21,950 research outputs found
Optical spectroscopic observations of gamma-ray blazar candidates II. The 2013 KPNO campaign in the Northern Hemisphere
We recently started a systematic search of low-energy counterparts of the
unidentified gamma-ray sources (UGSs) listed in the Fermi-Large Area Telescope
(LAT) First Source Catalog (1FGL) and the Fermi-LAT 2-Year Source Catalog
(2FGL).} The main goal of our investigation is to find active galaxies
belonging to the blazar class that lie within the positional uncertainty region
of the UGSs and thus could be their potential low-energy counterparts. To
achieve our aims, we first adopted several procedures based on the peculiar
observational properties of blazars in the radio and in the IR. Then we carried
out a follow-up spectroscopic campaign in the optical band to verify the nature
of the candidates selected as potential counterparts of the UGSs. Here we
present the results of the observations carried out in 2013 in the Northern
Hemisphere at Kitt Peak National Observatory (KPNO). Optical spectroscopy is
crucial to confirm the nature of the sources and can be used to estimate their
redshifts; it will also allow us to test the robustness of our methods when the
whole campaign is completed. Here we present the optical spectroscopic
observations of 39 sources. Within our sample we found that 6 sources are
blazars, candidates to be low-energy counterparts of the UGSs listed in the
2FGL. We confirm that an additional 8 sources, previously classified as active
galaxies of uncertain type and associated in the 2FGL, are also all BL Lac
objects. Moreover, we also present 20 new spectra for known blazars listed in
the Multi-frequency Catalogue of Blazars as having an uncertain redshift and/or
being classified as BL Lac candidates. We conclude that our methods for
selecting gamma-ray blazar candidates allows us to discover new blazars and
increase the list of potential low-energy counterparts for the Fermi UGSs.Comment: 27 pages, 39 figures, 1 table, A&A accepted for publication
(pre-proof version
New blazars from the cross-match of recent multi-frequency catalogs
Blazars are radio-loud active galactic nuclei well known for their non
thermal emission spanning a wide range of frequencies. The Roma-BZCAT is, to
date, the most comprehensive list of these sources. We performed the
cross-match of several catalogs obtained from recent surveys at different
frequencies to search for new blazars. We cross-matched the 1 Swift-XRT
Point Source catalog with the spectroscopic sample of the 9 Data Release
of the Sloan Digital Sky Survey. Then, we performed further cross-matches with
the catalogs corresponding to the Faint Images of the Radio Sky at Twenty cm
survey and to the AllWISE Data release, focusing on sources with infrared
colors similar to those of confirmed -ray blazars included in the
Second Fermi-LAT catalog. As a result, we obtained a preliminary list of
objects with all the elements needed for a proper blazar classification
according to the prescriptions of the Roma-BZCAT. We carefully investigated
additional properties such as their morphology and the slope of their spectral
energy distribution in the radio domain, the features shown in their optical
spectrum, and the luminosity in the soft X rays to exclude generic active
galactic nuclei and focus on authentic blazar-like sources. At the end of our
screening we obtained a list of 15 objects with firmly established blazar
properties.Comment: 8 pages, 3 figures, 1 table. Accepted for publication in Astrophysics
and Space Science on 2015 April 25. Corrected typo in Section
Unveiling the nature of the unidentified gamma-ray sources III: gamma-ray blazar-like counterparts at low radio frequencies
About one third of the gamma-ray sources listed in the second Fermi LAT
catalog (2FGL) have no firmly established counterpart at lower energies so
being classified as unidentified gamma-ray sources (UGSs). Here we propose a
new approach to find candidate counterparts for the UGSs based on the 325 MHz
radio survey performed with Westerbork Synthesis Radio Telescope (WSRT) in the
northern hemisphere. First we investigate the low-frequency radio properties of
blazars, the largest known population of gamma-ray sources; then we search for
sources with similar radio properties combining the information derived from
the Westerbork Northern Sky Survey (WENSS) with those of the NRAO VLA Sky
survey (NVSS). We present a list of candidate counterparts for 32 UGSs with at
least one counterpart in the WENSS. We also performed an extensive research in
literature to look for infrared and optical counterparts of the gamma-ray
blazar candidates selected with the low-frequency radio observations to confirm
their nature. On the basis of our multifrequency research we identify 23 new
gamma-ray blazar candidates out of 32 UGSs investigated. Comparison with
previous results on the UGSs are also presented. Finally, we speculate on the
advantages on the use of the low-frequency radio observations to associate UGSs
and to search for gamma-ray pulsar candidates.Comment: 15 pages, 13 figures, 3 tables, ApJS accepted for publication
(version pre-proof corrections
Refining the associations of the Fermi Large Area Telescope Source Catalogs
The Fermi-Large Area Telescope (LAT) First Source Catalog (1FGL) was released
in February 2010 and the Fermi-LAT 2-Year Source Catalog (2FGL) appeared in
April 2012, based on data from 24 months of operation. Since their releases,
many follow up observations of unidentified gamma-ray sources (UGSs) were
performed and new procedures to associate gamma-ray sources with potential
counterparts at other wavelengths were developed. Here we review and
characterize all the associations as published in the 1FGL and 2FGL catalog on
the basis of multifrequency archival observations. In particular we located 177
spectra for the low-energy counterparts that were not listed in the previous
Fermi catalogs, and in addition we present new spectroscopic observations of 8
gamma-ray blazar candidates. Based on our investigations, we introduce a new
counterpart category of "candidate associations" and propose a refined
classification for the candidate low-energy counterparts of the Fermi sources.
We compare the 1FGL-assigned counterparts with those listed in the 2FGL to
determine which unassociated sources became associated in later releases of the
Fermi catalogs. We also search for potential counterparts to all the remaining
unassociated Fermi sources. Finally, we prepare a refined and merged list of
all the associations of the 1FGL plus 2FGL catalogs that includes 2219 unique
Fermi objects. This is the most comprehensive and systematic study of all the
associations collected for the gamma-ray sources available to date. We conclude
that 80% of the Fermi sources have at least one known plausible gamma-ray
emitter within their positional uncertainty regions.Comment: 26 pages, 24 figures, 7 tables, ApJS accepted for publication
(pre-proof version uploaded
Public Administration Education in Italy: a Statistical Analysis
The paper presents a statistical analysis exploring public administration education in Italian universities. It highlights the main specificities of PA education in Italy with reference to the disciplinary character, the geographical distribution, the type and level of PA programs, etc. and aims at describing how universities are adjusting curricula in relation to public sector modernization, by comparing the main faculties (economics and management sciences, law, political sciences, sociology, engineering, sciences of communication, social sciences) of all Italian universities.Public Administration; Education; Training; Disciplinary Approaches; Administrative Culture
Application of the MST clustering to the high energy gamma-ray sky. III - New detections of gamma-ray emission from blazars
We present the results of a photon cluster search in the gamma-ray sky
observed by the Fermi Large Area Telescope, using the new Pass 8 dataset, at
energies higher than 10 GeV. By means of the Minimum Spanning Tree (MST)
algorithm, we found 25 clusters associated with catalogued blazars not
previously known as gamma-ray emitters. The properties of these sources are
discussed.Comment: 10 pages, 3 figures. Accepted for publication in Astrophysics & Space
Scienc
Two new catalogs of blazar candidates in the WISE infrared sky
We present two catalogs of radio-loud candidate blazars whose WISE
mid-infrared colors are selected to be consistent with the colors of confirmed
gamma-ray emitting blazars. The first catalog is the improved and expanded
release of the WIBRaLS catalog presented by D'Abrusco et al. (2014): it
includes sources detected in all four WISE filters, spatially cross-matched
with radio source in one of three radio surveys and radio-loud based on their
q22 spectral parameter. WIBRaLS2 includes 9541 sources classified as BL Lacs,
FSRQs or mixed candidates based on their WISE colors. The second catalog,
called KDEBLLACS, based on a new selection technique, contains 5579 candidate
BL Lacs extracted from the population of WISE sources detected in the first
three WISE passbands ([3.4], [4.6] and [12]) only, whose mid-infrared colors
are similar to those of confirmed, gamma-ray BL Lacs. KDBLLACS members area
also required to have a radio counterpart and be radio-loud based on the
parameter q12, defined similarly to q22 used for the WIBRaLS2. We describe the
properties of these catalogs and compare them with the largest samples of
confirmed and candidate blazars in the literature. We crossmatch the two new
catalogs with the most recent catalogs of gamma-ray sources detected by Fermi
LAT instrument. Since spectroscopic observations of candidate blazars from the
first WIBRaLS catalog within the uncertainty regions of gamma-ray unassociated
sources confirmed that ~90% of these candidates are blazars, we anticipate that
these new catalogs will play again an important role in the identification of
the gamma-ray sky.Comment: 20 pages, 7 figures. Accepted for publication in The Astrophysical
Journal Supplement Serie
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