User profiles for L. Seco

Lucas F. Secco

- Verified email at uchicago.edu - Cited by 7297

Luis Seco

- Verified email at math.utoronto.ca - Cited by 1676

Margaret Loretta Secco

- Verified email at unb.ca - Cited by 1566

The essential spectrum of Neumann Laplacians on some bounded singular domains

R Hempel, LA Seco, B Simon - Journal of functional analysis, 1991 - Elsevier
… be the set of all functions in L*(Q) whose distributional gradients are in L, and we define -A:
via … (0, L) x (0, w) of fixed length L and width w 6 L, with two adjoining rectangles S, and S, of …

[PDF][PDF] On the energy of a large atom

CL Fefferman, LA Seco - 1990 - community.ams.org
We announce a proof of an asymptotic formula for the groundstate energy of a large atom.
The early work of Thomas-Fermi, Hartree-Fock, Dirac, and Scott predicted that for an atomic …

The electromagnetic counterpart of the binary neutron star merger LIGO/Virgo GW170817. II. UV, optical, and near-infrared light curves and comparison to kilonova …

…, M Sauseda, DJ Schlegel, LF Secco… - The Astrophysical …, 2017 - iopscience.iop.org
We present UV, optical, and near-infrared (NIR) photometry of the first electromagnetic
counterpart to a gravitational wave source from Advanced Laser Interferometer Gravitational-…

Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear

…, J Blazek, O Friedrich, S Samuroff, J Prat, LF Secco… - Physical Review D, 2018 - APS
We use 26× 10 6 galaxies from the Dark Energy Survey (DES) Year 1 shape catalogs over
1321 deg 2 of the sky to produce the most significant measurement of cosmic shear in a …

Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing

…, DS Cid, V Scarpine, M Schubnell, D Scolnic, LF Secco… - Physical Review D, 2022 - APS
We present the first cosmology results from large-scale structure using the full 5000 deg 2 of
imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis …

Living in a world of our own: The experience of parents who have a child with autism

RL Woodgate, C Ateah, L Secco - Qualitative health …, 2008 - journals.sagepub.com
In this article, we discuss findings of a hermeneutic phenomenological study that sought to
describe the experiences of parents who have a child with autism. Qualitative interviews were …

Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration

…, N MacCrann, S Dodelson, A Choi, C Doux, LF Secco… - Physical Review D, 2022 - APS
… The lightcones are run with the LGADGET2 N-body code, a memory optimized version of
GADGET2 [… in terms of the convergence power spectrum Cκ(l) at an angular wave number l as …

The electromagnetic counterpart of the binary neutron star merger LIGO/Virgo GW170817. I. Discovery of the optical counterpart using the dark energy camera

…, M Sauseda, DJ Schlegel, LF Secco… - The Astrophysical …, 2017 - iopscience.iop.org
We present the Dark Energy Camera (DECam) discovery of the optical counterpart of the first
binary neutron star merger detected through gravitational-wave emission, GW170817. Our …

Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty

LF Secco, S Samuroff, E Krause, B Jain, J Blazek… - Physical Review D, 2022 - APS
… Under the Limber approximation [112,113], the 2D convergence power spectrum in
tomographic bins i and j, C ij κ (l) is related to the full 3D matter power spectrum as: …

[PDF][PDF] Eigenvalues and eigenfunctions of ordinary differential operators

C Fefferman, L Seco - Advances in Mathematics, 1992 - core.ac.uk
… When V(x) is given by (l), our results are essentially as … Hence the successive terms uk (x)L
-’ decrease rapidly, … 9, modulo a high power of l/L With the integration constants picked in this …