Consider a fixed voting rule R. In the Possible President problem, we are given an election where the candidates are partitioned into parties, and the problem is to determine if, given a party P, it is possible for every party to nominate a candidate such that the nominee from P is a winner of the election that is obtained by restricting the votes to the nominated candidates. In the Necessary President problem, we would like to find a nominee who wins no matter who else is nominated. In this talk, we explore the complexity of these problems, which can be thought of as the two natural extremes of the party nomination problem, with an emphasis on a parameterized perspective and algorithms on structured profiles.
Brute force effects of mass media presence and social media activity on elect...Marko Kovic
Note: This presentation was given ath the 69th annual conference of the World Association of Public Opinion Research in Austin, Texas, on May 11, 2016.
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In this study, we analyze whether the mere volume of presence in mass media and the mere volume of activity on social media conveys advantages to candidates in parliamentary elections. Based on the theoretical model of bounded rationality, we call these potential effects \textit{brute force effects}. During the last month of the election campaign of the Swiss general election of 2015, we have tracked the presence of all 873 candidates from the canton of Zurich in a broad sample of mass media as well as their activity on Facebook and Twitter. The results of our multilevel Bayesian estimates show that neither direct activity on social media nor indirect resonance on social media has substantial effects. Mass media presence, in contrast, has consistent small, but substantial effects. Our results suggest that the brute force effect of mass media presence can have a tangible impact, but only a small one.
The document provides instructions and materials for a classroom lesson on the US election process. It includes directions for students to write party platforms, participate in a mock primary election, national convention, and general election. It also explains the roles and process for the electoral college in determining the winner. The lesson culminates in the announcement of election winners and an inauguration speech.
The document criticizes the media's reliance on and handling of political polls in several ways: it says polls are given too much attention over substantive issues; results are often oversimplified and not put in proper context; and polls can distort the election process and freeze out lesser known candidates. It also argues that polls are designed more to influence public opinion rather than objectively measure it.
The spotlight is on pollsters in the UK, following the performance of the polls at the 2015 General Election. Are we alone in facing this challenge, or is it a global issue? Does the experience in other countries point to what we should be doing in the UK?
Ipsos has many of the leading polling experts from around the world, and we brought them together in London to provide unique combined insight. Our panel members from the US, Canada, Italy and Sweden talked us through the role and challenges of polling in their countries and what we need to do to get it right. They also updated us on the political landscape of their countries, with outlines of the major elections they have recently had, and in the case of the US, the on-going race to the White House.
This document provides an overview of political parties in the United States. It discusses how the two-party system has evolved over time and compares it to party systems in other democracies. Key points covered include the decline in party identification among Americans; differences between the US and European party structures; the historical development and changing nature of political parties; and ongoing debates around reforming the two-party system.
Efficient algorithms for hard problems on structured electoratesNeeldhara Misra
This talk explores possibilities for exploiting structure in voting profiles to obtain efficient algorithms for problems that are computationally intractable in general.
We consider a natural variant of the well-known Feedback Vertex Set problem, namely the problem of deleting a small subset of vertices or edges to a full binary tree. This version of the problem is motivated by real-world scenarios that are best modeled by full binary trees. We establish that both versions of the problem are NP-hard, which stands in contrast to the fact that deleting edges to obtain a forest or a tree is equivalent to the problem of finding a minimum cost spanning tree, which can be solved in polynomial time. We also establish that both problems are FPT by the standard parameter.
Brute force effects of mass media presence and social media activity on elect...Marko Kovic
Note: This presentation was given ath the 69th annual conference of the World Association of Public Opinion Research in Austin, Texas, on May 11, 2016.
---
In this study, we analyze whether the mere volume of presence in mass media and the mere volume of activity on social media conveys advantages to candidates in parliamentary elections. Based on the theoretical model of bounded rationality, we call these potential effects \textit{brute force effects}. During the last month of the election campaign of the Swiss general election of 2015, we have tracked the presence of all 873 candidates from the canton of Zurich in a broad sample of mass media as well as their activity on Facebook and Twitter. The results of our multilevel Bayesian estimates show that neither direct activity on social media nor indirect resonance on social media has substantial effects. Mass media presence, in contrast, has consistent small, but substantial effects. Our results suggest that the brute force effect of mass media presence can have a tangible impact, but only a small one.
The document provides instructions and materials for a classroom lesson on the US election process. It includes directions for students to write party platforms, participate in a mock primary election, national convention, and general election. It also explains the roles and process for the electoral college in determining the winner. The lesson culminates in the announcement of election winners and an inauguration speech.
The document criticizes the media's reliance on and handling of political polls in several ways: it says polls are given too much attention over substantive issues; results are often oversimplified and not put in proper context; and polls can distort the election process and freeze out lesser known candidates. It also argues that polls are designed more to influence public opinion rather than objectively measure it.
The spotlight is on pollsters in the UK, following the performance of the polls at the 2015 General Election. Are we alone in facing this challenge, or is it a global issue? Does the experience in other countries point to what we should be doing in the UK?
Ipsos has many of the leading polling experts from around the world, and we brought them together in London to provide unique combined insight. Our panel members from the US, Canada, Italy and Sweden talked us through the role and challenges of polling in their countries and what we need to do to get it right. They also updated us on the political landscape of their countries, with outlines of the major elections they have recently had, and in the case of the US, the on-going race to the White House.
This document provides an overview of political parties in the United States. It discusses how the two-party system has evolved over time and compares it to party systems in other democracies. Key points covered include the decline in party identification among Americans; differences between the US and European party structures; the historical development and changing nature of political parties; and ongoing debates around reforming the two-party system.
Efficient algorithms for hard problems on structured electoratesNeeldhara Misra
This talk explores possibilities for exploiting structure in voting profiles to obtain efficient algorithms for problems that are computationally intractable in general.
We consider a natural variant of the well-known Feedback Vertex Set problem, namely the problem of deleting a small subset of vertices or edges to a full binary tree. This version of the problem is motivated by real-world scenarios that are best modeled by full binary trees. We establish that both versions of the problem are NP-hard, which stands in contrast to the fact that deleting edges to obtain a forest or a tree is equivalent to the problem of finding a minimum cost spanning tree, which can be solved in polynomial time. We also establish that both problems are FPT by the standard parameter.
Elicitation for Preferences Single Peaked on Trees Neeldhara Misra
This talk will focus on the problem of preference elicitation, where the goal is to understand the preferences of agents (which we model by total orders) by querying them about their pairwise preferences. We will survey known results, which have studied the problem both on general domains and structured ones, such as the domain of single-peaked preferences. As one might expect, structured domains admit a lower query complexity. We will consider domains that are single peaked over trees, which generalize the notion of single-peakedness.
The document presents algorithms for finding the largest induced q-colorable subgraph of a given graph G. It first describes a randomized algorithm that runs in time proportional to enumerating maximal independent sets and a polynomial in n and q. For perfect graphs, where maximum independent sets can be found efficiently, it gives a deterministic algorithm running in similar time. It also shows that the problem does not admit a polynomial kernel when parameterized by the solution size for split and perfect graphs under standard assumptions.
The document describes research into the maximum edge coloring problem, which involves coloring the edges of a graph such that each vertex sees at most two colors. The goal is to maximize the number of colors used. The problem is known to be NP-complete. The authors present a fixed-parameter tractable algorithm that runs in time O*(20k) by reducing the problem into smaller subproblems involving color palettes, vertex covers, and independent sets. They also discuss some open problems regarding improving the running time and determining whether the problem admits a polynomial kernel.
This document discusses reasons for pursuing research in computer science, including the challenges, joys, and mindset required. It addresses circumstances around research, fascination with problems, eureka moments versus dull periods, the importance of persistence and breadth versus depth. It provides advice on coming to terms with limitations, the social aspects of research, balancing theory and practice, and having other interests besides work. Overall, the document presents research as rewarding but requiring hard work.
This document provides an overview of techniques for solving hard computational problems. It discusses the complexity classes P, NP, and NP-complete, and provides examples of NP-complete problems like the travelling salesman problem. The document then discusses heuristic approaches like approximation and randomized algorithms. It also discusses exploiting additional structure in problem inputs and parameterized/exact analysis. Finally, it provides an example of using vertex cover techniques like degree bounds to solve the vertex cover problem in polynomial time for certain cases.
The document discusses matchings in graphs and the Erdos-Ko-Rado (EKR) theorem. It introduces Baranyai partitions, which is a decomposition of the edges of a complete bipartite graph K2n into (2n-1) perfect matchings. Considering cyclic permutations of the edges within each perfect matching partition provides a way to set up "Katona-like local environments" to prove bounds on intersecting families of matchings, in analogy to Katona's proof technique for intersecting families of sets.
The document discusses connected separators and 2-connected separators in graphs. It presents the treewidth reduction theorem, which shows that the 2-connected separator problem can be solved by finding an equivalent instance on a graph of small treewidth. It also discusses properties of 2-connected Steiner trees, including that the non-terminal vertices induce a forest, and presents an algorithm that guesses and maps the structure of the 2-connected Steiner tree.
The document describes a generic algorithm for the F-deletion problem, where the goal is to remove at most k vertices from a graph such that the remaining graph does not contain graphs from F as minors. It shows that when F contains only planar graphs, the algorithm provides a constant-factor approximation. It analyzes special cases where the algorithm works with different constants, such as when the graph minus the solution is independent, a matching, or acyclic. It then discusses how the algorithm extends to more general graphs by exploiting that the graph minus solution must have bounded treewidth when F contains planar graphs.
A Kernel for Planar F-deletion: The Connected CaseNeeldhara Misra
The document discusses polynomial kernels for planar F-deletion problems. It presents an algorithm that works by guessing the existence of protrusions and either reducing them or inferring irrelevant edges. If every guess finds an irrelevant edge, those edges can safely be removed from the graph. The algorithm aims to obtain a graph with constant treewidth by repeatedly guessing and reducing protrusions or deleting irrelevant edges. This leads to a polynomial kernel for certain cases of planar F-deletion.
Kernels for Planar F-Deletion (Restricted Variants)Neeldhara Misra
The document discusses kernelization for the F-deletion problem, where graphs in F are connected and at least one is planar. It is shown that the planar F-deletion problem admits a polynomial kernel whenever F contains a planar graph called the "onion" graph. Several other positive and negative results are also presented, including that planar F-deletion admits an approximation algorithm and a polynomial kernel on claw-free graphs. The document concludes by outlining the ingredients for showing that planar F-deletion admits a polynomial kernel.
Efficient Simplification: The (im)possibilitiesNeeldhara Misra
The document discusses techniques for simplifying problems, including kernelization procedures. It proposes definitions for what constitutes a good simplification procedure and kernelization procedure. A kernelization procedure takes an input of size n and parameter k and maps it to an equivalent instance of size only g(k) in polynomial time, where g is some computable function. This implies the problem is fixed-parameter tractable. The document also discusses how some NP-complete problems may still admit efficient simplification procedures when restricted to instances with certain properties, like bounded degree graphs.
This document discusses the kernelization complexity of finding colorful motifs in graphs. It introduces colorful motifs as a problem with applications in bioinformatics. It shows the problem is NP-complete even on very simple graph classes from the kernelization perspective. It presents an observation that leads to many polynomial kernels in a special case of comb graphs, but notes this does not generalize. It also provides NP-hardness results and observations ruling out polynomial kernels for more general graph classes and problems.
The document discusses q-expansions and their applications to problems like vertex cover and feedback vertex set. It introduces the q-expansion lemma, which states that if the neighborhood of a set S is at least q times the size of S, then there exist q matchings saturating S that are disjoint in the neighborhood. This lemma is then used to obtain polynomial kernelizations for problems like vertex cover and feedback vertex set by finding a high-degree vertex v and using q-expansions to find a small hitting set that does not contain v. The technique can be generalized to finding solutions for graphs excluding a fixed minor H by using q-expansions to find a small set avoiding a high degree vertex v.
The document discusses kernelization procedures for parameterized problems. It begins by defining kernelization as a polynomial-time preprocessing function that maps an input instance to an equivalent, compressed instance whose size depends only on the parameter. It then proves that a problem admits a kernel (can be kernelized) if and only if it is fixed-parameter tractable. Specifically, a kernel implies an FPT algorithm, and an FPT runtime implies the existence of a kernel. The document advocates for polynomial-sized kernels as the most efficient type of kernelization.
The document discusses connected dominating sets and short cycles. It begins by explaining that excluding longer cycles makes related problems easier to solve. Specifically, it shows that on graphs with girth at least five, high degree vertices must be in any minimum dominating set. However, this does not hold for connected dominating sets, since connectivity must also be maintained. It then describes how to obtain fixed-parameter tractable algorithms for connected dominating set problems by guessing the minimum dominating set and extending it. It also shows that these problems do not admit polynomial kernels by providing a reduction from Fair Connected Colors, which is W-hard.
Compositions of iron-meteorite parent bodies constrainthe structure of the pr...Sérgio Sacani
Magmatic iron-meteorite parent bodies are the earliest planetesimals in the Solar System,and they preserve information about conditions and planet-forming processes in thesolar nebula. In this study, we include comprehensive elemental compositions andfractional-crystallization modeling for iron meteorites from the cores of five differenti-ated asteroids from the inner Solar System. Together with previous results of metalliccores from the outer Solar System, we conclude that asteroidal cores from the outerSolar System have smaller sizes, elevated siderophile-element abundances, and simplercrystallization processes than those from the inner Solar System. These differences arerelated to the formation locations of the parent asteroids because the solar protoplane-tary disk varied in redox conditions, elemental distributions, and dynamics at differentheliocentric distances. Using highly siderophile-element data from iron meteorites, wereconstruct the distribution of calcium-aluminum-rich inclusions (CAIs) across theprotoplanetary disk within the first million years of Solar-System history. CAIs, the firstsolids to condense in the Solar System, formed close to the Sun. They were, however,concentrated within the outer disk and depleted within the inner disk. Future modelsof the structure and evolution of the protoplanetary disk should account for this dis-tribution pattern of CAIs.
SDSS1335+0728: The awakening of a ∼ 106M⊙ black hole⋆Sérgio Sacani
Context. The early-type galaxy SDSS J133519.91+072807.4 (hereafter SDSS1335+0728), which had exhibited no prior optical variations during the preceding two decades, began showing significant nuclear variability in the Zwicky Transient Facility (ZTF) alert stream from December 2019 (as ZTF19acnskyy). This variability behaviour, coupled with the host-galaxy properties, suggests that SDSS1335+0728 hosts a ∼ 106M⊙ black hole (BH) that is currently in the process of ‘turning on’. Aims. We present a multi-wavelength photometric analysis and spectroscopic follow-up performed with the aim of better understanding the origin of the nuclear variations detected in SDSS1335+0728. Methods. We used archival photometry (from WISE, 2MASS, SDSS, GALEX, eROSITA) and spectroscopic data (from SDSS and LAMOST) to study the state of SDSS1335+0728 prior to December 2019, and new observations from Swift, SOAR/Goodman, VLT/X-shooter, and Keck/LRIS taken after its turn-on to characterise its current state. We analysed the variability of SDSS1335+0728 in the X-ray/UV/optical/mid-infrared range, modelled its spectral energy distribution prior to and after December 2019, and studied the evolution of its UV/optical spectra. Results. From our multi-wavelength photometric analysis, we find that: (a) since 2021, the UV flux (from Swift/UVOT observations) is four times brighter than the flux reported by GALEX in 2004; (b) since June 2022, the mid-infrared flux has risen more than two times, and the W1−W2 WISE colour has become redder; and (c) since February 2024, the source has begun showing X-ray emission. From our spectroscopic follow-up, we see that (i) the narrow emission line ratios are now consistent with a more energetic ionising continuum; (ii) broad emission lines are not detected; and (iii) the [OIII] line increased its flux ∼ 3.6 years after the first ZTF alert, which implies a relatively compact narrow-line-emitting region. Conclusions. We conclude that the variations observed in SDSS1335+0728 could be either explained by a ∼ 106M⊙ AGN that is just turning on or by an exotic tidal disruption event (TDE). If the former is true, SDSS1335+0728 is one of the strongest cases of an AGNobserved in the process of activating. If the latter were found to be the case, it would correspond to the longest and faintest TDE ever observed (or another class of still unknown nuclear transient). Future observations of SDSS1335+0728 are crucial to further understand its behaviour. Key words. galaxies: active– accretion, accretion discs– galaxies: individual: SDSS J133519.91+072807.4
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...Sérgio Sacani
Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation
Elicitation for Preferences Single Peaked on Trees Neeldhara Misra
This talk will focus on the problem of preference elicitation, where the goal is to understand the preferences of agents (which we model by total orders) by querying them about their pairwise preferences. We will survey known results, which have studied the problem both on general domains and structured ones, such as the domain of single-peaked preferences. As one might expect, structured domains admit a lower query complexity. We will consider domains that are single peaked over trees, which generalize the notion of single-peakedness.
The document presents algorithms for finding the largest induced q-colorable subgraph of a given graph G. It first describes a randomized algorithm that runs in time proportional to enumerating maximal independent sets and a polynomial in n and q. For perfect graphs, where maximum independent sets can be found efficiently, it gives a deterministic algorithm running in similar time. It also shows that the problem does not admit a polynomial kernel when parameterized by the solution size for split and perfect graphs under standard assumptions.
The document describes research into the maximum edge coloring problem, which involves coloring the edges of a graph such that each vertex sees at most two colors. The goal is to maximize the number of colors used. The problem is known to be NP-complete. The authors present a fixed-parameter tractable algorithm that runs in time O*(20k) by reducing the problem into smaller subproblems involving color palettes, vertex covers, and independent sets. They also discuss some open problems regarding improving the running time and determining whether the problem admits a polynomial kernel.
This document discusses reasons for pursuing research in computer science, including the challenges, joys, and mindset required. It addresses circumstances around research, fascination with problems, eureka moments versus dull periods, the importance of persistence and breadth versus depth. It provides advice on coming to terms with limitations, the social aspects of research, balancing theory and practice, and having other interests besides work. Overall, the document presents research as rewarding but requiring hard work.
This document provides an overview of techniques for solving hard computational problems. It discusses the complexity classes P, NP, and NP-complete, and provides examples of NP-complete problems like the travelling salesman problem. The document then discusses heuristic approaches like approximation and randomized algorithms. It also discusses exploiting additional structure in problem inputs and parameterized/exact analysis. Finally, it provides an example of using vertex cover techniques like degree bounds to solve the vertex cover problem in polynomial time for certain cases.
The document discusses matchings in graphs and the Erdos-Ko-Rado (EKR) theorem. It introduces Baranyai partitions, which is a decomposition of the edges of a complete bipartite graph K2n into (2n-1) perfect matchings. Considering cyclic permutations of the edges within each perfect matching partition provides a way to set up "Katona-like local environments" to prove bounds on intersecting families of matchings, in analogy to Katona's proof technique for intersecting families of sets.
The document discusses connected separators and 2-connected separators in graphs. It presents the treewidth reduction theorem, which shows that the 2-connected separator problem can be solved by finding an equivalent instance on a graph of small treewidth. It also discusses properties of 2-connected Steiner trees, including that the non-terminal vertices induce a forest, and presents an algorithm that guesses and maps the structure of the 2-connected Steiner tree.
The document describes a generic algorithm for the F-deletion problem, where the goal is to remove at most k vertices from a graph such that the remaining graph does not contain graphs from F as minors. It shows that when F contains only planar graphs, the algorithm provides a constant-factor approximation. It analyzes special cases where the algorithm works with different constants, such as when the graph minus the solution is independent, a matching, or acyclic. It then discusses how the algorithm extends to more general graphs by exploiting that the graph minus solution must have bounded treewidth when F contains planar graphs.
A Kernel for Planar F-deletion: The Connected CaseNeeldhara Misra
The document discusses polynomial kernels for planar F-deletion problems. It presents an algorithm that works by guessing the existence of protrusions and either reducing them or inferring irrelevant edges. If every guess finds an irrelevant edge, those edges can safely be removed from the graph. The algorithm aims to obtain a graph with constant treewidth by repeatedly guessing and reducing protrusions or deleting irrelevant edges. This leads to a polynomial kernel for certain cases of planar F-deletion.
Kernels for Planar F-Deletion (Restricted Variants)Neeldhara Misra
The document discusses kernelization for the F-deletion problem, where graphs in F are connected and at least one is planar. It is shown that the planar F-deletion problem admits a polynomial kernel whenever F contains a planar graph called the "onion" graph. Several other positive and negative results are also presented, including that planar F-deletion admits an approximation algorithm and a polynomial kernel on claw-free graphs. The document concludes by outlining the ingredients for showing that planar F-deletion admits a polynomial kernel.
Efficient Simplification: The (im)possibilitiesNeeldhara Misra
The document discusses techniques for simplifying problems, including kernelization procedures. It proposes definitions for what constitutes a good simplification procedure and kernelization procedure. A kernelization procedure takes an input of size n and parameter k and maps it to an equivalent instance of size only g(k) in polynomial time, where g is some computable function. This implies the problem is fixed-parameter tractable. The document also discusses how some NP-complete problems may still admit efficient simplification procedures when restricted to instances with certain properties, like bounded degree graphs.
This document discusses the kernelization complexity of finding colorful motifs in graphs. It introduces colorful motifs as a problem with applications in bioinformatics. It shows the problem is NP-complete even on very simple graph classes from the kernelization perspective. It presents an observation that leads to many polynomial kernels in a special case of comb graphs, but notes this does not generalize. It also provides NP-hardness results and observations ruling out polynomial kernels for more general graph classes and problems.
The document discusses q-expansions and their applications to problems like vertex cover and feedback vertex set. It introduces the q-expansion lemma, which states that if the neighborhood of a set S is at least q times the size of S, then there exist q matchings saturating S that are disjoint in the neighborhood. This lemma is then used to obtain polynomial kernelizations for problems like vertex cover and feedback vertex set by finding a high-degree vertex v and using q-expansions to find a small hitting set that does not contain v. The technique can be generalized to finding solutions for graphs excluding a fixed minor H by using q-expansions to find a small set avoiding a high degree vertex v.
The document discusses kernelization procedures for parameterized problems. It begins by defining kernelization as a polynomial-time preprocessing function that maps an input instance to an equivalent, compressed instance whose size depends only on the parameter. It then proves that a problem admits a kernel (can be kernelized) if and only if it is fixed-parameter tractable. Specifically, a kernel implies an FPT algorithm, and an FPT runtime implies the existence of a kernel. The document advocates for polynomial-sized kernels as the most efficient type of kernelization.
The document discusses connected dominating sets and short cycles. It begins by explaining that excluding longer cycles makes related problems easier to solve. Specifically, it shows that on graphs with girth at least five, high degree vertices must be in any minimum dominating set. However, this does not hold for connected dominating sets, since connectivity must also be maintained. It then describes how to obtain fixed-parameter tractable algorithms for connected dominating set problems by guessing the minimum dominating set and extending it. It also shows that these problems do not admit polynomial kernels by providing a reduction from Fair Connected Colors, which is W-hard.
Compositions of iron-meteorite parent bodies constrainthe structure of the pr...Sérgio Sacani
Magmatic iron-meteorite parent bodies are the earliest planetesimals in the Solar System,and they preserve information about conditions and planet-forming processes in thesolar nebula. In this study, we include comprehensive elemental compositions andfractional-crystallization modeling for iron meteorites from the cores of five differenti-ated asteroids from the inner Solar System. Together with previous results of metalliccores from the outer Solar System, we conclude that asteroidal cores from the outerSolar System have smaller sizes, elevated siderophile-element abundances, and simplercrystallization processes than those from the inner Solar System. These differences arerelated to the formation locations of the parent asteroids because the solar protoplane-tary disk varied in redox conditions, elemental distributions, and dynamics at differentheliocentric distances. Using highly siderophile-element data from iron meteorites, wereconstruct the distribution of calcium-aluminum-rich inclusions (CAIs) across theprotoplanetary disk within the first million years of Solar-System history. CAIs, the firstsolids to condense in the Solar System, formed close to the Sun. They were, however,concentrated within the outer disk and depleted within the inner disk. Future modelsof the structure and evolution of the protoplanetary disk should account for this dis-tribution pattern of CAIs.
SDSS1335+0728: The awakening of a ∼ 106M⊙ black hole⋆Sérgio Sacani
Context. The early-type galaxy SDSS J133519.91+072807.4 (hereafter SDSS1335+0728), which had exhibited no prior optical variations during the preceding two decades, began showing significant nuclear variability in the Zwicky Transient Facility (ZTF) alert stream from December 2019 (as ZTF19acnskyy). This variability behaviour, coupled with the host-galaxy properties, suggests that SDSS1335+0728 hosts a ∼ 106M⊙ black hole (BH) that is currently in the process of ‘turning on’. Aims. We present a multi-wavelength photometric analysis and spectroscopic follow-up performed with the aim of better understanding the origin of the nuclear variations detected in SDSS1335+0728. Methods. We used archival photometry (from WISE, 2MASS, SDSS, GALEX, eROSITA) and spectroscopic data (from SDSS and LAMOST) to study the state of SDSS1335+0728 prior to December 2019, and new observations from Swift, SOAR/Goodman, VLT/X-shooter, and Keck/LRIS taken after its turn-on to characterise its current state. We analysed the variability of SDSS1335+0728 in the X-ray/UV/optical/mid-infrared range, modelled its spectral energy distribution prior to and after December 2019, and studied the evolution of its UV/optical spectra. Results. From our multi-wavelength photometric analysis, we find that: (a) since 2021, the UV flux (from Swift/UVOT observations) is four times brighter than the flux reported by GALEX in 2004; (b) since June 2022, the mid-infrared flux has risen more than two times, and the W1−W2 WISE colour has become redder; and (c) since February 2024, the source has begun showing X-ray emission. From our spectroscopic follow-up, we see that (i) the narrow emission line ratios are now consistent with a more energetic ionising continuum; (ii) broad emission lines are not detected; and (iii) the [OIII] line increased its flux ∼ 3.6 years after the first ZTF alert, which implies a relatively compact narrow-line-emitting region. Conclusions. We conclude that the variations observed in SDSS1335+0728 could be either explained by a ∼ 106M⊙ AGN that is just turning on or by an exotic tidal disruption event (TDE). If the former is true, SDSS1335+0728 is one of the strongest cases of an AGNobserved in the process of activating. If the latter were found to be the case, it would correspond to the longest and faintest TDE ever observed (or another class of still unknown nuclear transient). Future observations of SDSS1335+0728 are crucial to further understand its behaviour. Key words. galaxies: active– accretion, accretion discs– galaxies: individual: SDSS J133519.91+072807.4
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...Sérgio Sacani
Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation
Discovery of An Apparent Red, High-Velocity Type Ia Supernova at 𝐳 = 2.9 wi...Sérgio Sacani
We present the JWST discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS
+
53.13485
−
27.82088
with a host spectroscopic redshift of
2.903
±
0.007
. The transient was identified in deep James Webb Space Telescope (JWST)/NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) program. Photometric and spectroscopic followup with NIRCam and NIRSpec, respectively, confirm the redshift and yield UV-NIR light-curve, NIR color, and spectroscopic information all consistent with a Type Ia classification. Despite its classification as a likely SN Ia, SN 2023adsy is both fairly red (
�
(
�
−
�
)
∼
0.9
) despite a host galaxy with low-extinction and has a high Ca II velocity (
19
,
000
±
2
,
000
km/s) compared to the general population of SNe Ia. While these characteristics are consistent with some Ca-rich SNe Ia, particularly SN 2016hnk, SN 2023adsy is intrinsically brighter than the low-
�
Ca-rich population. Although such an object is too red for any low-
�
cosmological sample, we apply a fiducial standardization approach to SN 2023adsy and find that the SN 2023adsy luminosity distance measurement is in excellent agreement (
≲
1
�
) with
Λ
CDM. Therefore unlike low-
�
Ca-rich SNe Ia, SN 2023adsy is standardizable and gives no indication that SN Ia standardized luminosities change significantly with redshift. A larger sample of distant SNe Ia is required to determine if SN Ia population characteristics at high-
�
truly diverge from their low-
�
counterparts, and to confirm that standardized luminosities nevertheless remain constant with redshift.
The cost of acquiring information by natural selectionCarl Bergstrom
This is a short talk that I gave at the Banff International Research Station workshop on Modeling and Theory in Population Biology. The idea is to try to understand how the burden of natural selection relates to the amount of information that selection puts into the genome.
It's based on the first part of this research paper:
The cost of information acquisition by natural selection
Ryan Seamus McGee, Olivia Kosterlitz, Artem Kaznatcheev, Benjamin Kerr, Carl T. Bergstrom
bioRxiv 2022.07.02.498577; doi: https://doi.org/10.1101/2022.07.02.498577
Mechanisms and Applications of Antiviral Neutralizing Antibodies - Creative B...Creative-Biolabs
Neutralizing antibodies, pivotal in immune defense, specifically bind and inhibit viral pathogens, thereby playing a crucial role in protecting against and mitigating infectious diseases. In this slide, we will introduce what antibodies and neutralizing antibodies are, the production and regulation of neutralizing antibodies, their mechanisms of action, classification and applications, as well as the challenges they face.
Signatures of wave erosion in Titan’s coastsSérgio Sacani
The shorelines of Titan’s hydrocarbon seas trace flooded erosional landforms such as river valleys; however, it isunclear whether coastal erosion has subsequently altered these shorelines. Spacecraft observations and theo-retical models suggest that wind may cause waves to form on Titan’s seas, potentially driving coastal erosion,but the observational evidence of waves is indirect, and the processes affecting shoreline evolution on Titanremain unknown. No widely accepted framework exists for using shoreline morphology to quantitatively dis-cern coastal erosion mechanisms, even on Earth, where the dominant mechanisms are known. We combinelandscape evolution models with measurements of shoreline shape on Earth to characterize how differentcoastal erosion mechanisms affect shoreline morphology. Applying this framework to Titan, we find that theshorelines of Titan’s seas are most consistent with flooded landscapes that subsequently have been eroded bywaves, rather than a uniform erosional process or no coastal erosion, particularly if wave growth saturates atfetch lengths of tens of kilometers.
PPT on Sustainable Land Management presented at the three-day 'Training and Validation Workshop on Modules of Climate Smart Agriculture (CSA) Technologies in South Asia' workshop on April 22, 2024.
On the Parameterized Complexity of Party Nominations
1. Neeldhara Misra, IIT Gandhinagar
Dominik Peters, Carnegie-Mellon University
2019 Conference on
Algorithmic Decision Theory
Parameterized Complexity of Party Nominations
9. AB
C P
R
X
Z
S
T
Votes
B C A S P Q YZ TRX
Candidates
Every party nominates a candidate.
Q
Y
The votes are “projected” on the nominees.
10. AB
C P
R
X
Z
S
T
Votes
B C A S P Q YZ TRX
Candidates
Every party nominates a candidate.
Q
Y
The winner is declared based on the plurality voting rule.
18. If we know who the other parties are nominating,
it is easy to “evaluate” a candidate in our party.
Plurality
19. If we know who the other parties are nominating,
it is easy to “evaluate” a candidate in our party.
Plurality
20. If we know who the other parties are nominating,
it is easy to “evaluate” a candidate in our party.
Plurality
21. Plurality
If we know who the other parties are nominating,
it is easy to “evaluate” a candidate in our party.
22. A more natural scenario
We have no idea who the other nominees are.
23. A more natural scenario
We have no idea who the other nominees are.
The Optimist’s Question
Do we have a superstar candidate who ensures a party win,
irrespective of who is nominated from the other parties?
24. A more natural scenario
We have no idea who the other nominees are.
The Optimist’s Question
Do we have a superstar candidate who ensures a party win,
irrespective of who is nominated from the other parties?
The Pessimist’s Question
Do we have a promising candidate who makes the party win
in at least one of the many possible parallel universes?
25. A more natural scenario
We have no idea who the other nominees are.
Do we have a superstar candidate who ensures a party win,
irrespective of who is nominated from the other parties?
The Pessimist’s Question
Do we have a promising candidate who makes the party win
in at least one of the many possible parallel universes?
Necessary President
26. A more natural scenario
We have no idea who the other nominees are.
Do we have a superstar candidate who ensures a party win,
irrespective of who is nominated from the other parties?
Do we have a promising candidate who makes the party win
in at least one of the many possible parallel universes?
Necessary President
Possible President
27. Known Results
Do we have a superstar candidate who ensures a party win,
irrespective of who is nominated from the other parties?
Necessary President
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
28. Known Results
Do we have a superstar candidate who ensures a party win,
irrespective of who is nominated from the other parties?
Necessary President
co-NP complete even when the size of the largest party is two.
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
29. Known Results
Do we have a superstar candidate who ensures a party win,
irrespective of who is nominated from the other parties?
Necessary President
co-NP complete even when the size of the largest party is two.
polynomial-time when the profiles are single-peaked.
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
30. Known Results
Possible President
Do we have a promising candidate who makes the party win
in at least one of the many possible parallel universes?
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
31. Known Results
Possible President
Do we have a promising candidate who makes the party win
in at least one of the many possible parallel universes?
NP-complete even when the size of the largest party is two.
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
32. Known Results
Possible President
Do we have a promising candidate who makes the party win
in at least one of the many possible parallel universes?
NP-complete even when the size of the largest party is two.
NP-complete also when the profiles are 1D-Euclidean.
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
33. Known Results
Possible President
Do we have a promising candidate who makes the party win
in at least one of the many possible parallel universes?
NP-complete even when the size of the largest party is two.
NP-complete also when the profiles are 1D-Euclidean.
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
(a subclass of single-peaked & single-crossing profiles)
36. Possible President
NP-complete also when the profiles are 1D-Euclidean.
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
Our Contributions
NP-complete even when the size of the largest party is two.
37. Possible President
NP-complete even when the size of the largest party is two,
Our Contributions
NP-complete also when the profiles are 1D-Euclidean.and the
38. Possible President
NP-complete even when the size of the largest party is two,
Our Contributions
NP-complete also when the profiles are 1D-Euclidean.
(A stronger hardness result.)
and the
39. Possible President
NP-complete even when the size of the largest party is two,
Our Contributions
NP-complete also when the profiles are 1D-Euclidean.
(A stronger hardness result.)
and the
XP and W[2]-hard parameterized by the number of parties.
40. Possible President
NP-complete even when the size of the largest party is two,
Our Contributions
NP-complete also when the profiles are 1D-Euclidean.
(A stronger hardness result.)
and the
XP and W[2]-hard parameterized by the number of parties.
FPT parameterized by number of parties on 1D-Euclidean profiles.
41. Possible President
NP-complete even when the size of the largest party is two,
Our Contributions
NP-complete also when the profiles are 1D-Euclidean.
(A stronger hardness result.)
and the
XP and W[2]-hard parameterized by the number of parties.
FPT parameterized by number of parties on 1D-Euclidean profiles.
(Parameterized Results)
43. Necessary President
Our Contributions
co-NP complete even when the size of the largest party is two.
polynomial-time when the profiles are single-peaked.
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
44. Necessary President
Our Contributions
co-NP complete even when the size of the largest party is two.
polynomial-time when the profiles are single-peaked.
Piotr Faliszewski, Laurent Gourvès, Jérôme Lang, Julien Lesca, Jèrôme Monnot.
How hard is it for a party to nominate an election winner? AAAI 2016
polynomial-time when the profiles are single-crossing.
47. The Parameterized Paradigm
Beyond Worst-Case
Classical complexity: measure the performance of an algorithm
as a function of the input size.
48. Parameterized complexity: acknowledge the presence of additional structure,
which manifests as a secondary measurement — a parameter.
The Parameterized Paradigm
Beyond Worst-Case
49. Parameterized complexity: acknowledge the presence of additional structure,
which manifests as a secondary measurement — a parameter.
🎯 Design algorithms that restrict the combinatorial explosion
to a function of the parameter.
The Parameterized Paradigm
Beyond Worst-Case
50. Parameterized complexity: acknowledge the presence of additional structure,
which manifests as a secondary measurement — a parameter.
🎯 Design algorithms that restrict the combinatorial explosion
to a function of the parameter.
The Parameterized Paradigm
Beyond Worst-Case
f(k)p(n)
Input size
Parameter
fixed-parameter tractability
51. ⚠ W-hardness: a framework for arguing the
likely non-existence of FPT algorithms
for parameterized problems
The Parameterized Paradigm
Beyond Worst-Case
f(k)p(n)
Input size
Parameter
fixed-parameter tractability
52. ⚠ W-hardness: a framework for arguing the
likely non-existence of FPT algorithms
for parameterized problems
The Parameterized Paradigm
Beyond Worst-Case
😰
Hard
problem
X
FPT-Reductions
53. ⚠ W-hardness: a framework for arguing the
likely non-existence of FPT algorithms
for parameterized problems
The Parameterized Paradigm
Beyond Worst-Case
😰
Hard
problem
X
Runs in FPT time ● Preserves the parameter ● Maintains equivalence
FPT-Reductions
55. Possible President
High Level Methodology
XP and W[2]-hard parameterized by the number of parties.
FPT parameterized by number of parties on 1D-Euclidean profiles.
NP-complete even when the size of the largest party is two,
profiles are 1D-Euclidean.and the
56. Possible President
High Level Methodology
Reduction from “Linear” SAT aka LSAT
(a structured variation of SAT,
originally used in the context of geometric problems*)
NP-complete even when the size of the largest party is two,
profiles are 1D-Euclidean.and the
XP and W[2]-hard parameterized by the number of parties.
FPT parameterized by number of parties on 1D-Euclidean profiles.
* Esther M. Arkin, Aritra Banik, Paz Carmi, Gui Citovsky, Matthew J. Katz, Joseph S. B. Mitchell,
Marina Simakov. Choice is Hard, ISAAC 2015
57. Possible President
High Level Methodology
Brute-force
(guess the nominee from each party)
XP and W[2]-hard parameterized by the number of parties.
FPT parameterized by number of parties on 1D-Euclidean profiles.
NP-complete even when the size of the largest party is two,
profiles are 1D-Euclidean.and the
58. Possible President
High Level Methodology
FPT-reduction
(from a variant of Dominating Set,
also coming up in this talk)
XP and W[2]-hard parameterized by the number of parties.
FPT parameterized by number of parties on 1D-Euclidean profiles.
NP-complete even when the size of the largest party is two,
profiles are 1D-Euclidean.and the
59. Possible President
High Level Methodology
Dynamic Programming
(updates along the 1D-Euclidean axis,
also appeals to “SP and SC aspects” of 1D-Euclidean profiles)
XP and W[2]-hard parameterized by the number of parties.
FPT parameterized by number of parties on 1D-Euclidean profiles.
NP-complete even when the size of the largest party is two,
profiles are 1D-Euclidean.and the
60. Possible President
High Level Methodology
XP and W[2]-hard parameterized by the number of parties.
FPT parameterized by number of parties on 1D-Euclidean profiles.
Necessary President
polynomial-time when the profiles are single-crossing.
NP-complete even when the size of the largest party is two,
profiles are 1D-Euclidean.and the
61. Possible President
High Level Methodology
XP and W[2]-hard parameterized by the number of parties.
FPT parameterized by number of parties on 1D-Euclidean profiles.
Necessary President
polynomial-time when the profiles are single-crossing.
Adversarial approach: guess a nominee + a rival candidate
(use a “block property” and reduce to a structured Hitting Set instance)
NP-complete even when the size of the largest party is two,
profiles are 1D-Euclidean.and the
70. W[2]-hardness of Possible President
(parameterized by #parties)
Introduce a candidate for every red vertex;
and two special candidates p and q.
71. W[2]-hardness of Possible President
(parameterized by #parties)
Introduce a candidate for every red vertex;
and two special candidates p and q.
Parties. p,q are singletons.
The other parties correspond to color classes of the CRBDS instance.
72. Introduce a vote for every blue vertex with the ordering:
neighbours
non-neighbours
W[2]-hardness of Possible President
(parameterized by #parties)
74. Also introduce n copies of two special votes:
W[2]-hardness of Possible President
(parameterized by #parties)
75. Also introduce n copies of two special votes:
W[2]-hardness of Possible President
(parameterized by #parties)
76. Also introduce n copies of two special votes:
W[2]-hardness of Possible President
(parameterized by #parties)
Ask if p is a possible president.
77. Also introduce n copies of two special votes:
W[2]-hardness of Possible President
(parameterized by #parties)
Ask if p is a possible president.
Answer: Yes if and only if the “other nominees”
correspond to a colourful red-blue dominating set.
78. Also introduce n copies of two special votes:
W[2]-hardness of Possible President
(parameterized by #parties)
Ask if p is a possible president.
To begin with, p and q tie at a score of n each.
p’s score is “locked in” at n.
Nominees from a dominating set
“block” q from acquiring any additional score.
80. Parameterized complexity when
parameterized by the number of voters?
Open Problems
🤔
Is Possible President parameterized by the number of parties FPT
on single-peaked or single-crossing domains?
81. Open Problems
🤔
Intermediate notions of incomplete information.
What if we have partial information about the other nominees,
served either in a stochastic fashion or
as a fixed fraction of the number of parties?