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We report on discovery results from a quasar lens search in the ATLAS-DR3 public footprint. Spectroscopic follow-up campaigns, conducted at the 2.6 m Nordic Optical Telescope (La Palma) and 3.6mNew Technology Telescope (La Silla) in 2016, yielded seven pairs of quasars exhibiting the same lines a...


Agnello, A.Schechter, P.L.Morgan, N.D.Treu, T.Grillo, C.Malesani, D.Anguita, T.Apostolovski, Y.Rusu, C.E.Motta, V.Rojas, K.Chehade, B.Shanks, T.[Quasar lenses and pairs in the VST-ATLAS and Gaia]Quasar lenses and pairs in the VST-ATLAS and Gaia

Blazars, one of the most extreme classes of active galaxies, constitute so far the largest known population of.-ray sources, and their number is continuously growing in the Fermi catalogs. However, in the latest release of the Fermi catalog there is still a large fraction of sources that are clas...


Crespo, NAMassaro, FMilisavljevic, DLandoni, MChavushyan, VPatino-Alvarez, VMasetti, NJimenez-Bailon, EStrader, JChomiuk, LKatagiri, HKagaya, MCheung, CCPaggi, AD'Abrusco, RRicci, FLa Franca, FSmith, HATosti, G[OPTICAL SPECTROSCOPIC OBSERVATIONS OF GAMMA-RAY BLAZAR CANDIDATES. VI. FURTHER OBSERVATIONS FROM TNG, WHT, OAN, SOAR, AND MAGELLAN TELESCOPES]OPTICAL SPECTROSCOPIC OBSERVATIONS OF GAMMA-RAY BLAZAR CANDIDATES. VI. FURTHER OBSERVATIONS FROM TNG, WHT, OAN, SOAR, AND MAGELLAN TELESCOPES

We investigate the observed relationship between black hole mass (M-BH), bolometric luminosity (L-bol) and Eddington ratio (lambda(Edd)) with optical emission-line ratios ([N II] lambda 6583/H alpha, [S II] lambda lambda 6716, 6731/H alpha, [O I] lambda 6300/H alpha, [O III] lambda 5007/H beta, [...


Oh, KSchawinski, KKoss, MTrakhtenbrot, BLamperti, IRicci, CMushotzky, RVeilleux, SBerney, SCrenshaw, DMGehrels, NHarrison, FMasetti, NSoto, KTStern, DTreister, EUeda, Y[BAT AGN Spectroscopic Survey – III. An observed link between AGN Eddington ratio and narrow-emission-line ratios]BAT AGN Spectroscopic Survey – III. An observed link between AGN Eddington ratio and narrow-emission-line ratios

The existence of "radio-weak BL Lac objects" (RWBLs) has been an open question, and has remained unsolved since the discovery that quasars could be radio-quiet or radio-loud. Recently, several groups identified RWBL candidates, mostly found while searching for low-energy counterparts of the unide...


Massaro, FMarchesini, EJD'Abrusco, RMasetti, NAndruchow, ISmith, HA[RADIO-WEAK BL LAC OBJECTS IN THE FERMI ERA]RADIO-WEAK BL LAC OBJECTS IN THE FERMI ERA

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