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, NA
,
Massaro, F
,
Milisavljevic, D
,
Landoni, M
,
Chavushyan, V
,
Patino-Alvarez, V
,
Masetti, N
,
Jimenez-Bailon, E
,
Strader, J
,
Chomiuk, L
,
Katagiri, H
,
Kagaya, M
,
Cheung, CC
,
Paggi, A
,
D'Abrusco, R
,
Ricci, F
,
La Franca, F
,
Smith, HA
,
Tosti, 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
Oh, K
,
Schawinski, K
,
Koss, M
,
Trakhtenbrot, B
,
Lamperti, I
,
Ricci, C
,
Mushotzky, R
,
Veilleux, S
,
Berney, S
,
Crenshaw, DM
,
Gehrels, N
,
Harrison, F
,
Masetti, N
,
Soto, KT
,
Stern, D
,
Treister, E
,
Ueda, 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, F
,
Marchesini, EJ
,
D'Abrusco, R
,
Masetti, N
,
Andruchow, I
,
Smith, HA
,
[RADIO-WEAK BL LAC OBJECTS IN THE FERMI ERA]
,
RADIO-WEAK BL LAC OBJECTS IN THE FERMI ERA
Context. Based on their overwhelming dominance among associated Fermi gamma-ray catalogue sources, it is expected that a large fraction of the unidentified Fermi objects are blazars. Through crossmatching between the positions of unidentified gamma-ray sources from the First Fermi Catalog of gamm...
Marchesini, EJ
,
Masetti, N
,
Chavushyan, V
,
Cellone, SA
,
Andruchow, I
,
Bassani, L
,
Bazzano, A
,
Jimenez-Bailon, E
,
Landi, R
,
Malizia, A
,
Palazzi, E
,
Patino-Alvarez, V
,
Rodriguez-Castillo, GA
,
Stephen, JB
,
Ubertini, P
,
[Looking for blazars in a sample of unidentified high-energy emitting Fermi sources]
,
Looking for blazars in a sample of unidentified high-energy emitting Fermi sources
We present two-dimensional stellar and gaseous kinematics of the inner 0.7 × 1.2 kpc2 of the Seyfert 1.5 galaxy ESO 362-G18, derived from optical (4092-7338 Å) spectra obtained with the GMOS integral field spectrograph on the Gemini South telescope at a spatial resolution of ≈ 170 pc and spectral...
Humire, P.K.
,
Nagar, N.M.
,
Finlez, C.
,
Firpo, V.
,
Slater, R.
,
Lena, D.
,
Soto-Pinto, P.
,
Muñoz-Vergara, D.
,
Riffel, R.A.
,
Schmitt, H.R.
,
Kraemer, S.B.
,
Schnorr-Müller, A.
,
Fischer, T.C.
,
Robinson, A.
,
Storchi-Bergmann, T.
,
Crenshaw, M.
,
Elvis, M.S.
,
[An outflow in the Seyfert ESO 362-G18 revealed by Gemini-GMOS/IFU observations]
,
An outflow in the Seyfert ESO 362-G18 revealed by Gemini-GMOS/IFU observations
PBC J2333.9-2343 is a peculiar active nucleus with two giant radio lobes and a weak blazarlike nucleus at their centre. In this work we show new optical, ultraviolet (UV), and X-ray data taken from the San Pedro Mártir telescope, the New Technology Telescope, NTT/EFOSC2, and the Swift/XRT satelli...
Hernández-García, L.
,
Vietri, G.
,
Panessa, F.
,
Piconcelli, E.
,
Chavushyan, V.
,
Jiménez-Andrade, E.F.
,
Bassani, L.
,
Bazzano, A.
,
Cazzoli, S.
,
Malizia, A.
,
Masetti, N.
,
Monaco, L.
,
Pović, M.
,
Saviane, I.
,
Ubertini, P.
,
[Variable broad lines and outflow in the weak blazar PBC J2333.9-2343]
,
Variable broad lines and outflow in the weak blazar PBC J2333.9-2343