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Related papers: Broad Line Emission in Low-Metallicity Blue Compac…

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We present 3.5m Apache Point Observatory second-epoch spectra of four low-metallicity emission-line dwarf galaxies discovered serendipitously in the Data Release 5 of the Sloan Digital Sky Survey (SDSS) to have extraordinary large broad…

Astrophysics · Physics 2018-05-30 Y. I. Izotov , T. X. Thuan

We present a sample of 22 massive galaxies with stellar masses $>10^{10} M_{\odot}$ at $3<z<4$ with deep H and K-band high resolution spectra (R=3500-3000) from Keck/MOSFIRE and VLT/KMOS near-infrared spectrographs. We find a large fraction…

Astrophysics of Galaxies · Physics 2024-05-24 M. Martínez-Marín , K. Glazebrook , T. Nanayakkara , C. Jacobs , I. Labbé , G. G. Kacprzak , C. Papovich , C. Schreiber

We report on continued, $\sim$15 year-long, broad Balmer emission lines in three metal-poor dwarf emission-line galaxies selected from Sloan Digital Sky Survey spectroscopy. The persistent luminosity of the broad Balmer emission indicates…

Astrophysics of Galaxies · Physics 2021-07-16 Colin J. Burke , Xin Liu , Yu-Ching Chen , Yue Shen , Hengxiao Guo

Using the Gemini Near-InfraRed Spectrograph (GNIRS), we have assembled a complete sample of 20 K-selected galaxies at 2.0<z<2.7 with high quality near-infrared spectra. As described in a previous paper, 9 of these 20 galaxies have strongly…

We present a sample of 151 dwarf galaxies (10^8.5 < M_stellar < 10^9.5 Msun) that exhibit optical spectroscopic signatures of accreting massive black holes (BHs), increasing the number of known active galaxies in this stellar mass range by…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Amy E. Reines , Jenny E. Greene , Marla Geha

We have investigated the broad-line Balmer decrements (Halpha/Hbeta) for a large, homogeneous sample of Seyfert 1 galaxies and QSOs using spectroscopic data obtained in the Sloan Digital Sky Survey. The sample, drawn from the Fourth Data…

Astrophysics · Physics 2009-11-13 Xiaobo Dong , Tinggui Wang , Jianguo Wang , Weimin Yuan , Hongyan Zhou , Haifeng Dai , Kai Zhang

Broad emission lines are emitted in the surroundings of supermassive black holes in the centers of active galactic nuclei (AGN). This region is spatially not resolved. We intend to get information on the structure and geometry of this broad…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 W. Kollatschny , M. Zetzl

This is the second paper in a series studying the star formation rates, stellar components, metallicities, and star formation histories and evolution of a sample of blue compact galaxies. We analyzed spectral properties of 97 blue compact…

Astrophysics · Physics 2009-11-07 X. Kong , F. Z. Cheng , A. Weiss , S. Charlot

We use time-domain optical spectroscopy to distinguish between broad emission lines powered by accreting black holes (BHs) or stellar processes (i.e., supernovae) for 16 galaxies identified as AGN candidates by Reines \etal (2013). Our…

We used the $H\alpha$ images from a large sample of nearby late-type dwarf galaxies to investigate properties of their emission structure. The sample consists of three hundred galaxies of the irregular (Irr), Magellanic irregular (Im), blue…

Astrophysics of Galaxies · Physics 2020-12-16 Karachentsev I. D. , Kaisin S. S

We present the results of an optical spectroscopic survey designed to search for low-luminosity, "dwarf" Seyfert nuclei in a magnitude-limited sample of 486 bright, northern galaxies. Moderate-resolution spectra of exceptionally high…

Astrophysics · Physics 2010-12-09 Luis C. Ho , Alexei V. Filippenko , Wallace L. W. Sargent , Chien Y. Peng

We selected 27244 nearby, red, giant early-type galaxies (RGEs) from the Sloan Digital Sky Survey (SDSS). In a large fraction (53%) of their spectra the [O III] emission line is detected, with an equivalent width (EW) distribution strongly…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Alessandro Capetti , Ranieri D. Baldi

According to the classical AGN model, broad emission lines originate from the broad-line region (BLR) and are observable only when the attenuation by the dusty torus is small. However, we recently found several heavily-obscured ($A_V > 50$…

Many classes of active galactic nuclei (AGN) have been observed and recorded since the discovery of Seyfert galaxies. In this paper, we examine the sample of luminous galaxies in the Baryon Oscillation Spectroscopic Survey (BOSS). We find a…

Astrophysics of Galaxies · Physics 2013-12-05 Ben Roig , Michael R. Blanton , Nicolas P. Ross

We present 6.5-meter MMT and 3.5m APO spectrophotometry of 69 H II regions in 42 low-metallicity emission-line galaxies, selected from the Data Release 7 of the Sloan Digital Sky Survey to have mostly [O III]4959/Hbeta < 1 and [N…

Cosmology and Nongalactic Astrophysics · Physics 2018-05-29 Y. I. Izotov , T. X. Thuan , N. G. Guseva

We present an analysis of the mid-infrared emission lines for a sample of 12 low metallicity Blue Compact Dwarf (BCD) galaxies based on high resolution observations obtained with Infrared Spectrograph on board the {\rm Spitzer} Space…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Lei Hao , Yanling Wu , V. Charmandaris , H. W. W. Spoon , J. Bernard-Salas , D. Devost , V. Lebouteiller , J. R. Houck

We present 6.5-meter MMT spectrophotometry of 20 H II regions in 13 extremely metal-poor emission-line galaxies selected from the Data Release 5 of the Sloan Digital Sky Survey to have [O III] 4959/Hbeta < 1 and [N II] 6583/Hbeta < 0.05.…

Astrophysics · Physics 2009-11-13 Y. I. Izotov , T. X. Thuan

Long-slit spectroscopy has been obtained for a sample of 22 blue dwarf galaxies selected in the direction of the Virgo Cluster as part of a larger sample of Virgo blue dwarf galaxies for which deep Halpha imaging has been collected. Most of…

Astrophysics · Physics 2009-11-07 J. M. Vilchez , J. Iglesias-Paramo

We compare the gas distribution, kinematics and the current star formation in a sample of 10 very faint (-13.37 < M_B < -9.55) dwarf galaxies. For 5 of these galaxies we present fresh, high sensitivity, GMRT HI 21cm observations. For all…

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