We requested observation time from the 0.9m WIYN telescope to be in coincidence with VERITAS observations of the three blazars. Time was allocated in the period ...
1. WIYN One Degree Imager. 2. Filter Changer. 3. Demonstration Filters ... IO is new to the filter business, but has a lot of experience with complex and ...
Photometric Determination of Binary Mass Ratios in the WIYN Open Cluster Study ... we suspect that rapid rotation restricts us to masses less than a few M ...
... radiation ionizes part of H I tail Change in accretion launches expanding gas ring from nucleus. ... parts Dramatic drop in ionizing radiation, nucleus ...
M86 has very weak radio source, so AGN heating of ISM unlikely at present. Although extreme case, ISM easy to study in M86: should teach us about general ...
Persistent and Transient Blank Field Sources A. Treves Insubria University, Italy S. Campana Brera Observatory, Italy M. Chieregato Insubria University, Italy ...
WD accretes H-rich material from its low-mass, Roche-lobe filling companion ... Not many CVs known in globular/open clusters. Only 3 CVs known in all open clusters! ...
Why do they appear in groups sometimes? What can they tell us ... What still confuses us? Details, details... ( Sigh.) e.g. how to calibrate luminosities, etc? ...
or at least the ejection process is strongly influenced by ... Hydra spectrograph, 2002-04. Dispersion 0.33 A/pix; resolution ~7500. RV precision ~3-3.7 km/s ...
map. ALMA Workshop UMD. Margaret Meixner (STScI) 14 May 2004. The Sun: Quiet component: ... ALMA Workshop UMD. Margaret Meixner (STScI) 14 May 2004. NGC 7027 ...
We have requested suggestions for membership from members of ... Gemini Aspen instruments need $7M/year (US share) LSST Design & Development (already funded) ...
Mt. Palomar Observatory - CA. With the increasing light pollution from Los Angeles, Mount Wilson ... Mt. Palomar Dome (1) This dome houses the famous 200 inch ...
Image Deconvolution Applied to CCD astronomical images with astrometric purposes Maria Teresa Merino Espasa Universidad de Barcelona (Spain) Summary Introduction to ...
Bowling Green State University. Variable Stars 2004, BGSU, April 3. Et al... Brad Boswell ... m-M = 5 log d - 5 Av. Reddening maps iffy near Galactic Plane. ...
... Spirals in Ursa Major and Canes Venatici: Global Properties. Kwayera Davis (College of Charleston) Advisor: Eric Wilcots (University of Wisconsin-Madison) ...
Determine any relationships between the amount of star formation and the color of the galaxy. ... HII regions fluoresce in the H . HII Regions & Star Formation ...
Characterized by very soft emission - no flux at energies 1 keV ... Unerstanding whether they are the 'single degenerate' progenitors of type Ia SN is crucial ...
OPTIC is the prototype OTCCD camera. OPTIC contains two ... Asteroid FC5 2003. V~17, Both are 200 sec exposures. S/N ~6 times higher. High Speed (Video) Mode ...
HI Column Densities (DLAs and sub-DLAs) Kinematics. Element Abundances. Model Implications ... IRTF K-band imaging of DLA and sub-DLA fields at z 1. Strong MgII ...
M33 (3 fields) Phoenix. IC 10 IC 1613. NGC 6822 Sextans A. WLM Sextans B. How Are We Doing? ... Phoenix. WLM. What's Next? Spectroscopy! M31. N206 in M31. ob78 ...
... in order to provide uided correction for the ODI camera ... SU Investment Club. September 2003 May 2004. SU Ambassadors. September 2003 May 2004 ...
Anomalous Cosmic Rays (ACR) Radio emissions. Inferred complications. Inner/Outer heliosheaths ... No evidence of local generation of Anomalous Cosmic Rays (ACRs) ...
The survey data consists of imaging and spectroscopy of ~2500 elliptical within ... Thus is expected to increase over time as a result of the merging process. ...
R 17 mag 'NOT' already in one of the official optical target lists for 6dFGS ... Visually matched by 3 people to minimise galaxy selection bias. Results ...
The Imaging Chain for Optical Astronomy Review/overview The imaging chain typically includes the following elements: energy source object collection detection ...
The Chandra Multi-wavelength Project (ChaMP) PIs: Paul Green & Belinda Wilkes X-ray: Dong-Woo Kim Imaging: Rob Cameron, Wayne Barkhouse Spectroscopy: John Silverman
Dark matter cusps in galaxy centers, in particular absent in ... dynamical friction and smooth any cusp. in dwarf galaxies. The material is more dissipative, ...
Bruzual and Charlot (2003) single burst stellar population evolutionary model. H ... is reasonable; there are no large bursts of star formation at the time of ...
In astronomy, the source of energy (1) and the object (2) are almost always ... tertiary mirror to redirect light to external instruments (e.g., a spectrograph) ...