output
19952026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 2002 · astro-phShow all

69 papers · 2 filters

astro-ph2002★ 32 cited

Active star formation in N11B Nebula in the Large Magellanic Cloud: a sequential star formation scenario confirmed

Rodolfo H. Barba, Monica Rubio, Miguel R. Roth +1

The second largest HII region in the Large Magellanic Cloud, N11B has been surveyed in the near IR.We present JHKs images of the N11B nebula.These images are combined with CO(1-0)…

astro-ph2002★ 28 cited

Radio-selected Galaxies in Very Rich Clusters at z < 0.25: I. Multi-wavelength Observations and Data Reduction Techniques

G. E. Morrison, F. N. Owen, M. J. Ledlow +4

Radio observations were used to detect the `active' galaxy population within rich clusters of galaxies in a non-biased manner that is not plagued by dust extinction or the K-correc…

astro-ph2002★ 49 cited

Discovery of a High-Redshift (z=0.96) Cluster of Galaxies Using a FIRST Wide-Angle Tailed Radio Source

Elizabeth L. Blanton, Michael D. Gregg, David J. Helfand +2

Using a combination of near-infrared and optical photometry, along with multi-object spectroscopy, we have confirmed the existence of a high-redshift cluster of galxies at z = 0.96…

astro-ph2002★ 41 cited

uvbyCaHbeta CCD Photometry of Clusters. III. The Most Metal-Rich Open Cluster, NGC 6253

B. A. Twarog, B. J. Anthony-Twarog, N. De Lee

CCD photometry on the intermediate-band uvbyCaH-beta system is presented for the old open cluster, NGC 6253. Despite a high level of field star contamination due to its location to…

astro-ph2002★ 197 cited

Weak Lensing Results from the 75 Square Degree CTIO Survey

M. Jarvis, G. Bernstein, B. Jain +4

We measure seeing-corrected ellipticities for 2 x 10^6 galaxies with magnitude R<23 in 12 widely separated fields totalling 75 deg^2 of sky. At angular scales >30\arcmin, elliptici…

astro-ph2002★ 69 cited

Superhumps in Cataclysmic Binaries. XXIII. V442 Ophiuchi and RX J1643.7+3402

Joseph Patterson, William Fenton, John Thorstensen +15

We report the results of long observing campaigns on two novalike variables: V442 Ophiuchi and RX J1643.7+3402. These stars have high-excitation spectra, complex line profiles sign…

astro-ph2002★ 49 cited

Massive Ellipticals at High Redshift: NICMOS Imaging of Z~1 Radio Galaxies

A. W. Zirm, M. Dickinson, A. Dey

We present deep, continuum images of eleven high-redshift (0.811 < z < 1.875) 3CR radio galaxies observed with NICMOS. Our images probe the rest-frame optical light where stars are…

astro-ph2002★ 75 cited

ISM Abundances in Sculptor Group Dwarf Irregular Galaxies

Evan D. Skillman, Stephanie Cote, Bryan W. Miller

Using the CTIO 4-m telescope, we have obtained optical spectra of HII regions in five Sculptor Group dwarf irregular galaxies. We derive oxygen, nitrogen, and sulfur abundances fro…

astro-ph2002★ 66 cited

The unusual optical afterglow of the gamma-ray burst GRB 021004: Color changes and short-time-scale variability

D. Bersier, K. Z. Stanek, J. Winn +11

We report UBVRI observations of the optical afterglow of the gamma-ray burst GRB 021004. We observed significant (10-20%) deviations from a power law decay on several time scales,…

astro-ph2002★ 175 cited

Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el

Kevin Krisciunas, Nicholas B. Suntzeff, Pablo Candia +8

We present well sampled optical (UBVRI) and infrared (JHK) light curves of the nearby (~18.0 Mpc) Type Ia supernova SN 2001el, from 11 days before to 142 days after the time of B-b…

astro-ph2002★ 30 cited

The Ringed Spiral Galaxy NGC 4622. I. Photometry, Kinematics, and the Case for Two Strong Leading Outer Spiral Arms

Ronald J. Buta, Gene G. Byrd, Tarsh Freeman

The intriguing nearly face-on southern ringed spiral galaxy NGC 4622, the first galaxy definitively shown to have leading spiral structure, is revisited in this paper with new imag…

astro-ph2002★ 203 cited

Spectroscopic Confirmation of Three Redshift 5.7 Lyman-alpha Emitters from the Large Area Lyman Alpha Survey

James E. Rhoads, Arjun Dey, Sangeeta Malhotra +5

Narrow-band searches for Lyman alpha emission are an efficient way of identifying star-forming galaxies at high redshifts. We present Keck telescope spectra confirming redshifts z…

astro-ph2002★ 18 cited

Confirmation of SBS 1150+599A As An Extremely Metal-Poor Planetary Nebula

George Jacoby, John Feldmeier, Charles F. Claver +4

SBS 1150+599A is a blue stellar object at high galactic latitude discovered in the Second Byurakan Survey. New high-resolution images of SBS 1150+599A are presented, demonstrating…

astro-ph2002★ 4 cited

The BTC40 Survey for Quasars at 4.8 < z < 6

E. M. Monier, J. D. Kennefick, P. B. Hall +4

The BTC40 Survey for high-redshift quasars is a multicolor search using images obtained with the Big Throughput Camera (BTC) on the CTIO 4-m telescope in V, I, and z filters to sea…

astro-ph2002★ 84 cited

A Young Blue Tidal Stream in NGC 5128

Eric W. Peng, Holland C. Ford, Kenneth C. Freeman +1

Stellar streams in galaxy halos are the natural consequence of a history of merging and accretion. We present evidence for a blue tidal stream of young stars in the nearest giant e…

astro-ph2002★ 295 cited

Structure of Disk Dominated Galaxies I. Bulge/Disk Parameters, Simulations, and Secular Evolution

Lauren A. MacArthur, Stephane Courteau, Jon A. Holtzman

(Abridged) A robust analysis of galaxy structural parameters, based on the modeling of bulge and disk brightnesses in the BVRH bandpasses, is presented for 121 face-on and moderate…

astro-ph2002★ 13 cited

A Simple Prediction on the Surface Density of Galaxies at z ~ 6

Haojing Yan, Rogier A. Windhorst, Stephen C. Odewahn +3

Systematic surveys are being proposed to discover a significant number of galaxies at z ~ 6, which is now suggested as the epoch when the reionization era of the Universe ends. To…

astro-ph2002★ 100 cited

The Diversity of Extremely Red Objects

Ian Smail, F. N. Owen, G. E. Morrison +3

We present a multi-wavelength study of Extremely Red Objects (EROs) employing deep RIzJHK photometry of a 8.5'x8.5' region to identify 68 EROs with R-K>5.3 and K<20.5 (5-sigma). Th…

astro-ph2002★ 144 cited

Molecular Gas and Star Formation in Bars of Nearby Spiral Galaxies

Kartik Sheth, Stuart N. Vogel, Michael W. Regan +3

We compare the distribution of molecular gas and star formation activity in the bar region of six spirals (NGC 2903, NGC 3627, NGC 4321, NGC 5457, NGC 6946, & IC 342) from the BIMA…

astro-ph2002★ 68 cited

Evolution of Star Forming and Active Galaxies in Nearby Clusters

Neal A. Miller, Frazer N. Owen

(Abridged) We have used optical spectroscopy to investigate the radio- selected active galaxy populations in a sample of 20 nearby Abell clusters. The spectra were used to characte…

astro-ph2002★ 16 cited

A New Orbital Ephemeris and Reinterpretation of Spectroscopic Data for the Supersoft X-ray Binary RX J0513.9-6951

A. P. Cowley, P. C. Schmidtke, D. Crampton +1

We have analyzed nearly eight years of MACHO optical photometry of the supersoft X-ray binary RX J0513.9-6951 and derived a revised orbital period and ephemeris. Previously publish…

astro-ph2002★ 28 cited

K-Band Red Clump Distances to the LMC Clusters Hodge 4 and NGC 1651

Ata Sarajedini, Aaron J. Grocholski, Joanna Levine +1

We present near-infrared color-magnitude diagrams for the LMC star clusters Hodge 4 and NGC 1651 revealing the helium burning red clump stars for the first time in the JK passbands…

astro-ph2002★ 27 cited

The Stellar and Gas Kinematics of Several Irregular Galaxies

Deidre A. Hunter, Vera C. Rubin, Rob A. Swaters +2

We present long-slit spectra of three irregular galaxies from which we determinethe stellar kinematics in two of the galaxies (NGC 1156 and NGC 4449) and ionized-gas kinematics in…

astro-ph2002★ 23 cited

Carbon Isotopic Abundances in the Red Giants of Omega Centauri (NGC5139)

Verne V. Smith, Donald M. Terndrup, Nicholas B. Suntzeff

Carbon-12 and carbon-13 abundances are measured in eleven red-giant members of the globular cluster Omega Centauri via observations of first-overtone CO bands near 2.3 microns. The…