activity
19982023
most citedChandra Studies of the X-ray Point Source Luminosity Functions of M31

51 citations · 89 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2023★ 1 cited

Maximizing science return by coordinating the survey strategies of Roman with Rubin, and other major facilities

R. A. Street, S. Gough-Kelly, C. Lam +13

[Abridged] The Nancy Grace Roman Space Telescope will be one of several flagship survey facilities operating over the next decade starting 2025. The deep near-IR imaging that…

astro-ph.SR2011★ 12 cited

On the detectability of a predicted mesolensing event associated with the high proper motion star VB 10

Sebastien Lepine, Rosanne DiStefano

Extrapolation of the astrometric motion of the nearby low-mass star VB 10 indicates that sometime in late December 2011 or during the first 2-3 months of 2012, the star will make a…

astro-ph2003★ 23 cited

Chandra ACIS and Newton EPIC Observations of the X-ray Luminous SN1978K in NGC 1313

Eric M. Schlegel, Albert Kong, Philip Kaaret +2

We describe an observation of the X-ray luminous SN1978K in NGC 1313 using the ACIS detector on Chandra and an archival Newton EPIC observation. The models that provided good fits…

astro-ph2002★ 51 cited

Chandra Studies of the X-ray Point Source Luminosity Functions of M31

A. K. H. Kong, R. Di Stefano, M. R. Garcia +1

Three different M31 disk fields, spanning a range of stellar populations, were observed by Chandra. We report the X-ray point source luminosity function (LF) of each region, and th…

astro-ph1998★ 2 cited

Transient supersoft X-ray emission from V751 Cyg during the optical low-state

J. Greiner, G. H. Tovmassian, R. DiStefano +4

We have observed V751 Cyg with the ROSAT HRI during its recent optical low state and clearly detect it at a count rate of 0.015 cts/s. The X-ray intensity is a factor of ~20 higher…

astro-ph1998

Relation between supersoft X-ray sources and VY Scl stars

Jochen Greiner, Rosanne DiStefano

In a recent ROSAT observation, taken during its optical low state, we found that the VY Scl star V751 Cyg was a highly luminous source of soft X-rays. The ROSAT HRI count rate of V…