X-ray optical depth diagnostics of T Tauri accretion shocks (2009)
Argiroffi, C., Maggio, A., Peres, G., Drake, J. J., Santiago, J. Lopez, Sciortino, S., ...
In classical T Tauri stars, X-rays are produced by two plasma components: a hot low-density plasma, with frequent flaring activity, and a high-density lower temperature plasma. The former is coronal...
Results from DROXO. II. - [Ne II] and X-ray emission from Rho Ophiuchi young stellar objects (2009)
Flaccomio, E., Stelzer, B., Sciortino, S., Micela, G., Pillitteri, I., Testi, L.
The infrared [Ne II] and [Ne III] fine structure lines at 12.81um and 15.55um are predicted to trace the circumstellar disk gas subject to X-ray heating and ionization. We investigate the origin of...
Guarcello, M. G., Micela, G., Damiani, F., Peres, G., Prisinzano, L., Sciortino, S.
Context: the observations of the proplyds in the Orion Nebula Cluster, showing clear evidence of ongoing photoevaporation, have provided a clear proof about the role of the externally induced...
X-ray observations of IC348 in light of an updated cluster census (2008)
Stelzer, B., Micela, G., Flaccomio, E., Sciortino, S.
IC348 is an excellent laboratory for studies of low-mass star formation being nearby, compact and rich. A Chandra observation was carried out early in the satellite's lifetime. The extensive new data...
An X-ray survey of low-mass stars in Trumpler 16 with Chandra (2008)
Albacete-Colombo, J. F., Damiani, F., Micela, G., Sciortino, S., Harnden Jr, F. R.
We identify and characterize low-mass stars in the ~3 Myr old Trumpler 16 (Tr16) region by means of a deep Chandra X-ray observation, and study their optical and near-IR properties. We compare X-ray...
Circumstellar Disks in the Outer Galaxy: the Star-Forming Region NGC 1893 (2008)
Caramazza, M., Micela, G., Prisinzano, L., Rebull, L., Sciortino, S., Stauffer, J. R.
It is still debated whether star formation process depends on environment. In particular it is yet unclear whether star formation in the outer Galaxy, where the environmental conditions are,...
The X-ray cycle in the solar-type star HD 81809 (2008)
Favata, F., Micela, G., Orlando, S., Sciortino, S., Hall, J.
(abridged) Our long-term XMM-Newton program of long-term monitoring of a solar-like star with a well-studied chromospheric cycle, HD 81809 aims to study whether an X-ray cycle is present, along with...
Circumstellar disks in the outer galaxy : the star-forming region NGC 1893 (2008)
Caramazza, M., Micela, G., Prisinzano, L., Rebull, L., Sciortino, S., Stauffer, J. R.
Context. It is still debated whether star formation process depends on environment. In particular it is yet unclear whether star formation in the outer Galaxy, where the environmental conditions are,...
Will Be Inserted, F. Favata, G. Micela, S. Sciortino
We present determinations of the lithium abundance (through observations of the Li i 6707.8 A line) in a sample of main sequence stars with spectral types ranging from late F down to M0, selected...
Will Be Inserted, F. Favata, G. Micela, S. Sciortino, F. Morale
We present spectroscopic determinations of the Fe abundance in a sample of K-type stars selected from the Xray flux-limited Einstein Extended Medium Sensitivity Survey. These stars have been shown to...
F. Bocchino, A. Maggio, S. Sciortino, Abstract. Wedevelopedandtestedanon-equilibrium
We developed and tested a Non-Equilibrium of Ionization (NEI) emission model to study the X-ray emission of supernova remnants (SNR's) with a parametric fitting approach. We present results of...
Astronomy Astrophysics manuscript no. 3630 August 8, 2005 (2008)
Doi Will Be, F. Damiani, G. Micela, S. Sciortino
We present a Chandra ACIS-I X-ray observation of the region near the Herbig early-Be star MWC 297, where we detect a tight group of point X-ray sources. These are probably physically associated to...
Will Be Inserted, A. Maggio, F. Favata, G. Peres, S. Sciortino
We present an X-ray observation of the active giant fi Cet, performed with the Low Energy Concentrator Spectrometer (LECS) on-board the SAX satellite. The resulting Xray spectrum is well fit by an...
Will Be Inserted, F. Morale, G. Micela, F. Favata, S. Sciortino
We present the results of a uvby-fi photometric study of a sample of active late-type stars (F--K) selected from the Einstein Extended Medium Sensitivity Survey. Our work shows the presence in the...
Damiani Prisinzano Micela, F. Damiani, L. Prisinzano, G. Micela, S. Sciortino
We present a combined X-ray, optical and IR (2MASS) study of NGC 6530, complementing our previous studies of this cluster. We consider di#erent indicators of IR excesses, taken as indicator of...
Aa 406, 629--638 (2003) Doi: 10.1051/0004-6361:20030689 (2008)
Eso Astronomy Astrophysics, A. Marino, G. Micela, G. Peres, S. Sciortino
We present a comprehensive analysis of X-ray variability of the late-type (dF7-dM) Pleiades stars, detected in all ROSAT-PSPC observations; X-ray variations on short (hours) and medium (months) time...
Istituto Ed Osservatorio, Italy G. Micela, S. Sciortino
We report the results of a deep X-ray survey of the core region of the Pleiades cluster carried out with the ROSAT Observatory. In a single PSPC field ( 1 radius), we detect 99 of 214 Pleiades member...
A Deep X-Ray Survey Of The Pms Population Of The Upper Sco-Cen Association (2008)
Sciortino Damiani, S. Sciortino, F. Damiani, G. Micela, F. Favata
han previously reported. A recent X-ray surveys, based on the ROSAT All-Sky Survey (RASS) data, studied a much larger areas of the sky, but with the same limiting sensitivity as the older Einstein...
X-Ray And Optical Observations Of The Star Forming Region Ngc 2264 (2008)
Flaccomio Sciortino, E. Flaccomio, S. Sciortino, G. Micela, F. Damiani, F. Favata, ...
. We present a ROSAT High Resolution Imager (HRI) observation of the star forming region NGC 2264. The analysis has detected more than 40 X-ray sources with Lx in the range 10 30 \Gamma10 31 erg/sec....
Astronomy Astrophysics manuscript no. (2008)
Will Be Inserted, A. Marino, G. Micela, G. Peres, S. Sciortino
We have analyzed the X-ray variability of dF7-dK2 stars in the solar neighborhood detected with the pointed ROSAT-PSPC observations. Our data base is the sample of all stars listed in the CNS3...
E. Flaccomio, F. Damiani, G. Micela, S. Sciortino, F. R. Harnden, S. S. Murray, ...
Using the results of our rst paper on the Chandra HRC observation of the Orion Nebula Cluster (ONC), here we explore the relation between the coronal activity of its 1-Myr-old pre-main sequence...
Hard X-ray view of Nearby Star Forming Regions (2007)
Chandra and XMM-Newton have surveyed several nearby star forming regions and have greatly advanced our knowledge of X-ray emission from Young Stellar Objects (YSOs). After briefly reviewing it I...
Results and Perspectives of Young Stellar Object long look programs (2007)
Both Chandra and XMM-Newton have performed long look programs for studying the YSO physics. I will discuss recent results on the controversial issue of Class 0 YSO X-ray emission, the observational...
A. Maggio, S. Orlando, F. Favata, G. Micela, G. Peres, S. Sciortino
We present the results of extensive sets of simulations, performed to evaluate the diagnostic potential of the analysis of EPIC spectra. 1.
G. Micela, S. Sciortino, F. Favata, R. Pallavicini, J. Pye
ABSTRACT. We present preliminary results from two deep HRI ROSAT exposures on the i Sculptoris open cluster. This cluster, younger than the Pleiades, has photometric indicators that seem to imply a...
G. Micela, S. Sciortino, F. R. Harnden, V. Kashyap, R. Rosner, F. Damiani, ...
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are:
ASTRONOMY AND ASTROPHYSICS (2007)
F. Favata, G. Micela, S. Sciortino
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are:
X-ray observations of the young open cluster Blanco 1 (2007)
G. Micela, S. Sciortino, F. Favata, R. Pallavicini, J. Pye
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are:
ASTRONOMY AND ASTROPHYSICS (2007)
F. Favata, G. Micela, S. Sciortino
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are:
A Source Detection Method for ROSAT/PSPC X-Ray Images based on Wavelet Transforms (2007)
F. Damiani, A. Maggio, G. Micela, S. Sciortino
. We have developed a method based on wavelet transforms (WT) to detect sources in ROSAT PSPC X-ray images. The WT, evaluated at a set of scale parameters a, detects efficiently both point-like and...
X-Ray Emitting Pms Stars In Upper Sco-Cen: The X-Ray Faint Population (2007)
Favata Sciortino Damiani, F. Favata, S. Sciortino, F. Damiani, G. Micela
. We have performed an X-ray-based survey of the upper Sco-Cen star forming region, combining a deep ROSAT HRI pointing performed explicitly for this purpose with shallower ROSAT PSPC and HRI...
Lithium abundance in a volume limited sample of nearby main sequence G and K stars (2007)
Favata Micela And, F. Favata, G. Micela, S. Sciortino
. We present observations of the Li I 6707.8 A line in a volume limited sample of main sequence stars of spectral types ranging from late F down to M0, selected from the Gliese catalog of nearby...
X-Ray Variability And Rotation In The Pleiades Cluster (2007)
Micela And, G. Micela, S. Sciortino, F. R. Harnden, R. Rosner
Introduction The issue of coronal emission variability is one of the current problems of stellar physics. The Sun exhibits large variability in X-rays with amplitude of more than one order of...
X-ray spectroscopy of the active dM stars: AD Leo and EV Lac (2007)
Sciortino Maggio, S. Sciortino, A. Maggio, F. Favata
. We present results of an analysis of new observations of the active M dwarfs AD Leo (GJ 388) and EV Lac (GJ 873), performed with the X-ray satellite SAX, and compare them with both published and...
An optimized time screening algorithm for ROSAT PSPC and HRI observations. (2007)
Bocchino Barbera, F. Bocchino, M. Barbera, S. Sciortino
. We have developed a model-independent time screening optimization algorithm to cope with significant contamination spikes in the ROSAT PSPC/HRI bacground light-curves. The rejection criteria are...
The Evolutionary Status Of High-Lithium, High-Activity Cool Dwarfs (2007)
Favata Micela, F. Favata, G. Micela, S. Sciortino
. We have used the newly available Hipparcos parallaxes to study the evolutionary status of a number of high-lithium, high-activity late-type dwarfs found in X-ray based surveys, i.e. the Einstein...
Astronomy And Astrophysics (2007)
February Bvri, E. Flaccomio, G. Micela, S. Sciortino, F. Favata, C. Corbally, ...
. The pre-main sequence (PMS) population in the mass range between ß 0:2 and ß 3M fi in southern part of the star-forming region NGC 2264 has been studied, determining both the Initial Mass...
X-Ray Emission, Stellar Populations and Determination of IMF (2007)
Sciortino Micela, S. Sciortino, G. Micela, F. Damiani, E. Flaccomio, Osservatorio Astronomico, ...
X-ray observations allow investigation of the relation among coronal emission level and other stellar parameters, still poorly considered in the standard evolutionary models, such as rotation rate,...
BeppoSAX and ROSAT Observations of the Supernova Remnant RCW86 (2007)
Bocchino Favata, F. Bocchino, F. Favata, A. Maggio, S. Sciortino
Introduction The supernova remnant RCW86 (also known as G315.4-2.3, MSH14-63) is one of the brightest objects in its category of all the X-ray sky. Recently, it has received renewed attention...
ASTRONOMY AND ASTROPHYSICS (2007)
F. Favata, G. Micela, S. Sciortino
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are:
Discovery of X-ray emission from the proto-stellar jet (2007)
F. Favata, J. Drake, L Irs (hh, Fabio Favata, G. Micela, ...
Abstract. We have for the rst time detected X-ray emission associated with a proto-stellar jet, on the jet emanating from L1551 IRS5. The IRS5 proto-star is hidden beyond a very large absorbing...
Astron. Nachr./AN 32X (200X) X, XXX--XXX (2007)
The Hellas Xmm, A. Baldi, F. Cocchia, F. Favata, F. Fiore, S. Molendi, ...
d to consider separately stars of different age. We consider three age ranges, each characterized by different X-ray luminosity functions and coronal temperature. At our typical sensitivities, for a...
Mon. Not. R. Astron. Soc. 000, 000-000 (0000) Printed 25 April 2001 (MN L A T E X style (2007)
Le Rosat Medium, J. E. Morley, K. R. Briggs, J. P. Pye, F. Favata, G. Micela, ...
We have performed a moderately deep soft X-ray (0.1-2 keV) survey of the Galactic Plane using pointed observations with the ROSAT Position Sensitive Proportional Counter (PSPC). The survey is more...
Astronomy Astrophysics manuscript no. (2007)
Will Be Inserted, N. Pizzolato, P. Ventura, A. Maggio, G. Micela, S. Sciortino
We present an extensive study on the dependence of the convective turnover time (conv ) on the stellar metallicity and age for main-sequence stars of masses 0.6-1.6 M . To this aim we have used and...
Astronomy Astrophysics manuscript no. (2007)
Will Be Inserted, F. Favata, G. Micela, S. Sciortino, A. Kaas
We have for the rst time detected X-ray emission associated with a protostellar jet, on the jet emanating from the L1551 IRS5 protostar. The IRS5 protostar is hidden behind a very large absorbing...
Astron. Nachr./AN 32X (200X) X, XXX--XXX (2007)
The Stellar Content, G. Micela, F. Favata, E. Feigelson, S. Sciortino
Introduction We present our ongoing work on the stellar content of Chandra Deep Field North survey based on the analysis of the 1 Msec data (Brandt et al. 2001) in the 0.5-2.0 keV band. The optical...
E. Flaccomio, F. Damiani, G. Micela, S. Sciortino, F. R. Harnden, S. S. Murray, ...
In this rst of two companion papers on the Orion Nebula Cluster (ONC), we present our analysis of a 63 Ksec Chandra HRC-I observation that yielded 742 X-ray detections within the 30 eld of view. To...
Young Stars Near Earth: Progress and Prospects (2007)
Asp Conference Series, Ray Jayawardhana, Thomas Greene, S. Sciortino, F. Damiani, F. Favata, ...
We present results of our ongoing study of the low-mass members of Upper Sco-Cen based on deep BVRI photometry and XMMNewton EPIC observations purposely obtained as part of the GTO program. Analyzing...
Pillitteri Micela Sciortino, I. Pillitteri, G. Micela, S. Sciortino, F. Favata
We present X-ray Luminosity Distributions (XLDs) of late-type members (dF, dG, dK, dM) of the Blanco 1 cluster, based on ROSAT-HRI data and new astrometric-photometric membership obtained from the...
Astronomy Astrophysics manuscript no. H4001 February 17, 2003 (2007)
Doi Will Be, E. Flaccomio, G. Micela, S. Sciortino
We investigate the evolution of X-ray stellar activity from the age of the youngest known star forming regions (SFR), . 1Myr, to about 100 Myr, i.e. the zero age main sequence (ZAMS) for a 1M star....
Astronomy Astrophysics manuscript no. (2007)
Will Be Inserted, L. Prisinzano, G. Micela, S. Sciortino, F. Favata
We present UBVRI photometry of the open cluster NGC 2422 (age 10 yr) down to a limiting magnitude V ' 19. These data are used to derive the Luminosity and Mass Functions and to study the cluster...
Stellar Coronae in the Chandra and XMM-Newton Era (2007)
Asp Conference Series, J. Drake, S. Sciortino, F. Damiani, F. Favata, F. Favata, ...
As part of our long-term eort to characterize the low-mass stellar population of the Upper Sco-Cen association based on deep Xray surveys and follow-up optical observations we present results from a...
Bocchino Damiani Micela, F. Bocchino, F. Damiani, G. Micela, S. Sciortino, F. Favata
We present the results of a ROSAT study of NGC 2422, a southern open cluster at a distance of about 470 pc, with an age close to the Pleiades. Source detection was performed on two observations, a...
Giardino, G., Favata, F., Pillitteri, I., Flaccomio, E., Micela, G., Sciortino, S.
AIMS. We study the variability of the Fe 6.4 KeV emission line from the Class I young stellar object Elias 29 in the Rho-Oph cloud. METHODS. We analysed the data from Elias 29 collected by XMM during...
X-ray flaring from the young stars in CygnusOB2 (2007)
Colombo, J. F. Albacete, Caramazza, M., Flaccomio, E., Micela, G., Sciortino, S.
Aims: We characterize individual and ensemble properties of X-ray flares from stars in the CygOB2 and ONC star-forming regions. Method: We analyzed X-ray lightcurves of 1003 CygOB2 sources observed...
Coronal Abundances in Orion Nebula Cluster Stars (2007)
Maggio, A., Flaccomio, E., Favata, F., Micela, G., Sciortino, S., Feigelson, E. D., ...
Following the Chandra Orion Ultradeep Project (COUP) observation, we have studied the chemical composition of the hot plasma in a sample of 146 X-ray bright pre-main sequence stars in the Orion...
Giardino, G., Favata, F., Micela, G., Sciortino, S., Winston, E.
AIMS: To study the properties of X-ray emissions from young stellar objects (YSOs), through their evolution from Class I to Class III and determine whether Class 0 protostars emit in X-rays. METHODS:...
Guarcello, M. G., Prisinzano, L., Micela, G., Damiani, F., Peres, G., Sciortino, S.
Context: the observation of young stars with circumstellar disks suggests that the disks are dissipated, starting from the inner region, by the radiation of the central star and eventually by the...
Unveiling the Cygnus OB2 stellar population with Chandra (2006)
Colombo, J. F. Albacete, Flaccomio, E., Micela, G., Damiani, F., Sciortino, S.
The aim of this work is to identify the so far unknown low mass stellar population of the ~2Myr old Cygnus OB2 region, and to investigate the X-ray and near-IR stellar properties of its members. We...
The stellar content of the XMM-Newton Bright Serendipitous Survey (2006)
Lopez-Santiago, J., Micela, G., Sciortino, S., Favata, F., Caccianiga, A., Della Ceca, R., ...
Context: The comparison of observed counts in a given sky direction with predictions by Galactic models yields constraints to the spatial distribution and the stellar birthrate of young stellar...
XMM-Newton survey of two Upper Scorpius regions (2006)
Argiroffi, C., Favata, F., Flaccomio, E., Maggio, A., Micela, G., Peres, G., ...
We study X-ray emission from young stars by analyzing deep XMM-Newton observations of two regions of the Upper Scorpius association, having an age of 5 Myr. Based on near infrared and optical...
ACIS-I observations of NGC2264. Membership and X-ray properties of PMS stars (2006)
Flaccomio, E., Micela, G., Sciortino, S.
We analyze a deep, 100 ksec long, Chandra ACIS observation of NGC2264. We detect 420 sources, 85% of which are associated with known optical and NIR counterparts. More than 90% of these counterparts...
Giardino, G., Favata, F., Silva, B., Micela, G., Reale, F., Sciortino, S.
We present the results of a five-day monitoring campaign with XMM-Newton of six X-ray bright young stellar objects (YSOs) in the star-forming complex L1551 in Taurus. All stars present significant...
The discovery of an expanding X-ray source in the HH 154 protostellar jet (2006)
Favata, F., Bonito, R., Micela, G., Fridlund, M., Orlando, S., Sciortino, S., ...
We have performed, in October 2005, a deep Chandra X-ray observation of HH 154. Comparison with the previous (2001) Chandra observation allows to detect proper motion down to the level predicted by...
Chandra X-Ray Observations of Young Clusters. III. NGC 2264 and the Orion Flanking Fields (2006)
Rebull, L. M., Stauffer, J. R., Ramirez, S. V., Flaccomio, E., Sciortino, S., Micela, G., ...
Chandra observations of solar-like pre-main sequence (PMS) stars in the Orion Flanking Fields (age ~1 Myr) and NGC 2264 (~3 Myr) are compared with the results of the COUP survey of similar objects in...
Deep X-ray survey of the young open cluster NGC 2516 with XMM-Newton (2006)
Pillitteri, I., Micela, G., Damiani, F., Sciortino, S.
We report on a deep X-ray survey of the young (~ 140 Myr), rich open cluster NGC 2516 obtained with the EPIC camera on board the XMM-Newton satellite. By combining data from six observations, a high...
Radiation hard diamond sensors for future tracking applications (2006)
Adam, W., De Boer, W., Borchi, E., Bruzzi, M., Colledani, C., D'Angelo, P., ...
Astronomy Astrophysics manuscript no. example c (2006)
Eso October Correlation, M. G. Guarcello, L. Prisinzano, G. Micela, F. Damiani, G. Peres, ...
Context. The observation of young stars with circumstellar disks suggests that the disks are dissipated, starting from the inner region, by the radiation of the central star and eventually by the...
Astronomy Astrophysics manuscript no. 5011 c (2006)
Eso September The, F. Damiani, G. Micela, S. Sciortino, N. Huélamo, A. Moitinho, ...
Context. We study the stellar population of the very young cluster NGC 2362, using a deep Chandra ACIS-I X-ray observation. This cluster, only 5 Myr old, has already cleared most of its inter- and...
Astronomy Astrophysics manuscript no. 4003 c (2006)
Eso January Deep, I. Pillitteri, G. Micela, F. Damiani, S. Sciortino
Aims. We report a deep X-ray survey of the young ( 140 Myr), rich open cluster NGC 2516 obtained with the EPIC camera on board the XMM-Newton satellite.
Astronomy Astrophysics manuscript no. upsco c (2006)
Eso Th July, C. Argiroffi, F. Favata, E. Flaccomio, A. Maggio, G. Micela, ...
Aims. We study X-ray emission from young stars by analyzing deep XMM-Newton observations of two regions of the Upper Scorpius association, having an age of 5 Myr.
IMPROVEMENTS IN CVD DIAMOND PROPERTIES FOR RADIOTHERAPY DOSIMETRY (2006)
De Angelis, C., Bucciolini, M., Casati, M., Løvik, I., Bruzzi, M., Lagomarsino, S., ...
The goal of this work was to compare the behaviour of a chemical vapour deposited (CVD) diamond sample, grown at the University of Florence using a local procedure, with that of a commercial CVD...
Improvements in CVD diamond properties for radiotherapy dosimetry (2006)
De Angelis, C., Bucciolini, M., Casati, M., Løvik, I., Bruzzi, M., Lagomarsino, S., ...
The goal of this work was to compare the behaviour of a chemical vapour deposited (CVD) diamond sample, grown at the University of Florence using a local procedure, with that of a commercial CVD...
Rotational modulation of X-ray emission in Orion Nebula young stars (2005)
Flaccomio, E., Micela, G., Sciortino, S., Feigelson, E. D., Herbst, W., Favata, F., ...
We investigate the spatial distribution of X-ray emitting plasma in a sample of young Orion Nebula Cluster stars by modulation of their X-ray light-curves due to stellar rotation. The study, part of...
Bright X-ray flares in Orion young stars from COUP: evidence for star-disk magnetic fields? (2005)
Favata, F., Flaccomio, E., Reale, F., Micela, G., Sciortino, S., Shang, H., ...
We have analyzed a number of intense X-ray flares observed in the Chandra Orion Ultradeep Project (COUP), a 13 days observation of the Orion Nebula Cluster (ONC). Analysis of the flare decay allows...
X-ray emission from early-type stars in the Orion Nebula Cluster (2005)
Stelzer, B., Flaccomio, E., Montmerle, T., Micela, G., Sciortino, S., Favata, F., ...
The X-ray properties of twenty ~1 Myr old O, B, and A stars of the Orion Trapezium are examined with data from the Chandra Orion Ultradeep Project (COUP). On the basis of simple theories for X-ray...
COUP census of X-ray stars in BN-KL and OMC-1S (2005)
Grosso, N., Feigelson, E. D., Getman, K. V., Townsley, L., Broos, P., Flaccomio, E., ...
We present a study of the X-ray sources detected in the vicinity of two density peaks in the Orion Molecular Cloud 1 (OMC-1) behind the Orion Nebula Cluster (ONC), as seen in the exceptionally deep...
Development of radiation tolerant semiconductor detectors for the Super-LHC (2005)
Moll, M., Adey, J., Al-Ajili, A., Alfieri, G., Allport, P. P., Artuso, M., ...
The envisaged upgrade of the Large Hadron Collider (LHC) at CERN towards the Super-LHC (SLHC) with a 10 times increased luminosity of 10(35) cm(-2) s(-1) Will present severe challenges for the...
Radiation-hard semiconductor detectors for SuperLHC (2005)
Bruzzi, M., Adey, J., Al-Ajili, A., Alexandrov, P., Alfieri, G., Allport, P. P., ...
An option of increasing the luminosity of the Large Hadron Collider (LHC) at CERN to 1035 cm-2 s-1 has been envisaged to extend the physics reach of the machine. An efficient tracking down to a few...
Recent advancements in the development of radiation hard semiconductor detectors for S-LHC (2005)
Fretwurst, E., Adey, J., Al-Ajili, A., Alfieri, G., Allport, P. P., Artuso, M., ...
The proposed luminosity upgrade of the Large Hadron Collider (S-LHC) at CERN will demand the innermost layers of the vertex detectors to sustain fluences of about 10(16) hadrons/cm(2). Due to the...
Radiation-hard semiconductor detectors for SuperLHC (2005)
Bruzzi, M., Adey, J., Al-Ajili, A., Alexandrov, P., Alfieri, G., Allport, P. P., ...
An option of increasing the luminosity of the Large Hadron Collider (LHC) at CERN to 1035 cm-2 s-1 has been envisaged to extend the physics reach of the machine. An efficient tracking down to a few...
Recent advancements in the development of radiation hard semiconductor detectors for S-LHC (2005)
Fretwurst, E., Adey, J., Al-Ajili, A., Alfieri, G., Allport, P. P., Artuso, M., ...
The proposed luminosity upgrade of the Large Hadron Collider (S-LHC) at CERN will demand the innermost layers of the vertex detectors to sustain fluences of about 10(16) hadrons/cm(2). Due to the...
Development of radiation tolerant semiconductor detectors for the Super-LHC (2005)
Moll, M., Adey, J., Al-Ajili, A., Alfieri, G., Allport, P. P., Artuso, M., ...
The envisaged upgrade of the Large Hadron Collider (LHC) at CERN towards the Super-LHC (SLHC) with a 10 times increased luminosity of 10(35) cm(-2) s(-1) Will present severe challenges for the...
Chandra Orion Ultradeep Project : Observations and source lists (2005)
Getman, K. V., Flaccomio, E., Broos, P. S., Grosso, N., Tsujimoto, M., Townsley, L., ...
The origin of T tauri X-ray emission : New insights from the Chandra Orion Ultradeep Project (2005)
Preibisch, T., Kim, Y. C., Favata, F., Feigelson, E. D., Flaccomio, E., Getman, K., ...
X-ray emission from young brown dwarfs in the Orion Nebula Cluster (2005)
Preibisch, T., McCaughrean, M. J., Grosso, N., Feigelson, E. D., Flaccomio, E., Getman, K., ...
X-ray emission from early-type stars in the Orion Nebula Cluster (2005)
Stelzer, B., Flaccomio, E., Montmerle, T., Micela, G., Sciortino, S., Favata, F., ...
Favata, F., Micela, G., Silva, B., Sciortino, S., Tsujimoto, M.
We report the results of a search for 6.4 keV Fe fluorescent emission in Young Stellar Objects (YSOs) with measured accretion luminosities in the rho Oph cloud, using all existing chandra and...
High Resolution X-ray Spectroscopy of Pre-Main-Sequence Stars: TWA 5 and PZ Tel (2004)
Argiroffi, C., Drake, J. J., Harnden, F. R., Maggio, A., Peres, G., Sciortino, S., ...
We report on the analysis of high resolution X-ray spectra of two pre-main-sequence stars: TWA 5 (observed with XMM-Newton) and PZ Telescopii (observed with Chandra/HETGS). TWA 5 is a classical T...
X-ray spectral and timing characteristics of the stars in the young open cluster IC 2391 (2004)
Marino, A., Micela, G., Peres, G., Pillitteri, I., Sciortino, S.
We present X-ray spectral and timing analysis of members of the young open cluster IC 2391 observed with the XMM-Newton observatory. We detected 99 X-ray sources by analysing the summed data obtained...
Chandra Orion Ultradeep Project: Observations and Source Lists (2004)
Getman, K. V., Flaccomio, E., Broos, P. S., Grosso, N., Tsujimoto, M., Townsley, L., ...
We present a description of the data reduction methods and the derived catalog of more than 1600 X-ray point sources from the exceptionally deep January 2003 Chandra X-ray Observatory observation of...
The Star Formation Region NGC 6530: distance, ages and Initial Mass Function (2004)
Prisinzano, L., Damiani, F., Micela, G., Sciortino, S.
We present astrometry and $BVI$ photometry, down to $V\simeq22$, of the very young open cluster NGC6530, obtained from observations taken with the Wide Field Imager camera at the MPG/ESO 2.2 m...
X-ray spectroscopy of the unsteady quiescent corona of AD Leo with Chandra (2004)
Maggio, A., Drake, J. J., Kashyap, V., Harnden, F. R., Micela, G., ...
We present the analysis and interpretation of an observation of the flare star AD Leo (dM3e) with Chandra/LETG. The high resolution X-ray spectrum allowed us to infer the plasma emission measure...
Feigelson, E. D., Hornschemeier, A. E., Micela, G., Bauer, F. E., Alexander, D. M., Brandt, W. N., ...
The extremely sensitive Chandra Deep Field-North (CDF-N) pencil-beam X-ray survey is used to identify and characterize the X-ray emission from old high-latitude main sequence Galactic stars. Our...
New developments in CVD diamond for detector applications (2004)
Adam,A., Berdermann,E., Bergonzo,P., De Boer,W., Bogani,F., Borchi,E., ...
Chemical Vapor Deposition (CVD) diamond has been discussed extensively as an alternative sensor material for use very close to the interaction region of the LHC and other machines where extreme...
Pillitteri, I., Micela, G., Sciortino, S., Damiani, F., Harnden Jr, F. R.
We present an X-ray study of the high metallicity young open cluster Blanco 1 based on XMM--Newton data. X-ray spectroscopy of cluster members is presented for the first time as well as new X-ray...
High Resolution X-ray Spectroscopy of the Post-T Tauri Star PZ Tel (2004)
Argiroffi, C., Drake, J. J., Maggio, A., Peres, G., Sciortino, S., Harnden, F. R.
We present an analysis of the Chandra High Energy Transmission Grating Spectrometer observation of the rapidly rotating P_(rot)=0.94 d post T Tauri (~20 Myr old) star PZ Telescopii, in the Tucana...
Parameter properties and stellar population of the old open cluster NGC 3960 (2004)
Prisinzano, L., Micela, G., Sciortino, S., Favata, F.
We present a $BVI$ photometric and astrometric catalogue of the open cluster NGC 3960, down to limiting magnitude $V\sim22$, obtained from observations taken with the Wide Field Imager camera at the...
New developments in CVD diamond for detector applications (2004)
Adam, A., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., Borchi, E., ...
Chemical Vapor Deposition (CVD) diamond has been discussed extensively as an alternative sensor material for use very close to the interaction region of the LHC and other machines where extreme...
Parameter properties and stellar population of the old open cluster NGC 3960 (2004)
L. Prisinzano, G. Micela, S. Sciortino, F. Favata
We present a BVI photometric and astrometric catalogue of the open cluster NGC 3960, down to limiting magnitude V 22, obtained from observations taken with the Wide Field Imager camera at the MPG/ESO...
Astronomy Astrophysics manuscript no. gb041 March 5, 2004 (2004)
Doi Will Be, F. Favata, G. Micela, S. L. Baliunas, M. Güdel, ...
We present the initial results from our XMM-Newton program aimed at searching for X-ray activity cycles in solar-type stars. HD 81809 is a G2-type star (somewhat more evolved than the Sun, and with a...
X-ray rotational modulation of a supersaturated star in IC 2391 (2003)
Marino, A., Micela, G., Peres, G., Sciortino, S.
We present evidence of X-ray rotational modulation on VXR45, a young fast rotator star, member of IC 2391. It is a dG9 spectral type star whose rotational period and X-ray luminosity make it a...
Luminosity and Mass Function of the Galactic open cluster NGC 2422 (2003)
Prisinzano, L., Micela, G., Sciortino, S., Favata, F.
We present UBVRI photometry of the open cluster NGC 2422 (age $\sim 10^8$ yr) down to a limiting magnitude $V\simeq19$. These data are used to derive the Luminosity and Mass Functions and to study...
Favata, F., Giardino, G., Micela, G., Sciortino, S., Damiani, F.
We present a study of the X-ray sources present in the nearby L1551 star forming region, based on a deep XMM observation complemented with Chandra data for the brightest sources. All the known...
Flaccomio, E., Micela, G., Sciortino, S.
We investigate the evolution of X-ray stellar activity from the age of the youngest known star forming regions (SFR), < 1Myr, to about 100 Myr, i.e. the zero age main sequence (ZAMS) for a ~ 1M_sun...
Status of the R&D activity on diamond particle detectors (2003)
Adam, W., Bellini, B., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., ...
Status of the R&D activity on diamond particle detectors (2003)
Adam, W., Bellini, B., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., ...
The development of diamond tracking detectors for the LHC (2003)
Adam,W., Berdermann,E., Bergonzo,P., De Boer,W., Bogani,F., Borchi,E., ...
Chemical vapor deposition diamond has been discussed extensively as an alternate sensor material for use very close to the interaction region of the LHC where extreme radiation conditions exist....
Status ofthe R&D activity on diamond particle detectors (2003)
Adam,W., Berdermann,E., Bergonzo,P., De Boer,W., Bogani,F., Borchi,E., ...
Chemical Vapor Deposited (CVD) polycrystalline diamond has been proposed as a radiation-hard alternative to silicon in the extreme radiation levels occurring close to the interaction region ofthe...
New results on diamond pixel sensors using ATLAS frontend electronics (2003)
Adam,W., Berdermann,E., Bergonzo,P., De Boer,W., Bogani,F., Borchi,E., ...
Diamond is a promising sensor material for future collider experiments due to its radiation hardness. Diamond pixel sensors have been bump bonded to an ATLAS pixel readout chip using PbSn solder...
The development of diamond tracking detectors for the LHC (2003)
Adam, W., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., Borchi, E., ...
Chemical vapor deposition diamond has been discussed extensively as an alternate sensor material for use very close to the interaction region of the LHC where extreme radiation conditions exist....
Status ofthe R&D activity on diamond particle detectors (2003)
Adam, W., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., ...
Chemical Vapor Deposited (CVD) polycrystalline diamond has been proposed as a radiation-hard alternative to silicon in the extreme radiation levels occurring close to the interaction region ofthe...
New results on diamond pixel sensors using ATLAS frontend electronics (2003)
Adam, W., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., Borchi, E., ...
Diamond is a promising sensor material for future collider experiments due to its radiation hardness. Diamond pixel sensors have been bump bonded to an ATLAS pixel readout chip using PbSn solder...
Chandra X-Ray Observations of the Young Open Cluster NGC 2516 (2003)
Damiani Flaccomio Micela, F. Damiani, E. Flaccomio, G. Micela, S. Sciortino, F. R. Harnden, ...
We present a comprehensive study of the Chandra X-ray observations of the young open cluster NGC 2516. We have analyzed 8 individual Chandra observations. We have combined the data to achieve the...
Observational clues for a role of circumstellar accretion in PMS X-ray activity (2002)
Flaccomio, E., Micela, G., Sciortino, S.
We revisit the published analyses of ROSAT X-ray observations of the star forming regions NGC 2264 and Chamaeleon I (~3 and ~5 Myr old respectively) in the light of newly published optical data. At...
Flaccomio, E., Damiani, F., Micela, G., Sciortino, S., Harnden Jr., F. R., Murray, S. S., ...
In this first of two companion papers on the Orion Nebula Cluster (ONC), we present our analysis of a 63 Ksec Chandra HRC-I observation that yielded 742 X-ray detections within the 30'x30' field of...
Flaccomio, E., Damiani, F., Micela, G., Sciortino, S., Harnden Jr., F. R., Murray, S. S., ...
Using the results of our first paper on the Chandra HRC observation of the Orion Nebula Cluster (ONC), here we explore the relation between the coronal activity of its 1-Myr-old pre-main sequence...
A CVD diamond beam telescope for charged particle tracking (2002)
Adam,W., Berdermann,E., Bergonzo,P., De Boer,W., Bogani,F., Borchi,E., ...
Chemical vapor deposition (CVD) diamond is a radiation-hard sensor material that may be used for charged particle tracking near the interaction region in experiments at high-luminosity colliders. The...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W, Berdermann, E, Bergonzo, P, De Boer, W, Bogani, F, Borchi, E, ...
CVD diamond is a radiation hard sensor material which may be used for charged particle tracking near the interaction region in experiments at high luminosity colliders. The goal of the work described...
Performance of irradiated CVD diamond micro-strip sensors (2002)
Adam, W., Berdermann, E., Bergonzo, P., Bertuccio, G., Bogani, F., Borchi, E., ...
CVD diamond detectors are of interest for charged particle detection and tracking due to their high radiation tolerance. In this article we present, for the first time, beam test results from...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., Borchi, E., ...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W, Berdermann, E, Bergonzo, P, De Boer, W, Bogani, F, Borchi, E, ...
CVD diamond is a radiation hard sensor material which may be used for charged particle tracking near the interaction region in experiments at high luminosity colliders. The goal of the work described...
Performance of irradiated CVD diamond micro-strip sensors (2002)
Adam, W., Berdermann, E., Bergonzo, P., Bertuccio, G., Bogani, F., Borchi, E., ...
CVD diamond detectors are of interest for charged particle detection and tracking due to their high radiation tolerance. In this article we present, for the first time, beam test results from...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., Borchi, E., ...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W, Berdermann, E, Bergonzo, P, De Boer, W, Bogani, F, Borchi, E, ...
CVD diamond is a radiation hard sensor material which may be used for charged particle tracking near the interaction region in experiments at high luminosity colliders. The goal of the work described...
Performance of irradiated CVD diamond micro-strip sensors (2002)
Adam, W., Berdermann, E., Bergonzo, P., Bertuccio, G., Bogani, F., Borchi, E., ...
CVD diamond detectors are of interest for charged particle detection and tracking due to their high radiation tolerance. In this article we present, for the first time, beam test results from...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., Borchi, E., ...
A CVD diamond beam telescope for charged particle tracking (2002)
Adam, W., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., Borchi, E., ...
Chemical vapor deposition (CVD) diamond is a radiation-hard sensor material that may be used for charged particle tracking near the interaction region in experiments at high-luminosity colliders. The...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W, Berdermann, E, Bergonzo, P, De Boer, W, Bogani, F, Borchi, E, ...
CVD diamond is a radiation hard sensor material which may be used for charged particle tracking near the interaction region in experiments at high luminosity colliders. The goal of the work described...
Performance of irradiated CVD diamond micro-strip sensors (2002)
Adam, W., Berdermann, E., Bergonzo, P., Bertuccio, G., Bogani, F., Borchi, E., ...
CVD diamond detectors are of interest for charged particle detection and tracking due to their high radiation tolerance. In this article we present, for the first time, beam test results from...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., Borchi, E., ...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W, Berdermann, E, Bergonzo, P, De Boer, W, Bogani, F, Borchi, E, ...
CVD diamond is a radiation hard sensor material which may be used for charged particle tracking near the interaction region in experiments at high luminosity colliders. The goal of the work described...
Performance of irradiated CVD diamond micro-strip sensors (2002)
Adam, W., Berdermann, E., Bergonzo, P., Bertuccio, G., Bogani, F., Borchi, E., ...
CVD diamond detectors are of interest for charged particle detection and tracking due to their high radiation tolerance. In this article we present, for the first time, beam test results from...
A CVD Diamond Beam Telescope for Charged Particle Tracking (2002)
Adam, W., Berdermann, E., Bergonzo, P., De Boer, W., Bogani, F., Borchi, E., ...
Astronomy Astrophysics manuscript no. aa2680 (2002)
Doi Will Be, N. Pizzolato, A. Maggio, G. Micela, S. Sciortino, P. Ventura
We present the results of a new study on the relationship between coronal X-ray emission and stellar rotation in late-type main-sequence stars. We have selected a sample of 259 dwarfs in the B V...
A CVD diamond beam telescope for charged particle tracking (2001)
Adam, W, Berdermann, E, Bergonzo, P, De Boer, Wim, Bogani, F, Borchi, E, ...
CVD diamond is a radiation hard sensor material which may be used for charged particle tracking near the interaction region in experiments at high luminosity colliders. The goal of the work described...
The discovery of X-ray emission from the protostellar jet L1551 IRS5 (HH 154) (2001)
Favata, F., Fridlund, C. V. M., Micela, G., Sciortino, S., Kaas, A. A.
We have for the first time detected X-ray emission associated with a protostellar jet, on the jet emanating from the L1551 IRS5 protostar. The IRS5 protostar is hidden behind a very large absorbing...
Discovery of X-ray emission from the proto-stellar jet L1551 IRS5 (HH 154) (2001)
Favata, Fabio, Fridlund, C. V. M., Micela, G., Sciortino, S., Kaas, A. A.
We have for the first time detected X-ray emission associated with a proto-stellar jet, on the jet emanating from L1551 IRS5. The IRS5 proto-star is hidden beyond a very large absorbing column...
A ROSAT medium-sensitivity Galactic plane survey at 180 degrees (2001)
Morley, J.E., Briggs, K.R., Pye, J.P., Favata, F., Micela, G., Sciortino, S.
XMM-Newton survey of the low-metallicity open cluster NGC 2516 (2000)
Sciortino, S., Micela, G., Damiani, F., Flaccomio, E., Briggs, K., Denby, M., ...
We present the first results of an XMM-Newton EPIC survey of NGC 2516, a southern low-metallicity open cluster with an age close to the Pleiades. The attained limiting sensitivity is of ~ 2.4 10^-15...
Performance of irradiated CVD diamond micro-strip sensors (2000)
Adam, W, Berdermann, E, Bergonzo, P, Bertuccio, G, Bogani, F, Borchi, E, ...
CVD diamond detectors are of interest for charged particle detection and tracking due to their high radiation tolerance. In this article we present, for the first time, beam test results from...
A BeppoSAX and ROSAT view of the RCW86 supernova remnant (2000)
Bocchino, F., Vink, J., Favata, F., Maggio, A., Sciortino, S.
We present a spectral analysis of the Northern and Southwestern rim of the RCW86 X-ray shell, pointing out the remarkable differences between these two parts of the same object. In the North, a...
Micro-strip sensors based on CVD Diamond (2000)
Adam, W, Berdermann, E, Bergonzo, P, Bertuccio, G, Bogani, F, Borchi, E, ...
In this article we present the performance of recent chemical vapour deposition (CVD) diamond micro-strip sensors in beam tests. In addition we present the first comparison of a CVD diamond...
Micro-strip sensors based on CVD Diamond (2000)
Adam, W, Berdermann, E, Bergonzo, P, Bertuccio, G, Bogani, F, Borchi, E, ...
In this article we present the performance of recent chemical vapour deposition (CVD) diamond micro-strip sensors in beam tests. In addition we present the first comparison of a CVD diamond...
CMS : the TriDAS Project Technical Design Report; v.1, the Trigger Systems (2000)
L. Bayatyan, G., Grigorian, N., G. Khachatrian, V., T. Margarian, A., M. Sirunyan, A., Adam, W., ...
Pulse height distribution and radiation tolerance of CVD diamond detectors (2000)
Adam, W., Berdermann, E., Bergonzo, P., Bertuccio, G., Bogani, F., Borchi, E., ...
The paper reviews measurements of the radiation tolerance of CVD diamond for irradiation with 24 GeV/c protons, 300 MeV/c pions and 1 MeV neutrons. For proton and neutron irradiation, the measured...
CMS : the TriDAS Project Technical Design Report; v.1, the Trigger Systems (2000)
L. Bayatyan, G., Grigorian, N., G. Khachatrian, V., T. Margarian, A., M. Sirunyan, A., Adam, W., ...
Pulse height distribution and radiation tolerance of CVD diamond detectors (2000)
Adam, W., Berdermann, E., Bergonzo, P., Bertuccio, G., Bogani, F., Borchi, E., ...
The paper reviews measurements of the radiation tolerance of CVD diamond for irradiation with 24 GeV/c protons, 300 MeV/c pions and 1 MeV neutrons. For proton and neutron irradiation, the measured...
Will Be Inserted, F. Favata, G. Micela, F. Reale, S. Sciortino
We present a systematic analysis of the four known large X-ray flares detected to date on the eclipsing binary system Algol, using an approach based on hydrodynamic simulations of decaying flaring...
Will Be Inserted, N. Pizzolato, A. Maggio, S. Sciortino
We have investigated the variation of coronal X-ray emission during early post-main-sequence phases for a sample of 120 late-type stars within 100 pc, and with estimated masses in the range 1 -- 3 M...
An extreme X-ray flare observed on EV Lac by ASCA in July 1998 (1999)
Favata, F., Reale, F., Micela, G., Sciortino, S., Maggio, A., Matsumoto, H.
We present a long (150 ks elapsed time) ASCA X-ray observation of the dM3.5e star EV Lac, during which an exceptionally intense flaring event (lasting approximately 12 ks) was observed: at the...
Diamond particle detectors (1999)
Adam, W, Bauer, C, Berdermann, E, Bogani, F, Borchi, E, Bruzzi, Mara, ...
CVD diamond pixel detectors for LHC experiments (1999)
Wedenig, R., Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., ...
CVD diamond detectors for ionizing radiation (1999)
Friedl, M., Adam, W., Bauer, C., Berfermann, E., Bergonzo, P., Bogani, F., ...
In future HEP accelerators, such as the LHC (CERN), detectors and electronics in the vertex region of the experiments will suffer from extreme radiation. Thus radiation hardness is required for both...
Proton irradiation of CVD diamond detectors for high-luminosity experiments at the LHC (1999)
Meier, D., Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., ...
CVD diamond shows promising properties for use as a position sensitive detector for experiments in the highest radiation areas at the Large Hadron Collider. In order to study the radiation hardn ess...
Review of the development of diamond radiation sensors (1999)
Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., Borchi, E., ...
Diamond radiation sensors produced by chemical vapour deposition are studied for the application as tracking detectors in high luminosity experiments. Sensors with a charge collection distance up to...
The first bump-bonded pixel detectors on CVD diamond (1999)
Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., Borchi, E., ...
Diamond is a nearly ideal material for detecting ionising radiation. Its outstanding radiation hardness, fast charge collection and low leakage current allow it to be used in high radiation...
CVD diamond pixel detectors for LHC experiments (1999)
Wedenig, R., Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., ...
CVD diamond detectors for ionizing radiation (1999)
Friedl, M., Adam, W., Bauer, C., Berfermann, E., Bergonzo, P., Bogani, F., ...
In future HEP accelerators, such as the LHC (CERN), detectors and electronics in the vertex region of the experiments will suffer from extreme radiation. Thus radiation hardness is required for both...
Proton irradiation of CVD diamond detectors for high-luminosity experiments at the LHC (1999)
Meier, D., Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., ...
CVD diamond shows promising properties for use as a position sensitive detector for experiments in the highest radiation areas at the Large Hadron Collider. In order to study the radiation hardn ess...
Review of the development of diamond radiation sensors (1999)
Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., Borchi, E., ...
Diamond radiation sensors produced by chemical vapour deposition are studied for the application as tracking detectors in high luminosity experiments. Sensors with a charge collection distance up to...
The first bump-bonded pixel detectors on CVD diamond (1999)
Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., Borchi, E., ...
Diamond is a nearly ideal material for detecting ionising radiation. Its outstanding radiation hardness, fast charge collection and low leakage current allow it to be used in high radiation...
Proton irradiation of CVD diamond detectors for high-luminosity experiments at the LHC (1999)
Meier, D., Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., ...
CVD diamond shows promising properties for use as a position sensitive detector for experiments in the highest radiation areas at the Large Hadron Collider. In order to study the radiation hardn ess...
Proton irradiation of CVD diamond detectors for high-luminosity experiments at the LHC (1999)
Meier, D., Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., ...
CVD diamond shows promising properties for use as a position sensitive detector for experiments in the highest radiation areas at the Large Hadron Collider. In order to study the radiation hardn ess...
Proton irradiation of CVD diamond detectors for high-luminosity experiments at the LHC (1999)
Meier, D., Adam, W., Bauer, C., Berdermann, E., Bergonzo, P., Bogani, F., ...
CVD diamond shows promising properties for use as a position sensitive detector for experiments in the highest radiation areas at the Large Hadron Collider. In order to study the radiation hardn ess...
ROSAT PSPC Observation of the NE Region of the Vela Supernova Remnant (1999)
Iii The, F. Bocchino, A. Maggio, S. Sciortino
. We reconsider two ROSAT observations of the Vela SNR shock region, with the aim to overcome the problems encountered in interpreting the X-ray spectra in terms of single-temperature NEI emission...
Proton Irradiation of CVD Diamond Detectors for High Luminosity Experiments at the LHC (1998)
Meier, D, Adam, W, Bauer, C, Berdermann, E, Bergonzo, P, Bogani, F, ...
CVD diamond shows promising properties for use as a position sensitive detector for experiments in the highest radiation areas at the Large Hadron Collider. In order to study the radiation hardn ess...
Development of CVD diamond radiation detectors (1998)
Adam, W, Bauer, C, Berdermann, E, Bogani, F, Borchi, E, Bruzzi, Mara, ...
Diamond is a nearly ideal material for detecting ionizing radiation. Its outstanding radiation hardness, fast charge collection and low leakage current allow a diamond detector to be used in high ra...
Recent results on CVD diamond radiation sensors (1998)
Weilhammer, P., Adam, W., Bauer, C., Berdermann, E., Bogani, F., Borchi, E., ...
Status of diamond particle detectors (1998)
Krammer, M., Adam, W., Bauer, C., Berdermann, E., Bogani, F., Borchi, E., ...
Recent results on CVD diamond radiation sensors (1998)
Weilhammer, P., Adam, W., Bauer, C., Berdermann, E., Bogani, F., Borchi, E., ...
Status of diamond particle detectors (1998)
Krammer, M., Adam, W., Bauer, C., Berdermann, E., Bogani, F., Borchi, E., ...
On the widespread Weak-Line T-Tauri population detected in the ROSAT All-Sky Survey (1997)
Favata, F., Micela, G., Sciortino, S.
We discuss the apparent widespread presence of Weak-Line T-Tauri stars (WTTS) among stellar coronal sources detected in the ROSAT All-Sky Survey (RASS), and their relative number with respect to...
On coronal abundances derived with the SAX/LECS and ASCA/SIS detectors (1997)
Favata, F., Maggio, A., Peres, G., Sciortino, S.
We have studied the performance of global chi^2 fitting of low-resolution X-ray spectra in retrieving intrinsic source parameters, with emphasis on the coronal metallicity. The study has been...
Will Be Inserted, F. Favata, G. Micela, S. Sciortino
We discuss the apparent widespread presence of Weak-Line T-Tauri stars (WTTS) among stellar coronal sources detected in the ROSAT All-Sky Survey (RASS), and their relative number with respect to...
Will Be Inserted, S. Sciortino, F. Damiani, F. Favata, G. Micela
We have searched for low-mass pre-main-sequence stars in the nearby Upper Sco-Cen star-forming region using ROSAT observations analyzed with an innovative source detection method based on wavelet...
Will Be Inserted, F. Favata, A. Maggio, G. Peres, S. Sciortino
We have studied the performance of global fitting of low-resolutionX-ray spectra in retrieving intrinsic source parameters, with emphasis on the coronal metallicity. The study has been conducted by...
The EPIC system onboard the ESA XMM mission (1996)
Villa, G. E., Abbey, A. F., Arnaud, M., Balasini, M., Bignami, G. F., Boer, M., ...
Investigation of thermoluminescent properties of synthetic (CVD) diamond (1995)
Biggeri, U, Borchi, E, Bruzzi, Mara, Leroy, C, Sciortino, S, Bacci, T, ...
Favata Sciortino, G. Micela, F. Favata, S. Sciortino
We present the parallaxes, measured by Hipparcos, for a sample of X-ray selected stars. The stars belong to the stellar sample of the Einstein Extended Medium Sensitivity Survey. They are all at...
THE EVOLUTIONARY STATUS OF HIGH-LITHIUM, HIGH-ACTIVITY COOL DWARFS F. Favata
Micela Sciortino Antona, F. Favata, G. Micela, S. Sciortino
We have used the newly available Hipparcos precise parallaxes to study the evolutionary status of a number of high-lithium, high-activity late-type dwarfs found in X-ray based surveys, the Einstein...