ASCA lightcurves of Source 2 in soft state. ASCA Observations of the two Ultra ... Kazuo Makishima(University of Tokyo), Tsunefumi Mizuno(Hiroshima University) ...
The Shape Model and Expected Phase Law for Mathilde. Small Body Lunch Talk. Jianyang Li ... of Shape on Lightcurves and Phase Functions. Small Body Lunch Talk ...
Wide-field, nearly-static science (Dark Energy) Near-Earth Asteroid search (NEA) ... Multicolor lightcurves of asteroids. Goals. Completeness as function of ...
Carnegie - M. Hamuy, S. Gonzalez, E. Persson, M. Roth, W. Freedman ... Y band at 1.035 m. Morphology of JHK lightcurves: Primary maxima occur a few days before ...
Exploration of the Universe Division, NASA Goddard Space Flight Center ... New software release OSA 5: more user friendly, more options, better responses, ...
Central Engines of Gamma-Ray Bursts & Supernovae S. R. Kulkarni California Institute of Technology http://www.astro.caltech.edu/~srk My summary of what we know about ...
An Introduction to X-ray Astronomy Keith Arnaud NASA Goddard University of Maryland X-ray Astronomy X-ray Processes X-rays from the Sun X-ray Binaries All-Sky Surveys ...
Modeling of type Ia supernovae. Simulation of radioactive ... Bruit ' extra noise ' : supprim par nouveau proc d . Mesur . Attendu. Objectif. Claire Juramy ...
Surveys monitor millions of stars for years to find rare lensing events ... 40 binary events, parallax, extended source, lensing of variable stars, etc. ...
... Simulations for GRB 041219a Polarisation with SPI GRB041219a Results IBIS Polarisation of GRB041219a Slide 14 Photoelectric Absorption - Theory Slide 16 ...
Observed variations in thermal flux in the submillimeter and mid ... that expected due to shape and albedo alone; evidence for variation in surface properties. ...
Not via multi-step accelerations, (in situ, Fermi 1, 2 , shock ... Rather by single-step sweeping via corotating magnetic fields, ... Post-cursors (offset by ...
Databases, software, etc. for X-ray astronomy Keith Arnaud NASA Goddard University of Maryland What I will cover Databases HEASARC Chandra Data Archive XMM Science ...
distance ladder: parallax, Cepheids, SuperNova Type Ia ... nearby stars with parallax (up to 1kpc) - nearby galaxies with variable stars (Cepheids) ...
Produces highest spatial resolution images. Also best time resolution (but be careful) ... High resolution spectroscopy on extended objects that are larger than 10 ...
Gamma-Ray Burst Early Afterglows. Bing Zhang. Physics Department. University of Nevada, Las Vegas ... gamma-ray. UV/opt/IR/radio. Why is the early afterglow ...
compatible with a cosmological constant, WL~0.7. SNe: ... Produces calibrated star catalogs in the CFHTLS Deep fields, in natural Megacam magnitudes. ...
... GRB models. Lecture 5: Black Hole Accretion Disk Models. Black Hole ... Future models and future observational missions. GRBs The Historical Perspective ...
... flare, moon, EGRET Unids ... It is clear that the moon is something that we are going to have ... the details of the impacts of choices made at the ...
Published Eros's photometric parameters (Domingue et al. 2002) 35th LPSC, ... Move Eros closer to the values of average S-type. Consistent with Eros spectrum ...
Lawrence Berkeley National Laboratory. The Super/Nova Acceleration Probe (SNAP) ... Lawrence Berkeley National Laboratory. Ancillary Science From SNAP. Galaxy ...
Colors & Reddening. Absolute magnitudes & Hubble diagram. SNe II ... Secondary maximum appears to have been significantly stronger than primary maximum! ...
Asteroids/satellites shine from reflected sunlight-- prop. ... shapes for irregular asteroids & satellites. ... Rocket body in geosynchronous transfer orbit: ...
High resolution spectroscopy by two gratings that can be placed in the optical ... highest spatial resolution images. Also best time resolution (but be careful) ...
Also many general catalogs and datasets held at other data centers (eg ... for HEASARC archival and current missions and for Chandra but not (alas) for XMM. ...
Implies 'zero' metallicity, where zero is the big bang abundance of elements 12C ... Photosphere is a massive, optically thick wind during eruption at 7000-9000 K ...
Getting Started with Kepler Kepler Science & Guest Observer Offices Steve Bryson Douglas Caldwell Jessie Christiansen Michael Fanelli Michael Haas Jon Jenkins
The misbehaving black hole candidate 4U 1630-47: a brief look at its outburst history ... during 1998 outburst. K - 16. Summary of outbursts since discovery in ...
FAST spectrograph. 3700 7500 . Recent upgrade to optics. Three or four spectra per night, ... Capability of Spectrograph. SN with R = 19.8 mag. Recent Examples ...
(Kulkarni et al. 1998; Li & Chevalier 1999) SN1998bw an engine-driven SN. Case 1: off-axis (0.5 ... (Li & Chevalier 1999) Energy. Density. Radius. Mass Loss ...
Scanning-free-automatized detection pipeline has been set up (shapelet-neural ... 250H/year of photo. Rencontre de Monriond 2006 SNLS 1st year cosmological results ...
Common superhumps shown by Whitehurst and several others to be the result of ... Bonnet-Bidaud, Motch, & Mouchet (1985) first to suggest the 5.2-hr period in TV ...
... (CVs) in the Hamburg Quasar Survey and Sloan Digital Sky ... Project to observe fainter CVs detected in Hamburg Quasar Survey, Sloan Digital Sky Survey etc ...