234 results on '"MILIA S."'
Search Results
2. The High Time Resolution Universe Survey - XI. Discovery of five recycled pulsars and the optical detectability of survey white dwarf companions
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Bates, S. D., Thornton, D., Bailes, M., Barr, E., Bassa, C. G., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., Champion, D. J., Flynn, C. M. L., Jameson, A., Johnston, S., Keith, M. J., Kramer, M., Levin, L., Lyne, A., Milia, S., Ng, C., Petroff, E., Possenti, A., Stappers, B. W., van Straten, W., and Tiburzi, C.
- Subjects
Astrophysics - Solar and Stellar Astrophysics - Abstract
We present the discovery of a further five recycled pulsar systems in the mid-Galactic latitude portion of the High Time Resolution Universe (HTRU) Survey. The pulsars have rotational periods ranging from 2 ms to 66 ms, and four are in binary systems with orbital periods between 10.8 hours and 9.0 days. Three of these binary systems are particularly interesting; PSR J1227-6208 has a pulse period of 34.5 ms and the highest mass function of all pulsars with near-circular orbits. The circular orbit suggests that the companion is not another neutron star, so future timing experiments may reveal one of the heaviest white dwarfs ever found ($>$ 1.3 M$_\odot$). Timing observations of PSR J1431$-$4715 indicate that it is eclipsed by its companion which has a mass indicating it belongs to the redback class of eclipsing millisecond pulsars. PSR J1653-2054 has a companion with a minimum mass of only $0.08$ M$_\odot$, placing it among the class of pulsars with low-mass companions. Unlike the majority of such systems, however, no evidence of eclipses is seen at 1.4 GHz., Comment: 11 pages, 6 figures, 4 tables
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- 2014
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3. The High Time Resolution Universe Survey - IX: Polarimetry of long-period pulsars
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Tiburzi, C., Johnston, S., Bailes, M., Bates, S. D., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., Champion, D., Coster, P., D'Amico, N., Keith, M. J., Kramer, M., Levin, L., Milia, S., Ng, C., Possenti, A., Stappers, B. W., Thornton, D., and van Straten, W.
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present a polarimetric analysis of 49 long-period pulsars discovered as part of the High Time Resolution Universe (HTRU) southern survey. The sources exhibit the typical characteristics of "old" pulsars, with low fractional linear and circular polarisation and narrow, multicomponent profiles. Although the position angle swings are generally complex, for two of the analysed pulsars (J1622-3751 and J1710-2616) we obtained an indication of the geometry via the rotating vector model. We were able to determine a value of the rotation measure (RM) for 34 of the sources which, when combined with their dispersion measures (DM), yields an integrated magnetic field strength along the line of sight. With the data presented here, the total number of values of RM associated to pulsars discovered during the HTRU southern survey sums to 51. The RMs are not consistent with the hypothesis of a counter-clockwise direction of the Galactic magnetic field within an annulus included between 4 and 6 kpc from the Galactic centre. A partial agreement with a counter-clockwise sense of the Galactic magnetic field within the spiral arms is however found in the area of the Carina-Sagittarius arm., Comment: 18 pages, 5 figures, 2 tables, accepted by MNRAS
- Published
- 2013
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4. The High Time Resolution Universe Pulsar Survey - VII: discovery of five millisecond pulsars and the different luminosity properties of binary and isolated recycled pulsars
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Burgay, M., Bailes, M., Bates, S. D., Bhat, N. D. R., Burke-Spolaor, S., Champion, D. J., Coster, P., D'Amico, N., Johnston, S., Keith, M. J., Kramer, M., Levin, L., Lyne, A. G., Milia, S., Ng, C., Possenti, A., Stappers, B. W., Thornton, D., Tiburzi, C., van Straten, W., and Bassa, C. G.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
This paper presents the discovery and timing parameters for five millisecond pulsars (MSPs), four in binary systems with probable white dwarf companions and one isolated, found in ongoing processing of the High Time Resolution Universe Pulsar Survey (HTRU). We also present high quality polarimetric data on four of them. These further discoveries confirm the high potential of our survey in finding pulsars with very short spin periods. At least two of these five MSPs are excellent candidates to be included in the Pulsar Timing Array projects. Thanks to the wealth of MSP discoveries in the HTRU survey, we revisit the question of whether the luminosity distributions of isolated and binary MSPs are different. Using the Cordes and Lazio distance model and our new and catalogue flux density measurements, we find that 41 of the 42 most luminous MSPs in the Galactic disk are in binaries and a statistical analysis suggests that the luminosity functions differ with 99.9% significance. We conclude that the formation process that leads to solitary MSPs affects their luminosities, despite their period and period derivatives being similar to those of pulsars in binary systems., Comment: 11 pages, 7 figures
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- 2013
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5. A Population of Fast Radio Bursts at Cosmological Distances
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Thornton, D., Stappers, B., Bailes, M., Barsdell, B. R., Bates, S. D., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., Champion, D. J., Coster, P., D'Amico, N., Jameson, A., Johnston, S., Keith, M. J., Kramer, M., Levin, L., Milia, S., Ng, C., Possenti, A., and van Straten, W.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
Searches for transient astrophysical sources often reveal unexpected classes of objects that are useful physical laboratories. In a recent survey for pulsars and fast transients we have uncovered four millisecond-duration radio transients all more than 40{\deg} from the Galactic plane. The bursts' properties indicate that they are of celestial rather than terrestrial origin. Host galaxy and intergalactic medium models suggest that they have cosmological redshifts of 0.5 to 1, and distances of up to 3 gigaparsecs. No temporally coincident x- or gamma-ray signature was identified in association with the bursts. Characterization of the source population and identification of host galaxies offers an opportunity to determine the baryonic content of the Universe., Comment: 20 pages, 6 figures, 2 tables. Energies in table 1 corrected from hard-copy version
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- 2013
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6. The High Time Resolution Universe Pulsar Survey VIII: The Galactic millisecond pulsar population
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Levin, L., Bailes, M., Barsdell, B. R., Bates, S. D., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., Champion, D. J., Coster, P., D'Amico, N., Jameson, A., Johnston, S., Keith, M. J., Kramer, M., Milia, S., Ng, C., Possenti, A., Stappers, B., Thornton, D., and van Straten, W.
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We have used millisecond pulsars (MSPs) from the southern High Time Resolution Universe (HTRU) intermediate latitude survey area to simulate the distribution and total population of MSPs in the Galaxy. Our model makes use of the scale factor method, which estimates the ratio of the total number of MSPs in the Galaxy to the known sample. Using our best fit value for the z-height, z=500 pc, we find an underlying population of MSPs of 8.3(\pm 4.2)*10^4 sources down to a limiting luminosity of L_min=0.1 mJy kpc^2 and a luminosity distribution with a steep slope of d\log N/d\log L = -1.45(\pm 0.14). However, at the low end of the luminosity distribution, the uncertainties introduced by small number statistics are large. By omitting very low luminosity pulsars, we find a Galactic population above L_min=0.2 mJy kpc^2 of only 3.0(\pm 0.7)*10^4 MSPs. We have also simulated pulsars with periods shorter than any known MSP, and estimate the maximum number of sub-MSPs in the Galaxy to be 7.8(\pm 5.0)*10^4 pulsars at L=0.1 mJy kpc^2. In addition, we estimate that the high and low latitude parts of the southern HTRU survey will detect 68 and 42 MSPs respectively, including 78 new discoveries. Pulsar luminosity, and hence flux density, is an important input parameter in the model. Some of the published flux densities for the pulsars in our sample do not agree with the observed flux densities from our data set, and we have instead calculated average luminosities from archival data from the Parkes Telescope. We found many luminosities to be very different than their catalogue values, leading to very different population estimates. Large variations in flux density highlight the importance of including scintillation effects in MSP population studies., Comment: 13 pages, 5 figures, 5 tables. Accepted for publication in MNRAS
- Published
- 2013
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7. The High Time Resolution Universe Survey VI: An Artificial Neural Network and Timing of 75 Pulsars
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Bates, S. D., Bailes, M., Barsdell, B. R., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., Champion, D. J., Coster, P., D'Amico, N., Jameson, A., Johnston, S., Keith, M. J., Kramer, M., Levin, L., Lyne, A., Milia, S., Ng, C., Nietner, C., Possenti, A., Stappers, B., Thornton, D., and van Straten, W.
- Subjects
Astrophysics - Solar and Stellar Astrophysics - Abstract
We present 75 pulsars discovered in the mid-latitude portion of the High Time Resolution Universe survey, 54 of which have full timing solutions. All the pulsars have spin periods greater than 100 ms, and none of those with timing solutions are in binaries. Two display particularly interesting behaviour; PSR J1054-5944 is found to be an intermittent pulsar, and PSR J1809-0119 has glitched twice since its discovery. In the second half of the paper we discuss the development and application of an artificial neural network in the data-processing pipeline for the survey. We discuss the tests that were used to generate scores and find that our neural network was able to reject over 99% of the candidates produced in the data processing, and able to blindly detect 85% of pulsars. We suggest that improvements to the accuracy should be possible if further care is taken when training an artificial neural network; for example ensuring that a representative sample of the pulsar population is used during the training process, or the use of different artificial neural networks for the detection of different types of pulsars., Comment: 15 pages, 8 figures
- Published
- 2012
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8. Radio emission evolution, polarimetry and multifrequency single pulse analysis of the radio magnetar PSR J1622-4950
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Levin, L., Bailes, M., Bates, S. D., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., D'Amico, N., Johnston, S., Keith, M. J., Kramer, M., Milia, S., Possenti, A., Stappers, B., and van Straten, W.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
Here we report on observations of the radio magnetar PSR J1622-4950 at frequencies from 1.4 to 17 GHz. We show that although its flux density is varying up to a factor of ~10 within a few days, it has on average decreased by a factor of 2 over the last 700 days. At the same time, timing analysis indicates a trend of decreasing spin-down rate over our entire data set, again of about a factor of 2 over 700 days, but also an erratic variability in the spin-down rate within this time span. Integrated pulse profiles are often close to 100 per cent linearly polarized, but large variations in both the profile shape and fractional polarization are regularly observed. Furthermore, the behaviour of the position angle of the linear polarization is very complex - offsets in both the absolute position angle and the phase of the position angle sweep are often seen and the occasional presence of orthogonal mode jumps further complicates the picture. However, model fitting indicates that the magnetic and rotation axes are close to aligned. Finally, a single pulse analysis has been carried out at four observing frequencies, demonstrating that the wide pulse profile is built up of narrow spikes of emission, with widths that scale inversely with observing frequency. All three of the known radio magnetars seem to have similar characteristics, with highly polarized emission, time-variable flux density and pulse profiles, and with spectral indices close to zero., Comment: 12 pages, 8 figures, 2 tables; Monthly Notices of the Royal Astronomical Society, Online Early
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- 2012
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9. The High Time Resolution Universe Pulsar Survey IV: Discovery and polarimetry of millisecond pulsars
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Keith, M. J., Johnston, S., Bailes, M., Bates, S. D., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., D'Amico, N., Jameson, A., Kramer, M., Levin, L., Milia, S., Possenti, A., Stappers, B. W., van Straten, W., and Parent, D.
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present the discovery of six millisecond pulsars (MSPs) in the High Time Resolution Universe (HTRU) survey for pulsars and fast transients carried out with the Parkes radio telescope. All six are in binary systems with approximately circular orbits and are likely to have white dwarf companions. PSR J1017-7156 has a high flux density and a narrow pulse width, making it ideal for precision timing experiments. PSRs J1446-4701 and J1125-5825 are coincident with gamma-ray sources, and folding the high-energy photons with the radio timing ephemeris shows evidence of pulsed gamma-ray emission. PSR J1502-6752 has a spin period of 26.7 ms, and its low period derivative implies that it is a recycled pulsar. The orbital parameters indicate it has a very low mass function, and therefore a companion mass much lower than usually expected for such a mildly recycled pulsar. In addition we present polarisation profiles for all 12 MSPs discovered in the HTRU survey to date. Similar to previous observations of MSPs, we find that many have large widths and a wide range of linear and circular polarisation fractions. Their polarisation profiles can be highly complex, and although the observed position angles often do not obey the rotating vector model, we present several examples of those that do. We speculate that the emission heights of MSPs are a substantial fraction of the light cylinder radius in order to explain broad emission profiles, which then naturally leads to a large number of cases where emission from both poles is observed., Comment: Update to correct affiliation for CAASTRO. 16 pages, 18 figures. Accepted for publication in MNRAS
- Published
- 2011
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10. Transformation of a Star into a Planet in a Millisecond Pulsar Binary
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Bailes, M., Bates, S. D., Bhalerao, V., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., D'Amico, N., Johnsto, S., Keith, M. J., Kramer, M., Kulkarni, S. R., Levin, L., Lyne, A. G., Milia, S., Possenti, A., Spitler, L., Stappers, B., and van Straten, W.
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Earth and Planetary Astrophysics - Abstract
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter from a binary companion. Although most are in binary systems, some 30% are solitary, and their origin is therefore mysterious. PSR J1719-1438, a 5.7 ms pulsar, was detected in a recent survey with the Parkes 64m radio telescope. We show that it is in a binary system with an orbital period of 2.2 h. Its companion's mass is near that of Jupiter, but its minimum density of 23 g cm$^{-3}$ suggests that it may be an ultra-low mass carbon white dwarf. This system may thus have once been an Ultra Compact Low-Mass X-ray Binary, where the companion narrowly avoided complete destruction., Comment: 16 pages, 3 figures. Science Express, in press
- Published
- 2011
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11. The High Time Resolution Universe Survey - III. Single-pulse searches and preliminary analysis
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Burke-Spolaor, S., Bailes, M., Johnston, S., Bates, S. D., Bhat, N. D. R, Burgay, M., D'Amico, N., Jameson, A., Keith, M. J., Kramer, M., Levin, L., Milia, S., Possenti, A., Stappers, B., and van Straten, W.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
We present the search methods and initial results for transient radio signals in the High Time Resolution Universe (HTRU) Survey. The HTRU survey's single-pulse search, the software designed to perform the search, and a determination of the HTRU survey's sensitivity to single pulses are described. Initial processing of a small fraction of the survey has produced 11 discoveries, all of which are sparsely-emitting neutron stars, as well as provided confirmation of two previously unconfirmed neutron stars. Most of the newly discovered objects lie in regions surveyed previously, indicating both the improved sensitivity of the HTRU survey observing system and the dynamic nature of the radio sky. The cycles of active and null states in nulling pulsars, rotating radio transients (RRATs), and long-term intermittent pulsars are explored in the context of determining the relationship between these populations, and of the sensitivity of a search to the various radio-intermittent neutron star populations. This analysis supports the case that many RRATs are in fact high-null-fraction pulsars (i. e. with null fraction >~0.95), and indicates that intermittent pulsars appear distinct from nulling pulsars in their activity cycle timescales. We find that in the measured population, there is a deficit of pulsars with typical emission timescales greater than ~300 s that is not readily explained by selection effects. The HTRU low-latitude survey will be capable of addressing whether this deficit is physical. We predict that the HTRU survey will explore pulsars with a broad range of nulling fractions (up to and beyond 0.999), and at its completion is likely to increase the currently known RRATs by a factor of more than two., Comment: 14 pages, 7 figures. Accepted to MNRAS
- Published
- 2011
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12. The High Time Resolution Universe Survey II: Discovery of 5 Millisecond Pulsars
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Bates, S. D., Bailes, M., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., D'Amico, N., Jameson, A., Johnston, S., Keith, M. J., Kramer, M., Levin, L., Lyne, A., Milia, S., Possenti, A., Stappers, B., and van Straten, W.
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present the discovery of 5 millisecond pulsars found in the mid-Galactic latitude portion of the High Time Resolution Universe (HTRU) Survey. The pulsars have rotational periods from ~2.3 to ~7.5 ms, and all are in binary systems with orbital periods ranging from ~0.3 to ~150 d. In four of these systems, the most likely companion is a white dwarf, with minimum masses of ~0.2 Solar Masses. The other pulsar, J1731-1847, has a very low mass companion and exhibits eclipses, and is thus a member of the "black widow" class of pulsar binaries. These eclipses have been observed in bands centred near frequencies of 700, 1400 and 3000 MHz, from which measurements have been made of the electron density in the eclipse region. These measurements have been used to examine some possible eclipse mechanisms. The eclipse and other properties of this source are used to perform a comparison with the other known eclipsing and "black widow" pulsars. These new discoveries occupy a short-period and high-dispersion measure (DM) region of parameter space, which we demonstrate is a direct consequence of the high time and frequency resolution of the HTRU survey. The large implied distances to our new discoveries makes observation of their companions unlikely with both current optical telescopes and the Fermi Gamma-ray Space Telescope. The extremely circular orbits make any advance of periastron measurements highly unlikely. No relativistic Shapiro delays are obvious in any of the systems, although the low flux densities would make their detection difficult unless the orbits were fortuitously edge-on., Comment: 11 pages, 5 figures, 4 tables, for publication in MNRAS
- Published
- 2011
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13. The High Time Resolution Universe Pulsar Survey I: System configuration and initial discoveries
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Keith, M. J., Jameson, A., van Straten, W., Bailes, M., Johnston, S., Kramer, M., Possenti, A., Bates, S. D., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., D'Amico, N., Levin, L., McMahon, P. L., Milia, S., and Stappers, B. W.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Solar and Stellar Astrophysics - Abstract
We have embarked on a survey for pulsars and fast transients using the 13-beam Multibeam receiver on the Parkes radio telescope. Installation of a digital backend allows us to record 400 MHz of bandwidth for each beam, split into 1024 channels and sampled every 64 us. Limits of the receiver package restrict us to a 340 MHz observing band centred at 1352 MHz. The factor of eight improvement in frequency resolution over previous multibeam surveys allows us to probe deeper into the Galactic plane for short duration signals such as the pulses from millisecond pulsars. We plan to survey the entire southern sky in 42641 pointings, split into low, mid and high Galactic latitude regions, with integration times of 4200, 540 and 270 s respectively. Simulations suggest that we will discover 400 pulsars, of which 75 will be millisecond pulsars. With ~30% of the mid-latitude survey complete, we have re-detected 223 previously known pulsars and discovered 27 pulsars, 5 of which are millisecond pulsars. The newly discovered millisecond pulsars tend to have larger dispersion measures than those discovered in previous surveys, as expected from the improved time and frequency resolution of our instrument., Comment: Updated author list. 10 pages, 7 figures. For publication in MNRAS
- Published
- 2010
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14. Preliminary Evaluation of Sharon-Anammox Process Feasibility to Treat Ammonium-Rich Effluents Produced by Double-Stage Anaerobic Digestion of Food Waste
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Milia, S., Tocco, G., Erby, G., De Gioannis, G., Carucci, A., di Prisco, Marco, Series editor, Chen, Sheng-Hong, Series editor, Solari, Giovanni, Series editor, Vayas, Ioannis, Series editor, and Mannina, Giorgio, editor
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- 2017
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15. Transfer of results of the MAECI MINCYT proyect to areas impacted with heavy metals from volcanism
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Scotti, A., Silvani, V., Milia, S., Guglietta, D., Castaño-Gañan, A., Godeas, Alicia, García-Romera, Inmaculada, Cappai, G., Colombo, R., Trapasso, F., Gómez-Martín, P., Izaguirre, M.L., Ubaldini, S., Scotti, A., Silvani, V., Milia, S., Guglietta, D., Castaño-Gañan, A., Godeas, Alicia, García-Romera, Inmaculada, Cappai, G., Colombo, R., Trapasso, F., Gómez-Martín, P., Izaguirre, M.L., and Ubaldini, S.
- Published
- 2023
16. Bioaugmentation-Assisted Phytostabilisation of Abandoned Mine Sites in South West Sardinia
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Tamburini, E., Sergi, S., Serreli, L., Bacchetta, G., Milia, S., Cappai, G., and Carucci, A.
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- 2017
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17. Ammonium recovery from agro-industrial digestate using bioelectrochemical systems
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Carucci, A., primary, Erby, G., additional, Puggioni, G., additional, Spiga, D., additional, Frugoni, F., additional, and Milia, S., additional
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- 2022
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18. SRT performance measurements (2018-2021)
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Egron, Elise, Vacca, V., Carboni, G., Pili, M., Loru, S., Castangia, P., Pellizzoni, Alberto, SERRA, Giampaolo, IACOLINA, Maria Noemi, VALENTE, Giuseppe, ATTOLI, Alessandro, Buffa, F., Mulas, S., Perrodin, D., Poppi, S., Bachetti, M., Burgay, M., Caria, M. T., Carretti, E., Casu, S., Concu, R., Corongiu, A., Deiana, G. L., Fara, Antonietta, Gaudiomonte, F., Ladu, A., MARCHEGIANI, Paolo, MAXIA, PAOLO, Melis, A., Milia, S., Migoni, C., Navarrini, A., Orlati, A., Ortu, P., Palmas, S., Pilia, M., Pisanu, T., SABA, Andrea, Schirru, L., Soletta, P., Surcis, G., Tarchi, A., URRU, Enrico, VARGIU, GIAN PAOLO, RIGHINI, SIMONA, and BOLLI, Pietro
- Abstract
Tests of characterization are periodically performed at SRT in order to check the status of the antenna, ensure a good functioning of the different components (e.g. active surface, receivers, backends, etc), and improve the observing performances at the different frequencies. In particular, the tests include measurements of beam shape, pointing, gain curves and focus for the different receivers (L, C, X and K-bands). We report the results of the main tests carried out after a long stop of the antenna due to the reparation of the main servo motors chillers in 2020 and compare them with those carried out during the recommissioning in 2018 (after the change of the actuators of the active surface). These results will be useful in order to compare the new status of the antenna after the upgrade of the new receivers at higher frequency (PON).
- Published
- 2022
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19. Landfill gas generation after mechanical biological treatment of municipal solid waste. Estimation of gas generation rate constants
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Gioannis, G. De, Muntoni, A., Cappai, G., and Milia, S.
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- 2009
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20. Multidisciplinary Strategy for Optimised Management and Sustainable Recovery of Secondary and Critical Raw Materials from Mining Residues
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Milia S., Cappai G., Silvani V., Scotti A., Salvatori R., Passeri D., Trapasso F., Colombo R., Godeas A., Ubaldini S., and Guglietta D.
- Subjects
recovery ,mining residues ,circular economy ,critical raw materials ,secondary raw materials - Abstract
New strategies implementing a resource-efficient and competitive economy, which transforms environmental problems into opportunities, are encouraged at global scale (UN Sustainable Development Goals, SDG). In recent years, mine residues are attracting scientific interest, since they can turn into viable sources of secondary and critical raw materials (SRMs and CRMs). Planning the sustainable supply and circular use of resources, integrating incomplete information, providing environmentally sound technologies for the simultaneous reduction of environmental risks and recovery of SRMs and CRMs are the key steps for overcoming such ambitious challenges. In this study, a multidisciplinary and eco-sustainable strategy is presented for the characterization, mapping, classification and valorization of mine residues.
- Published
- 2021
21. DEVELOPMENT OF AN INTEGRATED MULTIDISCIPLINARY STRATEGY FOR GALLIUM, IRON AND MANGANESE RECOVERY FROM MINING RESIDUES IN A CONTEXT OF CIRCULAR ECONOMY
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Scotti A, Milia S, Cappai G, Silvani V, Guglietta D, Trapasso F, Belardi G, Salvatori R, Tempesta E, Passeri D, Ubaldini S, Godeas A, Babay P, Gonzalez F, Leguizamón R, and Gómez M.
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Phytomycoremediation ,Environmental technologies ,Hydrometallurgy ,Mining Resource Recovery ,Remote sensing ,Circular Economy ,Hydrometallurgy Techniques ,Remote Sensing Map ,Secondary raw materials ,Phytoremediation - Abstract
Mining and mineral-processing wastes have been giving a lot of concern in recent times. We have evaluated an integrated multidisciplinary strategy for mining residues characterization, as well as for the recovery of secondary (e.g., Fe, Mn) and critical (e.g., Ga) raw materials. After the in situ sampling campaigns in Bichakundi Joda West iron and manganese mine (Keonjhar district, State of Odisha, India), residues have been characterized and the acquired mineralogical, chemical and spectral information have been used to create a map of mining residue deposits by means of the new multispectral satellite Sentinel-2A classification. Furthermore, mycorrhizal-assisted phytoextraction of metals from previously classified soils, based on sunflowers colonized by an AM fungal strain GA5 Rhizophagus intraradices, was carried out in the perspective of subsequent recovery of Ga, Fe and Mn from biomass using hydrometallurgical and electrochemical techniques. The bioconcentration factors in aerial and radicular parts (BCS and BCR, respectively), and translocation factors (TF) followed the order Ga>Mn>Fe for BCS and TF, while for BCR was Ga>Fe>Mn. The results were used to estimate the bioextracting potential by phyto-mycoremediation into a Vegetable Depuration Module (VDM): the highest extraction was estimated for Fe (60 g/VDM), followed by Mn (35 g/VDM) and Ga (1.02 g/VDM), thus confirming a good potential for their subsequent recovery by hydrometallurgical techniques with final purification by selective electrodeposition. Results are encouraging and the application of such multidisciplinary approach can be important to develop a circular model for sustainable exploitation of mining residues.
- Published
- 2020
22. Simultaneous denitrification and desalination of groundwater in 3-chamber BES configuration
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Puggioni G., Milia S., Dessì E., Unali V., Pous N., Puig S., and Carucci A.
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denitrification ,BES ,groundwater - Published
- 2020
23. Sustainable management and optimization of mining wastes: an integrated multidisciplinary approach
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Daniela Guglietta, Belardi G., Cappai G., Godeas A., Milia S., Passeri D., Salvatori R., Scotti A., Silvani V., Tempesta E., and Trapasso F.
- Subjects
remediation ,recycle ,remote sensing analysis ,reuse ,mining wastes - Abstract
Our economy needs to collect raw materials (RMs) from mining activities and this produces an impressive amount of mining wastes and a number of environmental problems associated with the disposal of them. Nowadays, the advances of the innovative technologies and markets make mining waste sources of valuable minerals/elements, but, in order to exploit them, it is necessary to know accurate information and to develop smart strategies of management and planning. In this framework, we tested an integrated multidisciplinary approach for sustainable management and optimisation of mining wastes. We sampled iron (Fe) and manganese (Mn) wastes produced in Joda West Mine (State of Odisha-India). Afterward, X-Ray Powde r Diffraction, X-Ray Fluorescence and spectral signatures analysis were used in order to characterize the mining waste samples. Mineralogical, chemical and spectral data were used as input to classify Sentinel-2A image. The characterized mining waste map identified waste deposit areas with different percentage of Fe and Mn and represented a suitable tool for further optimizing strategies of mining waste management. In particular, the potentialities of phyto-mycoremediation of classified mining wastes for heavy metals up take and bioaccumulation were evaluated, in the perspective of their subsequent recovery from biomass through hydrometallurgical methods. The mycorrhized plant species tolerated the high concentrations of metals and were effective for the phytostabilization and phytoextraction of Cr, Cu, Ni, Sr, Zn, Mn, Fe, P, As, S, Sr, P and Rb although overall biomass growth was not suf ficient to sustain a significant recovery of heavy metals at this stage (i. e., process conditions should be optimized). Preliminary results showed that an approach based on both advanced techniques and low cost treatment methods successfully lead to significant waste reduction and materials recovery.
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- 2020
- Full Text
- View/download PDF
24. Application of the ELAN® anammox based process to treat digested blackwater in a decentralized wastewater system
- Author
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Tocco G., Pedrouso A., Val del Rio A., Carucci A., Morales N., Milia S., and Mosquera-Corral A.
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Anammox ,Nitritation ,Wastewater source separation ,Blackwater ,Starvation ,Decentralized systems - Abstract
Wastewater source-separation and on-site treatment systems face severe problems of wastewater availability. Therefore, the effect of repeated short-term starvation and reactivation periods on a partial nitritation-anammox (PN/AMX) based process was assessed treating digested blackwater at room temperature. First, two sequencing batch reactors (SBR) were operated in continuous mode (SBR-C, which served as control) and with repeated starvation/reactivation periods during the nights and the weekends (SBR-D), using simulated blackwater (300 mg N/L and 200 mg COD/L) as substrate. The results showed no remarkable difference in overall process performance between both reactors, achieving total nitrogen removal efficiencies (NRE) around 90 %. Furthermore, no significant variations were measured in specific activities, except for the aerobic heterotrophic one that was lower in SBR-D, presumably due to the exposure to anoxic conditions. Then, the technical feasibility of applying the PN/AMX system to treat real blackwater produced in an office building during working hours was successfully proved in a third reactor (SBR-R), with the same starvation/reactivation periods tested in SBR-D. Despite the low temperature, ranging from 14 to 21 °C, total NRE up to 95 % and total nitrogen concentration in the effluent lower than 10 mg N/L were achieved. Moreover, a good recovery of the PN/AMX process performance after a long starvation period of 15 days (simulating holidays) was observed. Results proved for the first time the feasibility and long-term stability (100 days) of the PN/AMX process for the treatment (and potential reuse) of blackwater in a decentralized system, with repeated starvation/reactivation periods and after long starvation.
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- 2019
25. Unbiodegradable soluble COD removal from industrial wastewater by a hybrid moving bed biofilm reactor
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Carucci A., Cappai G., Camedda C., Erby G., Puggioni G., Milia S., and Tocco G.
- Subjects
industrial wastewater ,usCOD ,recalcitrant organics ,MBBR ,plastics industry - Abstract
In this study, plastics industry wastewater (PIWW) characterized by high total and soluble chemical oxygen demand (tCOD and sCOD, up to ~2200 and ~1500 mg/L, respectively) and remarkable unbiodegradable soluble COD (usCOD, 508±224 mg/L, 31±14% of tCOD) concentrations was treated at laboratory scale using a hybrid moving bed biofilm reactor (MBBR). Interestingly, the MBBR showed average tCOD, sCOD and usCOD removal efficiencies of 26±6, 32±11 and 36±11%, respectively, which were comparable to those achieved by the coagulation/flocculation pre-treatment currently applied at full-scale. Such results encourage the application of MBBR as a cost-effective option for the removal of recalcitrant soluble organics from PIWW and other similar industrial wastewaters.
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- 2019
26. Identification of a new allele, HLA-DRB1*1366
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Milia, S., Lai, S., Valentini, T., Testi, M., Cappai, L., Moscetti, A., Mariani, M., Alba, F., and Carcassi, C.
- Published
- 2005
27. Cyclical variation of plasma lipids, apolipoproteins, and lipoprotein(a) during menstrual cycle of normal women
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Tonolo, G., Ciccarese, M., Brizzi, P., Milia, S., Dessole, S., Pussu, L., Secchi, G., and Maioli, M.
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Menstrual cycle -- Physiological aspects ,Lipid metabolism -- Physiological aspects ,Hormones, Sex -- Physiological aspects ,Coronary heart disease -- Risk factors ,Biological sciences - Abstract
Sixteen nulliparous healthy women with ages ranging from 25 to 36 yrs. participated in a study to determine the effects of hormonal changes associated with the menstrual cycle on lipid and lipoprotein levels in the blood. The results show that endogenous female sex hormones modulate the plasma levels of lipids and apolipoproteins, including lipoprotein(a). Thus, the phase of the menstrual cycle should be taken into consideration when evaluating the lipid risk profile of women who have not reached menopause.
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- 1995
28. Effects of different operating conditions on sediment slurry sequencing batch reactors treating marine port sediments contaminated by PAHs
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Milia S., Camedda C., Erby G., and Carucci A.
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polycyclic aromatic hydrocarbons ,sediment slurry ,marine sediments ,biostimulation ,SBR - Abstract
Due to intensive anthropic activities, marine port sediments are often contaminated by organic pollutants like polycyclic aromatic hydrocarbons (PAHs), which represent a significant environmental threat. In this study, two sediment slurry sequencing batch reactors (SS-SBRs) were used to biologically degrade a mixture of PAHs (namely fluorene, phenanthrene, fluoranthene and pyrene) from marine sediments dredged from Cagliari (Italy) and El Kantaoui (Tunisia) ports. To enhance PAHs removal by biostimulation, nutrients were added in both sediments, acetate was used as co-substrate (El Kantaoui, SS-SBR1), and saponins were used as surfactants (Cagliari, SS-SBR2). Moreover, different levels of contamination (up to 200 mgPAHtot/kgdw in SS-SBR1; up to 400 mgPAHtot/kgdw in SS-SBR2) and solid to liquid ratios (S/L, up to 0.2 in SS-SBR1; up to 0.1 in SS-SBR2) were applied. As to SS-SBR1, the highest average removal efficiencies (99-100% and 98-100% for 3- and 4-ring PAHs, respectively) were achieved when the level of contamination and S/L were set at 200 mgPAHtot/kgdw and 0.1, 150 mgPAHtot/kgdw and 0.13, and 150 mgPAHtot/kgdw and 0.20, respectively; as to SS-SBR2, very high average removal efficiencies (99,100% and 98,100% for 3- and 4-ring PAHs, respectively) were observed during the whole experimental campaign. Such results are promising and provide a useful background for testing other important operating parameters (e.g., the volumetric exchange ratio).
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- 2017
29. Preliminary evaluation of microbial fuel cells applicability to bioremediate marine sediments contaminated by polycyclic aromatic hydrocarbons
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Milia S., Camedda C., Erby G., Mascia M., Virdis B., and Carucci A.
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phenanthrene ,microbial fuel cells ,bioremediation ,polycyclic aromatic hydrocarbons ,marine sediments - Abstract
This study reports a preliminary evaluation of applicability of sediment microbial fuel cells (SMFCs) to bioremediate marine sediments contaminated by phenanthrene, a polycyclic aromatic hydrocarbon (PAH). The anodic compartments of two SMFCs were batch-fed with a slurry (5% w/w real dry sediment in artificial seawater) contaminated with phenanthrene (200 mg/kgdw), while the corresponding cathodic compartments were filled with 0.5 M K3[Fe(CN)6]. Both anode and cathode consisted of a piece of conductive graphite felt (4 cm2). A cation-permeable membrane was used to separate the compartments. SMFC-1 was operated in static conditions, whereas mechanical stirring was applied in SMFC-2. Good phenanthrene removals were achieved in SMFC-1 (61%) and SMFC-2 (88.5%) after 20 days of operation; mechanical stirring played a role in accelerating phenanthrene degradation. Biocatalytic activity was characterized by linear sweep voltammetries: maximum power densities and optimal current densities in SMFC-1 and -2 were 9.2 and 38.4 ?W/cm2, and 26.2 and 142.7 ?A/cm2, respectively. Such promising results are putatively associated to the capability of electroactive microorganisms to promote phenanthrene degradation at the anodes. The use of electrodes as electron sink in electrochemical remediation of contaminated slurries deserves further investigation, since it represents a cost-effective alternative to conventional treatments requiring energy-consuming aeration.
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- 2017
30. Evaluation of nitrous oxide gaseous emissions from a partial nitritation reactor operating under different conditions
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Milia S., Tocco G., Erby G., and Carucci A.
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ammonium ,nitrous oxide ,greenhouse gas emissions ,partial nitritation ,alkalinity - Abstract
In this study, continuous measurements of nitrous oxide gaseous emissions from a lab-scale partial nitritation (PN) chemostat treating ammonium-rich (1500 mgN/L) synthetic wastewater were performed, in order to achieve a deeper knowledge about its potential environmental impact. The reactor was operated at constant hydraulic retention time (HRT, 1 d) and nitrogen loading rate (NLR, 1500 mgN/L·d), with different influent alkalinity/nitrogen molar ratios (alk/N, 1 and 1.3) and dissolved oxygen concentrations (DO, 5.0, 3.0, 2.0, 1.5 and 1.0 mgO2/L). As DO ranged between 5.0 and 1.5 mgO2/L, the partial conversion of ammonium to nitrite was successfully achieved, with a negligible production of nitrate and nitrous oxide. When alk/N was increased from 1 to 1.3 (DO was not limiting, i.e. 2 mgO2/L), the increase in ammonium-nitrogen removal rate (ANRR, from 717±17 to 945±21 mgNH4-N/L·d) and the simultaneous decrease in specific N2O-N production (from 0.33±0.01 to 0.23±0.01% of ANRR) were observed. When DO was set to 1.0 mgO2/L, partial nitritation was irreversibly compromised, and a corresponding increase in specific N2O-N production was observed (from 0.22±0.01 to 0.61±0.03% of ANRR). The results indicate a clear correlation between N2O production and autotrophic ammonium to nitrite oxidation rate.
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- 2017
31. Multi-messenger observations of a binary neutron star merger
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Abbott, B., Abbott, R., Abbott, T., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R., Adya, V., Affeldt, C., Afrough, M., Agarwal, B., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O., Aiello, L., Ain, A., Ajith, P., Allen, B., Allen, G., Allocca, A., Altin, P., Amato, A., Ananyeva, A., Anderson, S., Anderson, W., Angelova, S., Antier, S., Appert, S., Arai, K., Araya, M., Areeda, J., Arnaud, N., Arun, K., Ascenzi, S., Ashton, G., Ast, M., Aston, S., Astone, P., Atallah, D., Aufmuth, P., Aulbert, C., AultONeal, K., Austin, C., Avila-Alvarez, A., Babak, S., Bacon, P., Bader, M., Bae, S., Baker, P., Baldaccini, F., Ballardin, G., Ballmer, S., Banagiri, S., Barayoga, J., Barclay, S., Barish, B., Barker, D., Barkett, K., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Barthelmy, S., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J., Bawaj, M., Bayley, J., Bazzan, M., Becsy, B., Beer, C., Bejger, M., Belahcene, I., Bell, A., Berger, B., Bergmann, G., Bero, J., Berry, C., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I., Billingsley, G., Billman, C., Birch, J., Birney, R., Birnholtz, O., Biscans, S., Biscoveanu, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M., Blackburn, J., Blackman, J., Blair, C., Blair, D., Blair, R., Bloemen, S., Bock, O., Bode, N., Boer, M., Bogaert, G., Bohe, A., Bondu, F., Bonilla, E., Bonnand, R., Boom, B., Bork, R., Boschi, V., Bose, S., Bossie, K., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P., Branchesi, M., Brau, J., Briant, T., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Broida, J., Brooks, A., Brown, D., Brunett, S., Buchanan, C., Buikema, A., Bulik, T., Bulten, H., Buonanno, A., Buskulic, D., Buy, C., Byer, R., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Bustillo, J., Callister, T., Calloni, E., Camp, J., Canepa, M., Canizares, P., Cannon, K., Cao, H., Cao, J., Capano, C., Capocasa, E., Carbognani, F., Caride, S., Carney, M., Diaz, J., Casentini, C., Caudill, S., Cavagli, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C., Cerd-Durn, P., Cerretani, G., Cesarini, E., Chamberlin, S., Chan, M., Chao, S., Charlton, P., Chase, E., Chassande-Mottin, E., Chatterjee, D., Chatziioannou, K., Cheeseboro, B., Chen, H., Chen, X., Chen, Y., Cheng, H., Chia, H., Chincarini, A., Chiummo, A., Chmiel, T., Cho, H., Cho, M., Chow, J., Christensen, N., Chu, Q., Chua, A., Chua, S., Chung, A., Chung, S., Ciani, G., Ciolfi, R., Cirelli, C., Cirone, A., Clara, F., Clark, J., Clearwater, P., Cleva, F., Cocchieri, C., Coccia, E., Cohadon, P., Cohen, D., Colla, A., Collette, C., Cominsky, L., Constancio, M., Conti, L., Cooper, S., Corban, P., Corbitt, T., Cordero-Carrion, I., Corley, K., Cornish, N., Corsi, A., Cortese, S., Costa, C., Coughlin, M., Coughlin, S., Coulon, J., Countryman, S., Couvares, P., Covas, P., Cowan, E., Coward, D., Cowart, M., Coyne, D., Coyne, R., Creighton, J., Creighton, T., Cripe, J., Crowder, S., Cullen, T., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., Dlya, G., Danilishin, S., D'Antonio, S., Danzmann, K., Dasgupta, A., Dattilo, V., Dave, I., Davier, M., Davis, D., Daw, E., Day, B., De, S., Debra, D., Degallaix, J., De laurentis, M., Deleglise, S., Del Pozzo, W., Demos, N., Denker, T., Dent, T., De Pietri, R., Dergachev, V., De Rosa, R., DeRosa, R., De Rossi, C., DeSalvo, R., De Varona, O., Devenson, J., Dhurandhar, S., Diaz, M., Di Fiore, L., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Di Pace, S., Di Palma, I., Di Renzo, F., Doctor, Z., Dolique, V., Donovan, F., Dooley, K., Doravari, S., Dorrington, I., Douglas, R., Alvarez, M., Downes, T., Drago, M., Dreissigacker, C., Driggers, J., Du, Z., Ducrot, M., Dupej, P., Dwyer, S., Edo, T., Edwards, M., Effler, A., Ehrens, P., Eichholz, J., Eikenberry, S., Eisenstein, R., Essick, R., Estevez, D., Etienne, Z., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Farinon, S., Farr, B., Farr, W., Fauchon-Jones, E., Favata, M., Fays, M., Fee, C., Fehrmann, H., Feicht, J., Fejer, M., Fernandez-Galiana, A., Ferrante, I., Ferreira, E., Ferrini, F., Fidecaro, F., Finstad, D., Fiori, I., Fiorucci, D., Fishbach, M., Fisher, R., Fitz-Axen, M., Flaminio, R., Fletcher, M., Fong, H., Font, J., Forsyth, P., Forsyth, S., Fournier, J., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fries, E., Fritschel, P., Frolov, V., Fulda, P., Fyffe, M., Gabbard, H., Gadre, B., Gaebel, S., Gair, J., Gammaitoni, L., Ganija, M., Gaonkar, S., Garcia-Quiros, C., Garufi, F., Gateley, B., Gaudio, S., Gaur, G., Gayathri, V., Gehrels, N., Gemme, G., Genin, E., Gennai, A., George, D., George, J., Gergely, L., Germain, V., Ghonge, S., Ghosh, A., Ghosh, S., Giaime, J., Giardina, K., Giazotto, A., Gill, K., Glover, L., Goetz, E., Goetz, R., Gomes, S., Goncharov, B., Gonzlez, G., Castro, J., Gopakumar, A., Gorodetsky, M., Gossan, S., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Granata, M., Grant, A., Gras, S., Gray, C., Greco, G., Green, A., Gretarsson, E., Griswold, B., Groot, P., Grote, H., Grunewald, S., Gruning, P., Guidi, G., Guo, X., Gupta, A., Gupta, M., Gushwa, K., Gustafson, E., Gustafson, R., Halim, O., Hall, B., Hall, E., Hamilton, E., Hammond, G., Haney, M., Hanke, M., Hanks, J., Hanna, C., Hannam, M., Hannuksela, O., Hanson, J., Hardwick, T., Harms, J., Harry, G., Harry, I., Hart, M., Haster, C., Haughian, K., Healy, J., Heidmann, A., Heintze, M., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I., Hennig, J., Heptonstall, A., Heurs, M., Hild, S., Hinderer, T., Hoak, D., Hofman, D., Holt, K., Holz, D., Hopkins, P., Horst, C., Hough, J., Houston, E., Howell, E., Hreibi, A., Hu, Y., Huerta, E., Huet, D., Hughey, B., Husa, S., Huttner, S., Huynh-Dinh, T., Indik, N., Inta, R., Intini, G., Isa, H., Isac, J., Isi, M., Iyer, B., Izumi, K., Jacqmin, T., Jani, K., Jaranowski, P., Jawahar, S., Jimenez-Forteza, F., Johnson, W., Jones, D., Jones, R., Jonker, R., Ju, L., Junker, J., Kalaghatgi, C., Kalogera, V., Kamai, B., Kandhasamy, S., Kang, G., Kanner, J., Kapadia, S., Karki, S., Karvinen, K., Kasprzack, M., Katolik, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kawabe, K., Kefelian, F., Keitel, D., Kemball, A., Kennedy, R., Kent, C., Key, J., Khalili, F., Khan, I., Khan, S., Khan, Z., Khazanov, E., Kijbunchoo, N., Kim, C., Kim, J., Kim, K., Kim, W., Kim, Y., Kimbrell, S., King, E., King, P., Kinley-Hanlon, M., Kirchhoff, R., Kissel, J., Kleybolte, L., Klimenko, S., Knowles, T., Koch, P., Koehlenbeck, S., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W., Kowalska, I., Kozak, D., Krmer, C., Kringel, V., Krishnan, B., Krlak, A., Kuehn, G., Kumar, P., Kumar, R., Kumar, S., Kuo, L., Kutynia, A., Kwang, S., Lackey, B., Lai, K., Landry, M., Lang, R., Lange, J., Lantz, B., Lanza, R., Larson, S., Lartaux-Vollard, A., Lasky, P., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lee, C., Lee, H., Lee, K., Lehmann, J., Lenon, A., Leonardi, M., Leroy, N., Letendre, N., Levin, Y., Li, T., Linker, S., Littenberg, T., Liu, J., Lo, R., Lockerbie, N., London, L., Lord, J., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J., Lousto, C., Lovelace, G., Lck, H., Lumaca, D., Lundgren, A., Lynch, R., Ma, Y., Macas, R., Macfoy, S., Machenschalk, B., MacInnis, M., Macleod, D., Hernandez, I., Magaa-Sandoval, F., Zertuche, L., Magee, R., Majorana, E., Maksimovic, I., Man, N., Mandic, V., Mangano, V., Mansell, G., Manske, M., Mantovani, M., Marchesoni, F., Marion, F., Mrka, S., Mrka, Z., Markakis, C., Markosyan, A., Markowitz, A., Maros, E., Marquina, A., Marsh, P., Martelli, F., Martellini, L., Martin, I., Martin, R., Martynov, D., Mason, K., Massera, E., Masserot, A., Massinger, T., Masso-Reid, M., Mastrogiovanni, S., Matas, A., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., McCarthy, R., McClelland, D., McCormick, S., McCuller, L., McGuire, S., McIntyre, G., McIver, J., McManus, D., McNeill, L., Mcrae, T., McWilliams, S., Meacher, D., Meadors, G., Mehmet, M., Meidam, J., Mejuto-Villa, E., Melatos, A., Mendell, G., Mercer, R., Merilh, E., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Metzdorff, R., Meyers, P., Miao, H., Michel, C., Middleton, H., Mikhailov, E., Milano, L., Mueller, A., Mueller, B., Miller, J., Millhouse, M., Milovich-Goff, M., Minazzoli, O., Minenkov, Y., Ming, J., Mishra, C., Mitra, S., Mitrofanov, V., Mitselmakher, G., Mittleman, R., Moffa, D., Moggi, A., Mogushi, K., Mohan, M., Mohapatra, S., Montani, M., Moore, C., Moraru, D., Moreno, G., Morriss, S., Mours, B., Mow-Lowry, C., Mueller, G., Muir, A., Mukherjee, A., Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Muniz, E., Muratore, M., Murray, P., Napier, K., Nardecchia, I., Naticchioni, L., Nayak, R., Neilson, J., Nelemans, G., Nelson, T., Nery, M., Neunzert, A., Nevin, L., Newport, J., Newton, G., Ng, K., Nguyen, P., Nguyen, T., Nichols, D., Nielsen, A., Nissanke, S., Nitz, A., Noack, A., Nocera, F., Nolting, D., North, C., Nuttall, L., Oberling, J., O'Dea, G., Ogin, G., Oh, J., Oh, S., Ohme, F., Okada, M., Oliver, M., Oppermann, P., Oram, R., O'Reilly, B., Ormiston, R., Ortega, L., O'Shaughnessy, R., Ossokine, S., Ottaway, D., Overmier, H., Owen, B., Pace, A., Page, J., Page, M., Pai, A., Pai, S., Palamos, J., Palashov, O., Palomba, C., Pal-Singh, A., Pan, H., Pang, B., Pang, P., Pankow, C., Pannarale, F., Pant, B., Paoletti, F., Paoli, A., Papa, M., Parida, A., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patil, M., Patricelli, B., Pearlstone, B., Pedraza, M., Pedurand, R., Pekowsky, L., Pele, A., Penn, S., Perez, C., Perreca, A., Perri, L., Pfeiffer, H., Phelps, M., Piccinni, O., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I., Pirello, M., Pitkin, M., Poe, M., Poggiani, R., Popolizio, P., Porter, E., Post, A., Powell, J., Prasad, J., Pratt, J., Pratten, G., Predoi, V., Prestegard, T., Price, L., Prijatelj, M., Principe, M., Privitera, S., Prodi, G., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Prrer, M., Qi, H., Quetschke, V., Quintero, E., Quitzow-James, R., Raab, F., Rabeling, D., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rajbhandari, B., Rakhmanov, M., Ramirez, K., Ramos-Buades, A., Rapagnani, P., Raymond, V., Razzano, M., Read, J., Regimbau, T., Rei, L., Reid, S., Reitze, D., Ren, W., Reyes, S., Ricci, F., Ricker, P., Rieger, S., Riles, K., Rizzo, M., Robertson, N., Robie, R., Robinet, F., Rocchi, A., Rolland, L., Rollins, J., Roma, V., Romano, R., Romel, C., Romie, J., Rosinska, D., Ross, M., Rowan, S., Rdiger, A., Ruggi, P., Rutins, G., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Salconi, L., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sampson, L., Sanchez, E., Sanchez, L., Sanchis-Gual, N., Sandberg, V., Sanders, J., Sassolas, B., Sathyaprakash, B., Saulson, P., Sauter, O., Savage, R., Sawadsky, A., Schale, P., Scheel, M., Scheuer, J., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R., Schonbeck, A., Schreiber, E., Schuette, D., Schulte, B., Schutz, B., Schwalbe, S., Scott, J., Scott, S., Seidel, E., Sellers, D., Sengupta, A., Sentenac, D., Sequino, V., Sergeev, A., Shaddock, D., Shaffer, T., Shah, A., Shahriar, M., Shaner, M., Shao, L., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D., Siellez, K., Siemens, X., Sieniawska, M., Sigg, D., Silva, A., Singer, L., Singh, A., Singhal, A., Sintes, A., Slagmolen, B., Smith, B., Smith, J., Smith, R., Somala, S., Son, E., Sonnenberg, J., Sorazu, B., Sorrentino, F., Souradeep, T., Spencer, A., Srivastava, A., Staats, K., Staley, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stevenson, S., Stone, R., Stops, D., Strain, K., Stratta, G., Strigin, S., Strunk, A., Sturani, R., Stuver, A., Summerscales, T., Sun, L., Sunil, S., Suresh, J., Sutton, P., Swinkels, B., Szczepanczyk, M., Tacca, M., Tait, S., Talbot, C., 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H., Sampedro, L., Schneiter, M., Sodre, L., Starck, M., Torres-Flores, S., Tornatore, M., Castillo, M., Castro-Tirado, A., Tello, J., Zhang, B., Cunniffe, R., Castellon, A., Hiriart, D., Caballero-Garcia, M., Jelinek, M., Kubanek, P., Del Pulgar, C., Park, I., Jeong, S., Ceron, J., Pandey, S., Yock, P., Querel, R., Fan, Y., Wang, C., Beardsley, A., Brown, I., Crosse, B., Emrich, David, Franzen, T., Gaensler, B., Horsley, L., Johnston-Hollitt, Melanie, Kenney, David, Morales, M., Pallot, D., Sokolowski, Marcin, Steele, K., Tingay, Steven, Trott, Cathryn, Wayth, Randall, Williams, A., Wu, C., Yoshida, A., Sakamoto, T., Kawakubo, Y., Takahashi, I., Asaoka, Y., Ozawa, S., Torii, S., Shimizu, Y., Tamura, T., Ishizaki, W., Cherry, M., Ricciarini, S., Penacchioni, A., Marrocchesi, P., Pozanenko, A., Volnova, A., Mazaeva, E., Minaev, P., Krugov, M., Kusakin, A., Reva, I., Moskvitin, A., Rumyantsev, V., Inasaridze, R., Klunko, E., Tungalag, N., Schmalz, S., Burhonov, O., Abdalla, H., Abramowski, A., Aharonian, F., Benkhali, F., Angner, E., Arakawa, M., Arrieta, M., Aubert, P., Backes, M., Balzer, A., Barnard, M., Becherini, Y., Berge, D., Bernhard, S., Bernrhr, K., Blackwell, R., Bottcher, M., Boisson, C., Bolmont, J., Bonnefoy, S., Bordas, P., Brun, F., Brun, P., Bryan, M., Bchele, M., Capasso, M., Caroff, S., Carosi, A., Casanova, S., Cerruti, M., Chakraborty, N., Chaves, R., Chen, A., Chevalier, J., Condon, B., Davids, I., Decock, J., Deil, C., Devin, J., Dewilt, P., Dirson, L., Djannati-Atao, A., Donath, A., Drury, L., Dutson, K., Dyks, J., Edwards, T., Egberts, K., Emery, G., Ernenwein, J., Eschbach, S., Farnier, C., Fernandes, M., Fiasson, A., Fontaine, G., Fssling, M., Gabici, S., Gallant, Y., Garrigoux, T., Gate, F., Giavitto, G., Giebels, B., Glawion, D., Glicenstein, J., Gottschall, D., Hahn, J., Haupt, M., Hawkes, J., Heinzelmann, G., Henri, G., Hermann, G., Hinton, J., Hofmann, W., Hoischen, C., Holch, T., Holler, M., Horns, D., Ivascenko, A., Iwasaki, H., Jacholkowska, A., Jamrozy, M., Jankowsky, D., Jankowsky, F., Jingo, M., Jouvin, L., Jung-Richardt, I., Kastendieck, M., Katarzynski, K., Katsuragawa, M., Kerszberg, D., Khangulyan, D., Khelifi, B., King, J., Klepser, S., Klochkov, D., Kluzniak, W., Komin, N., Kosack, K., Krakau, S., Kraus, M., Krger, P., Laffon, H., Lamanna, G., Lau, J., Lees, J., Lefaucheur, J., Lemiere, A., Lenain, J., Leser, E., Lohse, T., Lorentz, M., Liu, R., Lypova, I., Malyshev, D., Marandon, V., Marcowith, A., Mariaud, C., Marx, R., Maurin, G., Maxted, N., Mayer, M., Meintjes, P., Mitchell, A., Moderski, R., Mohamed, M., Mohrmann, L., Mor, K., Moulin, E., Murach, T., Nakashima, S., De Naurois, M., Ndiyavala, H., Niederwanger, F., Niemiec, J., Oakes, L., Odaka, H., Ohm, S., Ostrowski, M., Oya, I., Padovani, M., Panter, M., Parsons, R., Pekeur, N., Pelletier, G., Perennes, C., Petrucci, P., Peyaud, B., Piel, Q., Pita, S., Poireau, V., Poon, H., Prokhorov, D., Prokoph, H., Phlhofer, G., Punch, M., Quirrenbach, A., Raab, S., Rauth, R., Renaud, M., Reyes, R., Rieger, F., Rinchiuso, L., Romoli, C., Rowell, G., Rudak, B., Rulten, C., Sahakian, V., Saito, S., Sanchez, D., Santangelo, A., Sasaki, M., Schlickeiser, R., Schssler, F., Schulz, A., Schwanke, U., Schwemmer, S., Seglar-Arroyo, M., Settimo, M., Seyffert, A., Shafi, N., Shilon, I., Shiningayamwe, K., Simoni, R., Sol, H., Spanier, F., Spir-Jacob, M., Stawarz, L., Steenkamp, R., Stegmann, C., Steppa, C., Sushch, I., Takahashi, T., Tavernet, J., Tavernier, T., Taylor, A., Terrier, R., Tiziani, D., Tluczykont, M., Trichard, C., Tsirou, M., Tsuji, N., Tuffs, R., Uchiyama, Y., Van der Walt, D., Van Eldik, C., Van Rensburg, C., Vasileiadis, G., Veh, J., Venter, C., Viana, A., Vincent, P., Vink, J., Voisin, F., Volk, H., Vuillaume, T., Wadiasingh, Z., Wagner, S., Wagner, P., Wagner, R., White, R., Wierzcholska, A., Willmann, P., WRnlein, A., Wouters, D., Yang, R., Zaborov, D., Zacharias, M., Zanin, R., Zdziarski, A., Zech, A., Zefi, F., Ziegler, A., Zorn, J., Zywucka, N., Fender, R., Broderick, J., Stewart, A., Ter Veen, S., Shulevski, A., Kavic, M., Simonetti, J., League, C., Tsai, J., Obenberger, K., Nathaniel, K., Taylor, G., Dowell, J., Liebling, S., Estes, J., Lippert, M., Sharma, I., Farella, B., Abeysekara, A., Alfaro, R., Alvarez, C., Arceo, R., Arteaga-Velzquez, J., Rojas, D., Solares, H., Barber, A., Becerril, A., Belmont-Moreno, E., BenZvi, S., Berley, D., Bernal, A., Brisbois, C., Caballero-Mora, K., Capistrn, T., Carramiana, A., Cotti, U., Cotzomi, J., De Leon, S., De Leon, C., De la Fuente, E., Hernandez, R., Dichiara, S., Dingus, B., DuVernois, M., Ellsworth, R., Engel, K., Enriquez-Rivera, O., Fiorino, D., Fleischhack, H., Fraija, N., Garcia-Gonzlez, J., Garfias, F., Gerhardt, M., Muoz, A., Gonzlez, M., Goodman, J., Hampel-Arias, Z., Harding, J., Hernandez, S., Hernandez-Almada, A., Hona, B., Hntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kieda, D., Lara, A., Lauer, R., Lennarz, D., Vargas, H., Linnemann, J., Longinotti, A., Raya, G., Luna-Garcia, R., Lopez-Coto, R., Malone, K., Marinelli, S., Martinez, O., Martinez-Castellanos, I., Martinez-Castro, J., Martinez-Huerta, H., Matthews, J., Miranda-Romagnoli, P., Moreno, E., Mostaf, M., Nellen, L., Newbold, M., Nisa, M., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Perez-Perez, E., Ren, Z., Rho, C., Riviere, C., Rosa-Gonzlez, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F., Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A., Springer, R., Surajbali, P., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T., Weisgarber, T., Westerhoff, S., Wisher, I., Wood, J., Yapici, T., Younk, P., Zhou, H., Alvarez, J., Aab, A., Abreu, P., Aglietta, M., Albuquerque, I., Albury, J., Allekotte, I., Almela, A., Castillo, J., Alvarez-Muiz, J., Anastasi, G., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Arsene, N., Asorey, H., Assis, P., Avila, G., Badescu, A., Balaceanu, A., Barbato, F., Luz, R., Becker, K., Bellido, J., Berat, C., Bertaina, M., Bertou, X., Biermann, P., Biteau, J., Blaess, S., Blanco, A., Blazek, J., Bleve, C., Bohacova, M., Bonifazi, C., Borodai, N., Botti, A., Brack, J., Brancus, I., Bretz, T., Bridgeman, A., Briechle, F., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caccianiga, L., Cancio, A., Canfora, F., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Chavez, A., Chinellato, J., Chudoba, J., Clay, R., Cerutti, A., Colalillo, R., Coleman, A., Collica, L., Coluccia, M., Conceicao, R., Consolati, G., Contreras, F., Cooper, M., Coutu, S., Covault, C., Cronin, J., D'Amico, S., Daniel, B., Dasso, S., Daumiller, K., Dawson, B., Day, J., De Almeida, R., De Jong, S., De Mauro, G., Neto, J., De Mitri, I., De Oliveira, J., De Souza, V., Debatin, J., Deligny, O., Castro, M., Diogo, F., Dobrigkeit, C., D'Olivo, J., Dorosti, Q., Dos Anjos, R., Dova, M., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C., Espadanal, J., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J., Filipcic, A., Freire, M., Fujii, T., Fuster, A., Gaior, R., Garcia, B., Gemmeke, H., Gherghel-Lascu, A., Ghia, P., Giaccari, U., Giammarchi, M., Giller, M., Glas, D., Glaser, C., Golup, G., Berisso, M., Vitale, P., Gonzlez, N., Gorgi, A., Gottowik, M., Grillo, A., Grubb, T., Guarino, F., Guedes, G., Halliday, R., Hampel, M., Hansen, P., Harari, D., Harrison, T., Harvey, V., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A., Hojvat, C., Holt, E., Homola, P., Horandel, J., Horvath, P., Hrabovsky, M., Huege, T., Hulsman, J., Insolia, A., Isar, P., Jandt, I., Johnsen, J., Josebachuili, M., Jurysek, J., Kaapa, A., Kampert, K., Keilhauer, B., Kemmerich, N., Kemp, J., Kieckhafer, R., Klages, H., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Kuempel, D., Mezek, G., Kunka, N., Awad, A., Lago, B., LaHurd, D., Lauscher, M., Legumina, R., De Oliveira, M., Letessier-Selvon, A., Lhenry-Yvon, I., Link, K., Lo Presti, D., Lopes, L., Lopez, R., Casado, A., Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mandat, D., Mantsch, P., Mariazzi, A., Maris, I., Marsella, G., Martello, D., Martinez, H., Bravo, O., Meza, J., Mathes, H., Mathys, S., Matthiae, G., Mayotte, E., Mazur, P., Medina, C., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K., Michal, S., Micheletti, M., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mueller, M., Mueller, S., Mussa, R., Naranjo, I., Niculescu-Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nozka, L., Nunez, L., Oikonomou, F., Olinto, A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pedreira, F., Kala, J., Pea-Rodriguez, J., Pereira, L., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Poh, J., Porowski, C., Prado, R., Privitera, P., Prouza, M., Quel, E., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., De Carvalho, W., Fernandez, G., Rojo, J., Roncoroni, M., Roth, M., Roulet, E., Rovero, A., Ruehl, P., Saffi, S., Saftoiu, A., Salamida, F., Saleh, A., Salina, G., Sanchez, F., Sanchez-Lucas, P., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Schauer, M., Scherini, V., Schieler, H., Schimp, M., Schmidt, D., Scholten, O., Schovnek, P., Schroder, F., Schumacher, J., Sciutto, S., Segreto, A., Shadkam, A., Shellard, R., Sigl, G., Silli, G., Smida, R., Snow, G., Sommers, P., Sonntag, S., Soriano, J., Squartini, R., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Strafella, F., Streich, A., Suarez, F., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A., Supik, J., Swain, J., Szadkowski, Z., Taboada, A., Taborda, O., Timmermans, C., Peixoto, C., Tomankova, L., Tome, B., Elipe, G., Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J., Valio, I., Valore, L., Van Aar, G., Van Bodegom, P., Van den Berg, A., Van Vliet, A., Varela, E., Cardenas, B., Vazquez, R., Veberic, D., Ventura, C., Quispe, I., Verzi, V., Vicha, J., Villaseor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A., Weber, M., Weindl, A., Wiedenski, M., Wiencke, L., Wilczynski, H., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Schulze, S., Corral-Santana, J., De Gregorio-Monsalvo, I., Gonzlez-Lopez, J., Hartmann, D., Ishwara-Chandra, C., Martin, S., Mehner, A., Misra, K., Michalowski, M., Resmi, L., Paragi, Z., Agudo, I., An, T., Beswick, R., Casadio, C., Frey, S., Kettenis, M., Marcote, B., Moldon, J., Szomoru, A., Langevelde, H., Cwiek, A., Cwiok, M., Czyrkowski, H., Dabrowski, R., Kasprowicz, G., Mankiewicz, L., Nawrocki, K., Opiela, R., Piotrowski, L., Wrochna, G., Zaremba, M., Zarnecki, A., Haggard, D., Nynka, M., Ruan, J., Bland, Phil, Booler, T., Devillepoix, H., De Gois, J., Hancock, Paul, Howie, Robert, Paxman, Jonathan, Sansom, Eleanor, Towner, Martin, Tonry, J., Stubbs, C., Denneau, L., Heinze, A., Stalder, B., Weiland, H., Eatough, R., Kramer, M., Kraus, A., Piro, L., Gonzlez, J., Butler, N., Khandrika, H., Kutyrev, A., Lee, W., Ricci, R., Ryan, R., Sanchez-Ramirez, R., Veilleux, S., Wieringa, M., Burgess, J., Van Eerten, H., Fontes, C., Korobkin, O., Wollaeger, R., Camilo, F., Foley, A., Goedhart, S., Makhathini, S., Oozeer, N., Smirnov, O., and Woudt, P.
- Abstract
© 2017. The American Astronomical Society. All rights reserved. On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma -ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40 8 8-+ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 M. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nu
- Published
- 2017
32. The Sardinia Radio Telescope (SRT): A large modern radio telescope for observations from meter to mm wavelengths
- Author
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Carretti, E., primary, Aresu, G., additional, Bachetti, M., additional, Bartolini, M., additional, Buffa, F., additional, Burgay, M., additional, Buttu, M., additional, Caria, T., additional, Carretti, E., additional, Castangia, P., additional, Casu, S., additional, Concu, R., additional, Corongiu, A., additional, Deiana, G. L., additional, Egron, E., additional, Fara, A., additional, Gaudiomonte, F., additional, Gusai, V., additional, Iacolina, N., additional, Ladu, A., additional, Loru, S., additional, Marongiu, P., additional, Melis, A., additional, Melis, P., additional, Migoni, C., additional, Milia, S., additional, Navarrini, A., additional, Orlati, A., additional, Ortu, P., additional, Palmas, S., additional, Pellizzoni, A., additional, Perrodin, D., additional, Pilia, M., additional, Pisanu, T., additional, Poppi, S., additional, Porceddu, I., additional, Righini, S., additional, Saba, A., additional, Serra, G., additional, Serrau, L., additional, Surcis, G., additional, Tarchi, A., additional, Trois, A., additional, Vacca, V., additional, Valente, G., additional, and Vargiu, G. P., additional
- Published
- 2017
- Full Text
- View/download PDF
33. The anammox process as the second step for the treatment of ammonium rich refinery wastewater with high Corg/N ratio
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MILIA S., PERRA M., TOCCO G., and CARUCCI A.
- Subjects
ammonium ,industrial wastewater ,organic carbon ,autotrophic nitrogen removal ,anammox - Abstract
The combination of partial nitritation and anammox (anaerobic ammonium oxidation) has been mainly applied to the treatment of wastewaters with high ammonium concentration and low content of biodegradable organic carbon. So far, only few studies have focused on the application of partial nitritation-anammox process to the treatment of ammonium-rich wastewaters characterized also by a high organic carbon to nitrogen ratio (Corg/N), as well as by the presence of toxic substances: in this study, an anammox reactor was started-up and fed with the effluent from a partial nitritation reactor treating IGCC (Integrated Gasification Combined Cycle) wastewater, in order to evaluate its feasibility as an alternative to the currently applied chemical-physical-biological treatment. A sequencing batch reactor was inoculated with granular anammox biomass and run at controlled temperature (35±0.5 °C) and pH (7.7±0.3). The synthetic influent containing NH4-N (up to 250 mg/L) and NO2-N (up to 330 mg/L) was progressively replaced by the IGCC wastewater, which had been pre-treated in the lab-scale partial nitritation reactor. When the reactor was fed with the synthetic medium at the target nitrogen loading rate (NLR, 0.350 gN/L?d), the observed NH4-N removal efficiency was 93±5%, and no nitrite was detected in the effluent. Good overall process performance was maintained as increasing amounts (up to 65%) of the effluent from the partial nitritation system were fed to the anammox reactor: NH4-N and NO2-N removal efficiencies were 98.9±1.0% and 96.6±2.1%, respectively, and nitrite specific removal rate peaked at 0.28 gNO2-N/gVSS?d. On day 154, a nitrogen shock load was applied to evaluate anammox stability during start-up: despite system sensitivity to the sudden increase of nitrogen load, process performance was recovered and the percentage of IGCC wastewater in the influent could be raised to 100% with fairly good NH4-N and NO2-N removal efficiencies (85.7±5.8% and 88.2±2.3%, respectively). Anammox granules were compact (diameter, 0.636±0.02 mm) and dense (86.5±3.4 gTSS/Lgran), with good settling properties. The total organic carbon (TOC) removal efficiency was low: since most of TOC (around 80±8%) had been removed in the preliminary partial nitritation step (results not shown), it can be assumed that the residual TOC entering the anammox reactor was slowly biodegradable, therefore heterotrophic denitrifiers did not compete with anammox biomass for nitrite. The results indicate that anammox start-up can be successfully achieved and the process can be applied in combination with a preliminary partial nitritation step for the treatment of ammonium-rich IGCC wastewater, thus providing useful information also for the treatment of similar wastewaters with high Corg/N ratio and containing toxic substances.
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- 2015
34. Il bambino resiliente: un'analisi degli interventi su minori e famiglia
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Casonato, M, Di Milia, S, CASONATO, MARCO MARIO, Di Milia, S., Casonato, M, Di Milia, S, CASONATO, MARCO MARIO, and Di Milia, S.
- Abstract
Nell'opera di Rousseau si crisrtallizza l'immagine dell'infanzia che pervade la teoria psicoanalitica, la psicologia dello sviluppo e dell'educazione, le pratiche di assistenza sociale e gli interventi dei giudici minorili, ed infine le credenze dei genitori.Tale immagine prevede che il bambino sia formato nella e dalla famiglia.Ma tutto ciò risulta errato e fuorviante alla luce della genetica comportamentale contemporanea.I bambini si formano infatti nell'ambiente in cui essi imparano a vivere riconoscendosi e identificandosi nella categoria sociali cui appartengono: il gruppo dei bambini.
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- 2010
35. Il bambino resiliente: un'analisi degli interventi su minori e famiglia
- Author
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CASONATO, MARCO MARIO, Di Milia, S., Casonato, M, and Di Milia, S
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Genetica comportamentale, resilienza, sviluppo infantile, giustizia minorile, servizi sociali, pregiudizi, falsi abusi, sottrazione di minori, apprendimento sciale - Abstract
Nell'opera di Rousseau si crisrtallizza l'immagine dell'infanzia che pervade la teoria psicoanalitica, la psicologia dello sviluppo e dell'educazione, le pratiche di assistenza sociale e gli interventi dei giudici minorili, ed infine le credenze dei genitori.Tale immagine prevede che il bambino sia formato nella e dalla famiglia.Ma tutto ciò risulta errato e fuorviante alla luce della genetica comportamentale contemporanea.I bambini si formano infatti nell'ambiente in cui essi imparano a vivere riconoscendosi e identificandosi nella categoria sociali cui appartengono: il gruppo dei bambini.
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- 2010
36. Accelerated Carbonation of Waelz Slag: Effect of Particle Size on CO2 Sequestration Capacity
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Cappai G., De Giudici G., Medas D., Milia S., Muntoni A., Orrù G., Nieddu A., and Piredda M.
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- 2014
37. Bioaugmentation-Assisted Phytostabilisation of Abandoned Mine Sites in South West Sardinia
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Tamburini, E., primary, Sergi, S., additional, Serreli, L., additional, Bacchetta, G., additional, Milia, S., additional, Cappai, G., additional, and Carucci, A., additional
- Published
- 2016
- Full Text
- View/download PDF
38. The High Time Resolution Universe survey - XI. Discovery of five recycled pulsars and the optical detectability of survey white dwarf companions
- Author
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Bates, S., Thornton, D., Bailes, M., Barr, E., Bassa, C., Bhat, Ramesh, Burgay, M., Burke-Spolaor, S., Champion, D., Flynn, C., Jameson, A., Johnston, S., Keith, M., Kramer, M., Levin, L., Lyne, A., Milia, S., Ng, C., Petroff, E., Possenti, A., Stappers, B., van Straten, W., Tiburzi, C., Bates, S., Thornton, D., Bailes, M., Barr, E., Bassa, C., Bhat, Ramesh, Burgay, M., Burke-Spolaor, S., Champion, D., Flynn, C., Jameson, A., Johnston, S., Keith, M., Kramer, M., Levin, L., Lyne, A., Milia, S., Ng, C., Petroff, E., Possenti, A., Stappers, B., van Straten, W., and Tiburzi, C.
- Abstract
We present the discovery of a further five recycled pulsar systems in the mid-Galactic latitude portion of the High Time Resolution Universe survey. The pulsars have rotational periods ranging from 2 to 66 ms, and four are in binary systems with orbital periods between 10.8 h and 9 d. Three of these binary systems are particularly interesting; PSR J1227-6208 has a pulse period of 34.5 ms and the highest mass function of all pulsars with near-circular orbits. The circular orbit suggests that the companion is not another neutron star, so future timing experiments may reveal one of the heaviest white dwarfs ever found (>1.3 M☉). Timing observations of PSR J1431-4715 indicate that it is eclipsed by its companion which has a mass indicating it belongs to the redback class of eclipsing millisecond pulsars. PSR J1653-2054 has a companion with a minimum mass of only 0.08M☉, placing it among the class of pulsars with low-mass companions. Unlike the majority of such systems, however, no evidence of eclipses is seen at 1.4 GHz.
- Published
- 2015
39. Pharmacokinetics and biotransformation of the new benzodiazepine, lormetazepam, in man: III. Repeated administration and transfer to neonates via breast milk
- Author
-
Hümpel, M., Stoppelli, I., Milia, S., and Rainer, E.
- Published
- 1982
- Full Text
- View/download PDF
40. The High Time Resolution Universe Pulsar Survey – V. Single-pulse energetics and modulation properties of 315 pulsars
- Author
-
Burke-Spolaor, S., Johnston, S., Bailes, M., Bates, S. D., Bhat, N. D. R., Burgay, M., Champion, D. J., D'Amico, N., Keith, M. J., Kramer, M., Levin, L., Milia, S., Possenti, S., Stappers, B., and van Straten, W.
- Subjects
Astrophysics::High Energy Astrophysical Phenomena - Abstract
We report on the pulse-to-pulse energy distributions and phase-resolved modulation properties for catalogued pulsars in the southern High Time Resolution Universe intermediate-latitude survey. We selected the 315 pulsars detected in a single-pulse search of this survey, allowing a large sample unbiased regarding any rotational parameters of neutron stars. We found that the energy distribution of many pulsars is well described by a log-normal distribution, with few deviating from a small range in log-normal scale and location parameters. Some pulsars exhibited multiple energy states corresponding to mode changes, and implying that some observed ‘nulling’ may actually be a mode-change effect. PSR J1900−2600 was found to emit weakly in its previously identified ‘null’ state. We found evidence for another state-change effect in two pulsars, which show bimodality in their nulling time-scales; that is, they switch between a continuous-emission state and a single-pulse-emitting state. Large modulation occurs in many pulsars across the full integrated profile, with increased sporadic bursts at leading and trailing sub-beam edges. Some of these high-energy outbursts may indicate the presence of ‘giant pulse’ phenomena. We found no correlation with modulation and pulsar period, age or other parameters. Finally, the deviation of integrated pulse energy from its average value was generally quite small, despite the significant phase-resolved modulation in some pulsars; we interpret this as tenuous evidence of energy regulation between distinct pulsar sub-beams.
- Published
- 2012
41. Radio emission evolution, polarimetry and multifrequency single pulse analysis of the radio magnetar PSR J1622−4950
- Author
-
Levin, L., Bailes, M., Bates, S. D., Bhat, N. D. R., Burgay, M., Burke-Spolaor, S., D'Amico, N., Johnston, S., Keith, M. J., Kramer, M., Milia, S., Possenti, A., Stappers, B., and van Straten, W.
- Subjects
High Energy Astrophysical Phenomena (astro-ph.HE) ,FOS: Physical sciences ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
Here we report on observations of the radio magnetar PSR J1622-4950 at frequencies from 1.4 to 17 GHz. We show that although its flux density is varying up to a factor of ~10 within a few days, it has on average decreased by a factor of 2 over the last 700 days. At the same time, timing analysis indicates a trend of decreasing spin-down rate over our entire data set, again of about a factor of 2 over 700 days, but also an erratic variability in the spin-down rate within this time span. Integrated pulse profiles are often close to 100 per cent linearly polarized, but large variations in both the profile shape and fractional polarization are regularly observed. Furthermore, the behaviour of the position angle of the linear polarization is very complex - offsets in both the absolute position angle and the phase of the position angle sweep are often seen and the occasional presence of orthogonal mode jumps further complicates the picture. However, model fitting indicates that the magnetic and rotation axes are close to aligned. Finally, a single pulse analysis has been carried out at four observing frequencies, demonstrating that the wide pulse profile is built up of narrow spikes of emission, with widths that scale inversely with observing frequency. All three of the known radio magnetars seem to have similar characteristics, with highly polarized emission, time-variable flux density and pulse profiles, and with spectral indices close to zero., Comment: 12 pages, 8 figures, 2 tables; Monthly Notices of the Royal Astronomical Society, Online Early
- Published
- 2012
42. Processi innovativi per il risanamento sostenibile di acque sotterranee contaminate da composti clorurati (Progetto PRIN 2008)
- Author
-
Majone M., Andreozzi R., Marotta R., Aulenta F., Rossetti S., Berlin L., Frascari D., Carucci A., and Milia S.
- Subjects
risanamento ,prin 2008 ,idrocarburi clorurati - Published
- 2012
43. Effects of the cometabolite/growth substrate ratio on the aerobic degradation of 4-monochlorophenol
- Author
-
Milia S., Cappai, De Gioannis, and Carucci
- Subjects
4-monochlorophenol ,cometabolite/growth ,aerobic degradation - Published
- 2011
44. A direct comparison amongst different technologies (aerobic granular sludge, SBR and MBR) for the treatment of wastewater contaminated by 4-chlorophenol
- Author
-
Carucci A., Milia S., Cappai G., and Muntoni A.
- Subjects
wastewater contaminated ,treatment ,4-chlorophenol - Abstract
Environmental concern on chlorinated phenols is rising due to their extreme toxicity even at low concentrations and their persistency in water and soils. Since the high amount of published data often lacks in terms of uniformity, direct comparisons amongst different treatment technologies are very difficult, or even impossible. In this study, granular sludge developed in an acetate-fed Granular sludge Sequencing Batch Reactor (GSBR) was used for the aerobic degradation of low chlorinated 4-chlorophenol (4CP), with readily biodegradable sodium acetate (NaAc) as growth substrate. A conventional Sequencing Batch Reactor (SBR) and a Membrane BioReactor (MBR) were operated in parallel under the same 4CP influent concentrations and/or 4CP volumetric organic loading rates as the GSBR, in order to carry out a direct comparison in terms of 4CP removal efficiencies and specific removal rates, effluent quality, waste sludge production, system simplicity, land area requirement, start-up times, NaAc dosage as growth substrate and maximum applied 4CP volumetric organic loading rate. A decision matrix was built to define the best technology to suit different scenarios: the GSBR was proved to be the most suitable technology when system simplicity, low land area requirement and short start-up times were considered as critical parameters for decision making.
- Published
- 2010
45. History, geography and population structure influence the distribution and heritability of blood and anthropometric quantitative traits in nine Sardinian genetic isolates
- Author
-
Portas L, Murgia F, Biino G, Concas MP, Casula L, Milia S, Whalen MB, Vaccargiu S, Cosso M, Parracciani D, Frongia B, and Pirastu M. Source
- Subjects
Heritability ,Quantitative Traits ,Isolated Populations - Abstract
Isolated founder populations which exhibit great genetic and environmental homogeneity provide an attractive setting for the study of quantitative traits (QTs). Geneticists have repeatedly turned to population isolates and the past successes have prompted increased interest among medical researchers. We studied nine small isolated villages of a secluded area of Sardinia (Ogliastra), all of them characterized by a few founders, high endogamy rates, slow population expansion and a distinct genetic makeup. Anthropometric and blood parameters, 43 QTs in all, were analysed in about 9000 voluntary subjects for whom extended genealogical information was available. We explored the distribution and examined mean differences of each trait among villages by analysis of variance (ANOVA). A heritability analysis with the variance component (VC) method was performed. Results show significant differences in the distribution of most traits between groups of villages located in two distinct geographical areas already identified by a previous population structure analysis, thus supporting the existence of differentiation among sub-populations in the same region. Heritability estimates range between 30 and 89%, demonstrating that genetic effects substantially contribute to phenotypic variation of all investigated traits and that this population provides excellent research conditions for gene-mapping projects. Results suggest that history, geographic location and population structure may have influenced the genetic and phenotypic features of these isolates. Our findings may be useful for the ongoing linkage and association studies in these isolates and suggest that a thorough characterization of population is valuable to better identify genes or variants that may be rare in the population at large and peculiar to single villages.
- Published
- 2010
46. The High Time Resolution Universe survey – XI. Discovery of five recycled pulsars and the optical detectability of survey white dwarf companions
- Author
-
Bates, S. D., primary, Thornton, D., additional, Bailes, M., additional, Barr, E., additional, Bassa, C. G., additional, Bhat, N. D. R., additional, Burgay, M., additional, Burke-Spolaor, S., additional, Champion, D. J., additional, Flynn, C. M. L., additional, Jameson, A., additional, Johnston, S., additional, Keith, M. J., additional, Kramer, M., additional, Levin, L., additional, Lyne, A., additional, Milia, S., additional, Ng, C., additional, Petroff, E., additional, Possenti, A., additional, Stappers, B. W., additional, van Straten, W., additional, and Tiburzi, C., additional
- Published
- 2014
- Full Text
- View/download PDF
47. Effect of accelerated carbonation on MSWI bottom ash and its particle size fractions
- Author
-
Cappai G., Milia S., Muntoni A., and Piredda M.
- Subjects
carbonation ,MSWI ,ash - Published
- 2009
48. A direct comparison between different technologies (aerobic granular sludge, SBR and MBR) for the treatment of wastewater contaminated by 4-mono-chlorophenol
- Author
-
Carucci A., Milia S., Cappai G., and Muntoni A.
- Subjects
4-chlorophenol ,wastewater ,contaminated - Published
- 2009
49. La rimozione dei composti organoclorurati dalle acque: possibili applicazioni di trattamenti biologici innovativi
- Author
-
Cappai G., Carucci A., Manigas L., and Milia S.
- Published
- 2007
50. Fanghi aerobici granulari per il trattamento biologico delle acque reflue
- Author
-
Carucci A. and Milia S.
- Published
- 2006
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