Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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Materials Map under construction

The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (1/1 displayed)

  • 2013The Spitzer Mid-infrared Active Galactic Nucleus Survey. I. Optical and Near-infrared Spectroscopy of Obscured Candidates and Normal Active Galactic Nuclei Selected in the Mid-infrared88citations

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Gates, E. L.
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Lacy, M.
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Storrie-Lombardi, L. J.
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Sajina, A.
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Nielsen, D. M.
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Petric, A. O.
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Seymour, N.
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Cox Drews, S.
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Harrison, C.
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Urrutia, Tanya
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2013

Co-Authors (by relevance)

  • Gates, E. L.
  • Lacy, M.
  • Storrie-Lombardi, L. J.
  • Sajina, A.
  • Nielsen, D. M.
  • Petric, A. O.
  • Seymour, N.
  • Cox Drews, S.
  • Harrison, C.
  • Urrutia, Tanya
OrganizationsLocationPeople

article

The Spitzer Mid-infrared Active Galactic Nucleus Survey. I. Optical and Near-infrared Spectroscopy of Obscured Candidates and Normal Active Galactic Nuclei Selected in the Mid-infrared

  • Ridgway, S. E.
  • Gates, E. L.
  • Lacy, M.
  • Storrie-Lombardi, L. J.
  • Sajina, A.
  • Nielsen, D. M.
  • Petric, A. O.
  • Seymour, N.
  • Cox Drews, S.
  • Harrison, C.
  • Urrutia, Tanya
Abstract

We present the results of a program of optical and near-infrared spectroscopic follow-up of candidate active galactic nuclei (AGNs) selected in the mid-infrared. This survey selects both normal and obscured AGNs closely matched in luminosity across a wide range, from Seyfert galaxies with bolometric luminosities L <SUB>bol</SUB> ~ 10<SUP>10</SUP> L <SUB>☉</SUB> to highly luminous quasars (L <SUB>bol</SUB> ~ 10<SUP>14</SUP> L <SUB>☉</SUB>), all with redshifts ranging from 0 to 4.3. Samples of candidate AGNs were selected with mid-infrared color cuts at several different 24 μm flux density limits to ensure a range of luminosities at a given redshift. The survey consists of 786 candidate AGNs and quasars, of which 672 have spectroscopic redshifts and classifications. Of these, 137 (20%) are type 1 AGNs with blue continua, 294 (44%) are type 2 objects with extinctions A<SUB>V</SUB> &gt;~ 5 toward their AGNs, 96 (14%) are AGNs with lower extinctions (A<SUB>V</SUB> ~ 1), and 145 (22%) have redshifts, but no clear signs of AGN activity in their spectra. Of the survey objects 50% have L <SUB>bol</SUB> &gt; 10<SUP>12</SUP> L <SUB>☉</SUB>, in the quasar regime. We present composite spectra for type 2 quasars and objects with no signs of AGN activity in their spectra. We also discuss the mid-infrared—emission-line luminosity correlation and present the results of cross correlations with serendipitous X-ray and radio sources. The results show that: (1) obscured objects dominate the overall AGN population, (2) mid-infrared selected AGN candidates exist which lack AGN signatures in their optical spectra but have AGN-like X-ray or radio counterparts, and (3) X-ray and optical classifications of obscured and unobscured AGNs often differ....

Topics
  • density
  • composite
  • infrared spectroscopy
  • Near-infrared spectroscopy