activity
19972004
most citedPrompt and afterglow X-ray emission from the X-Ray Flash of 2002 April 27

29 citations · 58 across the 8 of their papers we have counts for

collaborators

23 papers

astro-ph2004

Spectral states and transient behaviour of a sample of X-ray bursters observed by BeppoSax

L. Natalucci, A. Bazzano, F. Capitanio +3

During observation campaigns of the Galactic Bulge region, BeppoSAX detected a total of 21 new X-ray bursters in about 6 years of operation. These sources are mostly transient and…

astro-ph200429 cited

Prompt and afterglow X-ray emission from the X-Ray Flash of 2002 April 27

L. Amati, F. Frontera, J. J. M. in 't Zand +15

We report on the X-ray observations of the X-ray flash (XRF) which occurred on 2002 April 27, three days before BeppoSAX was switched off. The event was detected with the BeppoSAX…

astro-ph2004

A BeppoSAX-WFC viewpoint of new INTEGRAL sources, particularly IGR J17544-2619

Jean in 't Zand, John Heise, Pietro Ubertini +2

Of the 21 new sources that INTEGRAL discovered up to Feb. 1, 2004, five were detected with the BeppoSAX Wide Field Cameras at earlier times. IGR J16320-4751 appears to be a persist…

astro-ph2003

Application of the Variability -> Luminosity Indicator to X-Ray Flashes

D. E. Reichart, D. Q. Lamb, R. M. Kippen +3

We have applied the proposed variability -> luminosity indicator to ten "X-Ray Flashes" (XRFs) observed by the Wide-Field Cameras on BeppoSAX for which BATSE survey data exists. Ou…

astro-ph2003

Long and faint GRBs in archival BeppoSAX-WFC data

J. J. M. in 't Zand, J. Heise, R. M. Kippen +4

In an ongoing effort to search for X-ray transients on diverse time scales in the data archive of the BeppoSAX Wide Field Cameras we have identified four GRBs that are long (betwee…

astro-ph2003

X/gamma-ray measurements of the faint GRB 020321

J. J. M. in 't Zand, L. Kuiper, J. Heise +10

GRB 020321 is a faint GRB that received wide follow-up attention in X-rays (BeppoSAX/NFI, Chandra/ACIS-S, XMM-Newton), radio (ATCA) and optical (ESO, HST). We identify a weak X-ray…