# S. Chatterjee - Cornell Uni

## Contact Details

NameS. Chatterjee |
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AffiliationCornell Uni |
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CityIrvine |
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CountryUnited States |
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## Pubs By Year |
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## External Links |
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## Pub CategoriesHigh Energy Astrophysical Phenomena (10) Solar and Stellar Astrophysics (5) Instrumentation and Methods for Astrophysics (5) Cosmology and Nongalactic Astrophysics (5) High Energy Physics - Phenomenology (4) Physics - Materials Science (4) Physics - Strongly Correlated Electrons (4) Quantum Physics (4) Physics - Statistical Mechanics (3) High Energy Physics - Theory (3) Astrophysics of Galaxies (3) Computer Science - Computer Vision and Pattern Recognition (3) Quantitative Biology - Quantitative Methods (2) Statistics - Applications (2) Physics - Chemical Physics (2) Statistics - Theory (2) Physics - Instrumentation and Detectors (2) Physics - Biological Physics (2) High Energy Physics - Experiment (2) Mathematics - Statistics (2) Computer Science - Information Theory (1) Statistics - Machine Learning (1) General Relativity and Quantum Cosmology (1) Statistics - Methodology (1) Computer Science - Human-Computer Interaction (1) Mathematics - Information Theory (1) Nonlinear Sciences - Adaptation and Self-Organizing Systems (1) Nuclear Experiment (1) Nuclear Theory (1) Physics - Superconductivity (1) Nonlinear Sciences - Chaotic Dynamics (1) Mathematical Physics (1) Mathematics - Probability (1) Mathematics - Mathematical Physics (1) |

## Publications Authored By S. Chatterjee

**Authors:**C. J. Law

^{1}, M. W. Abruzzo

^{2}, C. G. Bassa

^{3}, G. C. Bower

^{4}, S. Burke-Spolaor

^{5}, B. J. Butler

^{6}, T. Cantwell

^{7}, S. H. Carey

^{8}, S. Chatterjee

^{9}, J. M. Cordes

^{10}, P. Demorest

^{11}, J. Dowell

^{12}, R. Fender

^{13}, K. Gourdji

^{14}, K. Grainge

^{15}, J. W. T. Hessels

^{16}, J. Hickish

^{17}, V. M. Kaspi

^{18}, T. J. W. Lazio

^{19}, M. A. McLaughlin

^{20}, D. Michilli

^{21}, K. Mooley

^{22}, Y. C. Perrott

^{23}, S. M. Ransom

^{24}, N. Razavi-Ghods

^{25}, M. Rupen

^{26}, A. Scaife

^{27}, P. Scott

^{28}, P. Scholz

^{29}, A. Seymour

^{30}, L. G. Spitler

^{31}, K. Stovall

^{32}, S. P. Tendulkar

^{33}, D. Titterington

^{34}, R. S. Wharton

^{35}, P. K. G. Williams

^{36}

**Affiliations:**

^{1}UC Berkeley,

^{2}Haverford College,

^{3}ASTRON,

^{4}ASIA-A,

^{5}NRAO-Socorro,

^{6}NRAO-Socorro,

^{7}JBCA,

^{8}Cambridge,

^{9}Cornell,

^{10}Cornell,

^{11}NRAO-Socorro,

^{12}UNM,

^{13}Oxford,

^{14}Amsterdam,

^{15}JBCA,

^{16}ASTRON,

^{17}UC Berkeley,

^{18}McGill,

^{19}JPL,

^{20}WVU,

^{21}ASTRON,

^{22}Oxford,

^{23}Cambridge,

^{24}NRAO-Charlottesville,

^{25}Cambridge,

^{26}DRAO,

^{27}JBCA,

^{28}Cambridge,

^{29}DRAO,

^{30}Arecibo,

^{31}MPIfR,

^{32}NRAO-Socorro,

^{33}McGill,

^{34}Cambridge,

^{35}Cornell,

^{36}Harvard-Smithsonian CfA

**Category:**High Energy Astrophysical Phenomena

We present results of the coordinated observing campaign that made the first subarcsecond localization of a Fast Radio Burst, FRB 121102. During this campaign, we made the first simultaneous detection of an FRB burst by multiple telescopes: the VLA at 3 GHz and the Arecibo Observatory at 1.4 GHz. Read More

**Authors:**C. G. Bassa

^{1}, S. P. Tendulkar

^{2}, E. A. K. Adams

^{3}, N. Maddox

^{4}, S. Bogdanov

^{5}, G. C. Bower

^{6}, S. Burke-Spolaor

^{7}, B. J. Butler

^{8}, S. Chatterjee

^{9}, J. M. Cordes

^{10}, J. W. T. Hessels

^{11}, V. M. Kaspi

^{12}, C. J. Law

^{13}, B. Marcote

^{14}, Z. Paragi

^{15}, S. M. Ransom

^{16}, P. Scholz

^{17}, L. G. Spitler

^{18}, H. J. van Langevelde

^{19}

**Affiliations:**

^{1}ASTRON,

^{2}McGill,

^{3}ASTRON,

^{4}ASTRON,

^{5}Columbia,

^{6}ASIAA,

^{7}NRAO/WVU,

^{8}NRAO,

^{9}Cornell,

^{10}Cornell,

^{11}ASTRON/Amsterdam,

^{12}McGill,

^{13}Berkeley,

^{14}JIVE,

^{15}JIVE,

^{16}NRAO,

^{17}DRAO,

^{18}MPIfR,

^{19}JIVE/Leiden

**Category:**High Energy Astrophysical Phenomena

We present optical, near- and mid-infrared imaging of the host galaxy of FRB 121102 with the Gemini North telescope, the Hubble Space Telescope and the Spitzer Space Telescope. The FRB 121102 host galaxy is resolved, revealing a bright star forming region located in the outskirts of the irregular, low-metallicity dwarf galaxy. The star forming region has a half-light radius of 0. Read More

**Authors:**P. Scholz, S. Bogdanov, J. W. T. Hessels, R. S. Lynch, L. G. Spitler, C. G. Bassa, G. C. Bower, S. Burke-Spolaor, B. J. Butler, S. Chatterjee, J. M. Cordes, K. Gourdji, V. M. Kaspi, C. J. Law, B. Marcote, M. A. McLaughlin, D. Michilli, Z. Paragi, S. M. Ransom, A. Seymour, S. P. Tendulkar, R. S. Wharton

**Category:**High Energy Astrophysical Phenomena

We undertook coordinated campaigns with the Green Bank, Effelsberg, and Arecibo radio telescopes during Chandra X-ray Observatory and XMM-Newton observations of the repeating fast radio burst FRB 121102 in late 2016 and early 2017 to search for simultaneous radio and X-ray bursts. We find 12 radio bursts from FRB 121102 during these 70 ks total of X-ray observations. We detect no X-ray photons at the times of radio bursts from FRB 121102 and further detect no X-ray bursts above the measured background at any time. Read More

We classify quantum states proximate to the semiclassical N\'eel state of the spin $S=1/2$ square lattice antiferromagnet with two-spin near-neighbor and four-spin ring exchange interactions. Motivated by a number of recent experiments on the cuprates and the iridates, we examine states with $\mathbb{Z}_2$ topological order, an order which is not present in the semiclassical limit. Some of the states break one or more of reflection, time-reversal, and lattice rotation symmetries, and can account for the observations. Read More

We prove that the bound-state momentum-space wave function $\phi(p)$ for the quasi-one-dimensional hydrogen atom as used by Olendski in two recent publications (Eur. J. Phys. Read More

The century-long (1907-2007) Ca II K spectroheliograms from Kodaikanal Solar Observatory, India, has recently been digitised and calibrated. Applying a fully-automated algorithm (which includes contrast enhancement and 'Watershed method') on this data, we have identified the supergranules and calculated the associated parameters, such as scale, circularity, fractal dimension. We have segregated the quiet and active regions and obtained the supergranule parameters separately for these two domains. Read More

Current 3$\nu$ global fits predict two degenerate solutions for $\theta_{23}$: one lies in lower octant ($\theta_{23} <\pi/4$), and the other belongs to higher octant ($\theta_{23} >\pi/4$). Here, we study how the measurement of $\theta_{23}$ octant would be affected in the upcoming Deep Underground Neutrino Experiment (DUNE) if there exist a light eV-scale sterile neutrino. We show that in 3+1 scheme, a new interference term in $\nu_\mu \to \nu_e$ oscillation probability can spoil the chances of measuring $\theta_{23}$ octant completely. Read More

We consider the "searching for a trail in a maze" composite hypothesis testing problem, in which one attempts to detect an anomalous directed path in a lattice 2D box of side n based on observations on the nodes of the box. Under the signal hypothesis, one observes independent Gaussian variables of unit variance at all nodes, with zero, mean off the anomalous path and mean \mu_n on it. Under the null hypothesis, one observes i. Read More

We study a coupled driven system in which two species of particles are advected by a fluctuating potential energy landscape. While the particles follow the potential gradient, each species affects the local shape of the landscape in different ways. As a result of this two-way coupling between the landscape and the particles, the system shows new interesting phases, characterized by different sorts of long ranged order in the particles and in the landscape. Read More

We study the dynamical properties of the ordered phases obtained in a coupled nonequilibrium system describing advection of two species of particles by a stochastically evolving landscape. The local dynamics of the landscape also gets affected by the particles. In a companion paper we have presented static properties of different phases that arise as the two-way coupling parameters are varied. Read More

We describe a tunable low-energy photon source consisting of a laser-driven xenon plasma lamp coupled to a Czerny-Turner monochromator. The combined tunability, brightness, and narrow spectral bandwidth make this light source useful in laboratory-based high-resolution photoemission spectroscopy experiments. The source supplies photons with energies up to ~7 eV, delivering under typical conditions >10^12 ph/s within a 10 meV spectral bandwidth, which is comparable to helium plasma lamps and many synchrotron beamlines. Read More

We investigate pseudorapidity correlations of the average transverse flow of particles emitted in relativistic heavy-ion collisions. We employ 3+1 dimensional viscous relativistic hydrodynamics with initial conditions from the quark Glauber Monte Carlo model to confront the recent measurements on the pseudorapidity correlations of the transverse momentum fluctuations in Pb+Pb collisions at $\sqrt{s_{NN}}=2760$GeV. We find good agreement between the model predictions and data. Read More

We study thermal and electrical transport in metals and superconductors near a quantum phase transition where antiferromagnetic order disappears. The same theory can also be applied to quantum phase transitions involving the loss of certain classes of intrinsic topological order. For a clean superconductor, we recover and extend the well-known universal results. Read More

This contribution reports an application of MultiFractal Detrended Fluctuation Analysis, MFDFA based novel feature extraction technique for automated detection of epilepsy. In fractal geometry, Multifractal Detrended Fluctuation Analysis MFDFA is a popular technique to examine the self-similarity of a nonlinear, chaotic and noisy time series. In the present research work, EEG signals representing healthy, interictal (seizure free) and ictal activities (seizure) are acquired from an existing available database. Read More

Sub-subgiants are a new class of stars that are optically redder than normal main-sequence stars and fainter than normal subgiant stars. Sub-subgiants, and the possibly related red stragglers (which fall to the red of the giant branch), occupy a region of the color-magnitude diagram that is predicted to be devoid of stars by standard stellar evolution theory. In previous papers we presented the observed demographics of these sources and defined possible theoretical formation channels through isolated binary evolution, the rapid stripping of a subgiant's envelope, and stellar collisions. Read More

Plasma lenses in the host galaxies of fast radio bursts (FRBs) can strongly modulate FRB amplitudes for a wide range of distances, including the $\sim $ Gpc distance of the repeater FRB121102. To produce caustics, the lens' dispersion-measure depth (${\rm DM}_{\ell}$), scale size ($a$), and distance from the source ($d_{\rm sl}$) must satisfy ${\rm DM}_{\ell} d_{\rm sl} / a^2 \gtrsim 0.65~ {\rm pc^2 \ AU^{-2} \ cm^{-3}}$. Read More

**Authors:**Kate D. Alexander

^{1}, Edo Berger

^{2}, Geoff Bower

^{3}, Sarah Casewell

^{4}, S. Brad Cenko

^{5}, Shami Chatterjee

^{6}, Ilse Cleeves

^{7}, Jim Cordes

^{8}, Jeremy Drake

^{9}, Maria Drout

^{10}, Trent Dupuy

^{11}, Tarraneh Eftekhari

^{12}, Giovanni Fazio

^{13}, Wen-fai Fong

^{14}, James Guillochon

^{15}, Mark Gurwell

^{16}, Michael Johnson

^{17}, Tomasz Kaminski

^{18}, Albert Kong

^{19}, Tanmoy Laskar

^{20}, Casey Law

^{21}, Stuart P. Littlefair

^{22}, Meredith MacGregor

^{23}, W. Peter Maksym

^{24}, Lynn Matthews

^{25}, Michael McCollough

^{26}, Stefanie Milam

^{27}, Arielle Moullet

^{28}, Matt Nicholl

^{29}, Aaron Rizzuto

^{30}, Barry Rothberg

^{31}, Andrew Seymour

^{32}, Eric Villard

^{33}, Belinda Wilkes

^{34}, Peter K. G. Williams

^{35}, Steven Willner

^{36}, Farhad Yusuf-Zadeh

^{37}

**Affiliations:**

^{1}ALMA Time-domain Special Interest Group,

^{2}ALMA Time-domain Special Interest Group,

^{3}ALMA Time-domain Special Interest Group,

^{4}ALMA Time-domain Special Interest Group,

^{5}ALMA Time-domain Special Interest Group,

^{6}ALMA Time-domain Special Interest Group,

^{7}ALMA Time-domain Special Interest Group,

^{8}ALMA Time-domain Special Interest Group,

^{9}ALMA Time-domain Special Interest Group,

^{10}ALMA Time-domain Special Interest Group,

^{11}ALMA Time-domain Special Interest Group,

^{12}ALMA Time-domain Special Interest Group,

^{13}ALMA Time-domain Special Interest Group,

^{14}ALMA Time-domain Special Interest Group,

^{15}ALMA Time-domain Special Interest Group,

^{16}ALMA Time-domain Special Interest Group,

^{17}ALMA Time-domain Special Interest Group,

^{18}ALMA Time-domain Special Interest Group,

^{19}ALMA Time-domain Special Interest Group,

^{20}ALMA Time-domain Special Interest Group,

^{21}ALMA Time-domain Special Interest Group,

^{22}ALMA Time-domain Special Interest Group,

^{23}ALMA Time-domain Special Interest Group,

^{24}ALMA Time-domain Special Interest Group,

^{25}ALMA Time-domain Special Interest Group,

^{26}ALMA Time-domain Special Interest Group,

^{27}ALMA Time-domain Special Interest Group,

^{28}ALMA Time-domain Special Interest Group,

^{29}ALMA Time-domain Special Interest Group,

^{30}ALMA Time-domain Special Interest Group,

^{31}ALMA Time-domain Special Interest Group,

^{32}ALMA Time-domain Special Interest Group,

^{33}ALMA Time-domain Special Interest Group,

^{34}ALMA Time-domain Special Interest Group,

^{35}ALMA Time-domain Special Interest Group,

^{36}ALMA Time-domain Special Interest Group,

^{37}ALMA Time-domain Special Interest Group

While the Atacama Large Millimeter/submillimeter Array (ALMA) is a uniquely powerful telescope, its impact in certain fields of astrophysics has been limited by observatory policies rather than the telescope's innate technical capabilities. In particular, several observatory policies present challenges for observations of variable, mobile, and/or transient sources --- collectively referred to here as "time-domain" observations. In this whitepaper we identify some of these policies, describe the scientific applications they impair, and suggest changes that would increase ALMA's science impact in Cycle 6 and beyond. Read More

The coordinate-space wave function $\psi(x)$ of quasi-one-dimensional atoms is defined in the $x\geq 0$ region only. This poses a typical problem to write a physically acceptable momentum-space wave function $\phi(p)$ from the Fourier transform of $\psi(x)$. We resolve the problem with special attention to the behavior of real and imaginary parts of the complex-valued function $\phi(p)$ as a function of $p$ and confirm that $\phi_i(p)$ (the imaginary part of $\phi(p)$) represents the correct momentum-space wave function. Read More

We make use of a Hylleraas-type wave function to derive an exact analytical model to quantify correlation in two-electron atomic/ionic systems and subsequently employ it to examine the role of inter-electronic repulsion in affecting (i) the bare (uncorrelated) single-particle position- and momentum-space charge distributions and (ii) corresponding Shannon's information entropies. The results presented for the first five members in the helium iso-electronic sequence, on the one hand, correctly demonstrate the effect of correlation on bare charge distributions and, on the other hand, lead us to some important results for the correlated and uncorrelated values of the entropies. These include the limiting behavior of the correlated entropy sum (sum of position- and momentum-space entropies) and geometrical realization for the variation of information entropies as a function of Z. Read More

Taking into account the current global information on neutrino oscillation parameters we forecast the capabilities of future long baseline experiments such as DUNE and T2HK in settling the atmospheric octant puzzle. We find that a good measurement of the reactor angle $\theta_{13}$ plays a key role in fixing the octant of the atmospheric angle $\theta_{23}$ with such future accelerator neutrino studies. Read More

The upcoming Ooty Wide Field Array (OWFA) will operate at $326.5 \, {\rm MHz}$ which corresponds to the redshifted 21-cm signal from neutral hydrogen (HI) at z = 3.35. Read More

Several analytic and numerical studies have indicated that the interstellar medium of a quasar host galaxy heated by feedback can contribute to a substantial secondary signal in the cosmic microwave background (CMB) through the thermal Sunyaev-Zel'dovich (SZ) effect. Recently, many groups have tried to detect this signal by cross-correlating CMB maps with quasar catalogs. Using a self-similar model for the gas in the intra-cluster medium and a realistic halo occupation distribution (HOD) prescription for quasars we estimate the level of SZ signal from gravitational heating of quasar hosts. Read More

Numerous experiments have reported discrete symmetry breaking in the high temperature pseudogap phase of the hole-doped cuprates, including breaking of one or more of lattice rotation, inversion, or time-reversal symmetries. In the absence of translational symmetry breaking or topological order, these conventional order parameters cannot explain the gap in the charged fermion excitation spectrum in the anti-nodal region. Zhao et al. Read More

The volume of data that will be produced by new-generation surveys requires automatic classification methods to select and analyze sources. Indeed, this is the case for the search for strong gravitational lenses, where the population of the detectable lensed sources is only a very small fraction of the full source population. In this paper, we present a morphological classification method for recognizing strong gravitational lenses. Read More

The poor contrast and the overlapping of cervical cell cytoplasm are the major issues in the accurate segmentation of cervical cell cytoplasm. This paper presents an automated unsupervised cytoplasm segmentation approach which can effectively find the cytoplasm boundaries in overlapping cells. The proposed approach first segments the cell clumps from the cervical smear image and detects the nuclei in each cell clump. Read More

We study trend filtering, a relatively recent method for univariate nonparametric regression. For a given integer $r \geq 1$, the trend filtering estimator of order $r$ is defined as the minimizer of the sum of squared errors when we constrain (or penalize) the sum of the absolute discrete derivatives of order $r$ over the input points. For $r = 1$, the estimator reduces to total variation regularization which has received much attention in the statistics and image processing literature. Read More

We perform realistic simulations of the current and future long baseline experiments such as T2K, NO$\nu$A, DUNE and T2HK in order to determine their ultimate potential in probing neutrino oscillation parameters. We quantify the potential of these experiments to underpin the octant of the atmospheric angle $\theta_{23}$ as well as the value and sign of the CP phase $\delta_{CP}$ Read More

In this work, we investigate the local and nonlocal broadcasting of entanglement and correlations in more general sense for the general two-qubit mixed state using asymmetric Pauli cloners. Interestingly, we claim that non-optimal broadcasting of entanglement is not different from optimal broadcasting using asymmetric cloners. Surprisingly, this is exactly opposite to the behaviour for geometric discord, a measure of correlation beyond entanglement. Read More

This study examines the presence of the day-of-the-week effect on daily returns of biotechnology stocks over a 16-year period from January 2002 to December 2015. Using daily returns from the NASDAQ Biotechnology Index (NBI), we find that the stock returns were the lowest on Mondays, and compared to the Mondays the stock returns were significantly higher on Wednesdays, Thursdays, and Fridays. Moreover, the results from using the asymmetric GARCH processes reveal that momentum and small-firm effect were positively associated with the market risk-adjusted returns of the biotechnology stocks during this period. Read More

**Authors:**S. Chatterjee, C. J. Law, R. S. Wharton, S. Burke-Spolaor, J. W. T. Hessels, G. C. Bower, J. M. Cordes, S. P. Tendulkar, C. G. Bassa, P. Demorest, B. J. Butler, A. Seymour, P. Scholz, M. W. Abruzzo, S. Bogdanov, V. M. Kaspi, A. Keimpema, T. J. W. Lazio, B. Marcote, M. A. McLaughlin, Z. Paragi, S. M. Ransom, M. Rupen, L. G. Spitler, H. J. van Langevelde

Fast radio bursts are astronomical radio flashes of unknown physical nature with durations of milliseconds. Their dispersive arrival times suggest an extragalactic origin and imply radio luminosities orders of magnitude larger than any other kind of known short-duration radio transient. Thus far, all FRBs have been detected with large single-dish telescopes with arcminute localizations, and attempts to identify their counterparts (source or host galaxy) have relied on contemporaneous variability of field sources or the presence of peculiar field stars or galaxies. Read More

**Authors:**B. Marcote

^{1}, Z. Paragi

^{2}, J. W. T. Hessels

^{3}, A. Keimpema

^{4}, H. J. van Langevelde

^{5}, Y. Huang

^{6}, C. G. Bassa

^{7}, S. Bogdanov

^{8}, G. C. Bower

^{9}, S. Burke-Spolaor

^{10}, B. J. Butler

^{11}, R. M. Campbell

^{12}, S. Chatterjee

^{13}, J. M. Cordes

^{14}, P. Demorest

^{15}, M. A. Garrett

^{16}, T. Ghosh

^{17}, V. M. Kaspi

^{18}, C. J. Law

^{19}, T. J. W. Lazio

^{20}, M. A. McLaughlin

^{21}, S. M. Ransom

^{22}, C. J. Salter

^{23}, P. Scholz

^{24}, A. Seymour

^{25}, A. Siemion

^{26}, L. G. Spitler

^{27}, S. P. Tendulkar

^{28}, R. S. Wharton

^{29}

**Affiliations:**

^{1}JIVE,

^{2}JIVE,

^{3}ASTRON,

^{4}JIVE,

^{5}JIVE,

^{6}Carleton College,

^{7}ASTRON,

^{8}Columbia U,

^{9}ASIAA,

^{10}NRAO Socorro,

^{11}NRAO Socorro,

^{12}JIVE,

^{13}Cornell U,

^{14}Cornell U,

^{15}NRAO Socorro,

^{16}U. of Manchester,

^{17}NAIC Arecibo,

^{18}McGill U,

^{19}UC Berkeley,

^{20}NASA JPL,

^{21}U. of West Virginia Dept. of Physics and Astronomy,

^{22}NRAO CV,

^{23}NAIC Arecibo,

^{24}DRAO,

^{25}NAIC Arecibo,

^{26}UC Berkeley,

^{27}MPIfR,

^{28}McGill U,

^{29}Cornell U

The millisecond-duration radio flashes known as Fast Radio Bursts (FRBs) represent an enigmatic astrophysical phenomenon. Recently, the sub-arcsecond localization (~ 100mas precision) of FRB121102 using the VLA has led to its unambiguous association with persistent radio and optical counterparts, and to the identification of its host galaxy. However, an even more precise localization is needed in order to probe the direct physical relationship between the millisecond bursts themselves and the associated persistent emission. Read More

**Authors:**Shriharsh P. Tendulkar

^{1}, Cees Bassa

^{2}, James M. Cordes

^{3}, Geoffery C. Bower

^{4}, Casey J. Law

^{5}, Shamibrata Chatterjee

^{6}, Elizabeth A. K. Adams

^{7}, Slavko Bogdanov

^{8}, Sarah Burke-Spolaor

^{9}, Bryan J. Butler

^{10}, Paul Demorest

^{11}, Jason W. T. Hessels

^{12}, Victoria M. Kaspi

^{13}, T. Joseph W. Lazio

^{14}, Natasha Maddox

^{15}, Benito Marcote

^{16}, Maura A. McLaughlin

^{17}, Zsolt Paragi

^{18}, Scott M. Ransom

^{19}, Paul Scholz

^{20}, Andrew Seymour

^{21}, Laura G. Spitler

^{22}, Huib J. van Langevelde

^{23}, Robert S. Wharton

^{24}

**Affiliations:**

^{1}McGill U.,

^{2}ASTRON,

^{3}Cornell U.,

^{4}ASIAA,

^{5}UC Berkeley,

^{6}Cornell U.,

^{7}ASTRON,

^{8}Columbia U.,

^{9}NRAO, WVU,

^{10}NRAO,

^{11}NRAO,

^{12}ASTRON, API,

^{13}McGill U.,

^{14}JPL,

^{15}ASTRON,

^{16}JIVE,

^{17}WVU,

^{18}JIVE,

^{19}NRAO,

^{20}DRAO,

^{21}Arecibo,

^{22}MPIfR,

^{23}JIVE, Leiden,

^{24}Cornell U.

The precise localization of the repeating fast radio burst (FRB 121102) has provided the first unambiguous association (chance coincidence probability $p\lesssim3\times10^{-4}$) of an FRB with an optical and persistent radio counterpart. We report on optical imaging and spectroscopy of the counterpart and find that it is an extended ($0.6^{\prime\prime}-0. Read More

**Affiliations:**

^{1}Dept. of Astronomy, University of Florida,

^{2}Dept. of Astronomy, University of Florida,

^{3}CIERA, Northwestern University

We investigate the formation and early evolution of star clusters assuming that they form from a turbulent starless clump of given mass bounded inside a parent self-gravitating molecular cloud characterized by a particular mass surface density. As a first step we assume instantaneous star cluster formation and gas expulsion. We draw our initial conditions from observed properties of starless clumps. Read More

Plages are the magnetically active chromospheric structures prominently visible in Ca $\scriptsize{{\textrm{II}}}$ K line (3933.67 \r{A}). A plage may or may not be associated with a sunspot which is a magnetic structure visible in the solar photosphere. Read More

Electron transfer (ET) in molecular donor-acceptor dye systems is crucial for charge transport in organic semiconductors. Classically, ET rates should decrease with increasing donor-acceptor distance while the microscopic mechanism is more complex and shows intricate dependencies on the excitation conditions. In this paper, we introduce highly soluble N,N'-dialkyl perylene dihydrazides (PDH) - perylene dyes with a dialkylamino -NR$_2$ donor functionality directly bonded to both of their imide nitrogen atoms. Read More

Carrier multiplication by singlet exciton fission enhances photovoltaic conversion efficiencies in organic solids. This decay of one singlet exciton into two triplet states promises to overcome the Shockley-Queisser limit as up to two electrons may be harvested per absorbed photon. Intermolecular coupling is deemed mandatory for both, singlet exciton fission and a band-like transport. Read More

Probabilistic models of directed polymers in random environment have received considerable attention in recent years. Much of this attention has focused on integrable models. In this paper, we introduce some new computational tools that do not require integrability. Read More

The great majority of electronic and optoelectronic devices depends on interfaces between n-type and p-type semiconductors. Finding such matching donor-acceptor systems in molecular crystals remains a challenging endeavor. Structurally compatible molecules may not necessarily be suitable with respect to their optical and electronic properties: large exciton binding energies may favor bound electron-hole pairs rather than charge separation by exciton dissociation, and free, band-like transport is challenging to achieve as hopping commonly dominates charge motion. Read More

**Authors:**M. L. Jones, M. A. McLaughlin, M. T. Lam, J. M. Cordes, L. Levin, S. Chatterjee, Z. Arzoumanian, K. Crowter, P. B. Demorest, T. Dolch, J. A. Ellis, R. D. Ferdman, E. Fonseca, M. E. Gonzalez, G. Jones, T. J. W. Lazio, D. J. Nice, T. T. Pennucci, S. M. Ransom, D. R. Stinebring, I. H. Stairs, K. Stovall, J. K. Swiggum, W. W. Zhu

**Category:**High Energy Astrophysical Phenomena

We analyze dispersion measure (DM) variations of 37 millisecond pulsars in the 9-year NANOGrav data release and constrain the sources of these variations. Variations are significant for nearly all pulsars, with characteristic timescales comparable to or even shorter than the average spacing between observations. Five pulsars have periodic annual variations, 14 pulsars have monotonically increasing or decreasing trends, and 13 pulsars show both effects. Read More

Plant electrical signals often contains low frequency drifts with or without the application of external stimuli. Quantification of the randomness in plant signals in a stimulus-specific way is hindered because the knowledge of vital frequency information in the actual biological response is not known yet. Here we design an optimum Infinite Impulse Response (IIR) filter which removes the low frequency drifts and preserves the frequency spectrum corresponding to the random component of the unstimulated plant signals by bringing the bias due to unknown artifacts and drifts to a minimum. Read More

Plants sense their environment by producing electrical signals which in essence represent changes in underlying physiological processes. These electrical signals, when monitored, show both stochastic and deterministic dynamics. In this paper, we compute 11 statistical features from the raw non-stationary plant electrical signal time series to classify the stimulus applied (causing the electrical signal). Read More

The study of solar active longitudes has generated a great interest in the recent years. In this work we have used an unique continuous sunspot data series obtained from Kodaikanal observatory and revisited the problem. Analysis of the data shows a persistent presence of the active longitude during the whole 90 years of data duration. Read More

We propose Hilbert transform (HT) and analytic signal (AS) construction for signals over graphs. This is motivated by the popularity of HT, AS, and modulation analysis in conventional signal processing, and the observation that complementary insight is often obtained by viewing conventional signals in the graph setting. Our definitions of HT and AS use a conjugate-symmetry-like property exhibited by the graph Fourier transform (GFT). Read More

In pulsar timing, timing residuals are the differences between the observed times of arrival and the predictions from the timing model. A comprehensive timing model will produce featureless residuals, which are presumably composed of dominating noise and weak physical effects excluded from the timing model (e.g. Read More

Cluster analysis has become one of the most exercised research areas over the past few decades in computer science. As a consequence, numerous clustering algorithms have already been developed to find appropriate partitions of a set of objects. Given multiple such clustering solutions, it is a challenging task to obtain an ensemble of these solutions. Read More

We propose a new class of nonconvex penalty functions in the paradigm of multitask sparse penalized regression that are based on data depth-based inverse ranking. Focusing on a one-step sparse estimator of the coefficient matrix using local linear approximation of the penalty function, we derive its theoretical properties and provide the algorithm for its computation. For orthogonal design and independent responses, the resulting thresholding rule enjoys near-minimax optimal risk performance, similar to the adaptive lasso (Zou, 2006). Read More

We report here the magneto-transport properties of the newly synthesized Heusler compound Cr2NiGa which crystallizes in a disordered cubic B2 structure belonging to Pm-3m space group. The sample is found to be paramagnetic down to 2 K with metallic character. On application of magnetic field, a significantly large increase in resistivity is observed which corresponds to magnetoresistance as high as 112% at 150 kOe of field at the lowest temperature. Read More

It is well known that Kasner geometry with spacelike singularity can be extended to bulk AdS-like geometry, furthermore one can study field theory on this Kasner space via its gravity dual. In this paper, we show that there exists a Kasner-like geometry with timelike singularity for which one can construct a dual gravity description. We then study various minimal surfaces including spacelike geodesics. Read More

**Authors:**M. T. Lam, J. M. Cordes, S. Chatterjee, Z. Arzoumanian, K. Crowter, P. B. Demorest, T. Dolch, J. A. Ellis, R. D. Ferdman, E. Fonseca, M. E. Gonzalez, G. Jones, M. L. Jones, L. Levin, D. R. Madison, M. A. McLaughlin, D. J. Nice, T. T. Pennucci, S. M. Ransom, R. M. Shannon, X. Siemens, I. H. Stairs, K. Stovall, J. K. Swiggum, W. W. Zhu

Gravitational wave astronomy using a pulsar timing array requires high-quality millisecond pulsars, correctable interstellar propagation delays, and high-precision measurements of pulse times of arrival. Here we identify noise in timing residuals that exceeds that predicted for arrival time estimation for millisecond pulsars observed by the North American Nanohertz Observatory for Gravitational Waves. We characterize the excess noise using variance and structure function analyses. Read More

The Galactic center has some of the highest stellar densities in the Galaxy and a range of interstellar scattering properties that may aid in the detection of new radio-selected transient events. Here we describe a search for radio transients in the Galactic center using over 200 hours of archival data from the Very Large Array (VLA) at 5 and 8.4 GHz. Read More