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Related papers: Type 1 low z AGN. I. Emission properties

200 papers

The mid-infrared to ultraviolet (0.1 -- 10 $\mu m$) spectral energy distribution (SED) shapes of 407 X-ray-selected radio-quiet type 1 AGN in the wide-field ``Cosmic Evolution Survey" (COSMOS) have been studied for signs of evolution. For a…

Active galactic nuclei (AGN) play a crucial role in galaxy evolution by influencing the observational properties of their host galaxies. We investigate the host galaxy properties of X-ray selected AGNs, focusing on differences between…

Astrophysics of Galaxies · Physics 2025-08-28 Carlos G. Bornancini , Gabriel A. Oio , Georgina Coldwell

JWST observations have unveiled faint active galactic nuclei (AGN) at high-redshift that provide insights on the formation of supermassive black holes (SMBHs) and their coevolution with galaxies. However, disentangling stellar from AGN…

The Two Micron All-Sky Survey (2MASS) has provided a uniform photometric catalog to search for previously unknown red AGN and QSOs. We have extended the search to the southern equatorial sky by obtaining spectra for 1182 AGN candidates…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Frank Masci , Roc Cutri , Paul Francis , Brant Nelson , John Huchra , D. Heath Jones , Matthew Colless , Will Saunders

Type 2 active galactic nuclei (AGN) represent the majority of the AGN population. However, due to the difficulties in measuring their black hole (BH) masses, it is still unknown whether they follow the same BH mass-host galaxy scaling…

Astrophysics of Galaxies · Physics 2017-11-08 F. Ricci , F. La Franca , A. Marconi , F. Onori , F. Shankar , R. Schneider , E. Sani , S. Bianchi , A. Bongiorno , M. Brusa , F. Fiore , R. Maiolino , C. Vignali

In this work, we investigated the X-ray emission for a sample of young radio AGNs by combining their data from Chandra/XMM-Newton and at other wavebands. We find strong correlations between the X-ray luminosity $L_{\rm X}$ in 2$-$10 keV and…

Astrophysics of Galaxies · Physics 2020-06-10 Mai Liao , Minfeng Gu , Minhua Zhou , Liang Chen

We study the large-scale environments and clustering properties of 28 low-luminosity AGNs at $z=3.9-6$ in the GOODS-N field. Our sample, identified from the JWST NIRCam Imaging and WFSS data in CONGRESS and FRESCO surveys with either broad…

The physics of active super massive black holes (BHs) is governed by their mass (M_BH), spin (a*) and accretion rate ($\dot{M}$). This work is the first in a series of papers with the aim of testing how these parameters determine the…

Astrophysics of Galaxies · Physics 2015-06-23 Daniel M. Capellupo , Hagai Netzer , Paulina Lira , Benny Trakhtenbrot , Julían Mejía-Restrepo

We determine the cumulative spectral energy distribution (SED) of local AGN in the 3-300 keV band and compare it with the spectrum of the cosmic X-ray background (CXB) in order to test the widely accepted paradigm that the CXB is a…

Astrophysics · Physics 2009-11-13 S. Sazonov , R. Krivonos , M. Revnivtsev , E. Churazov , R. Sunyaev

We present optical spectra for a representative sample of 27 nearby (z < 0.2) 2MASS-selected AGN with red near-IR colours (J-K 2.0). The spectra were taken with the ISIS spectrograph on the WHT with the aim of determining the nature of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Marvin Rose , Clive Tadhunter , Joanna Holt , Javier Rodríguez Zaurín

Although the super-massive (AGN) and stellar mass (XRBs) black holes have many properties in common, the broad emission lines (BELs) are exclusively signatures of the AGN. Based on the detection of these lines from SDSS data bases, there…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Susmita Chakravorty , Martin Elvis , Gary Ferland

Context: Narrow-band surveys for Ly-alpha emitters (LAEs) is a powerful tool in detecting high, and very high, redshift galaxies. Even though samples are growing at redshifts z = 3 - 6, the nature of these galaxies is still poorly known.…

We search for high-redshift (z>4.5) X-ray AGNs in the deep central (off-axis angle <5.7') region of the 7 Ms Chandra Deep Field-South X-ray image. We compile an initial candidate sample from direct X-ray detections. We then probe more…

Astrophysics of Galaxies · Physics 2020-03-11 L. L. Cowie , A. J. Barger , F. E. Bauer , J. Gonzalez-Lopez

The outshining light from active galactic nuclei (AGNs) poses significant challenges in studying the properties of AGN host galaxies. To address this issue, we propose a novel approach which combines image decomposition and spectral energy…

Astrophysics of Galaxies · Physics 2025-02-11 Haoran Yu , Lulu Fan , Yunkun Han , Weibin Sun , Yihang Zhang , Xuheng Ding , Yongquan Xue

We present medium resolution near infrared spectroscopic observations of 41 obscured and intermediate class AGN (type 2, 1.9 and 1.8; AGN2) with redshift $z \lesssim$0.1, selected from the Swift/BAT 70-month catalogue. The observations have…

Astrophysics of Galaxies · Physics 2016-10-21 F. Onori , F. La Franca , F. Ricci , M. Brusa , E. Sani , R. Maiolino , S. Bianchi , A. Bongiorno , F. Fiore , A. Marconi , C. Vignali

Chandra data in the COSMOS, AEGIS-XD and 4Ms CDFS are combined with optical/near-IR photometry to determine the rest-frame U-V vs V-J colours of X-ray AGN hosts at mean redshifts 0.40 and 0.85. This combination of colours (UVJ) provides an…

We compute black hole masses and bolometric luminosities for 87 obscured AGN in the redshift range 0.25 < z < 1.25, selected from the GOODS deep multi-wavelength survey fields via their X-ray emission. We fit the optical images and obtain…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 B. D. Simmons , J. Van Duyne , C. M. Urry , E. Treister , A. M. Koekemoer , N. A. Grogin , the GOODS Team

We present analyses of host galaxy properties of type 1 and type 2 X-ray selected AGNs in the XMM-XXL field, which have available optical spectroscopic classification. We model their optical to far-infrared spectral energy distributions…

Astrophysics of Galaxies · Physics 2021-09-15 G. Mountrichas , V. Buat , I. Georgantopoulos , G. Yang , V. A. Masoura , M. Boquien , D. Burgarella
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