority 1 grating scans should sensibly be examined first. Both will reveal the presence of high-density, but low-ionization gas--in particular the dense molecular gas that is believed to form a thick obscuring torus surrounding the central engine (eg., Krolik and Begelman 1988). This dense region is probably too optically thick to emit strong lines at much shorter wavelengths. The trade-off between high optical depth, and the frequency-cubed dependence of the Einstein A values suggests that this one CO line may carry 7% of the entire cooling budget of the torus by all CO lines, for an assumed temperature of 1000 K (Krolik and Lepp 1989). The high spectral resolution can reveal broad wings, and even double-peaked lobes which would be produced by a rapidly rotating torus or thick disk. Measuring its kinematics will be of enormous importance and can lead to a direct measure of the mass of the central engine. If the grating scans show these lines are detectable but marginal, we intend to pursue them with modest additional follow-up time. Finally, the program includes multi-filter photometry and 40- point grating spectra using PHT22 and LWS01 respectively. These observations are designed to provide detailed definition of the continuum energy distribution of AGN and QSOs: The observations of these sources will include an off-source observation for accurate continuum photometry. Background and source observations are listed separately as concatenated AOTs. For the following 9 sources: PG1613+658, PHL 909, PG1211+143, PG1351+640, Mkn 478, 3C345, 3C48, NGC 2992, 3C120, LWS01 observations are designed to define the continuum only, and will be binned to 40 discrete points across the LWS wavelength range. The LWS01 observations of all other sources in this proposal are full spectral scans. The LWS observations of the above quasars will be supplemented by multi-filter photometry using PHT22. The PHT filters utilized are: 90 100, 120, 135, 160, 180, and 200 microns; the 120 and 135 micron filters will be used to confirm the background-subtracted fluxes obtained with LWS, and the longer wavelength filters will define the slope of the far- infrared cutoff for the first time. For the high z QSOs, since the maximum emission is expected at 300-400 micron, beyond the ISO range, the priority is put on measurements at the largest wavelengths. Observations in the PHT22 mode are planned with the PHT-C200 detector at its maximum sensitivity with the 160 filter in order to detect the weakest sources with a good S/N ratio, and with the 200 filter in order to get the maximum information at the longest wavelength possible. Additional observations with the C100 detector with the 90 and 60 filters will give a complete view of the emission in the middle IR. Observations will be performed in the chopper mode, with the proper throw (90" and 45" respectively) to always keep the source in one of the pixels of the C200 or C100 arrays. A S/N ratio ~10 at least is requested with the 160 and 90 filters for "weak" sources (expected fluxes S_160 ~ 25mJy, S_100 ~ 15 mJy) with a background emission (cirrus + background galaxies) twice the average one estimated from Gautier et al. 1992 (A.J. 103, 1313). Such requirements should be achieved with integration times of 256 and 128 sec. with C_200+F_160 and C_100+F_90 respectively. Equal integration times with C_200+F_200 and C_100+F_60 respectively should give a good probability of detection for every source at 200 and 60 micron (expected fluxes for "weak" sources S_200 ~ 25 mJy and S_60 ~ 10 mJy). Additional details can be found in the LWS Elmau Document: "ISO:LWS Guaranteed Time Proposals", LWS/90/P/SCI/135.00, November 1990. <=== scientific_justification ===> Tables: Table 1a => [Ne II]12.81, [Ne III]15.55, [Ne III]36.02, [Ne V]14.32, [Ne V]24.28, [Ne VI]7.64, [Al VI]9.12, [Mg V]13.54, [Mg VII]9.03, [Ca V]11.48, [Ca VI]24.30 [O IV]25.91, [S III]18.71 Table 1b => [Ne II]12.81, [Ne III]15.55, [Ne III]36.02, [Ne V]24.28, [Ne VI]7.64, [Al VI]9.12, [Mg V]13.54, [Mg VII]9.03, [Ca V]11.48, [Ca VI]24.30 Table 2 => [Ne II]12.81 [Al V]2.88 [Mg IV]4.49 [Ca IV]3.18 [Si VII]2.47 [Ne III]15.55 [Al VI]3.66 [Mg V]5.60 [Ca V]4.16 [Si VII]6.52 [Ne III]36.02 [Al VI]9.12 [Mg V]13.54 [Ca V]11.48 [Si IX]2.58 [Ne V]14.32 [Al VIII]2.72 [Mg VII]5.50 [Ca VI]24.30 [Si IX]3.92 [Ne V]24.28 [Al VIII]5.85 [Mg VII]9.03 [Ca VII]4.09 [Ne VI]7.64 [Al X]2.75 [Mg VIII]3.03 [Ca VII]6.15 [Ca IX]3.09 Time distribution for August launch: Team top 40% second 30% last 30% LWS: 83189 64701 58289 JLP: 5207 2025 total: 88396 66726 58289 Time distribution for Spring launch: Team top 40% second 30% last 30% LWS: 80748 49598 72226 JLP: 5207 2025 total: 85955 51623 72226 <=== autumn_launch_targets ===> 01, "LWS01", 1.,"N", "NGC 1068 ", 2.66863, -0.22542, 1950,0.,0., 5824, 0 02, "LWS01", 1.,"N", "NGC 4151 ", 12.13363, 39.68383, 1950,0.,0., 5824, 0 03, "LWS01", 1.,"N", "I Zw 92 ", 14.65071, 53.71778, 1950,0.,0., 3206, 0 04, "SWS01", 1.,"N", "I Zw 92 ", 14.65071, 53.71778, 1950,0.,0., 6498, 0 05, "SWS02", 1.,"N", "I Zw 92 ", 14.65071, 53.71778, 1950,0.,0., 4400, 0 06, "PHT40", 1.,"N", "I Zw 92 ", 14.65071, 53.71778, 1950,0.,0., 1800, 0 07, "PHT22", 1.,"N", "3C273 ", 12.44257, 2.32875, 1950,0.,0., 1133, 0 08, "LWS01", 1.,"N", "3C273 ", 12.44257, 2.32875, 1950,0.,0., 1736, 9 09, "LWS01", 1.,"N", "3C273 off ", 12.44257, 2.36875, 1950,0.,0., 1736, 0 10, "PHT22", 1.,"N", "HB89 1821+643", 18.36164, 64.31694, 1950,0.,0., 1133, 0 11, "LWS01", 1.,"N", "HB89 1821+643", 18.36164, 64.31694, 1950,0.,0., 1736, 12 12, "LWS01", 1.,"N", "HB89 1821+643", 18.36164, 64.35694, 1950,0.,0., 1736, 0 13, "PHT22", 1.,"N", "1335-04 ", 13.59100, -04.28916, 1950, 0, 0, 1157, 0 14, "PHT22", 1.,"N", "1114-08 ", 11.24866, -08.37611, 1950,0.,0., 1157, 0 15, "PHT22", 1.,"N", "1158+46 ", 11.96747, +46.59138, 1950,0.,0., 1157, 0 16, "PHT22", 1.,"N", "1202-07 ", 12.04700, -07.43055, 1950,0.,0., 1157, 0 17, "PHT22", 1.,"N", "1247+34 ", 12.78827, +34.10333, 1950,0.,0., 1157, 0 18, "PHT22", 1.,"N", "1302-14 ", 13.04633, -14.07722, 1950,0.,0., 1157, 0 19, "PHT22", 1.,"N", "1335-04 ", 13.59100, -04.28916, 1950,0.,0., 1157, 0 20, "PHT22", 1.,"N", "2203+29 ", 22.06306, +29.25667, 1950,0.,0., 1157, 0 21, "PHT22", 1.,"N", "2237-06 ", 22.62150, -06.13333, 1950,0.,0., 1157, 0 22, "PHT22", 1.,"N", "PG1211+143 ", 12.19578, 14.33139, 1950,0.,0., 1133, 0 23, "PHT22", 1.,"N", "PHL 909 ", 0.90887, 14.49961, 1950,0.,0., 1133, 0 24, "PHT22", 1.,"N", "1413+11 ", 14.22225, +11.72722, 1950, 0, 0, 1157, 0 25, "LWS01", 1.,"N", "Mkn 509 ", 20.69063, -10.90506, 1950,0.,0., 2196, 26 26, "LWS01", 1.,"N", "Mkn 509 ", 20.69063, -10.94506, 1950,0.,0., 2196, 0 27, "SWS01", 1.,"N", "Mkn 509 ", 20.69063, -10.90506, 1950,0.,0., 6498, 0 28, "SWS02", 1.,"N", "Mkn 509 ", 20.69063, -10.90506, 1950,0.,0., 4300, 0 29, "LWS01", 1.,"N", "I Zw 1 ", 0.84939, 12.42222, 1950,0.,0., 1736, 30 30, "LWS01", 1.,"N", "I Zw 1 off ", 0.84939, 12.46222, 1950,0.,0., 1736, 0 31, "SWS01", 1.,"N", "I Zw 1 ", 0.84939, 12.42222, 1950,0.,0., 6498, 0 32, "SWS02", 1.,"N", "I Zw 1 ", 0.84939, 12.42222, 1950,0.,0., 3900, 0 33, "PHT22", 1.,"N", "PG1613+658 ", 16.22673, 65.84375, 1950,0.,0., 1133, 0 34, "LWS01", 1.,"N", "PG1613+658 ", 16.22673, 65.84375, 1950,0.,0., 1500, 35 35, "LWS01", 1.,"N", "PG1613+658 ", 16.22673, 65.88375, 1950,0.,0., 1500, 0 36, "PHT22", 1.,"N", "Fairall 9 ", 1.36417, -59.06500, 1950,0.,0., 1133, 0 37, "LWS01", 1.,"N", "Fairall 9 ", 1.36417, -59.06500, 1950,0.,0., 1736, 38 38, "LWS01", 1.,"N", "Fairall 9 off", 1.36417, -59.10500, 1950,0.,0., 1736, 0 39, "SWS01", 2.,"N", "Fairall 9 ", 1.36417, -59.06500, 1950,0.,0., 6498, 0 40, "SWS02", 2.,"N", "Fairall 9 ", 1.36417, -59.06500, 1950,0.,0., 4282, 0 41, "LWS03", 1.,"N", "NGC 1068 ", 2.66863, -0.22542, 1950,0.,0., 3600, 0 42, "PHT40", 2.,"N", "Mkn 509 ", 20.69063, -10.90506, 1950,0.,0., 1800, 0 43, "SWS01", 2.,"N", "NGC 3783 ", 11.60917, -37.46167, 1950,0.,0., 6498, 0 44, "SWS02", 2.,"N", "NGC 3783 ", 11.60917, -37.46167, 1950,0.,0., 3800, 0 45, "LWS01", 2.,"N", "Mkn 551 ", 0.44631, 30.28139, 1950,0.,0., 3206, 0 46, "SWS01", 2.,"N", "Mkn 551 ", 0.44631, 30.28139, 1950,0.,0., 6498, 0 47, "SWS02", 2.,"N", "Mkn 551 ", 0.44631, 30.28139, 1950,0.,0., 4300, 0 48, "SWS01", 2.,"N", "Mkn 463 ", 13.89442, 18.61583, 1950,0.,0., 6498, 0 49, "SWS02", 2.,"N", "Mkn 463 ", 13.89442, 18.61583, 1950,0.,0., 3700, 0 50, "PHT22", 2.,"N", "1331+17 ", 13.51944, +17.73889, 1950,0.,0., 1157, 0 51, "PHT22", 2.,"N", "1302-14 ", 13.04633, -14.07722, 1950, 0, 0, 1157, 0 52, "PHT22", 2.,"N", "1700+64 ", 17.01125, +64.27361, 1950,0.,0., 1157, 0 53, "PHT22", 2.,"N", "2132+01 ", 21.54386, +01.43500, 1950, 0, 0, 1157, 0 54, "LWS03", 1.,"N", "NGC 1068 ", 2.66863, -0.22542, 1950,0.,0., 3600, 0 55, "PHT22", 2.,"N", "1233+47 ", 12.55230, +47.87694, 1950,0.,0., 1157, 0 56, "PHT22", 2.,"N", "1301+47 ", 13.03078, +47.79305, 1950,0.,0., 1157, 0 57, "LWS01", 2.,"N", "3C345 ", 16.68822, 39.90303, 1950,0.,0., 1736, 58 58, "LWS01", 2.,"N", "3C345 ", 16.68822, 39.94303, 1950,0.,0., 1736, 0 59, "PHT22", 2.,"N", "3C345 ", 16.68822, 39.90303, 1950,0.,0., 1133, 0 60, "PHT22", 2.,"N", "2331+02 ", 23.53291, +02.27972, 1950,0.,0., 1157, 0 61, "PHT22", 2.,"N", "0050-25 ", 00.83833, -25.38638, 1950,0.,0., 1157, 0 62, "PHT22", 2.,"N", "2235-03 ", 22.59650, -03.02500, 1950,0.,0., 1157, 0 63, "PHT22", 2.,"N", "1050-00 ", 10.84630, -00.01417, 1950,0.,0., 1157, 0 64, "PHT22", 2.,"N", "1246-05 ", 12.77741, -05.71611, 1950, 0, 0, 1157, 0 65, "PHT22", 2.,"N", "0100+13 ", 01.00928, +13.00306, 1950,0.,0., 1157, 0 66, "SWS01", 3.,"N", "HB89 1821+643", 18.36164, 64.31694, 1950,0.,0., 4698, 0 67, "PHT40", 3.,"N", "HB89 1821+643", 18.36164, 64.31694, 1950,0.,0., 1800, 0 68, "PHT40", 3.,"N", "Mkn 551 ", 0.44631, 30.28139, 1950,0.,0., 1800, 0 69, "PHT22", 3.,"N", "Mkn 509 ", 20.69063, -10.90506, 1950,0.,0., 1133, 0 70, "LWS01", 3.,"N", "Mkn 463 ", 13.89442, 18.61583, 1950,0.,0., 3206, 0 71, "LWS01", 3.,"N", "NGC 3783 ", 11.60917, -37.46167, 1950,0.,0., 3206, 0 72, "LWS01", 3.,"N", "Mkn 573 ", 1.68970, 2.09897, 1950,0.,0., 3206, 0 73, "SWS02", 3.,"N", "Mkn 573 ", 1.68970, 2.09897, 1950,0.,0., 4300, 0 74, "LWS01", 3.,"N", "PHL 909 ", 0.90887, 14.49961, 1950,0.,0., 3450, 75 75, "LWS01", 3.,"N", "PHL 909 ", 0.90887, 14.53961, 1950,0.,0., 3450, 0 76, "LWS01", 3.,"N", "PG1211+143 ", 12.19578, 14.33139, 1950,0.,0., 3600, 77 77, "LWS01", 3.,"N", "PG1211+143 ", 12.19578, 14.37139, 1950,0.,0., 3600, 0 78, "PHT22", 3.,"N", "I Zw 1 ", 0.84939, 12.42222, 1950,0.,0., 1133, 0 79, "LWS01", 3.,"N", "IC4329A ", 13.77417, -30.06139, 1950,0.,0., 3206, 0 80, "SWS06", 3.,"N", "IC4329A ", 13.77417, -30.06139, 1950,0.,0., 4568, 0 81, "PHT40", 3.,"N", "IC4329A ", 13.77417, -30.06139, 1950,0.,0., 1800, 0 82, "LWS01", 3.,"N", "Mkn 478 ", 14.66793, 35.65205, 1950,0.,0., 900, 83 83, "LWS01", 3.,"N", "Mkn 478 off ", 14.66793, 35.69205, 1950,0.,0., 900, 0 84, "PHT22", 3.,"N", "Mkn 478 ", 14.66793, 35.65205, 1950,0.,0., 1133, 0 85, "PHT22", 2.,"N", "2225-05 ", 22.43169, -05.57138, 1950,0.,0., 1157, 0 <=== spring_launch_targets ===> 01, "LWS01", 1.,"N", "NGC 1068 ", 2.66863, -0.22542, 1950, 0,0, 5824, 0 02, "LWS01", 1.,"N", "NGC 4151 ", 12.13363, 39.68383, 1950, 0,0, 5824, 0 03, "LWS01", 1.,"N", "I Zw 92 ", 14.65071, 53.71778, 1950, 0,0, 3206, 0 04, "SWS01", 1.,"N", "I Zw 92 ", 14.65071, 53.71778, 1950, 0,0, 6498, 0 05, "SWS02", 1.,"N", "I Zw 92 ", 14.65071, 53.71778, 1950, 0,0, 4400, 0 06, "PHT40", 1.,"N", "I Zw 92 ", 14.65071, 53.71778, 1950, 0,0, 1800, 0 07, "SWS01", 1.,"N", "Mkn 3 ", 6.16345, 71.05298, 1950, 0,0, 6498, 0 08, "SWS02", 1.,"N", "Mkn 3 ", 6.16345, 71.05298, 1950, 0,0, 2910, 0 09, "PHT22", 1.,"N", "3C273 ", 12.44257, 2.32875, 1950, 0,0, 1133, 0 10, "LWS01", 1.,"N", "3C273 ", 12.44257, 2.32875, 1950, 0,0, 1736, 11 11, "LWS01", 1.,"N", "3C273 off ", 12.44257, 2.36875, 1950, 0,0, 1736, 0 12, "PHT22", 1.,"N", "1335-04 ", 13.59100, -04.28916, 1950, 0, 0, 1157, 0 13, "PHT22", 1.,"N", "0307+02 ", 03.12094, +02.36667, 1950, 0,0, 1157, 0 14, "PHT22", 1.,"N", "0751+56 ", 07.86130, +56.38500, 1950, 0,0, 1157, 0 15, "PHT22", 1.,"N", "0910+56 ", 09.18258, +56.43027, 1950, 0,0, 1157, 0 16, "PHT22", 1.,"N", "0952-01 ", 09.87422, -01.26472, 1950, 0,0, 1157, 0 17, "PHT22", 1.,"N", "1033-03 ", 10.56430, -03.46277, 1950, 0,0, 1157, 0 18, "PHT22", 1.,"N", "1050-00 ", 10.84630, -00.01417, 1950, 0,0, 1157, 0 19, "PHT22", 1.,"N", "1114-08 ", 11.24866, -08.37611, 1950, 0,0, 1157, 0 20, "PHT22", 1.,"N", "1158+46 ", 11.96747, +46.59138, 1950, 0,0, 1157, 0 21, "PHT22", 1.,"N", "1202-07 ", 12.04700, -07.43055, 1950, 0,0, 1157, 0 22, "PHT22", 1.,"N", "1247+34 ", 12.78827, +34.10333, 1950, 0,0, 1157, 0 23, "PHT22", 1.,"N", "1413+11 ", 14.22225, +11.72722, 1950, 0, 0, 1157, 0 24, "PHT22", 1.,"N", "2132+01 ", 21.54386, +01.43500, 1950, 0, 0, 1157, 0 25, "PHT22", 1.,"N", "Fairall 9 ", 1.36417, -59.06500, 1950, 0,0, 1133, 0 26, "LWS01", 1.,"N", "Fairall 9 ", 1.36417, -59.06500, 1950, 0,0, 1736, 27 27, "LWS01", 1.,"N", "Fairall 9 off", 1.36417, -59.10500, 1950, 0,0, 1736, 0 28, "LWS01", 1.,"N", "I Zw 1 ", 0.84939, 12.42222, 1950, 0,0, 1736, 29 29, "LWS01", 1.,"N", "I Zw 1 off ", 0.84939, 12.46222, 1950, 0,0, 1736, 0 30, "SWS01", 1.,"N", "I Zw 1 ", 0.84939, 12.42222, 1950, 0,0, 6498, 0 31, "SWS02", 1.,"N", "I Zw 1 ", 0.84939, 12.42222, 1950, 0,0, 3900, 0 32, "PHT22", 1.,"N", "I Zw 1 ", 0.84939, 12.42222, 1950, 0,0, 1133, 0 33, "LWS01", 1.,"N", "Mkn 3 ", 6.16345, 71.05298, 1950, 0,0, 3206, 0 34, "PHT22", 1.,"N", "PG1613+658 ", 16.22673, 65.84375, 1950, 0,0, 1133, 0 35, "LWS01", 1.,"N", "PG1613+658 ", 16.22673, 65.84375, 1950, 0,0, 1500, 36 36, "LWS01", 1.,"N", "PG1613+658 ", 16.22673, 65.88375, 1950, 0,0, 1500, 0 37, "LWS01", 1.,"N", "PG1351+640 ", 13.86285, 64.00789, 1950, 0,0, 1200, 38 38, "LWS01", 1.,"N", "PG1351+640 ", 13.86285, 64.04789, 1950, 0,0, 1200, 0 39, "SWS01", 2.,"N", "Fairall 9 ", 1.36417, -59.06500, 1950, 0,0, 6498, 0 40, "SWS02", 2.,"N", "Fairall 9 ", 1.36417, -59.06500, 1950, 0,0, 4282, 0 41, "LWS03", 1.,"N", "NGC 1068 ", 2.66863, -0.22542, 1950, 0,0, 3600, 0 42, "SWS01", 2.,"N", "NGC 3783 ", 11.60917, -37.46167, 1950, 0,0, 6498, 0 43, "SWS02", 2.,"N", "NGC 3783 ", 11.60917, -37.46167, 1950, 0,0, 3800, 0 44, "LWS01", 2.,"N", "NGC 3783 ", 11.60917, -37.46167, 1950, 0,0, 3206, 0 45, "PHT22", 2.,"N", "PHL 909 ", 0.90887, 14.49961, 1950, 0,0, 1133, 0 46, "LWS01", 2.,"N", "PHL 909 ", 0.90887, 14.49961, 1950, 0,0, 3450, 47 47, "LWS01", 2.,"N", "PHL 909 ", 0.90887, 14.53961, 1950, 0,0, 3450, 0 48, "SWS01", 2.,"N", "HB89 1821+643", 18.36164, 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