L. Guglielmi

Publication List Details

Period

1989 - 2008

Number

179

Co-Authors

Results of X-shooter data reduction software on laboratory frames (2008)

Goldoni, P., Royer, F., Horrobin, M., François, P., Guglielmi, L., Haigron, R., ...

We present the current state of the Data Reduction Software (DRS) being developed at APC, Paris Observatory, Amsterdam University and ESO for the X-shooter echelle spectrograph. X-shooter is the...

The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2007)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...

The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2007)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...

The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2007)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...

Archeops In-flight Performance, Data Processing and Map Making (2007)

Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...

Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...

Archeops In-flight Performance, Data Processing and Map Making (2007)

Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...

Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...

Archeops In-flight Performance, Data Processing and Map Making (2007)

Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...

Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...

Archeops: A High Resolution, Large Sky Coverage Balloon Experiment for Mapping CMB Anisotropies (2007)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bartlett, J., ...

Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (8 arcminutes) over a large fraction (25%) of the...

Cosmological constraints from Archeops (2007)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...

Cosmological constraints from Archeops (2007)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...

Cosmological constraints from Archeops (2007)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...

Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by Archeops (2007)

Ponthieu, N., Macias-Perez, J.F., Tristram, M., Ade, P., Amblard, A., Ansari, R., ...

We present the first measurement of temperature and polarization angular power spectra of the diffuse emission of Galactic dust at 353 GHz as seen by Archeops on 20% of the sky. The temperature...

Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by Archeops (2007)

Ponthieu, N., Macias-Perez, J.F., Tristram, M., Ade, P., Amblard, A., Ansari, R., ...

We present the first measurement of temperature and polarization angular power spectra of the diffuse emission of Galactic dust at 353 GHz as seen by Archeops on 20% of the sky. The temperature...

Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by Archeops (2007)

Ponthieu, N., Macias-Perez, J.F., Tristram, M., Ade, P., Amblard, A., Ansari, R., ...

We present the first measurement of temperature and polarization angular power spectra of the diffuse emission of Galactic dust at 353 GHz as seen by Archeops on 20% of the sky. The temperature...

Cosmological constraints from Archeops (2007)

Benoit, A., Rosset, C., Patanchon, G., Bargot, S., Ade, P., Amblard, A., ...

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops (2006)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops (2006)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops (2006)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...

The CMB temperature power spectrum from an improved analysis of the Archeops data (2006)

Tristram, M., Patanchon, G., Macias-Perez, J.F., Ade, P., Amblard, A., Ansari, R., ...

We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops flight. This...

The CMB temperature power spectrum from an improved analysis of the Archeops data (2006)

Tristram, M., Patanchon, G., Macias-Perez, J.F., Ade, P., Amblard, A., Ansari, R., ...

We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops flight. This...

The CMB temperature power spectrum from an improved analysis of the Archeops data (2006)

Tristram, M., Patanchon, G., Macias-Perez, J.F., Ade, P., Amblard, A., Ansari, R., ...

We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops flight. This...

Archeops In-flight Performance, Data Processing and Map Making (2006)

Macias-Perez, J. F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...

Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...

Archeops In-flight Performance, Data Processing and Map Making (2006)

Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...

Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...

Archeops In-flight Performance, Data Processing and Map Making (2006)

Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...

Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops (2005)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...

Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by Archeops (2005)

Ponthieu, N., Tristram, M., Ade, P., Amblard, A., Ansari, R., ...

We present the first measurement of temperature and polarization angular power spectra of the diffuse emission of Galactic dust at 353 GHz as seen by Archeops on 20% of the sky. The temperature...

Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by Archeops (2005)

Ponthieu, N., Macias-Perez, J.F., Tristram, M., Ade, P., Amblard, A., Ansari, R., ...

We present the first measurement of temperature and polarization angular power spectra of the diffuse emission of Galactic dust at 353 GHz as seen by Archeops on 20% of the sky. The temperature...

The CMB temperature power spectrum from an improved analysis of the Archeops data (2005)

Tristram, M., Patanchon, G., Macias-Perez, J.F., Ade, P., Amblard, A., Ansari, R., ...

We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops flight. This...

Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by Archeops (2005)

Ponthieu, N., Macias-Perez, J.F., Tristram, M., Ade, P., Amblard, A., Ansari, R., ...

We present the first measurement of temperature and polarization angular power spectra of the diffuse emission of Galactic dust at 353 GHz as seen by Archeops on 20% of the sky. The temperature...

The CMB temperature power spectrum from an improved analysis of the Archeops data (2005)

Tristram, M., Patanchon, G., Macias-Perez, J.F., Ade, P., Amblard, A., Ansari, R., ...

We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops flight. This...

Detection of Functional Platelet-Activating Factor Receptors on Leukemic B Cells of Chronic Lymphocytic Leukemic Patients. (2005)

Denizot, Y., Donnard, M., Guglielmi, L., Faucher, Jl, Jaccard, A., Bordessoule, D., ...

Although platelet-activating factor receptors (PAF-R) are reported on normal B cells, few results are available concerning leukemic ones. We demonstrated functional PAF-R on cell and nuclear surfaces...

The CMB temperature power spectrum from an improved analysis of the Archeops data (2004)

Tristram, M., Patanchon, G., Macias-Perez, J. F., Ade, P., Amblard, A., Ansari, R., ...

We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops flight. This...

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops (2004)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops (2004)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...

Mouse Embryonic Stem Cell Sorting for the Generation of Transgenic Mice by Sedimentation Field-Flow Fractionation. (2004)

Guglielmi, L., Battu, S., Le Bert, M., L. Faucher, J., Denizot, Y.

Mouse embryonic stem (ES) cells are an important tool for generation of transgenic mice and genetically modified mice. A rapid and efficient separation of ES cells that respects cell integrity,...

Hybrid Performance of the Pierre Auger Observatory and Reconstruction of Hybrid Events (2003)

Kick, B., Altmann, E., Alvarez, P., Bauleo, P., Bonifazi, C., Etchegoyen, A., ...

The Pierre Auger Observatory is a``hybrid'' UHECR detector. The surface detector (SD) and air fluorescence detector (FD) of the observatory are designed for observation of cosmic ray showers in...

The Lateral Distribution Function of Shower Signals in the Surface Detector of the Pierre Auger Observatory (2003)

Roth, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The surface detector (SD) array of the southern Pierre Auger Observatory will consist of a triangular grid of 1600 water Cherenkov tanks with 1.5 km spacing. For zenith angles less than 60deg the...

Processing of the Signals from the Surface Detectors of the Pierre - Auger Observatory (2003)

Suomijarvi, T., Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The detectors of the surface array of the Pierre Auger Observatory are water Cherenkov tanks. The signals from each tank are read out using three photomultipliers. The energy of the primary particle...

Calibration of the Pierre Auger fluorescence detector (2003)

Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The absolute calibration of an air fluorescence detector (FD) is an important element in correctly determining the energy of detected cosmic rays. The absolute calibration relates the flux of photons...

Performance of the Pierre Auger Fluorescence Detector and Analysis of well recontructed events (2003)

Argiro, S., Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The Pierre Auger Observatory is designed to elucidate the origin and nature of Ultra High Energy Cosmic Rays using a hybrid detection technique. A first run of data taking with a prototype version of...

Shower Studies at around $10^{18}$ eV with the Surface Detector of the Pierre Auger Observatory (2003)

Ghia, P-L., Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., ...

Three months of data taken by the Engineering Array Surface Detector of the Pierre Auger Observatory have been analyzed with the aim of setting a procedure for the study of showers at E_0 ~ 10^18 eV....

Atmospheric Monitoring for the Pierre Auger Fluorescence Detector (2003)

Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

Major uncertainties in the fluorescence energy measurement come from the precision of various atmospheric transmission, air Cerenkov subtraction, light multiple-scattering and cloud corrections. The...

The Anisotropy Search Program For the Pierre Auger Observatory (2003)

Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The Pierre Auger Southern Observatory in Argentina has begun taking data as it is being developed up to a final enclosed area of 3000 square kilometres. A key aspect of the project is to provide...

A Study Of Very Inclined Showers In The Pierre Auger Observatory (2003)

Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., Altmann, E., ...

The Engineering Array of the Auger Observatory has been running successfully since 2001 and inclined showers have been recorded from the start. We have analysed the events with zenith angle $>$...

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops (2003)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops (2003)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...

Cosmological constraints from Archeops (2003)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...

The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2003)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...

Hybrid Performance of the Pierre Auger Observatory and Reconstruction of Hybrid Events (2003)

Kick, B., Altmann, E., Alvarez, P., Bauleo, P., Bonifazi, C., Etchegoyen, A., ...

The Pierre Auger Observatory is a``hybrid'' UHECR detector. The surface detector (SD) and air fluorescence detector (FD) of the observatory are designed for observation of cosmic ray showers in...

The Lateral Distribution Function of Shower Signals in the Surface Detector of the Pierre Auger Observatory (2003)

Roth, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The surface detector (SD) array of the southern Pierre Auger Observatory will consist of a triangular grid of 1600 water Cherenkov tanks with 1.5 km spacing. For zenith angles less than 60deg the...

Processing of the Signals from the Surface Detectors of the Pierre - Auger Observatory (2003)

Suomijarvi, T., Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The detectors of the surface array of the Pierre Auger Observatory are water Cherenkov tanks. The signals from each tank are read out using three photomultipliers. The energy of the primary particle...

Calibration of the Pierre Auger fluorescence detector (2003)

Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The absolute calibration of an air fluorescence detector (FD) is an important element in correctly determining the energy of detected cosmic rays. The absolute calibration relates the flux of photons...

Performance of the Pierre Auger Fluorescence Detector and Analysis of well recontructed events (2003)

Argiro, S., Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The Pierre Auger Observatory is designed to elucidate the origin and nature of Ultra High Energy Cosmic Rays using a hybrid detection technique. A first run of data taking with a prototype version of...

Shower Studies at around $10^{18}$ eV with the Surface Detector of the Pierre Auger Observatory (2003)

Ghia, P-L., Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., ...

Three months of data taken by the Engineering Array Surface Detector of the Pierre Auger Observatory have been analyzed with the aim of setting a procedure for the study of showers at E_0 ~ 10^18 eV....

Atmospheric Monitoring for the Pierre Auger Fluorescence Detector (2003)

Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

Major uncertainties in the fluorescence energy measurement come from the precision of various atmospheric transmission, air Cerenkov subtraction, light multiple-scattering and cloud corrections. The...

The Anisotropy Search Program For the Pierre Auger Observatory (2003)

Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The Pierre Auger Southern Observatory in Argentina has begun taking data as it is being developed up to a final enclosed area of 3000 square kilometres. A key aspect of the project is to provide...

A Study Of Very Inclined Showers In The Pierre Auger Observatory (2003)

Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., Altmann, E., ...

The Engineering Array of the Auger Observatory has been running successfully since 2001 and inclined showers have been recorded from the start. We have analysed the events with zenith angle $>$...

Cosmological constraints from Archeops (2003)

Benoit, A., Rosset, C., Patanchon, G., Bargot, S., Ade, P., Amblard, A., ...

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...

The cosmic microwave background anisotropy power spectrum measured by Archeops (2003)

Benoit, A., Ade, P., Amblard, A., Ansari, R, Aubourg, E., Bargot, S., ...

We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...

Hybrid Performance of the Pierre Auger Observatory and Reconstruction of Hybrid Events (2003)

Kick, B., Altmann, E., Alvarez, P., Bauleo, P., Bonifazi, C., Etchegoyen, A., ...

The Pierre Auger Observatory is a``hybrid'' UHECR detector. The surface detector (SD) and air fluorescence detector (FD) of the observatory are designed for observation of cosmic ray showers in...

The Lateral Distribution Function of Shower Signals in the Surface Detector of the Pierre Auger Observatory (2003)

Roth, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The surface detector (SD) array of the southern Pierre Auger Observatory will consist of a triangular grid of 1600 water Cherenkov tanks with 1.5 km spacing. For zenith angles less than 60deg the...

Processing of the Signals from the Surface Detectors of the Pierre - Auger Observatory (2003)

Suomijarvi, T., Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The detectors of the surface array of the Pierre Auger Observatory are water Cherenkov tanks. The signals from each tank are read out using three photomultipliers. The energy of the primary particle...

Calibration of the Pierre Auger fluorescence detector (2003)

Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The absolute calibration of an air fluorescence detector (FD) is an important element in correctly determining the energy of detected cosmic rays. The absolute calibration relates the flux of photons...

Performance of the Pierre Auger Fluorescence Detector and Analysis of well recontructed events (2003)

Argiro, S., Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The Pierre Auger Observatory is designed to elucidate the origin and nature of Ultra High Energy Cosmic Rays using a hybrid detection technique. A first run of data taking with a prototype version of...

Shower Studies at around $10^{18}$ eV with the Surface Detector of the Pierre Auger Observatory (2003)

Ghia, P-L., Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., ...

Three months of data taken by the Engineering Array Surface Detector of the Pierre Auger Observatory have been analyzed with the aim of setting a procedure for the study of showers at E_0 ~ 10^18 eV....

Atmospheric Monitoring for the Pierre Auger Fluorescence Detector (2003)

Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

Major uncertainties in the fluorescence energy measurement come from the precision of various atmospheric transmission, air Cerenkov subtraction, light multiple-scattering and cloud corrections. The...

The Anisotropy Search Program For the Pierre Auger Observatory (2003)

Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The Pierre Auger Southern Observatory in Argentina has begun taking data as it is being developed up to a final enclosed area of 3000 square kilometres. A key aspect of the project is to provide...

A Study Of Very Inclined Showers In The Pierre Auger Observatory (2003)

Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., Altmann, E., ...

The Engineering Array of the Auger Observatory has been running successfully since 2001 and inclined showers have been recorded from the start. We have analysed the events with zenith angle $>$...

Cosmological constraints from Archeops (2003)

Benoit, A., Rosset, C., Patanchon, G., Bargot, S., Ade, P., Amblard, A., ...

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...

The cosmic microwave background anisotropy power spectrum measured by Archeops (2003)

Benoit, A., Ade, P., Amblard, A., Ansari, R, Aubourg, E., Bargot, S., ...

We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops (2003)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...

Cosmological constraints from Archeops (2003)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...

The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2003)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...

The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2002)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...

Cosmological constraints from Archeops (2002)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...

Archeops : a high resolution, large sky coverage balloon experiment for mapping cosmic microwave background anisotropies (2002)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bartlett, J., ...

Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (8 arcminutes) over a large fraction (25%) of the...

Archeops : a high resolution, large sky coverage balloon experiment for mapping cosmic microwave background anisotropies (2002)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bartlett, J., ...

Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (8 arcminutes) over a large fraction (25%) of the...

Membrane and Intracellular Platelet-Activating Factor Receptor Expression in Leukemic Blasts of Patients with Acute Myeloid and Lymphoid Leukemia (2002)

Donnard, M., Guglielmi, L., Turlure, P., Piguet, C., Couraud, M.J., Bordessoule, D., ...

Platelet-activating factor (PAF), a phospholipid mediator with a wide range of actions on mature leukocytes, acts through PAF-receptors (PAF-Rs) on the membranes of responsive cells. No results are...

Archeops: A High Resolution, Large Sky Coverage Balloon Experiment for Mapping CMB Anisotropies (2002)

Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bartlett, J., ...

Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (8 arcminutes) over a large fraction (25%) of the...

Gap-98-054 (1998)

Local Station Acquisition, Jm. Brunet, L. Guglielmi, C. Le Gall, G. Tristram

This paper is highly evolutive. You can nd the current version at : http://cd nfo.in2p3.fr/Experiences/Auger/auger.html : Discussion and Draft Papers / Local Station Controller Software / Acquisition...

Low-molecular-weight peptide inhibits RNA synthesis in human leukemic and phytohemagglutinin-stimulated leukocytes and globin mRNA transcription in differentiating Friend cells.

Amici, D, Rossi, G B, Cioé, L, Matarese, G P, Dolei, A, Guglielmi, L, ...

The RNA synthesis of human leukemic leukocytes and phytohemagglutinin-stimulated lymphocytes is markedly reduced by administration of a low-molecular-weight nonhistone peptide factor from calf...

Low-molecular-weight peptide inhibits RNA synthesis in human leukemic and phytohemagglutinin-stimulated leukocytes and globin mRNA transcription in differentiating Friend cells.

Amici, D, Rossi, G B, Cioé, L, Matarese, G P, Dolei, A, Guglielmi, L, ...

The RNA synthesis of human leukemic leukocytes and phytohemagglutinin-stimulated lymphocytes is markedly reduced by administration of a low-molecular-weight nonhistone peptide factor from calf...