Search Publications

Supernovae in deep Hubble Space Telescope galaxy cluster fields: cluster rates and field counts
DOI: 10.1046/j.1365-8711.2002.05274.x Bibcode: 2002MNRAS.332...37G

Maoz, Dan; Sharon, Keren; Gal-Yam, Avishay

We have searched for high-redshift supernova (SN) candidates in multiple deep Hubble Space Telescope (HST ) archival images of nine galaxy cluster fields. We detect six apparent SNe, with 21.6<=I 814 <=28.4mag. There is roughly 1 SN per deep (I 814 >26mag), doubly-imaged WFPC2 cluster field. Two SNe are associated wi…

2002 Monthly Notices of the Royal Astronomical Society
eHST 81
The PAH emission spectra of Large Magellanic Cloud H II regions
DOI: 10.1051/0004-6361:20011628 Bibcode: 2002A&A...382.1042V

Tielens, A. G. G. M.; Peeters, E.; van der Hulst, J. M. +1 more

A set of ISOPHOT spectra from a sample of H Ii regions in the Large Magellanic Cloud (LMC) is presented. In all the spectra, emission bands arising from Polycyclic Aromatic Hydrocarbons (PAHs) are clearly present. These features are observed to vary considerably in relative strength to each other from source to source and even within 30 Doradus. T…

2002 Astronomy and Astrophysics
ISO 81
Maximum-entropy weak lens reconstruction: improved methods and application to data
DOI: 10.1046/j.1365-8711.2002.05685.x Bibcode: 2002MNRAS.335.1037M

Marshall, P. J.; Bridle, S. L.; Hobson, M. P. +1 more

We develop the maximum-entropy weak shear mass reconstruction method presented in earlier papers by taking each background galaxy image shape as an independent estimator of the reduced shear field and incorporating an intrinsic smoothness into the reconstruction. The characteristic length-scale of this smoothing is determined by Bayesian methods. …

2002 Monthly Notices of the Royal Astronomical Society
eHST 80
A Chandra High Resolution Camera Observation of X-Ray Point Sources in M31
DOI: 10.1086/342475 Bibcode: 2002ApJ...578..114K

Kaaret, Philip

We present results from a 47 ks observation of the Andromeda galaxy, M31, using the High Resolution Camera of the Chandra X-Ray Observatory. We detect 142 point sources spanning 3 orders of magnitude in luminosity, from LX=2×1035 to 2×1038 ergs s-1 in the 0.1-10 keV band. The X-ray source location accura…

2002 The Astrophysical Journal
eHST 80
Density modulated whistler mode emissions observed near the plasmapause
DOI: 10.1029/2002GL015101 Bibcode: 2002GeoRL..29.1975M

Santolik, O.; Parrot, M.; Andre, M. +4 more

Electron density fluctuations are regularly observed near the plasmapause together with electromagnetic waves below the electron cyclotron frequency (usually called hiss or chorus). Instruments on board CLUSTER spacecraft often observe two such emission bands with fluctuating wave intensities that suggest wave ducting in density enhancements as we…

2002 Geophysical Research Letters
Cluster 80
Hubble Space Telescope Space Telescope Imaging System Observations of the He II Gunn-Peterson Effect toward HE 2347-4342
DOI: 10.1086/324397 Bibcode: 2002ApJ...564..542S

Tripp, Todd M.; Jenkins, Edward B.; Heap, Sara R. +3 more

We present an HST Space Telescope Imaging System (STIS) spectrum of the He II Gunn-Peterson effect toward HE 2347-4342. Compared to the previous HST Goddard High Resolution Spectrograph data obtained by Reimers et al. the STIS spectrum has a much improved resolution. The two-dimensional detector also allows us to better characterize the sky and da…

2002 The Astrophysical Journal
eHST 80
[CII] at 158 mu m as a star formation tracer in late-type galaxies
DOI: 10.1051/0004-6361:20020156 Bibcode: 2002A&A...385..454B

Boselli, A.; Gavazzi, G.; Lequeux, J. +1 more

We present a calibration of the massive star formation rate vs. [CII] luminosity relation based on a sample of nearby, late-type galaxies observed with ISO-LWS and imaged in the Hα +[NII] line. The relation holds for far-IR luminosities 108 <= LFIR <=1010.5 Lsun. The derived star formation rates ha…

2002 Astronomy and Astrophysics
ISO 80
Deep Hubble Space Telescope Imaging of Sextans A. I. The Spatially Resolved Recent Star Formation History
DOI: 10.1086/324635 Bibcode: 2002AJ....123..813D

Skillman, Evan D.; Dolphin, Andrew; Cole, Andrew A. +5 more

We have measured stellar photometry from deep Cycle 7 Hubble Space Telescope/WFPC2 imaging of the dwarf irregular galaxy Sextans A. The imaging was taken in three filters: F555W (V; eight orbits), F814W (I; 16 orbits), and F656N (Hα one orbit). Combining these data with Cycle 5 WFPC2 observations provides nearly complete coverage of the optically …

2002 The Astronomical Journal
eHST 80
The peculiar variable V838 Mon
DOI: 10.1046/j.1365-8711.2002.06017.x Bibcode: 2002MNRAS.336L..43K

Kimeswenger, S.; Lederle, C.; Schmeja, S. +1 more

V838 Mon underwent, after a first nova-like outburst in January and a usual decline, a second outburst after one month, and a third weak one again a month later. Moreover, a very small increase of the temperature at the beginning of April gives us a hint about a physical process with a period of one month. We obtained a BVRIC time-seque…

2002 Monthly Notices of the Royal Astronomical Society
eHST 79
An Enshrouded Active Galactic Nucleus in the Merging Starburst System Arp 299 Revealed by BeppoSAX
DOI: 10.1086/345925 Bibcode: 2002ApJ...581L...9D

Maraschi, L.; Cappi, M.; Franceschini, A. +9 more

Using a long (~=150 ks) broadband (0.1-40 keV) BeppoSAX observation of the merging starburst system Arp 299 (=IC 694+NGC 3690), we found the first unambiguous evidence of the presence of a deeply buried (NH~=2.5×1024 cm-2) active galactic nucleus (AGN) having  an intrinsic luminosity of L0.5-100keV~=1.9…

2002 The Astrophysical Journal
XMM-Newton 79