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Notification:

Date: Tue, 30 Aug 2005 11:07:04 +0200
From: Melania Del Santo <melania.delsanto@rm.iasf.cnr.it>
Subject: Poster
To: conference2005@sciops.esa.int
Cc: sidoli@mi.iasf.cnr.it

Dear Sir,
please, we would like to present a poster at the conference,
concerning a Galactic source observed by INTEGRAL, XMM and Chandra.
At the time of my registration to the conference,
the data analysis was not ready, so I did not send you any abstract.
Is it too late?

Thanks in advance.
Regards.

Melania Del Santo

Reply 1

From: Nora Loiseau <xmmhelp@xmm.vilspa.esa.es>
To: melania.delsanto@rm.iasf.cnr.it
Subject: Re: Poster (PR#19259)
Date: Tue Aug 30 10:37:30 2005

Dear Melania,

many thanks for your interest in 'The X-ray Universe 2005'.
Yes, you can present your poster, although it is late to be
included in the abstacts booklet. Please send us the Title and 
Abstract in reply to this mail, and let us know the 
Science Topic of your proposed poster
(see http://www.congrex.nl/05a11/ -> Programme)
Any co-authors (if so, please also let us know their institutes)?

Kind regards,
 Nora Loiseau (local organizing committee)

Followup 1

Date: Wed, 31 Aug 2005 16:19:04 +0200
From: Melania Del Santo <melania.delsanto@rm.iasf.cnr.it>
Subject: Re: Poster (PR#19259)
To: Nora Loiseau <xmmhelp@xmm.vilspa.esa.es>

Dear Nora,
the Science Topic of my poster should be:

Interacting binary systems, magnetars, isolated neutron stars & pulsars


> Any co-authors (if so, please also let us know their institutes)?


For the moment:

Melania Del Santo  (1), Lara Sidoli (2), Angela Bazzano (1), et al.

(1)  IASF/INAF, via del Fosso del Cavaliere 100, 00133 Roma
(2) IASF/INAF - sez. Milano, via E. Bassini 15, 20133 Milano

The title is:

X and soft-gamma ray behaviour of the Galactic source 1E 1743.1-2843


Abstract:

The X-ray persistent source 1E 1743.1-2843, located in the Galactic Centre
direction, has been observed by all
X-ray satellite above 2 keV. Due to the the high column density along the
line-of-sight, the nature of
the binary system remains still unknown.
The gamma-ray satellite INTEGRAL has longly observed the Galactic Centre region
in the framework of the Core Programme.
We report on results of roughly 2 years of INTEGRAL observations of 1E
1743.7-2843 detected for the first time in the soft gamma-ray band.
Since the source does not show any evidence for strong variabilities,
we present the broad band spectral analysis using not simultaneous Chandra and
XMM-Newton observations.


Thanks.

Regards

Melania Del Santo


>
> Kind regards,
>  Nora Loiseau (local organizing committee)
>
>
>
>
>
>

Reply 2

From: Nora Loiseau <xmmhelp@xmm.vilspa.esa.es>
To: Esa.Conference.Bureau@esa.int
Subject:  Poster  (PR#19259)
Date: Wed Aug 31 16:36:39 2005

Dear Yolanda,

 you may find attached a new abstract for the XMM-Newton Conference, just
arrived.

 Please, include it in your database, and send the routine confirmation e-mail
to the first author, Melania del Santo (melania.delsanto@rm.iasf.cnr.it)

 Thanks in advance. Regards, Nora

Science Topic:

Interacting binary systems, magnetars, isolated neutron stars & pulsars

Authors:

Melania Del Santo  (1), Lara Sidoli (2), Angela Bazzano (1), et al.

(1)  IASF/INAF, via del Fosso del Cavaliere 100, 00133 Roma
(2) IASF/INAF - sez. Milano, via E. Bassini 15, 20133 Milano

Title:

X and soft-gamma ray behaviour of the Galactic source 1E 1743.1-2843


Abstract:

The X-ray persistent source 1E 1743.1-2843, located in the Galactic Centre
direction, has been observed by all
X-ray satellite above 2 keV. Due to the the high column density along the
line-of-sight, the nature of
the binary system remains still unknown.
The gamma-ray satellite INTEGRAL has longly observed the Galactic Centre region
in the framework of the Core Programme.
We report on results of roughly 2 years of INTEGRAL observations of 1E
1743.7-2843 detected for the first time in the soft gamma-ray band.
Since the source does not show any evidence for strong variabilities,
we present the broad band spectral analysis using not simultaneous Chandra and
XMM-Newton observations.


----
Dr. Nora Loiseau
XMM-Newton User Support Group