Lech Mankiewicz
Research Subjects
Research Interests
Lech Mankiewicz has a total of 1000 co-authors. Here are the top co-authors by number of shared publications:
- Marcin Sokolowski
International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
53 shared publications - Grzegorz Kasprowicz
Warsaw University of Technology
32 shared publications K. Nawrocki
National Ctr. for Nuclear Research (Poland)
27 shared publicationsG. Wrochna
National Ctr. for Nuclear Research (Poland)
26 shared publications- Aleksander Fillip Zarnecki
Faculty of Physics, University of Warsaw, Warszawa, Poland
22 shared publications Grzegorz Wrochna
National Ctr. for Nuclear Research (Poland)
17 shared publications
Latest Publications
- Open Access
- 3 January 2025
- Published by American Association for the Advancement of Science (AAAS) in Science Advances
- Vol. 11 (1) , eadm7255
Information sharing within a social network is key to behavioral flexibility—Lessons from mice tested under seminaturalistic conditions
Being part of a social structure offers chances for social learning vital for survival and reproduction. Nevertheless, studying the neural mechanisms of social learning under laboratory conditions remains challenging. To investigate the impact of socially transmitted information about rewards on individual behavior, we used Eco-HAB, an automated system monitoring the voluntary behavior of group-housed mice under seminaturalistic conditions. In these settings, male mice spontaneously form social networks, with individuals occupying diverse positions. We show that a rewarded group member’s scent affects the ability of conspecifics to search for rewards in familiar and novel environments. The scent’s impact depends on the animal’s social position. Furthermore, disruption of neuronal plasticity in the prelimbic cortex (PL) disrupts the social networks and animals’ interest in social information related to rewards; only the latter is blocked by the acute PL inhibition. This experimental design represents a cutting-edge approach to studying the brain mechanisms of social learning.
- 3 January 2025
- Published by American Association for the Advancement of Science (AAAS) in Science Advances
- Vol. 11 (1) , eadm7255
Open AccessInformation sharing within a social network is key to behavioral flexibility—Lessons from mice tested under seminaturalistic conditions
Being part of a social structure offers chances for social learning vital for survival and reproduction. Nevertheless, studying the neural mechanisms of social learning under laboratory conditions remains challenging. To investigate the impact of socially transmitted information about rewards on individual behavior, we used Eco-HAB, an automated system monitoring the voluntary behavior of group-housed mice under seminaturalistic conditions. In these settings, male mice spontaneously form social networks, with individuals occupying diverse positions. We show that a rewarded group member’s scent affects the ability of conspecifics to search for rewards in familiar and novel environments. The scent’s impact depends on the animal’s social position. Furthermore, disruption of neuronal plasticity in the prelimbic cortex (PL) disrupts the social networks and animals’ interest in social information related to rewards; only the latter is blocked by the acute PL inhibition. This experimental design represents a cutting-edge approach to studying the brain mechanisms of social learning.
- 28 August 2020
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 125 (9) , 091101
Limits on the Flux of Nuclearites and Other Heavy Compact Objects from the Pi of the Sky Project
Many theories predict the existence of very heavy compact objects, that in terms of sizes would belong to the realms of nuclear or atomic physics, but in terms of masses could extend to the macroscopic world, reaching kilograms, tonnes, or more. If they exist, it is likely that they reach our planet with high speeds and cross the atmosphere. Because of their high mass-to-size ratio and huge energy, in many cases, they would leave behind a trail in the form of sound and seismic waves, etches, or light in transparent media. Here we show results of a search for such objects in visual photographs of the sky taken by the “Pi of the Sky” experiment, illustrated with the most stringent limits on the isotropic flux of incoming so-called nuclearites, spanning between and for masses between 100 g and 100 kg. In addition we establish a directional flux limit under an assumption of a static “sea” of nuclearites in the Galaxy, which spans between and in the same mass range. The general nature of the limits presented should allow one to constrain many specific models predicting the existence of heavy compact objects and both particle physics and astrophysical processes leading to their creation, and their sources.- 28 August 2020
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 125 (9) , 091101
Limits on the Flux of Nuclearites and Other Heavy Compact Objects from the Pi of the Sky Project
Many theories predict the existence of very heavy compact objects, that in terms of sizes would belong to the realms of nuclear or atomic physics, but in terms of masses could extend to the macroscopic world, reaching kilograms, tonnes, or more. If they exist, it is likely that they reach our planet with high speeds and cross the atmosphere. Because of their high mass-to-size ratio and huge energy, in many cases, they would leave behind a trail in the form of sound and seismic waves, etches, or light in transparent media. Here we show results of a search for such objects in visual photographs of the sky taken by the “Pi of the Sky” experiment, illustrated with the most stringent limits on the isotropic flux of incoming so-called nuclearites, spanning between and for masses between 100 g and 100 kg. In addition we establish a directional flux limit under an assumption of a static “sea” of nuclearites in the Galaxy, which spans between and in the same mass range. The general nature of the limits presented should allow one to constrain many specific models predicting the existence of heavy compact objects and both particle physics and astrophysical processes leading to their creation, and their sources.- 6 November 2019
- Published by SPIE-Intl Soc Optical Eng
- Vol. 11176, 111762N
Modular control system for behavioral experiments
The article presents the latest updates in the development of automated cage for optogenetic experiments. The new RFID module allows detecting the presence of mice in a given area of the cage. A brief description of the hardware and software parts has been presented.
- 6 November 2019
- Published by SPIE-Intl Soc Optical Eng
- Vol. 11176, 111762N
Modular control system for behavioral experiments
The article presents the latest updates in the development of automated cage for optogenetic experiments. The new RFID module allows detecting the presence of mice in a given area of the cage. A brief description of the hardware and software parts has been presented.
- 1 October 2018
- Published by SPIE-Intl Soc Optical Eng
- Vol. 10808, 181
Development of automated cage for optogenetic experiments with electromagnetic positioning system
Article presents latest updates in development of automated cage for optogenetic experiments. New hardware concept for data concentrator is presented with ability to fuse incoming data from multiple sources. Along with hardware updates, a new web interface for controlling the hardware is presented as well as localization system development.
- 1 October 2018
- Published by SPIE-Intl Soc Optical Eng
- Vol. 10808, 181
Development of automated cage for optogenetic experiments with electromagnetic positioning system
Article presents latest updates in development of automated cage for optogenetic experiments. New hardware concept for data concentrator is presented with ability to fuse incoming data from multiple sources. Along with hardware updates, a new web interface for controlling the hardware is presented as well as localization system development.
- 20 November 2017
- Published by Springer Nature in Nature Astronomy
- Vol. 2 (1) , 69-75
Transition from fireball to Poynting-flux-dominated outflow in the three-episode GRB 160625B
- 20 November 2017
- Published by Springer Nature in Nature Astronomy
- Vol. 2 (1) , 69-75
Transition from fireball to Poynting-flux-dominated outflow in the three-episode GRB 160625B
- 7 August 2017
- Published by SPIE-Intl Soc Optical Eng
- Vol. 10445, 104453Z-104453Z-6
An automated cage for optogenetic experiments with electromagnetic positioning system
- 7 August 2017
- Published by SPIE-Intl Soc Optical Eng
- Vol. 10445, 104453Z-104453Z-6
An automated cage for optogenetic experiments with electromagnetic positioning system
- 7 August 2017
- Published by SPIE-Intl Soc Optical Eng
- Vol. 10445, 104454C-104454C-12
Pi of the Sky observation of GRB160625B
- 7 August 2017
- Published by SPIE-Intl Soc Optical Eng
- Vol. 10445, 104454C-104454C-12
Pi of the Sky observation of GRB160625B
- 7 August 2017
- Published by SPIE-Intl Soc Optical Eng
- Vol. 10445, 104454I
Pi of the Sky in LSC-Virgo's EM follow-up in O1 science run
- 7 August 2017
- Published by SPIE-Intl Soc Optical Eng
- Vol. 10445, 104454I
Pi of the Sky in LSC-Virgo's EM follow-up in O1 science run
- Open Access
- 23 December 2016
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 466 (4) , 4009-4020
V473 Lyr, a modulated, period-doubled Cepheid, and U TrA, a double-mode Cepheid observed by MOST
Space-based photometric measurements first revealed low-amplitude irregularities in the pulsations of Cepheid stars, but their origins and how commonly they occur remain uncertain. To investigate this phenomenon, we present MOST space telescope photometry of two Cepheids. V473 Lyrae is a second-overtone, strongly modulated Cepheid, while U Trianguli Australis is a Cepheid pulsating simultaneously in the fundamental mode and first overtone. The nearly continuous, high-precision photometry reveals alternations in the amplitudes of cycles in V473 Lyr, the first case of period doubling detected in a classical Cepheid. In U TrA, we tentatively identify one peak as the fX or 0.61–type mode often seen in conjunction with the first radial overtone in Cepheids, but given the short length of the data, we cannot rule out that it is a combination peak instead. Ground-based photometry and spectroscopy were obtained to follow two modulation cycles in V473 Lyr and to better specify its physical parameters. The simultaneous data yield the phase lag parameter (the phase difference between maxima in luminosity and radial velocity) of a second-overtone Cepheid for the first time. We find no evidence for a period change in U TrA or an energy exchange between the fundamental mode and the first overtone during the last 50 yr, contrary to earlier indications. Period doubling in V473 Lyr provides a strong argument that mode interactions do occur in some Cepheids and we may hypothesize that it could be behind the amplitude modulation, as recently proposed for Blazhko RR Lyrae stars.
- 23 December 2016
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 466 (4) , 4009-4020
Open AccessV473 Lyr, a modulated, period-doubled Cepheid, and U TrA, a double-mode Cepheid observed by MOST
Space-based photometric measurements first revealed low-amplitude irregularities in the pulsations of Cepheid stars, but their origins and how commonly they occur remain uncertain. To investigate this phenomenon, we present MOST space telescope photometry of two Cepheids. V473 Lyrae is a second-overtone, strongly modulated Cepheid, while U Trianguli Australis is a Cepheid pulsating simultaneously in the fundamental mode and first overtone. The nearly continuous, high-precision photometry reveals alternations in the amplitudes of cycles in V473 Lyr, the first case of period doubling detected in a classical Cepheid. In U TrA, we tentatively identify one peak as the fX or 0.61–type mode often seen in conjunction with the first radial overtone in Cepheids, but given the short length of the data, we cannot rule out that it is a combination peak instead. Ground-based photometry and spectroscopy were obtained to follow two modulation cycles in V473 Lyr and to better specify its physical parameters. The simultaneous data yield the phase lag parameter (the phase difference between maxima in luminosity and radial velocity) of a second-overtone Cepheid for the first time. We find no evidence for a period change in U TrA or an energy exchange between the fundamental mode and the first overtone during the last 50 yr, contrary to earlier indications. Period doubling in V473 Lyr provides a strong argument that mode interactions do occur in some Cepheids and we may hypothesize that it could be behind the amplitude modulation, as recently proposed for Blazhko RR Lyrae stars.
- 28 September 2016
- Published by SPIE-Intl Soc Optical Eng
- p. 1003139-1003139-6
Miniature subcutaneous optogenetic device
- 28 September 2016
- Published by SPIE-Intl Soc Optical Eng
- p. 1003139-1003139-6
Miniature subcutaneous optogenetic device