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相关论文: The host galaxy of the BL Lacertae object 1ES 0647…

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We present results of an ongoing program at the ESO VLT for spectroscopy of BL Lac objects lacking a firm redshift estimate and here we report on 15 objects. For 11 sources we confirm the BL Lac classification, and we determine new…

天体物理学 · 物理学 2008-10-21 B. Sbarufatti , S. Ciprini , J. Kotilainen , R. Decarli , A. Treves , A. Veronesi , R. Falomo

We present the results of deep I-band imaging of two BL Lacerate objects, RGB 0136+391 and PKS 0735+178, during an epoch when the optical nucleus was in a faint state in both targets. In PKS 0735+178 we find a significant excess over a…

宇宙学与河外天体物理 · 物理学 2015-06-11 K. Nilsson , T. Pursimo , C. Villforth , E. Lindfors , L. O. Takalo , A. Sillanpää

We present optical images and spectroscopy for a dozen of BL Lac objects. Most of these objects were not previously studied and we give for the first time the properties of their host galaxies. The properties of the new host galaxies are…

天体物理学 · 物理学 2009-09-25 Renato Falomo , Marie-Helene Ulrich

The BL-Lac family of active galaxies possess almost featureless spectra and exhibit rapid variability over their entire spectral range. A number of models have been developed to explain these extreme properties, several of which have…

天体物理学 · 物理学 2016-08-30 G. F. Lewis , R. A. Ibata

Observations of the gamma-ray sky with Fermi led to significant advances towards understanding blazars, the most extreme class of Active Galactic Nuclei. A large fraction of the population detected by Fermi is formed by BL Lacertae (BL Lac)…

We report on ESO Very Large Telescope optical spectroscopy of 42 BL Lacertae objects of unknown redshift. Nuclear emission lines were observed in 12 objects, while for another six we detected absorption features due to their host galaxy.…

天体物理学 · 物理学 2008-11-26 B. Sbarufatti , A. Treves , R. Falomo , J. Heidt , J. Kotilainen , R. Scarpa

Context: The redshift of PG 1553+11, a bright BL Lac object (V~14), is still unknown. It has been recently observed in the TeV band, a fact that offers an upper limit for the redshift z<0.4. Aims: We intend to provide a lower limit for the…

天体物理学 · 物理学 2009-11-13 Aldo Treves , Renato Falomo , Michela Uslenghi

The HST NICMOS Camera 2 was used for H-band imaging of 12 BL Lacertae objects taken from the larger sample observed with the WFPC2 in the R band (Urry et al. 2000; Scarpa et al. 2000). Ten of the 12 BL Lacs are clearly resolved, and the…

天体物理学 · 物理学 2009-10-31 Riccardo Scarpa , C. Megan Urry , Paolo Padovani , Daniela Calzetti , Matthew O'Dowd

We analyze images of BL Lacertae objects obtained with the {\it Hubble Space Telescope} WFPC2 and the F814W filter. The nine objects cover a redshift range of 0.19 to 0.997. The relatively deep images are sufficient to detect galaxies at…

天体物理学 · 物理学 2009-10-31 J. E. Pesce , C. M. Urry , M. O'Dowd , R. Scarpa , R. Falomo , A. Treves

We present the results of the first systematic long-term multi-color optical monitoring of the BL Lacertae object 1ES 0806+52.4. The monitoring was performed in multiple passbands with a 60/90 cm Schmidt telescope from December 2005 to…

星系天体物理 · 物理学 2015-06-22 Zhongyi Man , Xiaoyuan Zhang , Jianghua Wu , Xu Zhou , Qirong Yuan

We report on the optical properties of a sample of 30 BL Lac host galaxies in the redshift range $0.03<z<0.2$, as derived from HST observations. All galaxies are fully resolved in the WFPC2 (F702W filter) images, allowing a quantitative…

天体物理学 · 物理学 2009-10-31 R. Falomo , R. Scarpa , A. Treves , C. M. Urry

The high-frequency-peaked BL Lacertae object 1ES 0229+200 is a relatively distant (z = 0.1396), hard-spectrum (Gamma ~ 2.5), very-high-energy-emitting (E > 100 GeV) gamma-ray blazar. Very-high-energy measurements of this active galactic…

We report on a large HST imaging survey of BL Lac objects, at spatial resolution ~10 times better than previous ground-based surveys. We focus on data reduction and analysis, describing the procedures used to model the host galaxy surface…

天体物理学 · 物理学 2009-10-31 Riccardo Scarpa , C. Megan Urry , Renato Falomo , Joseph E. Pesce , Aldo Treves

We present H-band imaging of 23 low redshift (z < 0.3) BL Lac objects that were previously investigated by us in the R-band. For all the observed objects, the host galaxy is well represented by an elliptical model, with average scale length…

天体物理学 · 物理学 2009-11-10 J. K. Kotilainen , R. Falomo

BL Lac objects (BLL) are defined by the presence of very weak (typically $<$ 5 {\AA}) or even absent spectral lines. This makes determining their distance particularly challenging, especially at high redshift, where the sources are fainter…

星系天体物理 · 物理学 2026-04-01 Renato Falomo , Aldo Treves , Simona Paiano , Riccardo Scarpa

PKS 1424+240 is a BL-Lac blazar with unknown redshift that was detected at high-energy gamma rays by Fermi-LAT with a hard spectrum. At VHE, it was first detected by VERITAS and later confirmed by MAGIC. Its spectral energy distribution is…

高能天体物理现象 · 物理学 2016-04-20 A. C. Rovero , H. Muriel , C. Donzelli , A. Pichel

BL Lacertae (BL Lac) objects at high redshifts ($z\geq 2$) are rarely detected. Through careful analysis of the SDSS spectrum, BZB J1450+5201 is confirmed to be a high-$z$ BL Lac object with $z\geq$ 2.471 by identifying the Ly$\alpha$ 1216…

高能天体物理现象 · 物理学 2016-03-23 N. H. Liao , J. M. Bai , J. G. Wang , H. T. Liu , J. J. Zhang , Ning Jiang , Z. L. Yuan , Liang Chen

Observations of the blazars 1ES 0647+250 and 1ES 0806+524 with VERITAS are reported here. These objects are among the favoured candidate extragalactic sources in the very high-energy regime due to the presence of high-energy electrons and…

天体物理学 · 物理学 2019-08-13 P. Cogan

The BL-Lac blazar PKS 0447-439 is one of the brightest HE gamma-ray sources that were first detected by Fermi-LAT. It was also detected by H.E.S.S. at VHE gamma-rays, which allowed constraining the redshift of PKS 0447-439 by considering…

星系天体物理 · 物理学 2015-06-23 H. Muriel , C. Donzelli , A. C. Rovero , A. Pichel

Six BL Lac objects from the complete 1 Jy radio-selected sample of 34 objects were observed in Cycle 5 with the HST WFPC2 camera to an equivalent limiting flux of mu_I~26 mag/arcsec^2. Here we report results for the second half of this…

天体物理学 · 物理学 2009-10-30 C. Megan Urry , Renato Falomo , Riccardo Scarpa , Joseph E. Pesce , Aldo Treves , Mauro Giavalisco