J/ApJ/866/133   Continuum-Hβ light curves of 5 Seyfert 1   (De Rosa+, 2018)

Velocity-resolved reverberation mapping of five bright Seyfert 1 galaxies. De Rosa G., Fausnaugh M.M., Grier C.J., Peterson B.M., Denney K.D., Horne K., Bentz M.C., Ciroi S., Bonta E.D., Joner M.D., Kaspi S., Kochanek C.S., Pogge R.W., Sergeev S.G., Vestergaard M., Adams S.M., Antognini J., Salvo C.A., Armstrong E., Bae J., Barth A.J., Beatty T.G., Bhattacharjee A., Borman G.A., Boroson T.A., Bottorff M.C., Brown J.E., Brown J.S., Brotherton M.S., Coker C.T., Clanton C., Cracco V., Crawford S.M., Croxall K.V., Eftekharzadeh S., Eracleous M., Fiorenza S.L., Frassati A., Hawkins K., Henderson C.B., Holoien T.W.-S., Hutchison T., Kellar J., Kilerci-Eser E., Kim S., King A.L., La Mura G., Laney C.D., Li M., Lochhaas C., Ma Z., MacInnis F., Manne-Nicholas E.R., Mason M., McGraw S.M., Mogren K., Montouri C., Moody J.W., Mosquera A.M., Mudd D., Musso R., Nazarov S.V., Nguyen M.L., Ochner P., Okhmat D.N., Onken C.A., Ou-Yang B., Pancoast A., Pei L., Penny M., Poleski R., Portaluri E., Prieto J.-L., Price-Whelan A.M., Pulatova N.G., Rafter S., Roettenbacher R.M., Romero-Colmenero E., Runnoe J., Schimoia J.S., Shappee B.J., Sherf N., Simonian G.V., Siviero A., Skowron D.M., Skowron J., Somers G., Spencer M., Starkey D.A., Stevens D.J., Stoll R., Tamajo E., Tayar J., van Saders J.L., Valenti S., Villanueva S.JR, Villforth C., Weiss Y., Winkler H., Zastrow J., Zhu W., Zu Y. <Astrophys. J., 866, 133 (2018)> =2018ApJ...866..133D 2018ApJ...866..133D
ADC_Keywords: Active gal. nuclei; Galaxies, spectra; Spectra, optical Keywords: galaxies: active ; galaxies: nuclei ; galaxies: Seyfert Abstract: We present the first results from a reverberation-mapping campaign undertaken during the first half of 2012, with additional data on one active galactic nucleus (AGN) (NGC 3227) from a 2014 campaign. Our main goals are (1) to determine the black hole masses from continuum-Hβ reverberation signatures, and (2) to look for velocity-dependent time delays that might be indicators of the gross kinematics of the broad-line region. We successfully measure Hβ time delays and black hole masses for five AGNs, four of which have previous reverberation mass measurements. The values measured here are in agreement with earlier estimates, though there is some intrinsic scatter beyond the formal measurement errors. We observe velocity-dependent Hβ lags in each case, and find that the patterns have changed in the intervening five years for three AGNs that were also observed in 2007. Description: The primary objective of this campaign is to determine the kinematics and structure of the BLR in a few well-studied bright AGNs. In particular, we are re-examining NGC 3227, NGC 3516, and NGC 5548 from Denney+ (2009ApJ...704L..80D 2009ApJ...704L..80D). We also included in our observing program NGC 4151, for which the best reverberation data are from a weather-abbreviated campaign in 2005 (Bentz+ 2006ApJ...651..775B 2006ApJ...651..775B). Sources included in the 2012 campaign were Mrk 374, Mrk 382, Mrk 478, Mrk 618, and Mrk 704. The principal data source for both the 2012 and 2014 campaigns was the Boller and Chivens CCD spectrograph on the MDM Observatory 1.3m McGraw-Hill telescope on Kitt Peak. The 2012 campaign ran from the beginning of 2012 January through the end of 2012 April. The spectral coverage is over the range 4400-5850Å and the resolution is 7.9Å. The 2012 campaign also included spectroscopic observations obtained at the Asiago Astrophysical Observatory of Padova University with the 1.22m Galileo telescope and the Cassegrain Boller & Chivens spectrograph. The spectral coverage is over the range 3200-8000Å and the resolution is 10.5Å. The Crimean Astrophysical Observatory (CrAO) provided spectra from the Nasmith spectrograph and SPEC-10 CCD on the 2.6m Shajn telescope. It covered wavelengths from 3900 to 6100Å. Finally, the 2.3m telescope at Wyoming Infrared Observatory (WIRO) and the WIRO Long Slit Spectrograph contributed a small number of observations. A spectral coverage between 4400 and 5600Å was used. We supplemented our spectroscopic continuum light curves with photometric observations. Observations in 2012 were obtained with the 0.5m Centurian 18 at Wise Observatory (WC18) and with the 0.9m at West Mountain Observatory (WMO). We also used data from the All-Sky Automated Survey for SuperNovae (ASAS-SN, Shappee+ 2014, J/ApJ/788/48). These data are from the first unit of ASAS-SN, Brutus, which consisted in 2012 of two 14cm aperture Nikon telephoto lenses on a single mount in the Faulkes Telescope North enclosure on Mount Haleakala, Hawaii. In addition, the 2014 campaign included imaging from CrAO, Fountainwood Observatory (FWO), and the Las Cumbres Observatory (LCO). The CrAO images were from the 0.7m telescope; observations from FWO were obtained with a 0.4m telescope. The LCO data were obtained using their worldwide network of 1m telescopes in the Sloan ugriz bands. When needed, we adopt a cosmological model with Ωm=0.30, ΩΛ=0.70, and H0=70km/s/Mpc. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 38 5 Source properties contlc.dat 34 976 Continuum light curves hbetalc.dat 33 507 Hβ light curves -------------------------------------------------------------------------------- See also: J/ApJ/613/682 : AGN central mass & broad-line region sizes (Peterson+, 2004) J/ApJ/702/1353 : Hβ and V-band light curves of NGC 4051 (Denney+, 2009) J/ApJ/714/1521 : Spectroscopy of galaxies around distant QSOs (Chen+, 2010) J/ApJ/716/993 : LAMP: reverberation mapping of H and He lines (Bentz+, 2010) J/ApJ/732/121 : V-band and Hβ monitoring of Z299-15 (Barth+, 2011) J/ApJ/733/124 : Cepheids in M101 observed with HST (Shappee+, 2011) J/ApJ/755/60 : Reverberation mapping for 5 Seyfert 1 galaxies (Grier+, 2012) J/ApJ/761/123 : KELT-1 photometry and spectroscopy follow-up (Siverd+, 2012) J/ApJ/779/109 : Long-term monitoring of NGC 5548 (Peterson+, 2013) J/ApJ/782/45 : SEAMBHs. I. Mrk 142, Mrk335, and IRAS F12397+3333 (Du+, 2014) J/ApJ/795/38 : Phot. & spec. measurements for KA1858+4850 (Pei+, 2014) J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014) J/ApJ/793/108 : SEAMBHs. II. Continuum and Hbeta LCs (Wang+, 2014) J/ApJS/217/26 : Lick AGN monitoring 2011: light curves (Barth+, 2015) J/ApJ/806/128 : Space telescope RM project. I. NGC 5548 (De Rosa+, 2015) J/ApJ/806/22 : SEAMBHs IV. Hβ time lags (Du+, 2015) J/ApJ/806/129 : Space telescope RM project. II. Swift data (Edelson+, 2015) J/ApJS/216/4 : SDSS-RM project: technical overview (Shen+, 2015) J/ApJ/821/56 : Space telescope RM project III. NGC5548 LCs (Fausnaugh+, 2016) J/ApJ/827/118 : A new reverberation mapping campaign on NGC 5548 (Lu+, 2016) J/ApJ/840/97 : Opt. reverberation map campaign of 5 AGNs (Fausnaugh+, 2017) J/ApJ/837/131 : Space telescope RM project V. NGC5548 sp. monitor (Pei+, 2017) J/A+A/625/A152 : Light-curve models of black hole (Barbieri+, 2019) J/MNRAS/448/2879 : Spectropolarimetry of 3C390.3 (Afanasiev+, 2015) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Name of the studied AGN 10- 15 F6.4 --- z [0.003/0.03] Redshift from the NASA Extragalactic Database (NED) 17- 21 F5.1 Mpc Dist [13.9/128] Luminosity distance (1) 23- 27 F5.2 [10-7W] logL5100 [42.6/43.8] log of observed 5100Å luminosity corrected for Galactic extinction; in erg/s units (2) 29- 33 F5.2 [10-7W] logLhost [42.3/43.3] log of host galaxy luminosity; in erg/s units 35- 38 F4.2 mag E(B-V) [0.02/0.04] Galactic reddening value from Schlafly & Finkbeiner (2011ApJ...737..103S 2011ApJ...737..103S) -------------------------------------------------------------------------------- Note (1): The luminosity distance in a consensus cosmology, except for NGC3227 which is interacting with an elliptical companion, NGC3226, which has a surface-brightness fluctuation distance of 23.5Mpc (Tonry+ 2001ApJ...546..681T 2001ApJ...546..681T). We therefore adopt this as the distance to NGC3227. In the case of NGC4151, we use the distance of 13.9Mpc adopted by Onken+ (2014ApJ...791...37O 2014ApJ...791...37O). See section 2.1 for further details. Note (2): Observed luminosity (corrected for Galactic extinction), calculated from the observed 5100Å rest-frame light curve. -------------------------------------------------------------------------------- Byte-by-byte Description of file: contlc.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name AGN name 10 I1 --- m_Name [1/2]? Multiple component on Name for NGC3227 12- 18 F7.2 d HJD [5931.5/6845.3] Heliocentric Julian Date of observation; HJD-2450000 21- 25 F5.2 10-17W/m2/nm Flux [4.2/37.6] Flux density in units of 10-15erg/s/cm2/Å 27- 30 F4.2 10-17W/m2/nm e_Flux [0.01/1.4]? Uncertainty in Flux 32- 34 A3 --- Obs Observatory (1) -------------------------------------------------------------------------------- Note (1): Contributing observatory as follows: M = MDM Observatory -- 1.3m McGraw-Hill telescope on Kitt Peak (405 occurrences); W1 = Wise Observatory -- 0.5m Centurian 18 (WC18) (232 occurrences); W2 = West Mountain Observatory (WMO) -- 0.9m telescope (169 occurrences); A1 = Asiago Astrophysical Observatory, Padova University -- 1.22m Galileo telescope (81 occurrences); A2 = ASAS-SN -- Faulkes Telescope North, Hawaii (28 occurrences); C = Crimean Astrophysical observatory (CrAO) -- 0.7m telescope (40 occurrences); FWO = Fountainwood Observatory -- 0.4m telescope (21 occurrences). -------------------------------------------------------------------------------- Byte-by-byte Description of file: hbetalc.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name AGN name 10 I1 --- m_Name [1/2]? Multiple component on Name for NGC3227 12- 18 F7.2 d HJD [5931.5/6820.7] Heliocentric Julian Date of observation; HJD-2450000 21- 25 F5.2 10-16W/m2 Flux [2.8/48.4] Flux density in units of 10-13erg/s/cm2 27- 30 F4.2 10-16W/m2 e_Flux [0.02/1.3]? Uncertainty in Flux 32- 33 A2 --- Obs Observatory (1) -------------------------------------------------------------------------------- Note (1): Contributing observatory as follows: M = MDM Observatory -- 1.3m McGraw-Hill telescope on Kitt Peak (410 occurrences); A1 = Asiago Astrophysical Observatory, Padova University -- 1.22m Galileo telescope (81 occurrences); C = Crimean Astrophysical observatory (CrAO) -- 0.7m telescope (16 occurrences). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS] 08-Oct-2019
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