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120 results on '"Carotenuto, Francesco"'

1. The Radio Counterpart to the Fast X-ray Transient EP240414a

Author: Bright, Joe S., Carotenuto, Francesco, Fender, Rob, Choza, Carmen, Mummery, Andrew, Jonker, Peter G., Smartt, Stephen J., DeBoer, David R., Farah, Wael, Matthews, James, Pollak, Alexander W., Rhodes, Lauren, and Siemion, Andrew
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Despite being operational for only a short time, the Einstein Probe mission has already significantly advanced the study of rapid variability in the soft X-ray sky. We report the discovery of luminous and variable radio emission from the Einstein Probe fast X-ray transient EP240414a, the second such source with a radio counterpart. The radio emission at $3\,\rm{GHz}$ peaks at $\sim30$ days post explosion and with a spectral luminosity $\sim2\times10^{30}\,\rm{erg}\,\rm{s}^{-1}\,\rm{Hz}^{-1}$, similar to what is seen from long gamma-ray bursts, and distinct from other extra-galactic transients including supernovae and tidal disruption events, although we cannot completely rule out emission from engine driven stellar explosions e.g. the fast blue optical transients. An equipartition analysis of our radio data reveals that an outflow with at least a moderate bulk Lorentz factor ($\Gamma\gtrsim1.6$) with a minimum energy of $\sim10^{48}\,\rm{erg}$ is required to explain our observations. The apparent lack of reported gamma-ray counterpart to EP240414a could suggest that an off-axis or choked jet could be responsible for the radio emission, although a low luminosity gamma-ray burst may have gone undetected. Our observations are consistent with the hypothesis that a significant fraction of extragalactic fast X-ray transients are associated with the deaths of massive stars., Comment: 11 pages, 6 figures, submitted to ApJL
Published: 2024

2. X-ray and Radio campaign of the Z-source GX 340+0: discovery of X-ray polarization and its implications

Author: Bhargava, Yash, Ng, Mason, Zhang, Liang, Balasubramanian, Arvind, Russell, Thomas D., Kaushik, Aman, Jadoliya, Vishal, Ravi, Swati, Bhattacharyya, Sudip, Pahari, Mayukh, Homan, Jeroen, Marshall, Herman L., Chakrabarty, Deepto, and Carotenuto, Francesco
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We present the discovery of X-ray polarization from the neutron star low-mass X-ray binary and Z-source, GX~340$+$0, using an Imaging X-ray Polarimetry Explorer (IXPE) observation in March 2024. Along with the IXPE observation, we conducted an extensive X-ray and radio monitoring campaign to ascertain the source properties during and around the IXPE observation. The source was within the horizontal branch throughout the multiwavelength campaign. We measured a significant X-ray polarization in 2--8 keV with polarization degree (PD) = $4.02 \pm 0.35$% and polarization angle (PA) = $37.6 \pm 2.5^\circ$. The energy-dependent polarization indicates that in the 2-2.5 keV energy range, the PA is much lower, $\sim9\pm8^\circ$, while other energy bands are consistent with the PA found over 2.5--8 keV. The simultaneous AstroSat-IXPE spectro-polarimetric observations provide some evidence for independent polarization from various spectral components, hinting at a disparity in the PA from the accretion disk and the Comptonized emission, while suggesting an unpolarized emission from the blackbody component. Radio observations in the 0.7--9 GHz frequency range reveal a non-detection of radio emission in 0.7-1.5 GHz and a significant detection in 5.5--9 GHz, suggesting the presence of a spectral break in 1.5-5.5 GHz. Using ATCA observation we place upper limits on the radio polarization at $<$6% on the linear polarization and $<$4% on the circular polarization at 3$\sigma$ level. We discuss the origin of the X-ray polarization and its implications on the geometry of the spectral components., Comment: Submitted in ApJL, 4 figures, 3 tables
Published: 2024

3. Constraining the physical properties of large-scale jets from black hole X-ray binaries and their impact on the local environment with blast-wave dynamical models

Author: Carotenuto, Francesco, Fender, Rob, Tetarenko, Alexandra J., Corbel, Stéphane, Zdziarski, Andrzej A., Shaik, Gulzar, Cooper, Alex J., and Di Palma, Irene
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Relativistic discrete ejecta launched by black hole X-ray binaries (BH XRBs) can be observed to propagate up to parsec-scales from the central object. Observing the final deceleration phase of these jets is crucial to estimate their physical parameters and to reconstruct their full trajectory, with implications for the jet powering mechanism, composition and formation. In this paper we present the results of the modelling of the motion of the ejecta from three BH XRBs: MAXI J1820+070, MAXI J1535$-$571 and XTE J1752$-$223, for which high-resolution radio and X-ray observations of jets propagating up to $\sim$15 arcsec ($\sim$0.6 pc at 3 kpc) from the core have been published in the recent years. For each jet, we modeled its entire motion with a dynamical blast-wave model, inferring robust values for the jet Lorentz factor, inclination angle and ejection time. Under several assumptions associated to the ejection duration, the jet opening angle and the available accretion power, we are able to derive stringent constraints on the maximum jet kinetic energy for each source (between $10^{43}$ and $10^{44}$ erg, including also H1743$-$322), as well as placing interesting upper limits on the density of the ISM through which the jets are propagating (from $n_{\rm ISM} \lesssim 0.4$ cm$^{-3}$ down to $n_{\rm ISM} \lesssim 10^{-4}$ cm$^{-3}$). Overall, our results highlight the potential of applying models derived from gamma-ray bursts to the physics of jets from BH XRBs and support the emerging picture of these sources as preferentially embedded in low-density environments., Comment: 22 pages, 9 figures. Accepted for publication in MNRAS
Published: 2024

4. Swift J1727.8-1613 has the Largest Resolved Continuous Jet Ever Seen in an X-ray Binary

Author: Wood, Callan M., Miller-Jones, James C. A., Bahramian, Arash, Tingay, Steven J., Prabu, Steve, Russell, Thomas D., Atri, Pikky, Carotenuto, Francesco, Altamirano, Diego, Motta, Sara E., Hyland, Lucas, Reynolds, Cormac, Weston, Stuart, Fender, Rob, Körding, Elmar, Maitra, Dipankar, Markoff, Sera, Migliari, Simone, Russell, David M., Sarazin, Craig L., Sivakoff, Gregory R., Soria, Roberto, Tetarenko, Alexandra J., and Tudose, Valeriu
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Multi-wavelength polarimetry and radio observations of Swift J1727.8-1613 at the beginning of its recent 2023 outburst suggested the presence of a bright compact jet aligned in the north-south direction, which could not be confirmed without high angular resolution images. Using the Very Long Baseline Array and the Long Baseline Array, we imaged Swift J1727.8-1613, during the hard/hard-intermediate state, revealing a bright core and a large, two-sided, asymmetrical, resolved jet. The jet extends in the north-south direction, at a position angle of $-0.60\pm0.07\deg$ East of North. At 8.4 GHz, the entire resolved jet structure is $\sim110 (d/2.7\,\text{kpc})/\sin i$ AU long, with the southern approaching jet extending $\sim80 (d/2.7\,\text{kpc})/\sin i$ AU from the core, where $d$ is the distance to the source and $i$ is the inclination of the jet axis to the line of sight. These images reveal the most resolved continuous X-ray binary jet, and possibly the most physically extended continuous X-ray binary jet ever observed. Based on the brightness ratio of the approaching and receding jets, we put a lower limit on the intrinsic jet speed of $\beta\geq0.27$ and an upper limit on the jet inclination of $i\leq74\deg$. In our first observation we also detected a rapidly fading discrete jet knot $66.89\pm0.04$ mas south of the core, with a proper motion of $0.66\pm0.05$ mas hour$^{-1}$, which we interpret as the result of a downstream internal shock or a jet-ISM interaction, as opposed to a transient relativistic jet launched at the beginning of the outburst., Comment: Accepted in ApJL
Published: 2024
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5. The fast X-ray transient EP240315a: a z ~ 5 gamma-ray burst in a Lyman continuum leaking galaxy

Author: Levan, Andrew J., Jonker, Peter G., Saccardi, Andrea, Malesani, Daniele Bjørn, Tanvir, Nial R., Izzo, Luca, Heintz, Kasper E., Sánchez, Daniel Mata, Quirola-Vásquez, Jonathan, Torres, Manuel A. P., Vergani, Susanna D., Schulze, Steve, Rossi, Andrea, D'Avanzo, Paolo, Gompertz, Benjamin, Martin-Carrillo, Antonio, Postigo, Antonio de Ugarte, Schneider, Benjamin, Yuan, Weimin, Ling, Zhixing, Zhang, Wenjie, Mao, Xuan, Liu, Yuan, Sun, Hui, Xu, Dong, Zhu, Zipei, Fernández, José Feliciano Agüí, Amati, Lorenzo, Bauer, Franz E., Campana, Sergio, Carotenuto, Francesco, Chrimes, Ashley, van Dalen, Joyce N. D., D'Elia, Valerio, Della Valle, Massimo, De Pasquale, Massimiliano, Dhillon, Vikram S., Galbany, Lluís, Gaspari, Nicola, Gianfagna, Giulia, Gomboc, Andreja, Habeeb, Nusrin, van Hoof, Agnes P. C., Hu, Youdong, Jakobsson, Pall, Julakanti, Yashaswi, Korth, Judith, Kouveliotou, Chryssa, Laskar, Tanmoy, Littlefair, Stuart P., Maiorano, Elisabetta, Mao, Jirong, Melandri, Andrea, Miller, M. Coleman, Mukherjee, Tamal, Oates, Samantha R., O'Brien, Paul, Palmerio, Jesse T., Parviainen, Hannu, Pieterse, Daniëlle L. A., Piranomonte, Silvia, Piro, Luigi, Pugliese, Giovanna, Ravasio, Maria E., Rayson, Ben, Salvaterra, Ruben, Sánchez-Ramírez, Rubén, Sarin, Nikhil, Shilling, Samuel P. R., Starling, Rhaana L. C., Tagliaferri, Gianpiero, Thakur, Aishwarya Linesh, Thöne, Christina C., Wiersema, Klaas, Worssam, Isabelle, and Zafar, Tayyaba
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: The nature of the minute-to-hour long Fast X-ray Transients (FXTs) localised by telescopes such as Chandra, Swift, and XMM-Newton remains mysterious, with numerous models suggested for the events. Here, we report multi-wavelength observations of EP240315a, a 1600 s long transient detected by the Einstein Probe, showing it to have a redshift of z=4.859. We measure a low column density of neutral hydrogen, indicating that the event is embedded in a low-density environment, further supported by direct detection of leaking ionising Lyman-continuum. The observed properties are consistent with EP240315a being a long-duration gamma-ray burst, and these observations support an interpretation in which a significant fraction of the FXT population are lower-luminosity examples of similar events. Such transients are detectable at high redshifts by the Einstein Probe and, in the (near) future, out to even larger distances by SVOM, THESEUS, and Athena, providing samples of events into the epoch of reionisation., Comment: 41 pages, 7 figures, submitted
Published: 2024

6. Tracking the X-ray Polarization of the Black Hole Transient Swift J1727.8-1613 during a State Transition

Author: Ingram, Adam, Bollemeijer, Niek, Veledina, Alexandra, Dovciak, Michal, Poutanen, Juri, Egron, Elise, Russell, Thomas D., Trushkin, Sergei A., Negro, Michela, Ratheesh, Ajay, Capitanio, Fiamma, Connors, Riley, Neilsen, Joseph, Kraus, Alexander, Iacolina, Maria Noemi, Pellizzoni, Alberto, Pilia, Maura, Carotenuto, Francesco, Matt, Giorgio, Mastroserio, Guglielmo, Kaaret, Philip, Bianchi, Stefano, Garcia, Javier A., Bachetti, Matteo, Wu, Kinwah, Costa, Enrico, Ewing, Melissa, Kravtsov, Vadim, Krawczynski, Henric, Loktev, Vladislav, Marinucci, Andrea, Marra, Lorenzo, Mikusincova, Romana, Nathan, Edward, Parra, Maxime, Petrucci, Pierre-Olivier, Righini, Simona, Soffitta, Paolo, Steiner, James F., Svoboda, Jiri, Tombesi, Francesco, Tugliani, Stefano, Ursini, Francesco, Yang, Yi-Jung, Zane, Silvia, Zhang, Wenda, Agudo, Ivan, Antonelli, Lucio A., Baldini, Luca, Baumgartner, Wayne H., Bellazzini, Ronaldo, Bongiorno, Stephen D., Bonino, Raffaella, Brez, Alessandro, Bucciantini, Niccolo, Castellano, Simone, Cavazzuti, Elisabetta, Chen, Chien-Ting, Ciprini, Stefano, De Rosa, Alessandra, Del Monte, Ettore, Di Gesu, Laura, Di Lalla, Niccolo, Di Marco, Alessandro, Donnarumma, Immacolata, Doroshenko, Victor, Ehlert, Steven R., Enoto, Teruaki, Evangelista, Yuri, Fabiani, Sergio, Ferrazzoli, Riccardo, Gunji, Shuichi, Hayashida, Kiyoshi, Heyl, Jeremy, Iwakiri, Wataru, Jorstad, Svetlana G., Karas, Vladimir, Kislat, Fabian, Kitaguchi, Takao, Kolodziejczak, Jeffery J., La Monaca, Fabio, Latronico, Luca, Liodakis, Ioannis, Maldera, Simone, Manfreda, Alberto, Marin, Frederic, Marscher, Alan P., Marshall, Herman L., Massaro, Francesco, Mitsuishi, Ikuyuki, Mizuno, Tsunefumi, Muleri, Fabio, Ng, Chi-Yung, O'Dell, Stephen L., Omodei, Nicola, Oppedisano, Chiara, Papitto, Alessandro, Pavlov, George G., Peirson, Abel L., Perri, Matteo, Pesce-Rollins, Melissa, Possenti, Andrea, Puccetti, Simonetta, Ramsey, Brian D., Rankin, John, Roberts, Oliver J., Romani, Roger W., Sgro, Carmelo, Slane, Patrick, Spandre, Gloria, Swartz, Douglas A., Tamagawa, Toru, Tavecchio, Fabrizio, Taverna, Roberto, Tawara, Yuzuru, Tennant, Allyn F., Thomas, Nicholas E., Trois, Alessio, Tsygankov, Sergey S., Turolla, Roberto, Vink, Jacco, Weisskopf, Martin C., and Xie, Fei
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We report on an observational campaign on the bright black hole X-ray binary Swift J1727.8$-$1613 centered around five observations by the Imaging X-ray Polarimetry Explorer (IXPE). These observations track for the first time the evolution of the X-ray polarization of a black hole X-ray binary across a hard to soft state transition. The 2--8 keV polarization degree decreased from $\sim$4\% to $\sim$3\% across the five observations, but the polarization angle remained oriented in the North-South direction throughout. Based on observations with the Australia Telescope Compact Array (ATCA), we find that the intrinsic 7.25 GHz radio polarization aligns with the X-ray polarization. Assuming the radio polarization aligns with the jet direction (which can be tested in the future with higher spatial resolution images of the jet), our results imply that the X-ray corona is extended in the disk plane, rather than along the jet axis, for the entire hard intermediate state. This in turn implies that the long ($\gtrsim$10 ms) soft lags that we measure with the Neutron star Interior Composition ExploreR (NICER) are dominated by processes other than pure light-crossing delays. Moreover, we find that the evolution of the soft lag amplitude with spectral state does not follow the trend seen for other sources, implying that Swift J1727.8$-$1613 is a member of a hitherto under-sampled sub-population., Comment: Accepted for publication in ApJ. 21 pages, 8 figures
Published: 2023

7. Discovery of a variable energy-dependent X-ray polarization in the accreting neutron star GX 5-1

Author: Fabiani, Sergio, Capitanio, Fiamma, Iaria, Rosario, Poutanen, Juri, Gnarini, Andrea, Ursini, Francesco, Farinelli, Ruben, Bobrikova, Anna, Steiner, James F., Svoboda, Jiri, Anitra, Alessio, Baglio, Maria C., Carotenuto, Francesco, Del Santo, Melania, Ferrigno, Carlo, Lewis, Fraser, Russell, David M., Russell, Thomas D., Eijnden, Jakob van den, Cocchi, Massimo, Di Marco, Alessandro, La Monaca, Fabio, Liu, Kuan, Rankin, John, Weisskopf, Martin C., Xie, Fei, Bianchi, Stefano, Burderi, Luciano, Di Salvo, Tiziana, Egron, Elise, Illiano, Giulia, Kaaret, Philip, Matt, Giorgio, Mikušincová, Romana, Muleri, Fabio, Papitto, Alessandro, Agudo, Iván, Antonelli, Lucio A., Bachetti, Matteo, Baldini, Luca, Baumgartner, Wayne H., Bellazzini, Ronaldo, Bongiorno, Stephen D., Bonino, Raffaella, Brez, Alessandro, Bucciantini, Niccolò, Castellano, Simone, Cavazzuti, Elisabetta, Chen, Chien-Ting, Ciprini, Stefano, Costa, Enrico, De Rosa, Alessandra, Del Monte, Ettore, Di Gesu, Laura, Di Lalla, Niccolò, Donnarumma, Immacolata, Doroshenko, Victor, Dovčiak, Michal, Ehlert, Steven R., Enoto, Teruaki, Evangelista, Yuri, Ferrazzoli, Riccardo, Garcia, Javier A., Gunji, Shuichi, Hayashida, Kiyoshi, Heyl, Jeremy, Iwakiri, Wataru, Jorstad, Svetlana G., Karas, Vladimir, Kislat, Fabian, Kitaguchi, Takao, Kolodziejczak, Jeffery J., Krawczynski, Henric, Latronico, Luca, Liodakis, Ioannis, Maldera, Simone, Manfreda, Alberto, Marin, Frédéric, Marinucci, Andrea, Marscher, Alan P., Marshall, Herman L., Massaro, Francesco, Mitsuishi, Ikuyuki, Mizuno, Tsunefumi, Negro, Michela, Ng, Chi-Yung, O'Dell, Stephen L., Omodei, Nicola, Oppedisano, Chiara, Pavlov, George G., Peirson, Abel L., Perri, Matteo, Pesce-Rollins, Melissa, Petrucci, Pierre-Olivier, Pilia, Maura, Possenti, Andrea, Puccetti, Simonetta, Ramsey, Brian D., Ratheesh, Ajay, Roberts, Oliver J., Romani, Roger W., Sgrò, Carmelo, Slane, Patrick, Soffitta, Paolo, Spandre, Gloria, Swartz, Douglas A., Tamagawa, Toru, Tavecchio, Fabrizio, Taverna, Roberto, Tawara, Yuzuru, Tennant, Allyn F., Thomas, Nicholas E., Tombesi, Francesco, Trois, Alessio, Tsygankov, Sergey S., Turolla, Roberto, Vink, Jacco, Wu, Kinwah, and Zane, Silvia
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We report on the coordinated observations of the neutron star low-mass X-ray binary (NS-LMXB) \gx in X-rays (IXPE, NICER, Nustar and INTEGRAL), optical (REM and LCO), near-infrared (REM), mid-infrared (VLT VISIR), and radio (ATCA). This Z-source was observed by \IXPE twice in March-April 2023 (Obs. 1 and 2). In the radio band, the source was detected, but only upper-limits to the linear polarization were obtained at a $3\sigma$ level of $6.1\%$ at 5.5 GHz and $5.9\%$ at 9 GHz in Obs.~1 and $12.5\%$ at 5.5~GHz and $20\%$ at 9~GHz in Obs.~2. The mid-IR, near-IR and optical observations suggest the presence of a compact jet which peaks in the mid- or far-IR. The X-ray polarization degree was found to be $3.7\% \pm 0.4 \%$ (at $90\%$ confidence level) during Obs.~1 when the source was in the horizontal branch of the Z-track and $1.8\% \pm 0.4 \%$ during Obs.~2 when the source was in the normal-flaring branch. These results confirm the variation of polarization degree as a function of the position of the source in the color-color diagram as for previously observed Z-track sources (Cyg~X-2 and XTE~1701$-$462). Evidence for a variation of the polarization angle $\sim 20^\circ$ with energy is found in both observations, likely related to the different, non-orthogonal polarization angles of the disk and Comptonization components which peak at different energies., Comment: Submitted to Astronomy and Astrophysics on 06 July 2023. Accepted on 21 November 2023
Published: 2023

8. First detection of X-ray polarization from the accreting neutron star 4U 1820-303

Author: Di Marco, Alessandro, La Monaca, Fabio, Poutanen, Juri, Russell, Thomas D., Anitra, Alessio, Farinelli, Ruben, Mastroserio, Guglielmo, Muleri, Fabio, Xie, Fei, Bachetti, Matteo, Burderi, Luciano, Carotenuto, Francesco, Del Santo, Melania, Di Salvo, Tiziana, Dovciak, Michal, Gnarini, Andrea, Iaria, Rosario, Kajava, Jari J. E., Liu, Kuan, Middei, Riccardo, O'Dell, Stephen L., Pilia, Maura, Rankin, John, Sanna, Andrea, Eijnden, Jakob van den, Weisskopf, Martin C., Bobrikova, Anna, Capitanio, Fiamma, Costa, Enrico, Kaaret, Philip, Marino, Alessio, Soffitta, Paolo, Ursini, Francesco, Ambrosino, Filippo, Cocchi, Massimo, Fabiani, Sergio, Marshall, Herman L., Matt, Giorgio, Motta, Sara Elisa, Papitto, Alessandro, Stella, Luigi, Tarana, Antonella, Zane, Silvia, Agudo, Ivan, Antonelli, Lucio A., Baldini, Luca, Baumgartner, Wayne H., Bellazzini, Ronaldo, Bianchi, Stefano, Bongiorno, Stephen D., Bonino, Raffaella, Brez, Alessandro, Bucciantini, Niccolo, Castellano, Simone, Cavazzuti, Elisabetta, Chen, Chien-Ting, Ciprini, Stefano, De Rosa, Alessandra, Del Monte, Ettore, Di Gesu, Laura, Di Lalla, Niccolo, Donnarumma, Immacolata, Doroshenko, Victor, Ehlert, Steven R., Enoto, Teruaki, Evangelista, Yuri, Ferrazzoli, Riccardo, Garcia, Javier A., Gunji, Shuichi, Hayashida, Kiyoshi, Heyl, Jeremy, Iwakiri, Wataru, Jorstad, Svetlana G., Karas, Vladimir, Kislat, Fabian, Kitaguchi, Takao, Kolodziejczak, Jeffery J., Krawczynski, Henric, Latronico, Luca, Liodakis, Ioannis, Maldera, Simone, Manfreda, Alberto, Marin, Frederic, Marinucci, Andrea, Marscher, Alan P., Massaro, Francesco, Mitsuishi, Ikuyuki, Mizuno, Tsunefumi, Negro, Michela, Ng, Chi-Yung, Omodei, Nicola, Oppedisano, Chiara, Pavlov, George G., Peirson, Abel L., Perri, Matteo, Pesce-Rollins, Melissa, Petrucci, Pierre-Olivier, Possenti, Andrea, Puccetti, Simonetta, Ramsey, Brian D., Ratheesh, Ajay, Roberts, Oliver J., Romani, Roger W., Sgrò, Carmelo, Slane, Patrick, Spandre, Gloria, Swartz, Douglas A., Tamagawa, Toru, Tavecchio, Fabrizio, Taverna, Roberto, Tawara, Yuzuru, Tennant, Allyn F., Thomas, Nicholas E., Tombesi, Francesco, Trois, Alessio, Tsygankov, Sergey S., Turolla, Roberto, Vink, Jacco, and Wu, Kinwah
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: This paper reports the first detection of polarization in the X-rays for atoll-source 4U 1820-303, obtained with the Imaging X-ray Polarimetry Explorer (IXPE) at 99.999% confidence level (CL). Simultaneous polarimetric measurements were also performed in the radio with the Australia Telescope Compact Array (ATCA). The IXPE observations of 4U 1820-303 were coordinated with Swift-XRT, NICER, and NuSTAR aiming to obtain an accurate X-ray spectral model covering a broad energy interval. The source shows a significant polarization above 4 keV, with a polarization degree of 2.0(0.5)% and a polarization angle of -55(7) deg in the 4-7 keV energy range, and a polarization degree of 10(2)% and a polarization angle of -67(7) deg in the 7-8 keV energy bin. This polarization also shows a clear energy trend with polarization degree increasing with energy and a hint for a position-angle change of about 90 deg at 96% CL around 4 keV. The spectro-polarimetric fit indicates that the accretion disk is polarized orthogonally to the hard spectral component, which is presumably produced in the boundary/spreading layer. We do not detect linear polarization from the radio counterpart, with a 99.97% upper limit of 50% at 7.25 GHz.
Published: 2023
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9. Bursts from Space: MeerKAT - The first citizen science project dedicated to commensal radio transients

Author: Andersson, Alex, Lintott, Chris, Fender, Rob, Bright, Joe, Carotenuto, Francesco, Driessen, Laura, Espinasse, Mathilde, Gaseahalwe, Kelebogile, Heywood, Ian, van der Horst, Alexander J., Motta, Sara, Rhodes, Lauren, Tremou, Evangelia, Williams, David R. A., Woudt, Patrick, Zhang, Xian, Bloemen, Steven, Groot, Paul, Vreeswijk, Paul, Giarratana, Stefano, Saikia, Payaswini, Andersson, Jonas, Arroyo, Lizzeth Ruiz, Baert, Loïc, Baumann, Matthew, Domainko, Wilfried, Eschweiler, Thorsten, Forsythe, Tim, Gaudenzi, Sauro, Grenier, Rachel Ann, Iannone, Davide, Lahoz, Karla, Melville, Kyle J., Nascimento, Marianne De Sousa, Navarro, Leticia, Parthasarathi, Sai, Piilonen, Rahman, Najma, Smith, Jeffrey, Stewart, B., Temoke, Newton, Tworek, Chloe, and Whittle, Isabelle
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The newest generation of radio telescopes are able to survey large areas with high sensitivity and cadence, producing data volumes that require new methods to better understand the transient sky. Here we describe the results from the first citizen science project dedicated to commensal radio transients, using data from the MeerKAT telescope with weekly cadence. Bursts from Space: MeerKAT was launched late in 2021 and received ~89000 classifications from over 1000 volunteers in 3 months. Our volunteers discovered 142 new variable sources which, along with the known transients in our fields, allowed us to estimate that at least 2.1 per cent of radio sources are varying at 1.28 GHz at the sampled cadence and sensitivity, in line with previous work. We provide the full catalogue of these sources, the largest of candidate radio variables to date. Transient sources found with archival counterparts include a pulsar (B1845-01) and an OH maser star (OH 30.1-0.7), in addition to the recovery of known stellar flares and X-ray binary jets in our observations. Data from the MeerLICHT optical telescope, along with estimates of long time-scale variability induced by scintillation, imply that the majority of the new variables are active galactic nuclei. This tells us that citizen scientists can discover phenomena varying on time-scales from weeks to several years. The success both in terms of volunteer engagement and scientific merit warrants the continued development of the project, whilst we use the classifications from volunteers to develop machine learning techniques for finding transients., Comment: Accepted to MNRAS, 14 pages + an appendix containing our main data table
Published: 2023
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10. The earliest Ethiopian wolf: implications for the species evolution and its future survival.

Author: Martínez-Navarro, Bienvenido, Gossa, Tegenu, Carotenuto, Francesco, Bartolini-Lucenti, Saverio, Palmqvist, Paul, Asrat, Asfawossen, Figueirido, Borja, Rook, Lorenzo, Niespolo, Elizabeth M, Renne, Paul R, Herzlinger, Gadi, and Hovers, Erella
Subjects: Animals, Wolves, Humans, Biodiversity, Phylogeny, Africa, Endangered Species, Life on Land
Abstract: In 2017, a hemimandible (MW5-B208), corresponding to the Ethiopian wolf (Canis simensis), was found in a stratigraphically-controlled and radio-isotopically-dated sequence of the Melka Wakena paleoanthropological site-complex, on the Southeastern Ethiopian Highlands, ~ 2300 m above sea level. The specimen is the first and unique Pleistocene fossil of this species. Our data provide an unambiguous minimum age of 1.6-1.4 Ma for the species' presence in Africa and constitutes the first empirical evidence that supports molecular interpretations. Currently, C. simensis is one of the most endangered carnivore species of Africa. Bioclimate niche modeling applied to the time frame indicated by the fossil suggests that the lineage of the Ethiopian wolf faced severe survival challenges in the past, with consecutive drastic geographic range contractions during warmer periods. These models help to describe future scenarios for the survival of the species. Projections ranging from most pessimistic to most optimistic future climatic scenarios indicate significant reduction of the already-deteriorating territories suitable for the Ethiopian Wolf, increasing the threat to the specie's future survival. Additionally, the recovery of the Melka Wakena fossil underscores the importance of work outside the East African Rift System in research of early human origins and associated biodiversity on the African continent.
Published: 2023

11. Search for gravitational-wave signals associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo

Author: Abbott, B. P., Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, C., Adhikari, R. X., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, G., Allocca, A., Aloy, M. A., Altin, P. A., Amato, A., Anand, S., Ananyeva, A., Anderson, S. B., Anderson, W. G., Angelova, S. V., Antier, S., Appert, S., Arai, K., Araya, M. C., Areeda, J. S., Arène, M., Arnaud, N., Aronson, S. M., Ascenzi, S., Ashton, G., Aston, S. M., Astone, P., Aubin, F., Aufmuth, P., AultONeal, K., Austin, C., Avendano, V., Avila-Alvarez, A., Babak, S., Bacon, P., Badaracco, F., Bader, M. K. M., Bae, S., Baird, J., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Bals, A., Banagiri, S., Barayoga, J. C., Barbieri, C., Barclay, S. E., Barish, B. C., Barker, D., Barkett, K., Barnum, S., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Bawaj, M., Bayley, J. C., Bazzan, M., Bécsy, B., Bejger, M., Belahcene, I., Bell, A. S., Beniwal, D., Benjamin, M. G., Berger, B. K., Bergmann, G., Bernuzzi, S., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhandare, R., Bidler, J., Biggs, E., Bilenko, I. A., Bilgili, S. A., Billingsley, G., Birney, R., Birnholtz, O., Biscans, S., Bischi, M., Biscoveanu, S., Bisht, A., Bitossi, M., Bizouard, M. A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bobba, F., Bode, N., Boer, M., Boetzel, Y., Bogaert, G., Bondu, F., Bonnand, R., Booker, P., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bossilkov, V., Bosveld, J., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Bramley, A., Branchesi, M., Brau, J. E., Breschi, M., Briant, T., Briggs, J. H., Brighenti, F., Brillet, A., Brinkmann, M., Brockill, P., Brooks, A. F., Brooks, J., Brown, D. D., Brunett, S., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Bustillo, J. Calderón, Callister, T. A., Calloni, E., Camp, J. B., Campbell, W. A., Canepa, M., Cannon, K. C., Cao, H., Cao, J., Carapella, G., Carbognani, F., Caride, S., Carney, M. F., Carullo, G., Diaz, J. Casanueva, Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cerdá-Durán, P., Cesarini, E., Chaibi, O., Chakravarti, K., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chase, E. A., Chassande-Mottin, E., Chatterjee, D., Chaturvedi, M., Cheeseboro, B. D., Chen, H. Y., Chen, X., Chen, Y., Cheng, H. -P., Cheong, C. K., Chia, H. Y., Chiadini, F., Chincarini, A., Chiummo, A., Cho, G., Cho, H. S., Cho, M., Christensen, N., Chu, Q., Chua, S., Chung, K. W., Chung, S., Ciani, G., Cieślar, M., Ciobanu, A. A., Ciolfi, R., Cipriano, F., Cirone, A., Clara, F., Clark, J. A., Clearwater, P., Cleva, F., Coccia, E., Cohadon, P. -F., Cohen, D., Colleoni, M., Collette, C. G., Collins, C., Colpi, M., Cominsky, L. R., Constancio Jr., M., Conti, L., Cooper, S. J., Corban, P., Corbitt, T. R., Cordero-Carrión, I., Corezzi, S., Corley, K. R., Cornish, N., Corre, D., Corsi, A., Cortese, S., Costa, C. A., Cotesta, R., Coughlin, M. W., Coughlin, S. B., Coulon, J. -P., Countryman, S. T., Couvares, P., Covas, P. B., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Creighton, J. D. E., Creighton, T. D., Cripe, J., Croquette, M., Crowder, S. G., Cullen, T. J., Cumming, A., Cunningham, L., Cuoco, E., Canton, T. Dal, Dálya, G., D'Angelo, B., Danilishin, S. L., D'Antonio, S., Danzmann, K., Dasgupta, A., Costa, C. F. Da Silva, Datrier, L. E. H., Dattilo, V., Dave, I., Davier, M., Davis, D., Daw, E. J., DeBra, D., Deenadayalan, M., Degallaix, J., De Laurentis, M., Deléglise, S., Del Pozzo, W., DeMarchi, L. M., Demos, N., Dent, T., De Pietri, R., De Rosa, R., De Rossi, C., DeSalvo, R., de Varona, O., Dhurandhar, S., Díaz, M. C., Dietrich, T., Di Fiore, L., DiFronzo, C., Di Giorgio, C., Di Giovanni, F., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Ding, B., Di Pace, S., Di Palma, I., Di Renzo, F., Divakarla, A. K., Dmitriev, A., Doctor, Z., Donovan, F., Dooley, K. L., Doravari, S., Dorrington, I., Downes, T. P., Drago, M., Driggers, J. C., Du, Z., Ducoin, J. -G., Dupej, P., Durante, O., Dwyer, S. E., Easter, P. J., Eddolls, G., Edo, T. B., Effler, A., Ehrens, P., Eichholz, J., Eikenberry, S. S., Eisenmann, M., Eisenstein, R. A., Errico, L., Essick, R. C., Estelles, H., Estevez, D., Etienne, Z. B., Etzel, T., Evans, M., Evans, T. M., Fafone, V., Fairhurst, S., Fan, X., Farinon, S., Farr, B., Farr, W. M., Fauchon-Jones, E. J., Favata, M., Fays, M., Fazio, M., Fee, C., Feicht, J., Fejer, M. M., Feng, F., Fernandez-Galiana, A., Ferrante, I., Ferreira, E. C., Ferreira, T. A., Fidecaro, F., Fiori, I., Fiorucci, D., Fishbach, M., Fisher, R. P., Fishner, J. M., Fittipaldi, R., Fitz-Axen, M., Fiumara, V., Flaminio, R., Fletcher, M., Floden, E., Flynn, E., Fong, H., Font, J. A., Forsyth, P. W. F., Fournier, J. -D., Vivanco, Francisco Hernandez, Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. V., Fronzè, G., Fulda, P., Fyffe, M., Gabbard, H. A., Gadre, B. U., Gaebel, S. M., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., García-Quirós, C., Garufi, F., Gateley, B., Gaudio, S., Gaur, G., Gayathri, V., Gemme, G., Genin, E., Gennai, A., George, D., George, J., Gergely, L., Ghonge, S., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giacomazzo, B., Giaime, J. A., Giardina, K. D., Gibson, D. R., Gill, K., Glover, L., Gniesmer, J., Godwin, P., Goetz, E., Goetz, R., Goncharov, B., González, G., Castro, J. M. Gonzalez, Gopakumar, A., Gossan, S. E., Gosselin, M., Gouaty, R., Grace, B., Grado, A., Granata, M., Grant, A., Gras, S., Grassia, P., Gray, C., Gray, R., Greco, G., Green, A. C., Green, R., Gretarsson, E. M., Grimaldi, A., Grimm, S. J., Groot, P., Grote, H., Grunewald, S., Gruning, P., Guidi, G. M., Gulati, H. K., Guo, Y., Gupta, A., Gupta, Anchal, Gupta, P., Gustafson, E. K., Gustafson, R., Haegel, L., Halim, O., Hall, B. R., Hall, E. D., Hamilton, E. Z., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hannuksela, O. A., Hansen, T. J., Hanson, J., Harder, T., Hardwick, T., Haris, K., Harms, J., Harry, G. M., Harry, I. W., Hasskew, R. K., Haster, C. J., Haughian, K., Hayes, F. J., Healy, J., Heidmann, A., Heintze, M. C., Heitmann, H., Hellman, F., Hello, P., Hemming, G., Hendry, M., Heng, I. S., Hennig, J., Heurs, M., Hild, S., Hinderer, T., Hochheim, S., Hofman, D., Holgado, A. M., Holland, N. A., Holt, K., Holz, D. E., Hopkins, P., Horst, C., Hough, J., Howell, E. J., Hoy, C. G., Huang, Y., Hübner, M. T., Huerta, E. A., Huet, D., Hughey, B., Hui, V., Husa, S., Huttner, S. H., Huynh-Dinh, T., Idzkowski, B., Iess, A., Inchauspe, H., Ingram, C., Inta, R., Intini, G., Irwin, B., Isa, H. N., Isac, J. -M., Isi, M., Iyer, B. R., Jacqmin, T., Jadhav, S. J., Jani, K., Janthalur, N. N., Jaranowski, P., Jariwala, D., Jenkins, A. C., Jiang, J., Johnson, D. S., Jones, A. W., Jones, D. I., Jones, J. D., Jones, R., Jonker, R. J. G., Ju, L., Junker, J., Kalaghatgi, C. V., Kalogera, V., Kamai, B., Kandhasamy, S., Kang, G., Kanner, J. B., Kapadia, S. J., Karki, S., Kashyap, R., Kasprzack, M., Katsanevas, S., Katsavounidis, E., Katzman, W., Kaufer, S., Kawabe, K., Keerthana, N. V., Kéfélian, F., Keitel, D., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, I., Khan, S., Khazanov, E. A., Khetan, N., Khursheed, M., Kijbunchoo, N., Kim, Chunglee, Kim, J. C., Kim, K., Kim, W., Kim, W. S., Kim, Y. -M., Kimball, C., King, P. J., Kinley-Hanlon, M., Kirchhoff, R., Kissel, J. S., Kleybolte, L., Klika, J. H., Klimenko, S., Knowles, T. D., Koch, P., Koehlenbeck, S. M., Koekoek, G., Koley, S., Kondrashov, V., Kontos, A., Koper, N., Korobko, M., Korth, W. Z., Kovalam, M., Kozak, D. B., Krämer, C., Kringel, V., Krishnendu, N., Królak, A., Krupinski, N., Kuehn, G., Kumar, A., Kumar, P., Kumar, Rahul, Kumar, Rakesh, Kuo, L., Kutynia, A., Kwang, S., Lackey, B. D., Laghi, D., Lai, K. H., Lam, T. L., Landry, M., Lane, B. B., Lang, R. N., Lange, J., Lantz, B., Lanza, R. K., Lartaux-Vollard, A., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lecoeuche, Y. K., Lee, C. H., Lee, H. K., Lee, H. M., Lee, H. W., Lee, J., Lee, K., Lehmann, J., Lenon, A. K., Leroy, N., Letendre, N., Levin, Y., Li, A., Li, J., Li, K. J. L., Li, T. G. F., Li, X., Lin, F., Linde, F., Linker, S. D., Littenberg, T. B., Liu, J., Liu, X., Llorens-Monteagudo, M., Lo, R. K. L., London, L. T., Longo, A., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lousto, C. O., Lovelace, G., Lower, M. E., Lück, H., Lumaca, D., Lundgren, A. P., Lynch, R., Ma, Y., Macas, R., Macfoy, S., MacInnis, M., Macleod, D. M., Macquet, A., Hernandez, I. Magaña, Magaña-Sandoval, F., Magee, R. M., Majorana, E., Maksimovic, I., Malik, A., Man, N., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Mapelli, M., Marchesoni, F., Marion, F., Márka, S., Márka, Z., Markakis, C., Markosyan, A. S., Markowitz, A., Maros, E., Marquina, A., Marsat, S., Martelli, F., Martin, I. W., Martin, R. M., Martinez, V., Martynov, D. V., Masalehdan, H., Mason, K., Massera, E., Masserot, A., Massinger, T. J., Masso-Reid, M., Mastrogiovanni, S., Matas, A., Matichard, F., Matone, L., Mavalvala, N., McCann, J. J., McCarthy, R., McClelland, D. E., McCormick, S., McCuller, L., McGuire, S. C., McIsaac, C., McIver, J., McManus, D. J., McRae, T., McWilliams, S. T., Meacher, D., Meadors, G. D., Mehmet, M., Mehta, A. K., Meidam, J., Villa, E. Mejuto, Melatos, A., Mendell, G., Mercer, R. A., Mereni, L., Merfeld, K., Merilh, E. L., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Messina, F., Metzdorff, R., Meyers, P. M., Meylahn, F., Miani, A., Miao, H., Michel, C., Middleton, H., Milano, L., Miller, A. L., Millhouse, M., Mills, J. C., Milovich-Goff, M. C., Minazzoli, O., Minenkov, Y., Mishkin, A., Mishra, C., Mistry, T., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Mo, G., Moffa, D., Mogushi, K., Mohapatra, S. R. P., Molina-Ruiz, M., Mondin, M., Montani, M., Moore, C. J., Moraru, D., Morawski, F., Moreno, G., Morisaki, S., Mours, B., Mow-Lowry, C. M., Muciaccia, F., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukherjee, Subroto, Mukund, N., Mullavey, A., Munch, J., Muñiz, E. A., Muratore, M., Murray, P. G., Nardecchia, I., Naticchioni, L., Nayak, R. K., Neil, B. F., Neilson, J., Nelemans, G., Nelson, T. J. N., Nery, M., Neunzert, A., Nevin, L., Ng, K. Y., Ng, S., Nguyen, C., Nguyen, P., Nichols, D., Nichols, S. A., Nissanke, S., Nocera, F., North, C., Nuttall, L. K., Obergaulinger, M., Oberling, J., O'Brien, B. D., Oganesyan, G., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Ohta, H., Okada, M. A., Oliver, M., Oppermann, P., Oram, Richard J., O'Reilly, B., Ormiston, R. G., Ortega, L. F., O'Shaughnessy, R., Ossokine, S., Ottaway, D. J., Overmier, H., Owen, B. J., Pace, A. E., Pagano, G., Page, M. A., Pagliaroli, G., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palomba, C., Pan, H., Panda, P. K., Pang, P. T. H., Pankow, C., Pannarale, F., Pant, B. C., Paoletti, F., Paoli, A., Parida, A., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patil, M., Patricelli, B., Payne, E., Pearlstone, B. L., Pechsiri, T. C., Pedersen, A. J., Pedraza, M., Pedurand, R., Pele, A., Penn, S., Perego, A., Perez, C. J., Périgois, C., Perreca, A., Petermann, J., Pfeiffer, H. P., Phelps, M., Phukon, K. S., Piccinni, O. J., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pirello, M., Pitkin, M., Plastino, W., Poggiani, R., Pong, D. Y. T., Ponrathnam, S., Popolizio, P., Powell, J., Prajapati, A. K., Prasad, J., Prasai, K., Prasanna, R., Pratten, G., Prestegard, T., Principe, M., Prodi, G. A., Prokhorov, L., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Quetschke, V., Quinonez, P. J., Raab, F. J., Raaijmakers, G., Radkins, H., Radulesco, N., Raffai, P., Raja, S., Rajan, C., Rajbhandari, B., Rakhmanov, M., Ramirez, K. E., Ramos-Buades, A., Rana, Javed, Rao, K., Rapagnani, P., Raymond, V., Razzano, M., Read, J., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Rettegno, P., Ricci, F., Richardson, C. J., Richardson, J. W., Ricker, P. M., Riemenschneider, G., Riles, K., Rizzo, M., Robertson, N. A., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romanelli, M., Romano, R., Romel, C. L., Romie, J. H., Rose, C. A., Rose, D., Rose, K., Rosińska, D., Rosofsky, S. G., Ross, M. P., Rowan, S., Rüdiger, A., Ruggi, P., Rutins, G., Ryan, K., Sachdev, S., Sadecki, T., Sakellariadou, M., Salafia, O. S., Salconi, L., Saleem, M., Samajdar, A., Sammut, L., Sanchez, E. J., Sanchez, L. E., Sanchis-Gual, N., Sanders, J. R., Santiago, K. A., Santos, E., Sarin, N., Sassolas, B., Sathyaprakash, B. S., Sauter, O., Savage, R. L., Schale, P., Scheel, M., Scheuer, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Schönbeck, A., Schreiber, E., Schulte, B. W., Schutz, B. F., Scott, J., Scott, S. M., Seidel, E., Sellers, D., Sengupta, A. S., Sennett, N., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaddock, D. A., Shaffer, T., Shahriar, M. S., Shaner, M. B., Sharma, A., Sharma, P., Shawhan, P., Shen, H., Shink, R., Shoemaker, D. H., Shoemaker, D. M., Shukla, K., ShyamSundar, S., Siellez, K., Sieniawska, M., Sigg, D., Singer, L. P., Singh, D., Singh, N., Singhal, A., Sintes, A. M., Sitmukhambetov, S., Skliris, V., Slagmolen, B. J. J., Slaven-Blair, T. J., Smith, J. R., Smith, R. J. E., Somala, S., Son, E. J., Soni, S., Sorazu, B., Sorrentino, F., Souradeep, T., Sowell, E., Spencer, A. P., Spera, M., Srivastava, A. K., Srivastava, V., Staats, K., Stachie, C., Standke, M., Steer, D. A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stevenson, S. P., Stocks, D., Stone, R., Stops, D. J., Strain, K. A., Stratta, G., Strigin, S. E., Strunk, A., Sturani, R., Stuver, A. L., Sudhir, V., Summerscales, T. Z., Sun, L., Sunil, S., Sur, A., Suresh, J., Sutton, P. J., Swinkels, B. L., Szczepańczyk, M. J., Tacca, M., Tait, S. C., Talbot, C., Tanner, D. B., Tao, D., Tápai, M., Tapia, A., Tasson, J. D., Taylor, R., Tenorio, R., Terkowski, L., Thomas, M., Thomas, P., Thondapu, S. R., Thorne, K. A., Thrane, E., Tiwari, Shubhanshu, Tiwari, Srishti, Tiwari, V., Toland, K., Tonelli, M., Tornasi, Z., Torres-Forné, A., Torrie, C. I., Töyrä, D., Travasso, F., Traylor, G., Tringali, M. C., Tripathee, A., Trovato, A., Trozzo, L., Tsang, K. W., Tse, M., Tso, R., Tsukada, L., Tsuna, D., Tsutsui, T., Tuyenbayev, D., Ueno, K., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Valentini, M., van Bakel, N., van Beuzekom, M., Brand, J. F. J. van den, Broeck, C. Van Den, Vander-Hyde, D. C., van der Schaaf, L., VanHeijningen, J. V., van Veggel, A. A., Vardaro, M., Varma, V., Vass, S., Vasúth, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Venugopalan, G., Verkindt, D., Vetrano, F., Viceré, A., Viets, A. D., Vinciguerra, S., Vine, D. J., Vinet, J. -Y., Vitale, S., Vo, T., Vocca, H., Vorvick, C., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walet, R., Walker, M., Wallace, L., Walsh, S., Wang, H., Wang, J. Z., Wang, S., Wang, W. H., Wang, Y. F., Ward, R. L., Warden, Z. A., Warner, J., Was, M., Watchi, J., Weaver, B., Wei, L. -W., Weinert, M., Weinstein, A. J., Weiss, R., Wellmann, F., Wen, L., Wessel, E. K., Weßels, P., Westhouse, J. W., Wette, K., Whelan, J. T., Whiting, B. F., Whittle, C., Wilken, D. M., Williams, D., Williamson, A. R., Willis, J. L., Willke, B., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Wofford, J. K., Wright, J. L., Wu, D. S., Wysocki, D. M., Xiao, S., Xu, R., Yamamoto, H., Yancey, C. C., Yang, L., Yang, Y., Yang, Z., Yap, M. J., Yazback, M., Yeeles, D. W., Yu, Hang, Yu, Haocun, Yuen, S. H. R., Zadrożny, A. K., Zadrożny, A., Zanolin, M., Zelenova, T., Zendri, J. -P., Zevin, M., Zhang, J., Zhang, L., Zhang, T., Zhao, C., Zhao, G., Zhou, M., Zhou, Z., Zhu, X. J., Zucker, M. E., Zweizig, J., Collaboration, The LIGO Scientific, Collaboration, the Virgo, Aptekar, R. L., Boynton, W. V., Frederiks, D. D., Golenetskii, S. V., Golovin, D. V., Hurley, K., Kozlova, A. V., Litvak, M. L., Mitrofanov, I. G., Sanin, A. B., Svinkin, D. S., Collaboration, IPN, Carotenuto, Francesco, and Krishnan, Badri
Subjects: Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
Abstract: We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of $<9.38 \times 10^{-6}$ (modeled) and $3.1 \times 10^{-4}$ (unmodeled). We do not find any significant evidence for gravitational-wave signals associated with the other gamma-ray bursts analyzed, and therefore we report lower bounds on the distance to each of these, assuming various source types and signal morphologies. Using our final modeled search results, short gamma-ray burst observations, and assuming binary neutron star progenitors, we place bounds on the rate of short gamma-ray bursts as a function of redshift for $z \leq 1$. We estimate 0.07-1.80 joint detections with Fermi-GBM per year for the 2019-20 LIGO-Virgo observing run and 0.15-3.90 per year when current gravitational-wave detectors are operating at their design sensitivities.
Published: 2019
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12. A Major Change in Rate of Climate Niche Envelope Evolution during Hominid History

Author: Mondanaro, Alessandro, Melchionna, Marina, Di Febbraro, Mirko, Castiglione, Silvia, Holden, Philip B., Edwards, Neil R., Carotenuto, Francesco, Maiorano, Luigi, Modafferi, Maria, Serio, Carmela, Diniz-Filho, Josè A.F., Rangel, Thiago, Rook, Lorenzo, O'Higgins, Paul, Spikins, Penny, Profico, Antonio, and Raia, Pasquale
Published: 2020
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13. Radio transients from compact objects across the mass spectrum in the era of multi-messenger astronomy.

Author: Corsi, Alessandra, Eddins, Avery, Lazio, T. Joseph W., Murphy, Eric J., Osten, Rachel A., and Carotenuto, Francesco
Subjects: MASS spectrometry, BLACK holes, NEUTRON stars, GRAVITATIONAL waves, BINARY black holes
Abstract: Compact objects across the mass spectrum-from neutron stars to supermassive black holes-are progenitors and/or central engines for some of the most cataclysmic phenomena in the Universe. As such, they are associated with radio emission on a variety of timescales and represent key targets for multi-messenger astronomy. Observations of transients in the radio band can unveil the physics behind their central engines, ejecta, and the properties of their surroundings, crucially complementing information on their progenitors gathered from observations of other messengers (such as gravitational waves and neutrinos). In this contribution, we summarize observational opportunities and challenges ahead in the multi-messenger study of neutron stars and black holes using radio observations. We highlight the specific contribution of current U.S. national radio facilities and discuss expectations for the field focusing on the science that could be enabled by facilities recommended by the 2020 Decadal survey such as the next generation Very Large Array (ngVLA). [ABSTRACT FROM AUTHOR]
Published: 2024
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14. First Detection of X-Ray Polarization from the Accreting Neutron Star 4U 1820−303

Author: Di Marco, Alessandro, primary, La Monaca, Fabio, additional, Poutanen, Juri, additional, Russell, Thomas D., additional, Anitra, Alessio, additional, Farinelli, Ruben, additional, Mastroserio, Guglielmo, additional, Muleri, Fabio, additional, Xie, Fei, additional, Bachetti, Matteo, additional, Burderi, Luciano, additional, Carotenuto, Francesco, additional, Del Santo, Melania, additional, Di Salvo, Tiziana, additional, Dovčiak, Michal, additional, Gnarini, Andrea, additional, Iaria, Rosario, additional, Kajava, Jari J. E., additional, Liu, Kuan, additional, Middei, Riccardo, additional, O’Dell, Stephen L., additional, Pilia, Maura, additional, Rankin, John, additional, Sanna, Andrea, additional, Eijnden, Jakob van den, additional, Weisskopf, Martin C., additional, Bobrikova, Anna, additional, Capitanio, Fiamma, additional, Costa, Enrico, additional, Kaaret, Philip, additional, Marino, Alessio, additional, Soffitta, Paolo, additional, Ursini, Francesco, additional, Ambrosino, Filippo, additional, Cocchi, Massimo, additional, Fabiani, Sergio, additional, Marshall, Herman L., additional, Matt, Giorgio, additional, Motta, Sara Elisa, additional, Papitto, Alessandro, additional, Stella, Luigi, additional, Tarana, Antonella, additional, Zane, Silvia, additional, Agudo, Iván, additional, Antonelli, Lucio A., additional, Baldini, Luca, additional, Baumgartner, Wayne H., additional, Bellazzini, Ronaldo, additional, Bianchi, Stefano, additional, Bongiorno, Stephen D., additional, Bonino, Raffaella, additional, Brez, Alessandro, additional, Bucciantini, Niccolò, additional, Castellano, Simone, additional, Cavazzuti, Elisabetta, additional, Chen, Chien-Ting, additional, Ciprini, Stefano, additional, De Rosa, Alessandra, additional, Del Monte, Ettore, additional, Di Gesu, Laura, additional, Di Lalla, Niccolò, additional, Donnarumma, Immacolata, additional, Doroshenko, Victor, additional, Ehlert, Steven R., additional, Enoto, Teruaki, additional, Evangelista, Yuri, additional, Ferrazzoli, Riccardo, additional, Garcia, Javier A., additional, Gunji, Shuichi, additional, Hayashida, Kiyoshi, additional, Heyl, Jeremy, additional, Iwakiri, Wataru, additional, Jorstad, Svetlana G., additional, Karas, Vladimir, additional, Kislat, Fabian, additional, Kitaguchi, Takao, additional, Kolodziejczak, Jeffery J., additional, Krawczynski, Henric, additional, Latronico, Luca, additional, Liodakis, Ioannis, additional, Maldera, Simone, additional, Manfreda, Alberto, additional, Marin, Frédéric, additional, Marinucci, Andrea, additional, Marscher, Alan P., additional, Massaro, Francesco, additional, Mitsuishi, Ikuyuki, additional, Mizuno, Tsunefumi, additional, Negro, Michela, additional, Ng, Chi-Yung, additional, Omodei, Nicola, additional, Oppedisano, Chiara, additional, Pavlov, George G., additional, Peirson, Abel L., additional, Perri, Matteo, additional, Pesce-Rollins, Melissa, additional, Petrucci, Pierre-Olivier, additional, Possenti, Andrea, additional, Puccetti, Simonetta, additional, Ramsey, Brian D., additional, Ratheesh, Ajay, additional, Roberts, Oliver J., additional, Romani, Roger W., additional, Sgrò, Carmelo, additional, Slane, Patrick, additional, Spandre, Gloria, additional, Swartz, Douglas A., additional, Tamagawa, Toru, additional, Tavecchio, Fabrizio, additional, Taverna, Roberto, additional, Tawara, Yuzuru, additional, Tennant, Allyn F., additional, Thomas, Nicholas E., additional, Tombesi, Francesco, additional, Trois, Alessio, additional, Tsygankov, Sergey S., additional, Turolla, Roberto, additional, Vink, Jacco, additional, and Wu, Kinwah, additional
Published: 2023
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15. Time-dependent visibility modelling of a relativistic jet in the X-ray binary MAXI J1803-298

Author: Forrest Research Foundation, Agenzia Spaziale Italiana, Istituto Nazionale di Astrofisica, National Aeronautics and Space Administration (US), National Natural Science Foundation of China, Wood, Callan M., Miller-Jones, J. C. A., Bahramian, Arash, Tingay, S. J., Russell, T. D., Tetarenko, A. J., Altamirano, Diego, Belloni, T., Carotenuto, Francesco, Ceccobello, Chiara, Corbel, S., Espinasse, Mathilde, Fender, R., Körding, E., Migliari, S., Russell, David M., Sarazin, C. L., Sivakoff, Gregory R., Soria, Roberto, Tudose, V., Forrest Research Foundation, Agenzia Spaziale Italiana, Istituto Nazionale di Astrofisica, National Aeronautics and Space Administration (US), National Natural Science Foundation of China, Wood, Callan M., Miller-Jones, J. C. A., Bahramian, Arash, Tingay, S. J., Russell, T. D., Tetarenko, A. J., Altamirano, Diego, Belloni, T., Carotenuto, Francesco, Ceccobello, Chiara, Corbel, S., Espinasse, Mathilde, Fender, R., Körding, E., Migliari, S., Russell, David M., Sarazin, C. L., Sivakoff, Gregory R., Soria, Roberto, and Tudose, V.
Abstract: Tracking the motions of transient jets launched by low-mass X-ray binaries (LMXBs) is critical for determining the moment of jet ejection, and identifying any corresponding signatures in the accretion flow. However, these jets are often highly variable and can travel across the resolution element of an image within a single observation, violating a fundamental assumption of aperture synthesis. We present a novel approach in which we directly fit a single time-dependent model to the full set of interferometer visibilities, where we explicitly parametrize the motion and flux density variability of the emission components, to minimize the number of free parameters in the fit, while leveraging information from the full observation. This technique allows us to detect and characterize faint, fast-moving sources, for which the standard time binning technique is inadequate. We validate our technique with synthetic observations, before applying it to three Very Long Baseline Array (VLBA) observations of the black hole candidate LMXB MAXI J1803−298 during its 2021 outburst. We measured the proper motion of a discrete jet component to be 1.37 ± 0.14 mas h−1, and thus we infer an ejection date of MJD 59348.08+0.05 −0.06, which occurs just after the peak of a radio flare observed by the Australia Telescope Compact Array (ATCA) and the Atacama Large Millimeter/Sub-Millimeter Array (ALMA), while MAXI J1803−298 was in the intermediate state. Further development of these new VLBI analysis techniques will lead to more precise measurements of jet ejection dates, which, combined with dense, simultaneous multiwavelength monitoring, will allow for clearer identification of jet ejection signatures in the accretion flow.
Published: 2023

16. The accretion/ejection link in the neutron star X-ray binary 4U 1820-30 I: a boundary layer-jet coupling?

Author: European Commission, European Research Council, Royal Society (UK), Department of Science and Technology (India), Istituto Nazionale di Fisica Nucleare, Agenzia Spaziale Italiana, National Aeronautics and Space Administration (US), Agencia Estatal de Investigación (España), Ministerio de Ciencia, Innovación y Universidades (España), Ministerio de Ciencia e Innovación (España), Marino, Alessio, Russell, T. D., Santo, Melania del, Beri, Aru, Sanna, Andrea, Coti Zelati, Francesco, Degenaar, Nathalie, Altamirano, Diego, Ambrosi, Elena, Anitra, A., Carotenuto, Francesco, D'Aí, Antonino, Salvo, Tiziana di, Manca, Arianna, Motta, S. E., Pinto, Ciro, Pintore, Fabio, Rea, Nanda, Eijnden, Jakob van den, European Commission, European Research Council, Royal Society (UK), Department of Science and Technology (India), Istituto Nazionale di Fisica Nucleare, Agenzia Spaziale Italiana, National Aeronautics and Space Administration (US), Agencia Estatal de Investigación (España), Ministerio de Ciencia, Innovación y Universidades (España), Ministerio de Ciencia e Innovación (España), Marino, Alessio, Russell, T. D., Santo, Melania del, Beri, Aru, Sanna, Andrea, Coti Zelati, Francesco, Degenaar, Nathalie, Altamirano, Diego, Ambrosi, Elena, Anitra, A., Carotenuto, Francesco, D'Aí, Antonino, Salvo, Tiziana di, Manca, Arianna, Motta, S. E., Pinto, Ciro, Pintore, Fabio, Rea, Nanda, and Eijnden, Jakob van den
Abstract: The accretion flow/jet correlation in neutron star (NS) low-mass X-ray binaries (LMXBs) is far less understood when compared to black hole (BH) LMXBs. In this paper we will present the results of a dense multiwavelength observational campaign on the NS LMXB 4U 1820-30, including X-ray (NICER, NuSTAR, and AstroSat) and quasi-simultaneous radio (ATCA) observations in 2022. 4U 1820-30 shows a peculiar 170 d super-orbital accretion modulation, during which the system evolves between ‘modes’ of high and low X-ray flux. During our monitoring, the source did not show any transition to a full hard state. X-ray spectra were well described using a disc blackbody, a Comptonization spectrum along with a Fe K emission line at ∼6.6 keV. Our results show that the observed X-ray flux modulation is almost entirely produced by changes in the size of the region providing seed photons for the Comptonization spectrum. This region is large (∼15 km) in the high mode and likely coincides with the whole boundary layer, while it shrinks significantly (≲10 km) in low mode. The electron temperature of the corona and the observed rms variability in the hard X-rays also exhibit a slight increase in low mode. As the source moves from high to low mode, the radio emission due to the jet becomes ∼5 fainter. These radio changes appear not to be strongly connected to the hard-to-soft transitions as in BH systems, while they seem to be connected mostly to variations observed in the boundary layer.
Published: 2023

17. Phylogenetic fields through time: temporal dynamics of geographical co-occurrence and phylogenetic structure within species ranges

Author: Villalobos, Fabricio, Carotenuto, Francesco, Raia, Pasquale, and Diniz-Filho, José Alexandre F.
Published: 2016

18. Chewing on the trees: Constraints and adaptation in the evolution of the primate mandible

Author: Meloro, Carlo, Cáceres, Nilton Carlos, Carotenuto, Francesco, Sponchiado, Jonas, Melo, Geruza Leal, Passaro, Federico, and Raia, Pasquale
Published: 2015

19. Zoogeographic significance of Dmanisi large mammal assemblage

Author: Bartolini-Lucenti, Saverio, primary, Cirilli, Omar, additional, Pandolfi, Luca, additional, Bernor, Raymond Louis, additional, Bukhsianidze, Maia, additional, Carotenuto, Francesco, additional, Lordkipanidze, David, additional, Tsikaridze, Nikoloz, additional, and Rook, Lorenzo, additional
Published: 2022
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20. Osservazioni sui meccanismi di locomozione dell’autore della Pista A delle 'Ciampate del diavolo'

Author: Mondanaro, Alessandro, Panarello, Adolfo, Modafferi, Maria, Melchionna, Marina, Serio, Carmela, Carotenuto, Francesco, Tavani, Stefano, Mietto, Paolo, and Raia, Pasquale
Subjects: Gait biomechanics, Stima della statura, Body mass estimate, Stima della massa corporea, Icnologia umana, Stature estimate, Human ichnology, Biomeccanica dell'andatura, Dynamic model, Modello dinamico
Published: 2022

21. One size does not fit all: no evidence for an optimal body size on islands

Author: Raia, Pasquale, Carotenuto, Francesco, and Meiri, Shai
Published: 2010
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22. Occupancy, range size, and phylogeny in Eurasian Pliocene to Recent large mammals

Author: Carotenuto, Francesco, Barbera, Carmela, and Raia, Pasquale
Published: 2010

23. THE SHAPE OF CONTENTION: ADAPTATION, HISTORY, AND CONTINGENCY IN UNGULATE MANDIBLES

Author: Raia, Pasquale, Carotenuto, Francesco, Meloro, Carlo, Piras, Paolo, and Pushkina, Diana
Published: 2010

24. Early Detection of Wild Rocket Tracheofusariosis Using Hyperspectral Image-Based Machine Learning

Author: Pane, Catello, primary, Manganiello, Gelsomina, additional, Nicastro, Nicola, additional, and Carotenuto, Francesco, additional
Published: 2021
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25. A 450 million years long latitudinal gradient in age-dependent extinction

Author: Silvestro, Daniele, Castiglione, Silvia, Mondanaro, Alessandro, Serio, Carmela, Melchionna, Marina, Piras, Paolo, Di Febbraro, Mirko, Carotenuto, Francesco, Rook Lorenzo, Raia Pasquale, Silvestro, Daniele, Castiglione, Silvia, Mondanaro, Alessandro, Serio, Carmela, Melchionna, Marina, Piras, Paolo, Di Febbraro, Mirko, Carotenuto, Francesco, Rook, Lorenzo, and Raia, Pasquale
Subjects: 'law of constant extinction', Letter, GE, Fossils, deep learning, fossil occurrences, mass extinction, neural networks, Animals, Biological Evolution, Invertebrates, Biodiversity, Extinction, Biological, social sciences, Extinction, musculoskeletal system, Biological, humanities, natural sciences, Letters, geographic locations
Abstract: Leigh Van Valen famously stated that under constant conditions extinction probability is independent of species age. To test this 'law of constant extinction', we developed a new method using deep learning to infer age‐dependent extinction and analysed 450 myr of marine life across 21 invertebrate clades. We show that extinction rate significantly decreases with age in > 90% of the cases, indicating that most species died out soon after their appearance while those which survived experienced ever decreasing extinction risk. This age‐dependent extinction pattern is stronger towards the Equator and holds true when the potential effects of mass extinctions and taxonomic inflation are accounted for. These results suggest that the effect of biological interactions on age‐dependent extinction rate is more intense towards the tropics. We propose that the latitudinal diversity gradient and selection at the species level account for this exceptional, yet little recognised, macroevolutionary and macroecological pattern., We developed a new method using deep learning to infer age‐dependent extinction and analyzed 450 myr of marine life across 21 invertebrate clades. We found that extinction rate significantly decreases with age in > 90% of the cases. We propose that the latitudinal diversity gradient and selection at the species level account for this exceptional, yet little recognized, macroevolutionary and macroecological pattern.
Published: 2020

26. Powdery Mildew Caused by Erysiphe cruciferarum on Wild Rocket (Diplotaxis tenuifolia): Hyperspectral Imaging and Machine Learning Modeling for Non-Destructive Disease Detection

Author: Pane, Catello, primary, Manganiello, Gelsomina, additional, Nicastro, Nicola, additional, Cardi, Teodoro, additional, and Carotenuto, Francesco, additional
Published: 2021
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27. Insights into Mechanical Properties of the 1980 Irpinia Fault System from the Analysis of a Seismic Sequence

Author: Festa, Gaetano, primary, Adinolfi, Guido Maria, additional, Caruso, Alessandro, additional, Colombelli, Simona, additional, De Landro, Grazia, additional, Elia, Luca, additional, Emolo, Antonio, additional, Picozzi, Matteo, additional, Scala, Antonio, additional, Carotenuto, Francesco, additional, Gammaldi, Sergio, additional, Iaccarino, Antonio Giovanni, additional, Nazeri, Sahar, additional, Riccio, Rosario, additional, Russo, Guido, additional, Tarantino, Stefania, additional, and Zollo, Aldo, additional
Published: 2021
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28. Past Extinctions of Homo Species Coincided with Increased Vulnerability to Climatic Change

Author: Raia, Pasquale, primary, Mondanaro, Alessandro, additional, Melchionna, Marina, additional, Di Febbraro, Mirko, additional, Diniz-Filho, Josè A.F., additional, Rangel, Thiago F., additional, Holden, Philip B., additional, Carotenuto, Francesco, additional, Edwards, Neil R., additional, Lima-Ribeiro, Matheus S., additional, Profico, Antonio, additional, Maiorano, Luigi, additional, Castiglione, Silvia, additional, Serio, Carmela, additional, and Rook, Lorenzo, additional
Published: 2020
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29. MInOSSE: A new method to reconstruct geographic ranges of fossil species

Author: Carotenuto, Francesco, primary, Di Febbraro, Mirko, additional, Mondanaro, Alessandro, additional, Castiglione, Silvia, additional, Serio, Carmela, additional, Melchionna, Marina, additional, Rook, Lorenzo, additional, and Raia, Pasquale, additional
Published: 2020
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30. Design and implementation of a mobile device app for network-based earthquake early warning systems (EEWSs): application to the PRESTo EEWS in southern Italy

Author: Colombelli, Simona, primary, Carotenuto, Francesco, additional, Elia, Luca, additional, and Zollo, Aldo, additional
Published: 2020
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31. A 450 million years long latitudinal gradient in age‐dependent extinction

Author: Silvestro, Daniele, primary, Castiglione, Silvia, additional, Mondanaro, Alessandro, additional, Serio, Carmela, additional, Melchionna, Marina, additional, Piras, Paolo, additional, Di Febbraro, Mirko, additional, Carotenuto, Francesco, additional, Rook, Lorenzo, additional, and Raia, Pasquale, additional
Published: 2019
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32. Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo

Author: Abbott, B. P., primary, Abbott, R., additional, Abbott, T. D., additional, Abraham, S., additional, Acernese, F., additional, Ackley, K., additional, Adams, C., additional, Adhikari, R. X., additional, Adya, V. B., additional, Affeldt, C., additional, Agathos, M., additional, Agatsuma, K., additional, Aggarwal, N., additional, Aguiar, O. D., additional, Aiello, L., additional, Ain, A., additional, Ajith, P., additional, Allen, G., additional, Allocca, A., additional, Aloy, M. A., additional, Altin, P. A., additional, Amato, A., additional, Anand, S., additional, Ananyeva, A., additional, Anderson, S. B., additional, Anderson, W. G., additional, Angelova, S. V., additional, Antier, S., additional, Appert, S., additional, Arai, K., additional, Araya, M. C., additional, Areeda, J. S., additional, Arène, M., additional, Arnaud, N., additional, Aronson, S. M., additional, Ascenzi, S., additional, Ashton, G., additional, Aston, S. M., additional, Astone, P., additional, Aubin, F., additional, Aufmuth, P., additional, AultONeal, K., additional, Austin, C., additional, Avendano, V., additional, Avila-Alvarez, A., additional, Babak, S., additional, Bacon, P., additional, Badaracco, F., additional, Bader, M. K. M., additional, Bae, S., additional, Baird, J., additional, Baker, P. T., additional, Baldaccini, F., additional, Ballardin, G., additional, Ballmer, S. W., additional, Bals, A., additional, Banagiri, S., additional, Barayoga, J. C., additional, Barbieri, C., additional, Barclay, S. E., additional, Barish, B. C., additional, Barker, D., additional, Barkett, K., additional, Barnum, S., additional, Barone, F., additional, Barr, B., additional, Barsotti, L., additional, Barsuglia, M., additional, Barta, D., additional, Bartlett, J., additional, Bartos, I., additional, Bassiri, R., additional, Basti, A., additional, Bawaj, M., additional, Bayley, J. C., additional, Bazzan, M., additional, Bécsy, B., additional, Bejger, M., additional, Belahcene, I., additional, Bell, A. S., additional, Beniwal, D., additional, Benjamin, M. G., additional, Berger, B. K., additional, Bergmann, G., additional, Bernuzzi, S., additional, Berry, C. P. L., additional, Bersanetti, D., additional, Bertolini, A., additional, Betzwieser, J., additional, Bhandare, R., additional, Bidler, J., additional, Biggs, E., additional, Bilenko, I. A., additional, Bilgili, S. A., additional, Billingsley, G., additional, Birney, R., additional, Birnholtz, O., additional, Biscans, S., additional, Bischi, M., additional, Biscoveanu, S., additional, Bisht, A., additional, Bitossi, M., additional, Bizouard, M. A., additional, Blackburn, J. K., additional, Blackman, J., additional, Blair, C. D., additional, Blair, D. G., additional, Blair, R. M., additional, Bloemen, S., additional, Bobba, F., additional, Bode, N., additional, Boer, M., additional, Boetzel, Y., additional, Bogaert, G., additional, Bondu, F., additional, Bonnand, R., additional, Booker, P., additional, Boom, B. A., additional, Bork, R., additional, Boschi, V., additional, Bose, S., additional, Bossilkov, V., additional, Bosveld, J., additional, Bouffanais, Y., additional, Bozzi, A., additional, Bradaschia, C., additional, Brady, P. R., additional, Bramley, A., additional, Branchesi, M., additional, Brau, J. E., additional, Breschi, M., additional, Briant, T., additional, Briggs, J. H., additional, Brighenti, F., additional, Brillet, A., additional, Brinkmann, M., additional, Brockill, P., additional, Brooks, A. F., additional, Brooks, J., additional, Brown, D. D., additional, Brunett, S., additional, Buikema, A., additional, Bulik, T., additional, Bulten, H. J., additional, Buonanno, A., additional, Buskulic, D., additional, Buy, C., additional, Byer, R. L., additional, Cabero, M., additional, Cadonati, L., additional, Cagnoli, G., additional, Cahillane, C., additional, Bustillo, J. Calderón, additional, Callister, T. A., additional, Calloni, E., additional, Camp, J. B., additional, Campbell, W. A., additional, Canepa, M., additional, Cannon, K. C., additional, Cao, H., additional, Cao, J., additional, Carapella, G., additional, Carbognani, F., additional, Caride, S., additional, Carney, M. F., additional, Carullo, G., additional, Diaz, J. Casanueva, additional, Casentini, C., additional, Caudill, S., additional, Cavaglià, M., additional, Cavalier, F., additional, Cavalieri, R., additional, Cella, G., additional, Cerdá-Durán, P., additional, Cesarini, E., additional, Chaibi, O., additional, Chakravarti, K., additional, Chamberlin, S. J., additional, Chan, M., additional, Chao, S., additional, Charlton, P., additional, Chase, E. A., additional, Chassande-Mottin, E., additional, Chatterjee, D., additional, Chaturvedi, M., additional, Cheeseboro, B. D., additional, Chen, H. Y., additional, Chen, X., additional, Chen, Y., additional, Cheng, H.-P., additional, Cheong, C. K., additional, Chia, H. Y., additional, Chiadini, F., additional, Chincarini, A., additional, Chiummo, A., additional, Cho, G., additional, Cho, H. S., additional, Cho, M., additional, Christensen, N., additional, Chu, Q., additional, Chua, S., additional, Chung, K. W., additional, Chung, S., additional, Ciani, G., additional, Cieślar, M., additional, Ciobanu, A. A., additional, Ciolfi, R., additional, Cipriano, F., additional, Cirone, A., additional, Clara, F., additional, Clark, J. A., additional, Clearwater, P., additional, Cleva, F., additional, Coccia, E., additional, Cohadon, P.-F., additional, Cohen, D., additional, Colleoni, M., additional, Collette, C. G., additional, Collins, C., additional, Colpi, M., additional, Cominsky, L. R., additional, Constancio, M., additional, Conti, L., additional, Cooper, S. J., additional, Corban, P., additional, Corbitt, T. R., additional, Cordero-Carrión, I., additional, Corezzi, S., additional, Corley, K. R., additional, Cornish, N., additional, Corre, D., additional, Corsi, A., additional, Cortese, S., additional, Costa, C. A., additional, Cotesta, R., additional, Coughlin, M. W., additional, Coughlin, S. B., additional, Coulon, J.-P., additional, Countryman, S. T., additional, Couvares, P., additional, Covas, P. B., additional, Cowan, E. E., additional, Coward, D. M., additional, Cowart, M. J., additional, Coyne, D. C., additional, Coyne, R., additional, Creighton, J. D. E., additional, Creighton, T. D., additional, Cripe, J., additional, Croquette, M., additional, Crowder, S. G., additional, Cullen, T. J., additional, Cumming, A., additional, Cunningham, L., additional, Cuoco, E., additional, Canton, T. Dal, additional, Dálya, G., additional, D’Angelo, B., additional, Danilishin, S. L., additional, D’Antonio, S., additional, Danzmann, K., additional, Dasgupta, A., additional, Costa, C. F. Da Silva, additional, Datrier, L. E. H., additional, Dattilo, V., additional, Dave, I., additional, Davier, M., additional, Davis, D., additional, Daw, E. J., additional, DeBra, D., additional, Deenadayalan, M., additional, Degallaix, J., additional, Laurentis, M. De, additional, Deléglise, S., additional, Pozzo, W. Del, additional, DeMarchi, L. M., additional, Demos, N., additional, Dent, T., additional, Pietri, R. De, additional, Rosa, R. De, additional, Rossi, C. De, additional, DeSalvo, R., additional, Varona, O. de, additional, Dhurandhar, S., additional, Díaz, M. C., additional, Dietrich, T., additional, Fiore, L. Di, additional, DiFronzo, C., additional, Giorgio, C. Di, additional, Giovanni, F. Di, additional, Giovanni, M. Di, additional, Girolamo, T. Di, additional, Lieto, A. Di, additional, Ding, B., additional, Pace, S. Di, additional, Palma, I. Di, additional, Renzo, F. Di, additional, Divakarla, A. K., additional, Dmitriev, A., additional, Doctor, Z., additional, Donovan, F., additional, Dooley, K. L., additional, Doravari, S., additional, Dorrington, I., additional, Downes, T. P., additional, Drago, M., additional, Driggers, J. C., additional, Du, Z., additional, Ducoin, J.-G., additional, Dupej, P., additional, Durante, O., additional, Dwyer, S. E., additional, Easter, P. J., additional, Eddolls, G., additional, Edo, T. B., additional, Effler, A., additional, Ehrens, P., additional, Eichholz, J., additional, Eikenberry, S. S., additional, Eisenmann, M., additional, Eisenstein, R. A., additional, Errico, L., additional, Essick, R. C., additional, Estelles, H., additional, Estevez, D., additional, Etienne, Z. B., additional, Etzel, T., additional, Evans, M., additional, Evans, T. M., additional, Fafone, V., additional, Fairhurst, S., additional, Fan, X., additional, Farinon, S., additional, Farr, B., additional, Farr, W. M., additional, Fauchon-Jones, E. J., additional, Favata, M., additional, Fays, M., additional, Fazio, M., additional, Fee, C., additional, Feicht, J., additional, Fejer, M. M., additional, Feng, F., additional, Fernandez-Galiana, A., additional, Ferrante, I., additional, Ferreira, E. C., additional, Ferreira, T. A., additional, Fidecaro, F., additional, Fiori, I., additional, Fiorucci, D., additional, Fishbach, M., additional, Fisher, R. P., additional, Fishner, J. M., additional, Fittipaldi, R., additional, Fitz-Axen, M., additional, Fiumara, V., additional, Flaminio, R., additional, Fletcher, M., additional, Floden, E., additional, Flynn, E., additional, Fong, H., additional, Font, J. A., additional, Forsyth, P. W. F., additional, Fournier, J.-D., additional, Vivanco, Francisco Hernandez, additional, Frasca, S., additional, Frasconi, F., additional, Frei, Z., additional, Freise, A., additional, Frey, R., additional, Frey, V., additional, Fritschel, P., additional, Frolov, V. V., additional, Fronzè, G., additional, Fulda, P., additional, Fyffe, M., additional, Gabbard, H. A., additional, Gadre, B. U., additional, Gaebel, S. M., additional, Gair, J. R., additional, Gammaitoni, L., additional, Gaonkar, S. G., additional, García-Quirós, C., additional, Garufi, F., additional, Gateley, B., additional, Gaudio, S., additional, Gaur, G., additional, Gayathri, V., additional, Gemme, G., additional, Genin, E., additional, Gennai, A., additional, George, D., additional, George, J., additional, Gergely, L., additional, Ghonge, S., additional, Ghosh, Abhirup, additional, Ghosh, Archisman, additional, Ghosh, S., additional, Giacomazzo, B., additional, Giaime, J. A., additional, Giardina, K. 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J., additional, McCarthy, R., additional, McClelland, D. E., additional, McCormick, S., additional, McCuller, L., additional, McGuire, S. C., additional, McIsaac, C., additional, McIver, J., additional, McManus, D. J., additional, McRae, T., additional, McWilliams, S. T., additional, Meacher, D., additional, Meadors, G. D., additional, Mehmet, M., additional, Mehta, A. K., additional, Meidam, J., additional, Villa, E. Mejuto, additional, Melatos, A., additional, Mendell, G., additional, Mercer, R. A., additional, Mereni, L., additional, Merfeld, K., additional, Merilh, E. L., additional, Merzougui, M., additional, Meshkov, S., additional, Messenger, C., additional, Messick, C., additional, Messina, F., additional, Metzdorff, R., additional, Meyers, P. M., additional, Meylahn, F., additional, Miani, A., additional, Miao, H., additional, Michel, C., additional, Middleton, H., additional, Milano, L., additional, Miller, A. L., additional, Millhouse, M., additional, Mills, J. C., additional, Milovich-Goff, M. C., additional, Minazzoli, O., additional, Minenkov, Y., additional, Mishkin, A., additional, Mishra, C., additional, Mistry, T., additional, Mitra, S., additional, Mitrofanov, V. P., additional, Mitselmakher, G., additional, Mittleman, R., additional, Mo, G., additional, Moffa, D., additional, Mogushi, K., additional, Mohapatra, S. R. P., additional, Molina-Ruiz, M., additional, Mondin, M., additional, Montani, M., additional, Moore, C. J., additional, Moraru, D., additional, Morawski, F., additional, Moreno, G., additional, Morisaki, S., additional, Mours, B., additional, Mow-Lowry, C. M., additional, Muciaccia, F., additional, Mukherjee, Arunava, additional, Mukherjee, D., additional, Mukherjee, S., additional, Mukherjee, Subroto, additional, Mukund, N., additional, Mullavey, A., additional, Munch, J., additional, Muñiz, E. A., additional, Muratore, M., additional, Murray, P. G., additional, Nardecchia, I., additional, Naticchioni, L., additional, Nayak, R. K., additional, Neil, B. F., additional, Neilson, J., additional, Nelemans, G., additional, Nelson, T. J. N., additional, Nery, M., additional, Neunzert, A., additional, Nevin, L., additional, Ng, K. Y., additional, Ng, S., additional, Nguyen, C., additional, Nguyen, P., additional, Nichols, D., additional, Nichols, S. A., additional, Nissanke, S., additional, Nocera, F., additional, North, C., additional, Nuttall, L. K., additional, Obergaulinger, M., additional, Oberling, J., additional, O’Brien, B. D., additional, Oganesyan, G., additional, Ogin, G. H., additional, Oh, J. J., additional, Oh, S. H., additional, Ohme, F., additional, Ohta, H., additional, Okada, M. A., additional, Oliver, M., additional, Oppermann, P., additional, Oram, Richard J., additional, O’Reilly, B., additional, Ormiston, R. G., additional, Ortega, L. F., additional, O’Shaughnessy, R., additional, Ossokine, S., additional, Ottaway, D. J., additional, Overmier, H., additional, Owen, B. J., additional, Pace, A. E., additional, Pagano, G., additional, Page, M. A., additional, Pagliaroli, G., additional, Pai, A., additional, Pai, S. A., additional, Palamos, J. R., additional, Palashov, O., additional, Palomba, C., additional, Pan, H., additional, Panda, P. K., additional, Pang, P. T. H., additional, Pankow, C., additional, Pannarale, F., additional, Pant, B. C., additional, Paoletti, F., additional, Paoli, A., additional, Parida, A., additional, Parker, W., additional, Pascucci, D., additional, Pasqualetti, A., additional, Passaquieti, R., additional, Passuello, D., additional, Patil, M., additional, Patricelli, B., additional, Payne, E., additional, Pearlstone, B. L., additional, Pechsiri, T. C., additional, Pedersen, A. 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M., additional, Shukla, K., additional, ShyamSundar, S., additional, Siellez, K., additional, Sieniawska, M., additional, Sigg, D., additional, Singer, L. P., additional, Singh, D., additional, Singh, N., additional, Singhal, A., additional, Sintes, A. M., additional, Sitmukhambetov, S., additional, Skliris, V., additional, Slagmolen, B. J. J., additional, Slaven-Blair, T. J., additional, Smith, J. R., additional, Smith, R. J. E., additional, Somala, S., additional, Son, E. J., additional, Soni, S., additional, Sorazu, B., additional, Sorrentino, F., additional, Souradeep, T., additional, Sowell, E., additional, Spencer, A. P., additional, Spera, M., additional, Srivastava, A. K., additional, Srivastava, V., additional, Staats, K., additional, Stachie, C., additional, Standke, M., additional, Steer, D. A., additional, Steinke, M., additional, Steinlechner, J., additional, Steinlechner, S., additional, Steinmeyer, D., additional, Stevenson, S. 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Published: 2019
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33. Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo

Author: Abbott, B, Abbott, R, Abbott, T, Abraham, S, Acernese, F, Ackley, K, Adams, C, Adhikari, R, Adya, V, Affeldt, C, Agathos, M, Agatsuma, K, Aggarwal, N, Aguiar, O, Aiello, L, Ain, A, Ajith, P, Allen, G, Allocca, A, Aloy, M, Altin, P, Amato, A, Anand, S, Ananyeva, A, Anderson, S, Anderson, W, Angelova, S, Antier, S, Appert, S, Arai, K, Araya, M, Areeda, J, Arène, M, Arnaud, N, Aronson, S, Ascenzi, S, Ashton, G, Aston, S, Astone, P, Aubin, F, Aufmuth, P, Aultoneal, K, Austin, C, Avendano, V, Avila-Alvarez, A, Babak, S, Bacon, P, Badaracco, F, Bader, M, Bae, S, Baird, J, Baker, P, Baldaccini, F, Ballardin, G, Ballmer, S, Bals, A, Banagiri, S, Barayoga, J, Barbieri, C, Barclay, S, Barish, B, Barker, D, Barkett, K, Barnum, S, Barone, F, Barr, B, Barsotti, L, Barsuglia, M, Barta, D, Bartlett, J, Bartos, I, Bassiri, R, Basti, A, Bawaj, M, Bayley, J, Bazzan, M, Bécsy, B, Bejger, M, Belahcene, I, Bell, A, Beniwal, D, Benjamin, M, Berger, B, Bergmann, G, Bernuzzi, S, Berry, C, Bersanetti, D, Bertolini, A, Betzwieser, J, Bhandare, R, Bidler, J, Biggs, E, Bilenko, I, Bilgili, S, Billingsley, G, Birney, R, Birnholtz, O, Biscans, S, Bischi, M, Biscoveanu, S, Bisht, A, Bitossi, M, Bizouard, M, Blackburn, J, Blackman, J, Blair, C, Blair, D, Blair, R, Bloemen, S, Bobba, F, Bode, N, Boer, M, Boetzel, Y, Bogaert, G, Bondu, F, Bonnand, R, Booker, P, Boom, B, Bork, R, Boschi, V, Bose, S, Bossilkov, V, Bosveld, J, Bouffanais, Y, Bozzi, A, Bradaschia, C, Brady, P, Bramley, A, Branchesi, M, Brau, J, Breschi, M, Briant, T, Briggs, J, Brighenti, F, Brillet, A, Brinkmann, M, Brockill, P, Brooks, A, Brooks, J, Brown, D, Brunett, S, 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, Campbell, W, Canepa, M, Cannon, K, Cao, H, Cao, J, Carapella, G, Carbognani, F, Caride, S, Carney, M, Carullo, G, Diaz, J, Casentini, C, Caudill, S, Cavaglià, M, Cavalier, F, Cavalieri, R, Cella, G, Cerdá-Durán, P, Cesarini, E, Chaibi, O, Chakravarti, K, Chamberlin, S, Chan, M, Chao, S, Charlton, P, Chase, E, Chassande-Mottin, E, Chatterjee, D, Chaturvedi, M, Cheeseboro, B, Chen, H, Chen, X, Chen, Y, Cheng, H, Cheong, C, Chia, H, Chiadini, F, Chincarini, A, Chiummo, A, Cho, G, Cho, H, Cho, M, Christensen, N, Chu, Q, Chua, S, Chung, K, Chung, S, Ciani, G, Cieślar, M, Ciobanu, A, Ciolfi, R, Cipriano, F, Cirone, A, Clara, F, Clark, J, Clearwater, P, Cleva, F, Coccia, E, Cohadon, P, Cohen, D, Colleoni, M, Collette, C, Collins, C, Colpi, M, Cominsky, L, Constancio, M, Conti, L, Cooper, S, Corban, P, Corbitt, T, Cordero-Carrión, I, Corezzi, S, Corley, K, Cornish, N, Corre, D, Corsi, A, Cortese, S, Costa, C, Cotesta, R, 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, Croquette, M, Crowder, S, Cullen, T, Cumming, A, Cunningham, L, Cuoco, E, Canton, T, Dálya, G, D’Angelo, B, Danilishin, S, D’Antonio, S, Danzmann, K, Dasgupta, A, Datrier, L, Dattilo, V, Dave, I, Davier, M, Davis, D, Daw, E, Debra, D, Deenadayalan, M, Degallaix, J, Laurentis, M, Deléglise, S, Pozzo, W, Demarchi, L, Demos, N, Dent, T, Pietri, R, Rosa, R, Rossi, C, Desalvo, R, Varona, O, Dhurandhar, S, Díaz, M, Dietrich, T, Fiore, L, Difronzo, C, Giorgio, C, Giovanni, F, Giovanni, M, Girolamo, T, Lieto, A, Ding, B, Pace, S, Palma, I, Renzo, F, Divakarla, A, Dmitriev, A, Doctor, Z, Donovan, F, Dooley, K, Doravari, S, Dorrington, I, Downes, T, Drago, M, Driggers, J, Du, Z, Ducoin, J, Dupej, P, Durante, O, Dwyer, S, Easter, P, Eddolls, G, Edo, T, Effler, A, Ehrens, P, Eichholz, J, Eikenberry, S, Eisenmann, M, Eisenstein, R, Errico, L, Essick, R, Estelles, H, Estevez, D, Etienne, Z, Etzel, T, Evans, M, Evans, T, Fafone, V, Fairhurst, S, Fan, X, Farinon, S, Farr, B, Farr, W, Fauchon-Jones, E, Favata, M, Fays, M, Fazio, M, Fee, C, Feicht, J, Fejer, M, Feng, F, Fernandez-Galiana, A, Ferrante, I, Ferreira, E, Ferreira, T, Fidecaro, F, Fiori, I, Fiorucci, D, Fishbach, M, Fisher, R, Fishner, J, Fittipaldi, R, Fitz-Axen, M, Fiumara, V, Flaminio, R, Fletcher, M, Floden, E, Flynn, E, Fong, H, Font, J, Forsyth, P, Fournier, J, Vivanco, F, Frasca, S, Frasconi, F, Frei, Z, Freise, A, Frey, R, Frey, V, Fritschel, P, Frolov, V, Fronzè, G, Fulda, P, Fyffe, M, Gabbard, H, Gadre, B, Gaebel, S, Gair, J, Gammaitoni, L, Gaonkar, S, García-Quirós, C, Garufi, F, Gateley, B, Gaudio, S, Gaur, G, Gayathri, V, Gemme, G, Genin, E, Gennai, A, George, D, George, J, Gergely, L, Ghonge, S, Ghosh, A, Ghosh, S, Giacomazzo, B, Giaime, J, Giardina, K, Gibson, D, Gill, K, Glover, L, Gniesmer, J, Godwin, P, Goetz, E, Goetz, R, Goncharov, B, González, G, Castro, J, Gopakumar, A, Gossan, S, Gosselin, M, Gouaty, R, Grace, B, Grado, A, Granata, M, Grant, A, Gras, S, Grassia, P, Gray, C, Gray, R, Greco, G, Green, A, Green, R, Gretarsson, E, Grimaldi, A, Grimm, S, Groot, P, Grote, H, Grunewald, S, Gruning, P, Guidi, G, Gulati, H, Guo, Y, Gupta, A, Gupta, P, Gustafson, E, Gustafson, R, Haegel, L, Halim, O, Hall, B, Hall, E, Hamilton, E, Hammond, G, Haney, M, Hanke, M, Hanks, J, Hanna, C, Hannam, M, Hannuksela, O, Hansen, T, Hanson, J, Harder, T, Hardwick, T, Haris, K, Harms, J, Harry, G, Harry, I, Hasskew, R, Haster, C, Haughian, K, Hayes, F, Healy, J, Heidmann, A, Heintze, M, Heitmann, H, Hellman, F, Hello, P, Hemming, G, Hendry, M, Heng, I, Hennig, J, Heurs, M, Hild, S, Hinderer, T, Hochheim, S, Hofman, D, Holgado, A, Holland, N, Holt, K, Holz, D, Hopkins, P, Horst, C, Hough, J, Howell, E, Hoy, C, Huang, Y, Hübner, M, Huerta, E, Huet, D, Hughey, B, Hui, V, Husa, S, Huttner, S, Huynh-Dinh, T, Idzkowski, B, Iess, A, Inchauspe, H, Ingram, C, Inta, R, Intini, G, Irwin, B, Isa, H, Isac, J, Isi, M, Iyer, B, Jacqmin, T, Jadhav, S, Jani, K, Janthalur, N, Jaranowski, P, Jariwala, D, Jenkins, A, Jiang, J, Johnson, D, Jones, A, Jones, D, Jones, J, Jones, R, Jonker, R, Ju, L, Junker, J, Kalaghatgi, C, Kalogera, V, Kamai, B, Kandhasamy, S, Kang, G, Kanner, J, Kapadia, S, Karki, S, Kashyap, R, Kasprzack, M, Katsanevas, S, Katsavounidis, E, Katzman, W, Kaufer, S, Kawabe, K, Keerthana, N, Kéfélian, F, Keitel, D, Kennedy, R, Key, J, Khalili, F, Khan, I, Khan, S, Khazanov, E, Khetan, N, Khursheed, M, Kijbunchoo, N, Kim, C, Kim, J, Kim, K, Kim, W, Kim, Y, Kimball, C, King, P, Kinley-Hanlon, M, Kirchhoff, R, Kissel, J, Kleybolte, L, Klika, J, Klimenko, S, Knowles, T, Koch, P, Koehlenbeck, S, Koekoek, G, Koley, S, Kondrashov, V, Kontos, A, Koper, N, Korobko, M, Korth, W, Kovalam, M, Kozak, D, Krämer, C, Kringel, V, Krishnendu, N, Królak, A, Krupinski, N, Kuehn, G, Kumar, A, Kumar, P, Kumar, R, Kuo, L, Kutynia, A, Kwang, S, Lackey, B, Laghi, D, Lai, K, Lam, T, Landry, M, Lane, B, Lang, R, Lange, J, Lantz, B, Lanza, R, Lartaux-Vollard, A, Lasky, P, Laxen, M, Lazzarini, A, Lazzaro, C, Leaci, P, Leavey, S, Lecoeuche, Y, Lee, C, Lee, H, Lee, J, Lee, K, Lehmann, J, Lenon, A, Leroy, N, Letendre, N, Levin, Y, Li, A, Li, J, Li, K, Li, T, Li, X, Lin, F, Linde, F, Linker, S, Littenberg, T, Liu, J, Liu, X, Llorens-Monteagudo, M, Lo, R, London, L, Longo, A, Lorenzini, M, Loriette, V, Lormand, M, Losurdo, G, Lough, J, Lousto, C, Lovelace, G, Lower, M, Lück, H, Lumaca, D, Lundgren, A, Lynch, R, Ma, Y, Macas, R, Macfoy, S, Macinnis, M, Macleod, D, Macquet, A, Hernandez, I, Magaña-Sandoval, F, Magee, R, Majorana, E, Maksimovic, I, Malik, A, Man, N, Mandic, V, Mangano, V, Mansell, G, Manske, M, Mantovani, M, Mapelli, M, Marchesoni, F, Marion, F, Márka, S, Márka, Z, Markakis, C, Markosyan, A, Markowitz, A, Maros, E, Marquina, A, Marsat, S, Martelli, F, Martin, I, Martin, R, Martinez, V, Martynov, D, Masalehdan, H, Mason, K, Massera, E, Masserot, A, Massinger, T, Masso-Reid, M, Mastrogiovanni, S, Matas, A, Matichard, F, Matone, L, Mavalvala, N, Mccann, J, Mccarthy, R, Mcclelland, D, Mccormick, S, Mcculler, L, Mcguire, S, Mcisaac, C, Mciver, J, Mcmanus, D, Mcrae, T, Mcwilliams, S, Meacher, D, Meadors, G, Mehmet, M, Mehta, A, Meidam, J, Villa, E, Melatos, A, Mendell, G, Mercer, R, Mereni, L, Merfeld, K, Merilh, E, Merzougui, M, Meshkov, S, Messenger, C, Messick, C, Messina, F, Metzdorff, R, Meyers, P, Meylahn, F, Miani, A, Miao, H, Michel, C, Middleton, H, Milano, L, Miller, A, Millhouse, M, Mills, J, Milovich-Goff, M, Minazzoli, O, Minenkov, Y, Mishkin, A, Mishra, C, Mistry, T, Mitra, S, Mitrofanov, V, Mitselmakher, G, Mittleman, R, Mo, G, Moffa, D, Mogushi, K, Mohapatra, S, Molina-Ruiz, M, Mondin, M, Montani, M, Moore, C, Moraru, D, Morawski, F, Moreno, G, Morisaki, S, Mours, B, Mow-Lowry, C, Muciaccia, F, Mukherjee, A, Mukherjee, D, Mukherjee, S, Mukund, N, Mullavey, A, Munch, J, Muñiz, E, Muratore, M, Murray, P, Nardecchia, I, Naticchioni, L, Nayak, R, Neil, B, Neilson, J, Nelemans, G, Nelson, T, Nery, M, Neunzert, A, Nevin, L, Ng, K, Ng, S, Nguyen, C, Nguyen, P, Nichols, D, Nichols, S, Nissanke, S, Nocera, F, North, C, Nuttall, L, Obergaulinger, M, Oberling, J, O’Brien, B, Oganesyan, G, Ogin, G, Oh, J, Oh, S, Ohme, F, Ohta, H, 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, Pagano, G, Page, M, Pagliaroli, G, Pai, A, Pai, S, Palamos, J, Palashov, O, Palomba, C, Pan, H, Panda, P, Pang, P, Pankow, C, Pannarale, F, Pant, B, Paoletti, F, Paoli, A, Parida, A, Parker, W, Pascucci, D, Pasqualetti, A, Passaquieti, R, Passuello, D, Patil, M, Patricelli, B, Payne, E, Pearlstone, B, Pechsiri, T, Pedersen, A, Pedraza, M, Pedurand, R, Pele, A, Penn, S, Perego, A, Perez, C, Périgois, C, Perreca, A, Petermann, J, Pfeiffer, H, Phelps, M, Phukon, K, Piccinni, O, Pichot, M, Piergiovanni, F, Pierro, V, Pillant, G, Pinard, L, Pinto, I, Pirello, M, Pitkin, M, Plastino, W, Poggiani, R, Pong, D, Ponrathnam, S, Popolizio, P, Powell, J, Prajapati, A, Prasad, J, Prasai, K, Prasanna, R, Pratten, G, Prestegard, T, Principe, M, Prodi, G, Prokhorov, L, Punturo, M, Puppo, P, Pürrer, M, Qi, H, Quetschke, V, Quinonez, P, Raab, F, Raaijmakers, G, Radkins, H, Radulesco, N, Raffai, P, Raja, S, Rajan, C, Rajbhandari, B, Rakhmanov, M, Ramirez, K, Ramos-Buades, A, Rana, J, Rao, K, Rapagnani, P, Raymond, V, Razzano, M, Read, J, Regimbau, T, Rei, L, Reid, S, Reitze, D, Rettegno, P, Ricci, F, Richardson, C, Richardson, J, Ricker, P, Riemenschneider, G, Riles, K, Rizzo, M, Robertson, N, Robinet, F, Rocchi, A, Rolland, L, Rollins, J, Roma, V, Romanelli, M, Romano, R, Romel, C, Romie, J, Rose, C, Rose, D, Rose, K, Rosińska, D, Rosofsky, S, Ross, M, Rowan, S, Rüdiger, A, Ruggi, P, Rutins, G, Ryan, K, Sachdev, S, Sadecki, T, Sakellariadou, M, Salafia, O, Salconi, L, Saleem, M, Samajdar, A, Sammut, L, Sanchez, E, Sanchez, L, Sanchis-Gual, N, Sanders, J, Santiago, K, Santos, E, Sarin, N, Sassolas, B, Sathyaprakash, B, Sauter, O, Savage, R, Schale, P, Scheel, M, Scheuer, J, Schmidt, P, Schnabel, R, Schofield, R, Schönbeck, A, Schreiber, E, Schulte, B, Schutz, B, Scott, J, Scott, S, Seidel, E, Sellers, D, Sengupta, A, Sennett, N, Sentenac, D, Sequino, V, Sergeev, A, Setyawati, Y, Shaddock, D, Shaffer, T, Shahriar, M, Shaner, M, Sharma, A, Sharma, P, Shawhan, P, Shen, H, Shink, R, Shoemaker, D, Shukla, K, Shyamsundar, S, Siellez, K, Sieniawska, M, Sigg, D, Singer, L, Singh, D, Singh, N, Singhal, A, Sintes, A, Sitmukhambetov, S, Skliris, V, Slagmolen, B, Slaven-Blair, T, Smith, J, Smith, R, Somala, S, Son, E, Soni, S, Sorazu, B, Sorrentino, F, Souradeep, T, Sowell, E, Spencer, A, Spera, M, Srivastava, A, Srivastava, V, Staats, K, Stachie, C, Standke, M, Steer, D, Steinke, M, Steinlechner, J, Steinlechner, S, Steinmeyer, D, Stevenson, S, Stocks, D, Stone, R, Stops, D, Strain, K, Stratta, G, Strigin, S, Strunk, A, Sturani, R, Stuver, A, Sudhir, V, Summerscales, T, Sun, L, Sunil, S, Sur, A, Suresh, J, Sutton, P, Swinkels, B, Szczepańczyk, M, Tacca, M, Tait, S, Talbot, C, Tanner, D, Tao, D, Tápai, M, Tapia, A, Tasson, J, Taylor, R, Tenorio, R, Terkowski, L, Thomas, M, Thomas, P, Thondapu, S, Thorne, K, Thrane, E, Tiwari, S, Tiwari, V, Toland, K, Tonelli, M, Tornasi, Z, Torres-Forné, A, Torrie, C, Töyrä, D, Travasso, F, Traylor, G, Tringali, M, Tripathee, A, Trovato, A, Trozzo, L, Tsang, K, Tse, M, Tso, R, Tsukada, L, Tsuna, D, Tsutsui, T, Tuyenbayev, D, Ueno, K, Ugolini, D, Unnikrishnan, C, Urban, A, Usman, S, Vahlbruch, H, Vajente, G, Valdes, G, Valentini, M, Bakel, N, Beuzekom, M, Brand, J, Broeck, C, Vander-Hyde, D, Schaaf, L, Vanheijningen, J, Veggel, A, Vardaro, M, Varma, V, Vass, S, Vasúth, M, Vecchio, A, Vedovato, G, Veitch, J, Veitch, P, Venkateswara, K, Venugopalan, G, Verkindt, D, Vetrano, F, Viceré, A, Viets, A, Vinciguerra, S, Vine, D, Vinet, J, Vitale, S, Vo, T, Vocca, H, Vorvick, C, Vyatchanin, S, Wade, A, Wade, L, Wade, M, Walet, R, Walker, M, Wallace, L, Walsh, S, Wang, H, Wang, J, Wang, S, Wang, W, Wang, Y, Ward, R, Warden, Z, Warner, J, Was, M, Watchi, J, Weaver, B, Wei, L, Weinert, M, Weinstein, A, Weiss, R, Wellmann, F, Wen, L, Wessel, E, Weßels, P, Westhouse, J, Wette, K, Whelan, J, Whiting, B, Whittle, C, Wilken, D, Williams, D, Williamson, A, Willis, J, Willke, B, Winkler, W, Wipf, C, Wittel, H, Woan, G, Woehler, J, Wofford, J, Wright, J, Wu, D, Wysocki, D, Xiao, S, Xu, R, Yamamoto, H, Yancey, C, Yang, L, Yang, Y, Yang, Z, Yap, M, Yazback, M, Yeeles, D, Yu, H, Yuen, S, Zadrożny, A, Zanolin, M, Zelenova, T, Zendri, J, Zevin, M, Zhang, J, Zhang, L, Zhang, T, Zhao, C, Zhao, G, Zhou, M, Zhou, Z, Zhu, X, Zucker, M, Zweizig, J, Aptekar, R, Boynton, W, Frederiks, D, Golenetskii, S, Golovin, D, Hurley, K, Kozlova, A, Litvak, M, Mitrofanov, I, Sanin, A, Svinkin, D, Carotenuto, F, Krishnan, B, Abbott, B. P., Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, C., Adhikari, R. X., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, G., Allocca, A., Aloy, M. A., Altin, P. A., Amato, A., Anand, S., Ananyeva, A., Anderson, S. B., Anderson, W. G., Angelova, S. V., Antier, S., Appert, S., Arai, K., Araya, M. C., Areeda, J. S., Arène, M., Arnaud, N., Aronson, S. M., Ascenzi, S., Ashton, G., Aston, S. M., Astone, P., Aubin, F., Aufmuth, P., AultONeal, K., Austin, C., Avendano, V., Avila-Alvarez, A., Babak, S., Bacon, P., Badaracco, F., Bader, M. K. M., Bae, S., Baird, J., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Bals, A., Banagiri, S., Barayoga, J. C., Barbieri, C., Barclay, S. E., Barish, B. C., Barker, D., Barkett, K., Barnum, S., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Bawaj, M., Bayley, J. C., Bazzan, M., Bécsy, B., Bejger, M., Belahcene, I., Bell, A. S., Beniwal, D., Benjamin, M. G., Berger, B. K., Bergmann, G., Bernuzzi, S., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhandare, R., Bidler, J., Biggs, E., Bilenko, I. A., Bilgili, S. A., Billingsley, G., Birney, R., Birnholtz, O., Biscans, S., Bischi, M., Biscoveanu, S., Bisht, A., Bitossi, M., Bizouard, M. A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bobba, F., Bode, N., Boer, M., Boetzel, Y., Bogaert, G., Bondu, F., Bonnand, R., Booker, P., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bossilkov, V., Bosveld, J., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Bramley, A., Branchesi, M., Brau, J. E., Breschi, M., Briant, T., Briggs, J. H., Brighenti, F., Brillet, A., Brinkmann, M., Brockill, P., Brooks, A. F., Brooks, J., Brown, D. D., Brunett, S., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. 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W., Wette, K., Whelan, J. T., Whiting, B. F., Whittle, C., Wilken, D. M., Williams, D., Williamson, A. R., Willis, J. L., Willke, B., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Wofford, J. K., Wright, J. L., Wu, D. S., Wysocki, D. M., Xiao, S., Xu, R., Yamamoto, H., Yancey, C. C., Yang, L., Yang, Y., Yang, Z., Yap, M. J., Yazback, M., Yeeles, D. W., Yu, Hang, Yu, Haocun, Yuen, S. H. R., Zadrożny, A. K., Zadrożny, A., Zanolin, M., Zelenova, T., Zendri, J. -P., Zevin, M., Zhang, J., Zhang, L., Zhang, T., Zhao, C., Zhao, G., Zhou, M., Zhou, Z., Zhu, X. J., Zucker, M. E., Zweizig, J., Aptekar, R. L., Boynton, W. V., Frederiks, D. D., Golenetskii, S. V., Golovin, D. V., Hurley, K., Kozlova, A. V., Litvak, M. L., Mitrofanov, I. G., Sanin, A. B., Svinkin, D. S., Carotenuto, Francesco, and Krishnan, Badri
Abstract: We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38 × 10−6 (modeled) and 3.1 × 10−4 (unmodeled). We do not find any significant evidence for gravitational-wave signals associated with the other gamma-ray bursts analyzed, and therefore we report lower bounds on the distance to each of these, assuming various source types and signal morphologies. Using our final modeled search results, short gamma-ray burst observations, and assuming binary neutron star progenitors, we place bounds on the rate of short gamma-ray bursts as a function of redshift for z ≤ 1. We estimate 0.07–1.80 joint detections with Fermi-GBM per year for the 2019–20 LIGO-Virgo observing run and 0.15–3.90 per year when current gravitational-wave detectors are operating at their design sensitivities.
Published: 2019

34. The blue lizard spandrel and the island syndrome

Author: Monti Daria M, Carotenuto Francesco, Rippa Daniela, Polese Gianluca, Turano Mimmo, Guarino Fabio M, Raia Pasquale, Cardi Manuela, and Fulgione Domenico
Subjects: Evolution, QH359-425
Abstract: Abstract Background Many small vertebrates on islands grow larger, mature later, lay smaller clutches/litters, and are less sexually dimorphic and aggressive than their mainland relatives. This set of observations is referred to as the 'Island Syndrome'. The syndrome is linked to high population density on islands. We predicted that when population density is low and/or fluctuating insular vertebrates may evolve correlated trait shifts running opposite to the Island Syndrome, which we collectively refer to as the 'reversed island syndrome' (RIS) hypothesis. On the proximate level, we hypothesized that RIS is caused by increased activity levels in melanocortin receptors. Melanocortins are postranslational products of the proopiomelanocortin gene, which controls pleiotropically pigmentation, aggressiveness, sexual activity, and food intake in vertebrates. Results We tested the RIS hypothesis performing a number of behavioral, genetic, and ontogenetic tests on a blue colored insular variant of the Italian Wall lizard Podarcis sicula, living on a small island off the Southern Italian coast. The population density of this blue-colored variant was generally low and highly fluctuating from one year to the next. In keeping with our predictions, insular lizards were more aggressive and sexually dimorphic than their mainland relatives. Insular males had wide, peramorphic heads. The growth rate of insular females was slower than growth rates of mainland individuals of both sexes, and of insular males. Consequently, size and shape dimorphism are higher on the Island. As predicted, melanocortin receptors were much more active in individuals of the insular population. Insular lizards have a higher food intake rate than mainland individuals, which is consistent with the increased activity of melanocortin receptors. This may be adaptive in an unpredictable environment such as Licosa Island. Insular lizards of both sexes spent less time basking than their mainland relatives. We suspect this is a by-product (spandrel) of the positive selection for increased activity of melanocortins receptors. Conclusions We contend that when population density is either low or fluctuating annually as a result of environmental unpredictability, it may be advantageous to individuals to behave more aggressively, to raise their rate of food intake, and allocate more energy into reproduction.
Published: 2010
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35. Character displacement under influence of Bergmann’s rule in Cerdocyon thous (Mammalia: Canidae)

Author: de Moura Bubadué, J., Cáceres, N., dos Santos Carvalho, R., Sponchiado, J., Saggese, F., Mondanaro, A., PASSARO, FEDERICO, RAIA, PASQUALE, CAROTENUTO, FRANCESCO, de Moura Bubadué, J., Cáceres, N., dos Santos Carvalho, R., Sponchiado, J., Passaro, Federico, Saggese, F., Mondanaro, A., Raia, Pasquale, and Carotenuto, Francesco
Subjects: Canidae, crab-eating fox, geometric morphometrics, sexual size dimorphism, shape disparity, South America, Bergmann’s rule, character displacement
Abstract: In South America, the crab-eating fox Cerdocyon thous occurs in sympatry to the ecologically similar, and phylogenetically close Lycalopex vetulus to the North, and Lycalopex gymnocercus to the South of its range. We studied character displacement in Cerdocyon under the effect of Bergmann's rule and the presence (or absence either) of Lycalopex within the crab-eating fox range. We performed skull shape analysis on 191 C. thous specimens and divided them in three distinct groups, depending on whether Cerdocyon occurs in sympatry or in allopatry to Lycalopex species. We tested for differences in size and shape between Cerdocyon groups and regressed both skull size and sexual size dimorphism against latitude and temperature, while controlling for spatial autocorrelation in the phenotypes. Southern Cerdocyon specimens present enlarged temporalis muscle and slender carnassial, both suggestive of a shift towards increased carnivory. Such a niche shift is interpreted as a mean to reduce competition to the larger Lycalopex species, which is still smaller than Cerdocyon. Consistently with the above, the degree of sexual shape and size dimorphism in Cerdocyon increases southward. We found a complex but coherent pattern of size and shape differentiation in Cerdocyon groups, which is consistent with the effects of both competition and Bergmann's rule. Cerdocyon reduces competition to Lycalopex by growing larger in the North. To the South, Cerdocyon is still larger, in keeping with Bergmann's rule, but strongly differs in skull shape from both its Lycalopex competitor and from any other Cerdocyon. Since the Southern Lycalopex species is much more similar in size to Cerdocyon than its Northern congeneric, this suggests that shape differences serve the goal of reducing competition between Cerdocyon and Lycalopex to the South, as size differences do to the North. The absence of the hypercarnivorous canid Speothos venaticus from the southern range of Cerdocyon may have allowed such a pattern to take place.
Published: 2016

36. Emotion Regulation and Parental Bonding in Families of Adolescents With Internalizing and Externalizing Symptoms

Author: Mannarini, Stefania, primary, Balottin, Laura, additional, Palmieri, Arianna, additional, and Carotenuto, Francesco, additional
Published: 2018
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37. Diversification Rates and the Evolution of Species Range Size Frequency Distribution

Author: Castiglione, Silvia, primary, Mondanaro, Alessandro, additional, Melchionna, Marina, additional, Serio, Carmela, additional, Di Febbraro, Mirko, additional, Carotenuto, Francesco, additional, and Raia, Pasquale, additional
Published: 2017
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38. Past Extinctions of HomoSpecies Coincided with Increased Vulnerability to Climatic Change

Author: Raia, Pasquale, Mondanaro, Alessandro, Melchionna, Marina, Di Febbraro, Mirko, Diniz-Filho, Josè A.F., Rangel, Thiago F., Holden, Philip B., Carotenuto, Francesco, Edwards, Neil R., Lima-Ribeiro, Matheus S., Profico, Antonio, Maiorano, Luigi, Castiglione, Silvia, Serio, Carmela, and Rook, Lorenzo
Abstract: At least six different Homospecies populated the World during the latest Pliocene to the Pleistocene. The extinction of all but one of them is currently shrouded in mystery, and no consistent explanation has yet been advanced, despite the enormous importance of the matter. Here, we use a recently implemented past climate emulator and an extensive fossil database spanning 2,754 archaeological records to model climatic niche evolution in Homo. We find statistically robust evidence that the three Homospecies representing terminating, independent lineages, H. erectus, H. heidelbergensis, and H. neanderthalensis, lost a significant portion of their climatic niche space just before extinction, with no corresponding reduction in physical range. This reduction coincides with increased vulnerability to climate change. In the case of Neanderthals, the increased extinction risk was probably exacerbated by competition with H. sapiens. This study suggests that climate change was the primary factor in the extinction of Homospecies.
Published: 2020
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39. Design and implementation of a mobile device APP for network-based EEW systems: application to PRESTo EEWS in Southern Italy.

Author: Colombelli, Simona, Carotenuto, Francesco, Elia, Luca, and Zollo, Aldo
Subjects: MOBILE apps, SEISMIC networks, EARTHQUAKE resistant design, LEAD time (Supply chain management), EARTHQUAKES
Abstract: A fundamental feature of any Earthquake Early Warning System is the ability of rapidly broadcast earthquake information to a wide audience of potential end users and stakeholders, in an intuitive, customizable way. Smartphones and other mobile devices are nowadays continuously connected to the internet and represent the ideal tools for earthquake alerts dissemination, to inform a large number of users about the potential damaging shaking of an impending earthquake. Here we present a mobile App (named ISNet EWApp) for Android devices which can receive the alerts generated by a network-based Early Warning system. Specifically, the app receives the earthquake alerts generated by the PRESTo EWS, which is currently running on the accelerometric stations of the Irpinia Seismic Network (ISNet) in Southern Italy. In the absence of alerts, the EWApp displays the standard bulletin of seismic events occurred within the network. In the event of a relevant earthquake, instead, the app has a dedicated module to predict the expected ground shaking intensity and the available lead-time at the user position and to provide customized messages to inform the user about the proper reaction during the alert. We first present the architecture of both network-based system and EWApp, and then and describe its essential operational modes. The app is designed in a way that is easily exportable to any other network-based early warning system. [ABSTRACT FROM AUTHOR]
Published: 2019
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40. THE PLIO-HOLOCENE LARGE MAMMALS OF THE WESTERN EURASIA: MACROECOLOGICAL AND EVOLUTIONARY ANALYSES OF THE FAUNAS

Author: Carotenuto, Francesco and Carotenuto, Francesco
Abstract: The climate during the Plio-Pleistocene was deeply influenced by the so called Milankovitch cycles (Zachos et al.,2001). These are combinations of different astronomical phenomena involving the variation of the Earth’s orbital eccentricity, the axis obliquity and precession. The first phenomenon was estimated to occur every 400-100 Ka, whereas the others occur over a time period of 41 and 23-19 Ka, respectively. These astronomical variations influenced the Earth-Sun distance and the angular incidence of solar rays with a net effect on the global climate change (Zachos et al., 2001). The Early Pliocene was characterized by a decrease of the global temperature, a trend that began during the Late Miocene. The measure of the mean 16O/18O values indicates a trend of warmer climate until 3.2 Mya, the latter that represents the onset of a new temperature cycle. During these cycles the ice sheet expanded and contracted according to the variation of the mean global temperature. Indeed, in the Middle Pliocene, the ice sheets began to cover the Northern Hemisphere, an event indicated as NHG (North Hemisphere Glaciation) (Shackleton et al., 1998; Maslin et al., 1998; Zachos et al., 2001). At ~2.5 Mya the oscillations of the temperature became quite a regular pattern determining the alternation between warmer (Interglacials) and cooler (Glacials) time periods, that were to characterize the Pleistocene. Some 1 May (period coincident with the Jaramillo Event of Earth’s Magnetic Field inversion) the time interval of a complete climatic cycle changed its duration from the 41-23-19 Kya., to a new longer cycle of 100 Kya, probably determined Earth’s orbital eccentricity variation. With the increase of the duration of the cycles the mean global temperatures reached more extreme values and there were stronger climate ranges between warm and cold periods. Moreover, the measures of the oxygen isotopes ratios confirm a net decrement of mean temperature values recorded from the Late Pliocen
Published: 2009

41. The blue lizard spandrel and the island syndrome

Author: Raia, Pasquale, primary, Guarino, Fabio M, additional, Turano, Mimmo, additional, Polese, Gianluca, additional, Rippa, Daniela, additional, Carotenuto, Francesco, additional, Monti, Daria M, additional, Cardi, Manuela, additional, and Fulgione, Domenico, additional
Published: 2010
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42. Early Detection of Wild Rocket Tracheofusariosis Using Hyperspectral Image-Based Machine Learning.

Author: Pane, Catello, Manganiello, Gelsomina, Nicastro, Nicola, and Carotenuto, Francesco
Subjects: MACHINE learning, FUSARIUM oxysporum, COLONIZATION (Ecology), DISEASE progression, SPECTRAL imaging
Abstract: Fusarium oxysporum f. sp. raphani is responsible for wilting wild rocket (Diplotaxis tenuifolia L. [D.C.]). A machine learning model based on hyperspectral data was constructed to monitor disease progression. Thus, pathogenesis after artificial inoculation was monitored over a 15-day period by symptom assessment, qPCR pathogen quantification, and hyperspectral imaging. The host colonization by a pathogen evolved accordingly with symptoms as confirmed by qPCR. Spectral data showed differences as early as 5-day post infection and 12 hypespectral vegetation indices were selected to follow disease development. The hyperspectral dataset was used to feed the XGBoost machine learning algorithm with the aim of developing a model that discriminates between healthy and infected plants during the time. The multiple cross-prediction strategy of the pixel-level models was able to detect hyperspectral disease profiles with an average accuracy of 0.8. For healthy pixel detection, the mean Precision value was 0.78, the Recall was 0.88, and the F1 Score was 0.82. For infected pixel detection, the average evaluation metrics were Precision: 0.73, Recall: 0.57, and F1 Score: 0.63. Machine learning paves the way for automatic early detection of infected plants, even a few days after infection. [ABSTRACT FROM AUTHOR]
Published: 2022
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43. Past extinctions of Homo species coincided with increased vulnerability to climatic change

Author: Raia, Pasquale, Mondanaro, Alessandro, Melchionna, Marina, Di Febbraro, Mirko, Diniz-Filho, Jose A F, Rangel, Thiago F, Holden, Philip B, Carotenuto, Francesco, Edwards, Neil R, Lima-Ribeiro, Matheus S, Profico, Antonio, Maiorano, Luigi, Castiglione, Silvia, Serio, Carmela, Rook, Lorenzo, Raia, Pasquale, Mondanaro, Alessandro, Melchionna, Marina, Di Febbraro, Mirko, Diniz-Filho, Jose A F, Rangel, Thiago F, Holden, Philip B, Carotenuto, Francesco, Edwards, Neil R, Lima-Ribeiro, Matheus S, Profico, Antonio, Maiorano, Luigi, Castiglione, Silvia, Serio, Carmela, and Rook, Lorenzo
Abstract: At least six different Homo species populated the World during the latest Pliocene to the Pleistocene. The extinction of all but one of them is currently shrouded in mystery, and no consistent explanation has yet been advanced, despite the enormous importance of the matter. Here, we use a recently implemented past climate emulator and an extensive fossil database spanning 2,754 archaeological records to model climatic niche evolution in Homo. We find statistically robust evidence that the three Homo species representing terminating, independent lineages, H. erectus, H. heidelbergensis, and H. neanderthalensis, lost a significant portion of their climatic niche space just before extinction, with no corresponding reduction in physical range. This reduction coincides with increased vulnerability to climate change. In the case of Neanderthals, the increased extinction risk was probably exacerbated by competition with H. sapiens. This study suggests that climate change was the primary factor in the extinction of Homo species.

44. A major change in rate of climate niche envelope evolution during hominid history

Author: Mondanaro, Alessandro, Melchiona, Marina, Di Febbraro, Mirko, Castiglione, Silvia, Holden, Philip B., Edwards, Neil R., Carotenuto, Francesco, Maiorano, Luigi, Modafferi, Maria, Serio, Carmela, Diniz-Filho, Josè A.F., Rangel, Thiago, Rook, Lorenzo, O'Higgins, Paul, Spikins, Penny, Profico, Antonia, Raia, Pasquale, Mondanaro, Alessandro, Melchiona, Marina, Di Febbraro, Mirko, Castiglione, Silvia, Holden, Philip B., Edwards, Neil R., Carotenuto, Francesco, Maiorano, Luigi, Modafferi, Maria, Serio, Carmela, Diniz-Filho, Josè A.F., Rangel, Thiago, Rook, Lorenzo, O'Higgins, Paul, Spikins, Penny, Profico, Antonia, and Raia, Pasquale
Abstract: Homo sapiens is the only species alive able to take advantage of its cognitive abilities to inhabit almost all environments on Earth. Humans are able to culturally construct, rather than biologically inherit, their occupied climatic niche to a degree unparalleled within the animal kingdom. Precisely when hominins acquired such an ability remains unknown, and scholars disagree on the extent to which our ancestors shared this same ability. Here, we settle this issue using fine-grained palaeoclimatic data, extensive archaeological data and phylogenetic comparative methods. Our results indicate that whereas early hominins were forced to live under physiologically suitable climatic conditions, with the emergence of H. heidelbergensis, the Homo climatic niche expanded beyond its natural limits, despite progressive harshening in global climates. This indicates that technological innovations providing effective exploitation of cold and seasonal habitats predated the emergence of Homo sapiens.

45. A major change in rate of climate niche envelope evolution during hominid history

Author: Mondanaro, Alessandro, Melchiona, Marina, Di Febbraro, Mirko, Castiglione, Silvia, Holden, Philip B., Edwards, Neil R., Carotenuto, Francesco, Maiorano, Luigi, Modafferi, Maria, Serio, Carmela, Diniz-Filho, Josè A.F., Rangel, Thiago, Rook, Lorenzo, O'Higgins, Paul, Spikins, Penny, Profico, Antonia, Raia, Pasquale, Mondanaro, Alessandro, Melchiona, Marina, Di Febbraro, Mirko, Castiglione, Silvia, Holden, Philip B., Edwards, Neil R., Carotenuto, Francesco, Maiorano, Luigi, Modafferi, Maria, Serio, Carmela, Diniz-Filho, Josè A.F., Rangel, Thiago, Rook, Lorenzo, O'Higgins, Paul, Spikins, Penny, Profico, Antonia, and Raia, Pasquale
Abstract: Homo sapiens is the only species alive able to take advantage of its cognitive abilities to inhabit almost all environments on Earth. Humans are able to culturally construct, rather than biologically inherit, their occupied climatic niche to a degree unparalleled within the animal kingdom. Precisely when hominins acquired such an ability remains unknown, and scholars disagree on the extent to which our ancestors shared this same ability. Here, we settle this issue using fine-grained palaeoclimatic data, extensive archaeological data and phylogenetic comparative methods. Our results indicate that whereas early hominins were forced to live under physiologically suitable climatic conditions, with the emergence of H. heidelbergensis, the Homo climatic niche expanded beyond its natural limits, despite progressive harshening in global climates. This indicates that technological innovations providing effective exploitation of cold and seasonal habitats predated the emergence of Homo sapiens.

46. Past extinctions of Homo species coincided with increased vulnerability to climatic change

Author: Raia, Pasquale, Mondanaro, Alessandro, Melchionna, Marina, Di Febbraro, Mirko, Diniz-Filho, Jose A F, Rangel, Thiago F, Holden, Philip B, Carotenuto, Francesco, Edwards, Neil R, Lima-Ribeiro, Matheus S, Profico, Antonio, Maiorano, Luigi, Castiglione, Silvia, Serio, Carmela, Rook, Lorenzo, Raia, Pasquale, Mondanaro, Alessandro, Melchionna, Marina, Di Febbraro, Mirko, Diniz-Filho, Jose A F, Rangel, Thiago F, Holden, Philip B, Carotenuto, Francesco, Edwards, Neil R, Lima-Ribeiro, Matheus S, Profico, Antonio, Maiorano, Luigi, Castiglione, Silvia, Serio, Carmela, and Rook, Lorenzo
Abstract: At least six different Homo species populated the World during the latest Pliocene to the Pleistocene. The extinction of all but one of them is currently shrouded in mystery, and no consistent explanation has yet been advanced, despite the enormous importance of the matter. Here, we use a recently implemented past climate emulator and an extensive fossil database spanning 2,754 archaeological records to model climatic niche evolution in Homo. We find statistically robust evidence that the three Homo species representing terminating, independent lineages, H. erectus, H. heidelbergensis, and H. neanderthalensis, lost a significant portion of their climatic niche space just before extinction, with no corresponding reduction in physical range. This reduction coincides with increased vulnerability to climate change. In the case of Neanderthals, the increased extinction risk was probably exacerbated by competition with H. sapiens. This study suggests that climate change was the primary factor in the extinction of Homo species.

47. Powdery Mildew Caused by Erysiphe cruciferarum on Wild Rocket (Diplotaxis tenuifolia): Hyperspectral Imaging and Machine Learning Modeling for Non-Destructive Disease Detection

Author: Nicola Nicastro, Teodoro Cardi, Francesco Carotenuto, Gelsomina Manganiello, Catello Pane, Pane, Catello, Manganiello, Gelsomina, Nicastro, Nicola, Cardi, Teodoro, and Carotenuto, Francesco
Subjects: 0106 biological sciences, business.product_category, Disease detection, Erysiphe cruciferarum, Random forest model, Plant Science, Biology, First report, 01 natural sciences, Xgboost model, Crop, 03 medical and health sciences, Non destructive, Digital detection, lcsh:Agriculture (General), Hyperspectral signature, 030304 developmental biology, 0303 health sciences, Chlorophyll absorption, Hyperspectral imaging, Diplotaxis tenuifolia, biology.organism_classification, lcsh:S1-972, Horticulture, Rocket, business, Agronomy and Crop Science, Powdery mildew, 010606 plant biology & botany, Food Science
Abstract: Wild rocket is a widely cultivated salad crop. Typical signs and symptoms of powdery mildew were observed on leaves of Diplotaxis tenuifolia, likely favored by climatic conditions occurring in a greenhouse. Based on morphological features and molecular analysis, the disease agent was identified as the fungal pathogen Erysiphe cruciferarum. To the best of our knowledge, this is the first report of E. cruciferarum on D. tenuifolia. Moreover, the present study provides a non-destructive high performing digital approach to efficiently detect the disease. Hyperspectral image analysis allowed to characterize the spectral response of wild rocket affected by powdery mildew and the adopted machine-learning approach (a trained Random Forest model with the four most contributory wavelengths falling in the range 403–446 nm) proved to be able to accurately discriminate between healthy and diseased wild rocket leaves. Shifts in the irradiance absorption by chlorophyll a of diseased leaves in the spectrum blue range seems to be at the base of the hyperspectral imaging detection of wild rocket powdery mildew.
Published: 2021

48. Insights into mechanical properties of the 1980 irpinia fault system from the analysis of a seismic sequence

Author: Luca Elia, Sergio Gammaldi, Gaetano Festa, Antonio Scala, Sahar Nazeri, Aldo Zollo, Alessandro Caruso, Guido Russo, Antonio Emolo, Antonio Giovanni Iaccarino, Grazia De Landro, Stefania Tarantino, Guido Maria Adinolfi, Francesco Carotenuto, Rosario Riccio, Matteo Picozzi, Simona Colombelli, Festa, Gaetano, Adinolfi, Guido Maria, Caruso, Alessandro, Colombelli, Simona, De Landro, Grazia, Elia, Luca, Emolo, Antonio, Picozzi, Matteo, Scala, Antonio, Carotenuto, Francesco, Gammaldi, Sergio, Iaccarino, Antonio Giovanni, Nazeri, Sahar, Riccio, Rosario, Russo, Guido, Tarantino, Stefania, and Zollo, Aldo
Subjects: 010504 meteorology & atmospheric sciences, Blind zone, Magnitude (mathematics), Fault (geology), 010502 geochemistry & geophysics, Earthquake seismology, Microseismicity, Seismic techniques, Seismotectonics, 01 natural sciences, Computer Science::Hardware Architecture, Sequence (geology), Computer Science::Operating Systems, Computer Science::Distributed, Parallel, and Cluster Computing, 0105 earth and related environmental sciences, geography, geography.geographical_feature_category, Autocorrelation technique, lcsh:QE1-996.5, Ranging, lcsh:Geology, seismotectonics, General Earth and Planetary Sciences, Geology, Seismology, Asperity (materials science)
Abstract: Seismic sequences are a powerful tool to locally infer geometrical and mechanical properties of faults and fault systems. In this study, we provided detailed location and characterization of events of the 3&ndash, 7 July 2020 Irpinia sequence (southern Italy) that occurred at the northern tip of the main segment that ruptured during the 1980 Irpinia earthquake. Using an autocorrelation technique, we detected more than 340 events within the sequence, with local magnitude ranging between &minus, 0.5 and 3.0. We thus provided double difference locations, source parameter estimation, and focal mechanisms determination for the largest quality events. We found that the sequence ruptured an asperity with a size of about 800 m, along a fault structure having a strike compatible with the one of the main segments of the 1980 Irpinia earthquake, and a dip of 50&ndash, 55&deg, at depth of 10.5&ndash, 12 km and 60&ndash, 65&deg, at shallower depths (7.5&ndash, 9 km). Low stress drop release (average of 0.64 MPa) indicates a fluid-driven initiation mechanism of the sequence. We also evaluated the performance of the earthquake early warning systems running in real-time during the sequence, retrieving a minimum size for the blind zone in the area of about 15 km.
Published: 2021

49. Past Extinctions of Homo Species Coincided with Increased Vulnerability to Climatic Change

Author: Mirko Di Febbraro, Antonio Profico, Thiago F. Rangel, Matheus S. Lima-Ribeiro, Alessandro Mondanaro, Pasquale Raia, José Alexandre Felizola Diniz-Filho, Silvia Castiglione, Luigi Maiorano, Carmela Serio, Marina Melchionna, Neil R. Edwards, Francesco Carotenuto, Lorenzo Rook, Philip B. Holden, Raia, Pasquale, Mondanaro, Alessandro, Melchionna, Marina, Di Febbraro, Mirko, Diniz-Filho, Josè A. F., Rangel, Thiago F., Holden, Philip B., Carotenuto, Francesco, Edwards, Neil R., Lima-Ribeiro, Matheus S., Profico, Antonio, Maiorano, Luigi, Castiglione, Silvia, Serio, Carmela, and Rook, Lorenzo
Subjects: human evolution, palaeoanthropology, climatic change, climate change-mediated, extinction, Homo neanderthalensis, climate niche factor analysis, niche overlap, global change, Pleistocene, Range (biology), media_common.quotation_subject, Niche, Vulnerability, Climate change, Competition (biology), climate change-mediated extinction, Earth and Planetary Sciences (miscellaneous), General Environmental Science, media_common, Extinction, Ecology, Global change, Climate change, Homo extinction, Pleistocene, Geography, Human evolution
Abstract: Summary At least six different Homo species populated the World during the latest Pliocene to the Pleistocene. The extinction of all but one of them is currently shrouded in mystery, and no consistent explanation has yet been advanced, despite the enormous importance of the matter. Here, we use a recently implemented past climate emulator and an extensive fossil database spanning 2,754 archaeological records to model climatic niche evolution in Homo. We find statistically robust evidence that the three Homo species representing terminating, independent lineages, H. erectus, H. heidelbergensis, and H. neanderthalensis, lost a significant portion of their climatic niche space just before extinction, with no corresponding reduction in physical range. This reduction coincides with increased vulnerability to climate change. In the case of Neanderthals, the increased extinction risk was probably exacerbated by competition with H. sapiens. This study suggests that climate change was the primary factor in the extinction of Homo species.
Published: 2020

50. Design and implementation of a mobile device APP for network-based EEW systems: application to PRESTo EEWS in Southern Italy

Author: Simona Colombelli, Luca Elia, Francesco Carotenuto, Aldo Zollo, Colombelli, Simona, Carotenuto, Francesco, Elia, Luca, and Zollo, Aldo
Subjects: 021110 strategic, defence & security studies, End user, business.industry, Computer science, 0211 other engineering and technologies, Earthquake warning system, 02 engineering and technology, Computer security, computer.software_genre, GeneralLiterature_MISCELLANEOUS, Early warning system, The Internet, Architecture, Android (operating system), business, Ground shaking, computer, Mobile device
Abstract: A fundamental feature of any Earthquake Early Warning System is the ability of rapidly broadcast earthquake information to a wide audience of potential end users and stakeholders, in an intuitive, customizable way. Smartphones and other mobile devices are nowadays continuously connected to the internet and represent the ideal tools for earthquake alerts dissemination, to inform a large number of users about the potential damaging shaking of an impending earthquake.Here we present a mobile App (named ISNet EWApp) for Android devices which can receive the alerts generated by a network-based Early Warning system. Specifically, the app receives the earthquake alerts generated by the PRESTo EWS, which is currently running on the accelerometric stations of the Irpinia Seismic Network (ISNet) in Southern Italy. In the absence of alerts, the EWApp displays the standard bulletin of seismic events occurred within the network. In the event of a relevant earthquake, instead, the app has a dedicated module to predict the expected ground shaking intensity and the available lead-time at the user position and to provide customized messages to inform the user about the proper reaction during the alert.We first present the architecture of both network-based system and EWApp, and then and describe its essential operational modes. The app is designed in a way that is easily exportable to any other network-based early warning system.
Published: 2020

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