From josla at kth.se  Fri Jan 27 09:23:32 2017
From: josla at kth.se (Josefin Larsson)
Date: Fri, 27 Jan 2017 08:23:32 +0000
Subject: [Okc-wp4] Fwd: Big Questions in Astrophysics (3-5 April 2017,
 Lund) - third announcement
References: <4898549E-D5CA-44EC-A44B-D1C49D0F510E@astro.lu.se>
Message-ID: <0B12B414-C9C7-4086-B47E-5DE795775F20@kth.se>


Reminder. Deadline for abstracts to the transients workshop is 31 Jan.

Josefin


Begin forwarded message:

From: Sofia Feltzing <sofia at astro.lu.se<mailto:sofia at astro.lu.se>>
Subject: Big Questions in Astrophysics (3-5 April 2017, Lund) - third announcement
Date: 9 Jan 2017 09:18:24 CET
To: <nordboard_info at astro.lu.se<mailto:nordboard_info at astro.lu.se>>
Reply-To: <eva at astro.lu.se<mailto:eva at astro.lu.se>>

Dear all,

We are very happy to announce that the full program for the plenary session of the
Big Questions in Astrophysics is now online (http://www.astro.lu.se/kawjubilee2017/plenary.shtml).

You find further information about the meeting, how to register and deadlines for registration at:

http://www.astro.lu.se/kawjubilee2017/

Note - participation is free, but you must register.

To attend the workshops on Monday and Wednesday you will have to attend the plenary meeting (4 April).

Deadline for abstracts to the workshops: 31 January 2017 (see also http://www.astro.lu.se/kawjubilee2017/registration.shtml)

If you have any questions you can reach the SOC/LOC via kawjubilee at astro.lu.se<mailto:kawjubilee at astro.lu.se>

On behalf of the SOC,
Sofia Feltzing


++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
Sofia Feltzing
Professor of astronomy
Lund Observatory, Sweden
Phone: +46-46-2227294
Email: sofia at astro.lu.se<mailto:sofia at astro.lu.se>
++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++






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From francesco.taddia at astro.su.se  Mon Feb  6 19:01:02 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Mon, 6 Feb 2017 18:01:02 +0000
Subject: [Okc-wp4] EO meeting Feb 9
Message-ID: <63C1CC85-BAEC-4E33-8B16-8B50A0B863DF@astro.su.se>

Dear all,

the first EO meeting of 2017 will be on Feb 9, at 13:00 in the usual KTH meeting room on floor 5.

We will have Raghnild Lunnan talking about: "Ca-rich Gap Transients: Extreme Objects in Extreme Locations”.

cheers

/Francesco


-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>








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From francesco.taddia at astro.su.se  Mon Feb 20 18:02:17 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Mon, 20 Feb 2017 17:02:17 +0000
Subject: [Okc-wp4] EO meeting Feb 23
Message-ID: <1BB72E5A-ED4A-4556-B34F-10C9C1E7FB54@astro.su.se>

Dear all,

on Thursday Feb 23rd (13:00-14:00) we have our next EO meeting.
Sergey Tsygankov from University of Turku, who is doing research in
 the field of accreting neutron stars, will talk about: "Low-level accretion onto highly magnetized neutron stars”.

Regards

/Francesco

-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From francesco.taddia at astro.su.se  Thu Feb 23 09:28:30 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 23 Feb 2017 08:28:30 +0000
Subject: [Okc-wp4] Reminder: EO meeting Feb 23
In-Reply-To: <1BB72E5A-ED4A-4556-B34F-10C9C1E7FB54@astro.su.se>
References: <1BB72E5A-ED4A-4556-B34F-10C9C1E7FB54@astro.su.se>
Message-ID: <CCDD1A40-E689-4E22-AA2F-FC747A30EF58@astro.su.se>

TODAY!!
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










On 20 Feb 2017, at 18:02, Francesco Taddia <ftadd at astro.su.se<mailto:ftadd at astro.su.se>> wrote:

Dear all,

on Thursday Feb 23rd (13:00-14:00) we have our next EO meeting.
Sergey Tsygankov from University of Turku, who is doing research in
 the field of accreting neutron stars, will talk about: "Low-level accretion onto highly magnetized neutron stars”.

Regards

/Francesco

-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











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From francesco.taddia at astro.su.se  Sun Mar  5 12:58:56 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Sun, 5 Mar 2017 11:58:56 +0000
Subject: [Okc-wp4] EO meeting on March 9th
Message-ID: <322A5880-F119-41CE-955B-85B142FA7330@astro.su.se>

Hi all,

this Thursday we will have our next EO meeting (13:00-14:00, KTHM meeting room on the 5th floor).
Giovanni Camelio (post-doc at the SU astronomy department) will give a talk titled:  Early evolution of newly born proto-neutron stars.

Here the abstract:
%%%%%%%%%%%
We evolve a proto-neutron star (PNS) with a nuclear many-body theory equation of state (EoS), for the first tens of seconds after the core bounce. In particular, we have determined the neutrino signal on terrestrial detectors and the frequencies of the gravitational waves due to stellar oscillations. Including rotation in an effective way, we also determine the time variation of the rotation rate and the neutrino angular momentum loss of the PNS with the GM3 mean-field EoS, and determine the corresponding gravitational wave signal due to rotation as the PNS contracts. We find that the mass shedding limit restricts the initial angular momentum and consequently the final rotation rate must be smaller than about 300 Hz for a PNS of about 1.6 solar masses. These results are obtained using a new code we have developed which describes the PNS evolution in spherical symmetry. This code integrates the neutrino number and energy transport equations together with the relativistic stellar structure equations by iteration. The neutrino cross sections are determined consistently with the underlying EoS. To include the many-body EoS in the evolution, we have find and tested a new fitting formula for the interacting part of the baryon free-energy, valid at finite temperature.
%%%%%%%%%%%

Regards


/Francesco


-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From francesco.taddia at astro.su.se  Sun Mar  5 15:16:24 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Sun, 5 Mar 2017 14:16:24 +0000
Subject: [Okc-wp4] EO meeting on March 9th
Message-ID: <F2DFB21D-B2DB-471E-9FE4-69C1D87FAF94@astro.su.se>

Hi all,

this Thursday we will have our next EO meeting (13:00-14:00, KTHM meeting room on the 5th floor).
Giovanni Camelio (post-doc at the SU astronomy department) will give a talk titled:  Early evolution of newly born proto-neutron stars.

Here the abstract:
%%%%%%%%%%%
We evolve a proto-neutron star (PNS) with a nuclear many-body theory equation of state (EoS), for the first tens of seconds after the core bounce. In particular, we have determined the neutrino signal on terrestrial detectors and the frequencies of the gravitational waves due to stellar oscillations. Including rotation in an effective way, we also determine the time variation of the rotation rate and the neutrino angular momentum loss of the PNS with the GM3 mean-field EoS, and determine the corresponding gravitational wave signal due to rotation as the PNS contracts. We find that the mass shedding limit restricts the initial angular momentum and consequently the final rotation rate must be smaller than about 300 Hz for a PNS of about 1.6 solar masses. These results are obtained using a new code we have developed which describes the PNS evolution in spherical symmetry. This code integrates the neutrino number and energy transport equations together with the relativistic stellar structure equations by iteration. The neutrino cross sections are determined consistently with the underlying EoS. To include the many-body EoS in the evolution, we have find and tested a new fitting formula for the interacting part of the baryon free-energy, valid at finite temperature.
%%%%%%%%%%%

Regards


/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From francesco.taddia at astro.su.se  Thu Mar  9 11:10:12 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 9 Mar 2017 10:10:12 +0000
Subject: [Okc-wp4] Reminder: EO meeting on March 9th
In-Reply-To: <F2DFB21D-B2DB-471E-9FE4-69C1D87FAF94@astro.su.se>
References: <F2DFB21D-B2DB-471E-9FE4-69C1D87FAF94@astro.su.se>
Message-ID: <D0CF0AA2-169E-4DA8-9ABC-A9DE16B5687D@astro.su.se>

TODAY!!
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










On 05 Mar 2017, at 15:16, Francesco Taddia <ftadd at astro.su.se<mailto:ftadd at astro.su.se>> wrote:

Hi all,

this Thursday we will have our next EO meeting (13:00-14:00, KTHM meeting room on the 5th floor).
Giovanni Camelio (post-doc at the SU astronomy department) will give a talk titled:  Early evolution of newly born proto-neutron stars.

Here the abstract:
%%%%%%%%%%%
We evolve a proto-neutron star (PNS) with a nuclear many-body theory equation of state (EoS), for the first tens of seconds after the core bounce. In particular, we have determined the neutrino signal on terrestrial detectors and the frequencies of the gravitational waves due to stellar oscillations. Including rotation in an effective way, we also determine the time variation of the rotation rate and the neutrino angular momentum loss of the PNS with the GM3 mean-field EoS, and determine the corresponding gravitational wave signal due to rotation as the PNS contracts. We find that the mass shedding limit restricts the initial angular momentum and consequently the final rotation rate must be smaller than about 300 Hz for a PNS of about 1.6 solar masses. These results are obtained using a new code we have developed which describes the PNS evolution in spherical symmetry. This code integrates the neutrino number and energy transport equations together with the relativistic stellar structure equations by iteration. The neutrino cross sections are determined consistently with the underlying EoS. To include the many-body EoS in the evolution, we have find and tested a new fitting formula for the interacting part of the baryon free-energy, valid at finite temperature.
%%%%%%%%%%%

Regards


/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











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From francesco.taddia at astro.su.se  Mon Mar 20 10:01:53 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Mon, 20 Mar 2017 09:01:53 +0000
Subject: [Okc-wp4] Next EO meeting on April 6th
Message-ID: <36378406-5B75-47A8-8478-E2446E5165C8@astro.su.se>

Dear all,

this week we do not plan our usual EO meeting, the next one will be on April 6th, and it will be about PoGOLite (plus a summary of the Lund
transient meeting).  Please contact me, Jesper, Stephan or Mette if you want to give one of our next EO talks.

cheers

/Francesco

-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From francesco.taddia at astro.su.se  Mon Mar 20 10:27:49 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Mon, 20 Mar 2017 09:27:49 +0000
Subject: [Okc-wp4] Next EO meeting on April 6th
In-Reply-To: <36378406-5B75-47A8-8478-E2446E5165C8@astro.su.se>
References: <36378406-5B75-47A8-8478-E2446E5165C8@astro.su.se>
Message-ID: <0F4A721D-CC7A-48D8-B9E7-094AC35C435A@astro.su.se>

PoGo+ of course :)
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>



On 20 Mar 2017, at 10:01, Francesco Taddia <francesco.taddia at astro.su.se<mailto:francesco.taddia at astro.su.se>> wrote:

Dear all,

this week we do not plan our usual EO meeting, the next one will be on April 6th, and it will be about PoGOLite (plus a summary of the Lund
transient meeting).  Please contact me, Jesper, Stephan or Mette if you want to give one of our next EO talks.

cheers

/Francesco

-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











-------------------------------------------------
okc-wp4 at albanova.se<mailto:okc-wp4 at albanova.se> mailing list

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From francesco.taddia at astro.su.se  Tue Apr  4 08:55:44 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Tue, 4 Apr 2017 06:55:44 +0000
Subject: [Okc-wp4] EO meeting on April 6th
Message-ID: <E354F85F-EC89-42AB-833B-0EFC79E569E4@astro.su.se>

Dear all,

this Thursday we have our EO meeting. Instead of the Pogo+ talk previously announced,
we will have Evan O’Connor talking about CC supernovae.

Usual place (KTH meeting room, 5th floor) and time (13:00-14:00).

cheers

/Francesco

-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From francesco.taddia at astro.su.se  Thu Apr  6 10:59:30 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 6 Apr 2017 08:59:30 +0000
Subject: [Okc-wp4] EO meeting on April 6th
In-Reply-To: <E354F85F-EC89-42AB-833B-0EFC79E569E4@astro.su.se>
References: <E354F85F-EC89-42AB-833B-0EFC79E569E4@astro.su.se>
Message-ID: <4C1FCA91-327A-40E7-A576-7AC41586FC06@astro.su.se>

In two hours!!
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










On 04 Apr 2017, at 08:55, Francesco Taddia <francesco.taddia at astro.su.se<mailto:francesco.taddia at astro.su.se>> wrote:

Dear all,

this Thursday we have our EO meeting. Instead of the Pogo+ talk previously announced,
we will have Evan O’Connor talking about CC supernovae.

Usual place (KTH meeting room, 5th floor) and time (13:00-14:00).

cheers

/Francesco

-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











-------------------------------------------------
okc-wp4 at albanova.se<mailto:okc-wp4 at albanova.se> mailing list

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From francesco.taddia at astro.su.se  Wed Apr 19 16:13:49 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Wed, 19 Apr 2017 14:13:49 +0000
Subject: [Okc-wp4] EO meeting on April 27th
Message-ID: <D047DC81-6674-4DC3-B5FF-D3A3DDFDF6DA@astro.su.se>

Hi all,

next EO meeting will be on April 27th, 13:00-14:00 (5th floor, KTH meeting room),
I will present two papers on stripped-envelope supernovae, that have been recently submitted for publication.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From francesco.taddia at astro.su.se  Thu Apr 27 09:27:26 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 27 Apr 2017 07:27:26 +0000
Subject: [Okc-wp4] Reminder: EO meeting on April 27th
In-Reply-To: <D047DC81-6674-4DC3-B5FF-D3A3DDFDF6DA@astro.su.se>
References: <D047DC81-6674-4DC3-B5FF-D3A3DDFDF6DA@astro.su.se>
Message-ID: <28088484-47AA-44AC-8379-25C08F8DCF9F@astro.su.se>


TODAY!!


On 19 Apr 2017, at 16:13, Francesco Taddia <ftadd at astro.su.se<mailto:ftadd at astro.su.se>> wrote:

Hi all,

next EO meeting will be on April 27th, 13:00-14:00 (5th floor, KTH meeting room),
I will present two papers on stripped-envelope supernovae, that have been recently submitted for publication.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











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From francesco.taddia at astro.su.se  Thu Apr 27 09:27:28 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 27 Apr 2017 07:27:28 +0000
Subject: [Okc-wp4] Reminder: EO meeting on April 27th
In-Reply-To: <D047DC81-6674-4DC3-B5FF-D3A3DDFDF6DA@astro.su.se>
References: <D047DC81-6674-4DC3-B5FF-D3A3DDFDF6DA@astro.su.se>
Message-ID: <8597086A-A1DF-4872-ABB7-9A6EC999401F@astro.su.se>


TODAY!!


On 19 Apr 2017, at 16:13, Francesco Taddia <ftadd at astro.su.se<mailto:ftadd at astro.su.se>> wrote:

Hi all,

next EO meeting will be on April 27th, 13:00-14:00 (5th floor, KTH meeting room),
I will present two papers on stripped-envelope supernovae, that have been recently submitted for publication.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











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From francesco.taddia at astro.su.se  Wed May 10 10:17:03 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Wed, 10 May 2017 08:17:03 +0000
Subject: [Okc-wp4] EO meeting tomorrow
Message-ID: <B7E8C48F-B014-4C2D-AC2B-BC0AE6474D7E@astro.su.se>

Hi all,

tomorrow at 13:00 on the 5th floor we will have our usual EO meeting, this time with two speakers:

a) Chloé Maury, an Erasmus student from Toulouse,  will talk about  “Constructing compact stars in a computer”.

b) Stephan Rosswog will talk about the experience of being the guest editor
   with Classical and Quantum Gravity of the special issue “Rattle and shine:
   the signals of compact binary mergers”. He will mostly discuss one of the papers
   in this special issue by Foucart on neutron star black hole mergers.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From francesco.taddia at astro.su.se  Thu May 11 09:45:48 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 11 May 2017 07:45:48 +0000
Subject: [Okc-wp4] EO meeting
In-Reply-To: <B7E8C48F-B014-4C2D-AC2B-BC0AE6474D7E@astro.su.se>
References: <B7E8C48F-B014-4C2D-AC2B-BC0AE6474D7E@astro.su.se>
Message-ID: <DE642EE6-A4CE-445C-8D2B-03F5086D9B07@astro.su.se>

TODAY!!
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










On 10 May 2017, at 10:17, Francesco Taddia <ftadd at astro.su.se<mailto:ftadd at astro.su.se>> wrote:

Hi all,

tomorrow at 13:00 on the 5th floor we will have our usual EO meeting, this time with two speakers:

a) Chloé Maury, an Erasmus student from Toulouse,  will talk about  “Constructing compact stars in a computer”.

b) Stephan Rosswog will talk about the experience of being the guest editor
   with Classical and Quantum Gravity of the special issue “Rattle and shine:
   the signals of compact binary mergers”. He will mostly discuss one of the papers
   in this special issue by Foucart on neutron star black hole mergers.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











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From francesco.taddia at astro.su.se  Thu May 11 09:45:46 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 11 May 2017 07:45:46 +0000
Subject: [Okc-wp4] EO meeting
In-Reply-To: <B7E8C48F-B014-4C2D-AC2B-BC0AE6474D7E@astro.su.se>
References: <B7E8C48F-B014-4C2D-AC2B-BC0AE6474D7E@astro.su.se>
Message-ID: <1D3E8F74-CD0C-4697-A60B-4DA37E90526A@astro.su.se>

TODAY!!
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










On 10 May 2017, at 10:17, Francesco Taddia <ftadd at astro.su.se<mailto:ftadd at astro.su.se>> wrote:

Hi all,

tomorrow at 13:00 on the 5th floor we will have our usual EO meeting, this time with two speakers:

a) Chloé Maury, an Erasmus student from Toulouse,  will talk about  “Constructing compact stars in a computer”.

b) Stephan Rosswog will talk about the experience of being the guest editor
   with Classical and Quantum Gravity of the special issue “Rattle and shine:
   the signals of compact binary mergers”. He will mostly discuss one of the papers
   in this special issue by Foucart on neutron star black hole mergers.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











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From francesco.taddia at astro.su.se  Mon May 29 14:30:16 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Mon, 29 May 2017 12:30:16 +0000
Subject: [Okc-wp4] EO meeting on June 1st
Message-ID: <4687F5EE-1C24-4C06-8758-F9D582764DBA@astro.su.se>

Hi all,

on Thursday (13:00-14:00, usual room on the 5th floor) Serena Falocco will give a talk titled: "The XMM view of NGC6217: evidence for an extended X-ray jet from a complex galactic nucleus”.

Here the abstract:

NGC6217 is a nearby (z=0.005) spiral galaxy. A variety of multi band data highlights various aspects of its central core resulting in multiple types of classifications, from a pure starburst to a Seyfert nucleus. Pietsch+2001 reported a jet emanating from the nucleus of NGC6217 in the Rosat X-ray images. The structure is composed by three knots and it is extended over 19 kpc.
We have studied four observations from XMM Newton satellite, studying the images and the spectra of the central core and the knots in order to understand their nature. The spectra of the central core are well represented by a complex starburst-AGN core. The XMM images confirm the presence of the jet structure. The spectra of the knots are harder than the spectrum of the core, in agreement with the jet hypothesis. Additional HST and VLA data display a complex nucleus with several condensations, suggesting a low luminosity AGN core coexisting with a starburst region. The accretion rate estimated in our study is consistent with an ADAF accretion mode.


cheers

/Francesco

-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From peter at astro.su.se  Tue May 30 17:26:42 2017
From: peter at astro.su.se (Peter Lundqvist)
Date: Tue, 30 May 2017 15:26:42 +0000
Subject: [Okc-wp4] Fwd: Licentiate seminar 31st May at 13:00
References: <1E773D5B-99D2-46C5-89FD-2BDF7AE4761F@astro.su.se>
Message-ID: <4203CA1C-6C0B-44CB-BE92-90F64C8DE2C4@astro.su.se>

Hi,

this is just to let you know about the licentiate seminar tomorrow.
It’s about modeling radio observations of Type Ia supernovae.

Best,
-Peter

Begin forwarded message:

From: Peter Lundqvist <peter at astro.su.se<mailto:peter at astro.su.se>>
Subject: Fwd: Licentiate seminar 31st May
Date: 30 May 2017 13:03:02 GMT+2
To: "alla at astro.su.se<mailto:alla at astro.su.se>" <alla at astro.su.se<mailto:alla at astro.su.se>>

Dear “alla”,

this is to remind you about tomorrow’s licentiate seminar by Esha at 13:00 in FB42.
(See below).

-Peter

Begin forwarded message:

From: Esha Kundu <esha.kundu at astro.su.se<mailto:esha.kundu at astro.su.se>>
Subject: Licentiate seminar 31st May
Date: 12 May 2017 17:27:44 GMT+2
To: "alla at astro.su.se<mailto:alla at astro.su.se>" <alla at astro.su.se<mailto:alla at astro.su.se>>

Dear all,

I will defend my licentiate thesis on 31st May 2017 at 13:00  in FB42. The title of the thesis is "Modeling of Radio Emission from Supernovae: Application to Type Ia" . The thesis can be found in the following link

https://ttt.astro.su.se/~esku1278/licentiate_thesis_esha.pdf

Regards,
Esha



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From francesco.taddia at astro.su.se  Thu Jun  1 09:37:40 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 1 Jun 2017 07:37:40 +0000
Subject: [Okc-wp4] Reminder: EO meeting on June 1st
In-Reply-To: <4687F5EE-1C24-4C06-8758-F9D582764DBA@astro.su.se>
References: <4687F5EE-1C24-4C06-8758-F9D582764DBA@astro.su.se>
Message-ID: <B27C82DE-C07C-4AFE-986D-AB4F089BAAAA@astro.su.se>

Today!!
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










On 29 May 2017, at 14:30, Francesco Taddia <ftadd at astro.su.se<mailto:ftadd at astro.su.se>> wrote:

Hi all,

on Thursday (13:00-14:00, usual room on the 5th floor) Serena Falocco will give a talk titled: "The XMM view of NGC6217: evidence for an extended X-ray jet from a complex galactic nucleus”.

Here the abstract:

NGC6217 is a nearby (z=0.005) spiral galaxy. A variety of multi band data highlights various aspects of its central core resulting in multiple types of classifications, from a pure starburst to a Seyfert nucleus. Pietsch+2001 reported a jet emanating from the nucleus of NGC6217 in the Rosat X-ray images. The structure is composed by three knots and it is extended over 19 kpc.
We have studied four observations from XMM Newton satellite, studying the images and the spectra of the central core and the knots in order to understand their nature. The spectra of the central core are well represented by a complex starburst-AGN core. The XMM images confirm the presence of the jet structure. The spectra of the knots are harder than the spectrum of the core, in agreement with the jet hypothesis. Additional HST and VLA data display a complex nucleus with several condensations, suggesting a low luminosity AGN core coexisting with a starburst region. The accretion rate estimated in our study is consistent with an ADAF accretion mode.


cheers

/Francesco

-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











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From francesco.taddia at astro.su.se  Fri Jun  2 11:13:32 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Fri, 2 Jun 2017 09:13:32 +0000
Subject: [Okc-wp4] Last EO meeting before summer on Thursday June 8th (13:00,
 KTH meeting room 5th floor)
Message-ID: <AD4CFA9D-915A-4652-9969-17FBD13891F4@astro.su.se>

Hi all,

next week we will have our last EO meeting before summer.
Lutz Köpke from University of Mainz will give a talk titled: "The next galactic supernova with the IceCube observatory”

Here the abstract:

Core collapse supernovae are expected to occur in our galaxy about twice per century.  As the inner region of the star cannot be studied with electromagnetic probes, neutrinos provide unique insights into the internal mechanisms in place during the core collapse.  With about 500.000 recorded O(10 MeV) neutrino interactions for a supernova at the galactic center, IceCube offers unrivaled statistical precision and will remain competitive even when future neutrino detectors are realized. The basic detection principle and simulations that address selected particle and astrophysical aspects will be discussed. As the signal is observed on top of a large dark rate background, IceCube cannot resolve individual neutrino interactions at these low energies to determine energy, direction and the neutrino type. Investigations that help to remedy this situation and joint measurements of various neutrino and gravitational wave experiments will be mentioned.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From cfinley at fysik.su.se  Wed Jun  7 22:44:02 2017
From: cfinley at fysik.su.se (Chad Finley)
Date: Wed, 7 Jun 2017 22:44:02 +0200
Subject: [Okc-wp4] Last EO meeting before summer, tomorrow
In-Reply-To: <AD4CFA9D-915A-4652-9969-17FBD13891F4@astro.su.se>
References: <AD4CFA9D-915A-4652-9969-17FBD13891F4@astro.su.se>
Message-ID: <12c835e1-966f-482a-c577-48f14a95de74@fysik.su.se>

Hi all,

Reminder for tomorrow's EO meeting, last before the summer.  Lutz is the 
coordinator of supernova neutrino detection with IceCube, he is spending 
his sabbatical in Uppsala and we are stealing him down for a talk for 
the day.

best,
chad


-------- Forwarded Message --------
Subject: 	[Okc-wp4] Last EO meeting before summer on Thursday June 8th 
(13:00, KTH meeting room 5th floor)
Date: 	Fri, 2 Jun 2017 09:13:32 +0000
From: 	Francesco Taddia <francesco.taddia at astro.su.se>
To: 	Okc-wp4 at fysik.su.se <Okc-wp4 at fysik.su.se>



Hi all,

next week we will have our last EO meeting before summer.
Lutz Köpke from University of Mainz will give a talk titled: "The next 
galactic supernova with the IceCube observatory”

Here the abstract:

Core collapse supernovae are expected to occur in our galaxy about twice 
per century.  As the inner region of the star cannot be studied with 
electromagnetic probes, neutrinos provide unique insights into the 
internal mechanisms in place during the core collapse.  With about 
500.000 recorded O(10 MeV) neutrino interactions for a supernova at the 
galactic center, IceCube offers unrivaled statistical precision and will 
remain competitive even when future neutrino detectors are realized. The 
basic detection principle and simulations that address selected particle 
and astrophysical aspects will be discussed. As the signal is observed 
on top of a large dark rate background, IceCube cannot resolve 
individual neutrino interactions at these low energies to determine 
energy, direction and the neutrino type. Investigations that help to 
remedy this situation and joint measurements of various neutrino and 
gravitational wave experiments will be mentioned.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se <mailto:ftadd at astro.su.se>










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From alexandra.veledina at su.se  Tue Aug 22 09:07:31 2017
From: alexandra.veledina at su.se (Alexandra Veledina)
Date: Tue, 22 Aug 2017 09:07:31 +0200
Subject: [Okc-wp4] Fwd: Nordita Astrophysics Seminar Wed. Aug 23 @ 13:30
In-Reply-To: <8e559fd82c1e4ebb8e4df195177cb5aa@ebox-prod-srv10.win.su.se>
References: <8e559fd82c1e4ebb8e4df195177cb5aa@ebox-prod-srv10.win.su.se>
Message-ID: <CADmUZa7=1RhO8TgD838o_hSiAaqJs1_QrinLjJ3f7C02J2U60g@mail.gmail.com>

There will be a seminar on magnetars tomorrow (Wednesday) in Nordita
Astrophysics building.

Welcome!

Alexandra

---------- Forwarded message ----------
From: Livia Vallini <livia.vallini at su.se>
Date: 22 August 2017 at 07:57
Subject: Nordita Astrophysics Seminar Wed. Aug 23 @ 13:30
To: "people at nordita.org" <people at nordita.org>, "alla at astro.su.se" <
alla at astro.su.se>


Dear All,

The next Nordita Astrophysics Seminar will be tomorrow *Wednesday Aug 23 at
13:30* (room 122:026*, Nordita West Building*).

Speaker:
Andrei M. Beloborodov (Columbia Univ.)

Title:
*Physics of magnetars*

Abstract:
Magnetars are neutron stars born with ultra-strong magnetic fields. Their
spectacular X-ray activity is fed by dissipation of magnetic energy. The
dissipation mechanism will be discussed, including processes inside and
around the star.

Welcome!

Add to calendar: http://agenda.albanova.se/conferenceDisplay.py/ica
l?confId=6315

-- 

Livia Vallini
Nordita Fellow
KTH Royal Institute of Technology
and Stockholm University
Roslagstullsbacken 23
106 91 Stockholm



-- 
Nordita fellow


KTH Royal Institute of Technology and Stockholm University
Roslagstullsbacken 23, SE-106 91 Stockholm, Sweden
E-mail : alexandra.veledina at gmail.com, alexandra.veledina at su.se
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From juri.poutanen at gmail.com  Fri Aug 25 15:20:17 2017
From: juri.poutanen at gmail.com (Juri Poutanen)
Date: Fri, 25 Aug 2017 15:20:17 +0200
Subject: [Okc-wp4] Nordita workshop on particle energization problems
Message-ID: <0F84EE5F-CDB8-47E2-84C8-5B57D27F8D9D@gmail.com>

Dear colleagues, 

during the next week we will hosting a workshop "Exascale thinking of particle energization problems” at Nordita 
astrophysics building. 

The workshop aims to discuss the state-of-the-art approaches, challenges for the next-generation hybrid MHD-PiC and radiation-PiC methods and outline the problems to be answered by the new exascale simulations of Nature in silico. It will bring together experts in high-performance computing, numerical methods, plasma physics and radiative processes. 

The program of the workshop is available at http://www.nordita.org/exa2017 

You are welcome to listen to the talks. 

Best regards,
workshop organizers

Axel Brandenburg 
Aake Nordlund 
Joonas Nättilä
Juri Poutanen 
Alexandra Veledina



From francesco.taddia at astro.su.se  Thu Aug 31 13:26:16 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 31 Aug 2017 11:26:16 +0000
Subject: [Okc-wp4] Next EO meetings
Message-ID: <4E38834B-0BA0-40B4-8892-CC7D013B3147@astro.su.se>

Dear all,

it is time to restart our extreme object meetings after the summer break.

Mark these first three dates on your calendar:

1) Next Thursday, 7/9, Federica Bianco (Center for Urban Science and Progress
 and NYU Center for Cosmology and Particle Physics) will talk about LSST and
the recent adventures of an astrophysicist in urban science.

2) On 28/9, we will have a talk titled "Shedding new light on the Crab with polarized X-rays" by the PoGo+ collaboration.

3) On 12/10 we want to have another EO meeting, and
we kindly ask for volunteers to give a talk!

The meetings will be at 13:00-14:00, @ KTH meeting room on the 5th floor.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>










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From francesco.taddia at astro.su.se  Thu Sep  7 11:48:04 2017
From: francesco.taddia at astro.su.se (Francesco Taddia)
Date: Thu, 7 Sep 2017 09:48:04 +0000
Subject: [Okc-wp4] Reminder: EO meeting today
In-Reply-To: <4E38834B-0BA0-40B4-8892-CC7D013B3147@astro.su.se>
References: <4E38834B-0BA0-40B4-8892-CC7D013B3147@astro.su.se>
Message-ID: <173DFE24-CF45-47E1-8BA1-1ECC1CEB2CD3@astro.su.se>



TODAY,

Federica Bianco (Center for Urban Science and Progress and
 NYU Center for Cosmology and Particle Physics) will talk about LSST and
the recent adventures of an astrophysicist in urban science.
 The meetings will be at 13:00-14:00, @ KTH meeting room on the 5th floor.


cheers

/Francesco

-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>




On 31 Aug 2017, at 13:26, Francesco Taddia <ftadd at astro.su.se<mailto:ftadd at astro.su.se>> wrote:

Dear all,

it is time to restart our extreme object meetings after the summer break.

Mark these first three dates on your calendar:

1) Next Thursday, 7/9, Federica Bianco (Center for Urban Science and Progress
 and NYU Center for Cosmology and Particle Physics) will talk about LSST and
the recent adventures of an astrophysicist in urban science.

2) On 28/9, we will have a talk titled "Shedding new light on the Crab with polarized X-rays" by the PoGo+ collaboration.

3) On 12/10 we want to have another EO meeting, and
we kindly ask for volunteers to give a talk!

The meetings will be at 13:00-14:00, @ KTH meeting room on the 5th floor.

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











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From ftadd at astro.su.se  Tue Sep 26 16:42:55 2017
From: ftadd at astro.su.se (Francesco Taddia)
Date: Tue, 26 Sep 2017 16:42:55 +0200
Subject: [Okc-wp4] EO meeting this Thursday
In-Reply-To: <4E38834B-0BA0-40B4-8892-CC7D013B3147@astro.su.se>
References: <4E38834B-0BA0-40B4-8892-CC7D013B3147@astro.su.se>
Message-ID: <0E1C8FA4-A8DA-45F5-8183-C5F1556931BF@astro.su.se>

Hi all,

here the speaker, the updated title and the abstract of the next EO talk, which will be this Thursday:

Speaker: Victor Mikhalev

Title:PoGO+ measurement of Crab emissions in the hard X-ray band.
 
Abstract: PoGO+ is a purpose-built and calibrated balloon borne polarimeter flown from the north of Sweden in the summer of 2016. The polarization of emissions from the Crab, as measured during the flight in 2016 is reported for the energy range (~20-160 keV). The Crab is a complex system consisting of a central pulsar, a diffuse pulsar wind nebula, as well as structures in the inner nebula including a jet and torus. Source and background observations are interspersed allowing for a rigorous background subtraction eliminating systematic effects. The polarization vector is found to be aligned with the spin axis of the pulsar for a polarization fraction, PF = (20.9 ± 5.0)%. Contrary to measurements at higher energies, no significant temporal evolution of phase-integrated polarisation parameters is observed. Through phase selections the off-pulse (OP) and pulsar (P1, P2) can be studied separately. The polarization properties of nebula dominated OP are compatible with the phase-integrated results. The polarization parameters for the pulsar itself (P2) are measured and are consistent with observations at optical wavelengths. Additionally, the instrument design and analysis methodology is detailed.



cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se <mailto:ftadd at astro.su.se>









> On 31 Aug 2017, at 13:26, Francesco Taddia <francesco.taddia at astro.su.se> wrote:
> 
> Dear all,
> 
> it is time to restart our extreme object meetings after the summer break.
> 
> Mark these first three dates on your calendar:
> 
> 1) Next Thursday, 7/9, Federica Bianco (Center for Urban Science and Progress
>  and NYU Center for Cosmology and Particle Physics) will talk about LSST and 
> the recent adventures of an astrophysicist in urban science.
> 
> 2) On 28/9, we will have a talk titled "Shedding new light on the Crab with polarized X-rays" by the PoGo+ collaboration.
> 
> 3) On 12/10 we want to have another EO meeting, and
> we kindly ask for volunteers to give a talk!
> 
> The meetings will be at 13:00-14:00, @ KTH meeting room on the 5th floor.
> 
> cheers
> 
> /Francesco
> -------------------------------------------
> Francesco Taddia
> Postdoctoral Researcher
> Department of Astronomy
> Stockholm University, Sweden
> ftadd at astro.su.se <mailto:ftadd at astro.su.se>
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> -------------------------------------------------
> okc-wp4 at albanova.se mailing list

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From ftadd at astro.su.se  Thu Sep 28 09:43:39 2017
From: ftadd at astro.su.se (Francesco Taddia)
Date: Thu, 28 Sep 2017 09:43:39 +0200
Subject: [Okc-wp4] Reminder: EO meeting today
In-Reply-To: <0E1C8FA4-A8DA-45F5-8183-C5F1556931BF@astro.su.se>
References: <4E38834B-0BA0-40B4-8892-CC7D013B3147@astro.su.se>
 <0E1C8FA4-A8DA-45F5-8183-C5F1556931BF@astro.su.se>
Message-ID: <49FA5D8D-E985-4956-9C84-AAF9597C9EEA@astro.su.se>

today!!
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se <mailto:ftadd at astro.su.se>

> On 26 Sep 2017, at 16:42, Francesco Taddia <ftadd at astro.su.se> wrote:
> 
> Hi all,
> 
> here the speaker, the updated title and the abstract of the next EO talk, which will be this Thursday:
> 
> Speaker: Victor Mikhalev
> 
> Title:PoGO+ measurement of Crab emissions in the hard X-ray band.
>  
> Abstract: PoGO+ is a purpose-built and calibrated balloon borne polarimeter flown from the north of Sweden in the summer of 2016. The polarization of emissions from the Crab, as measured during the flight in 2016 is reported for the energy range (~20-160 keV). The Crab is a complex system consisting of a central pulsar, a diffuse pulsar wind nebula, as well as structures in the inner nebula including a jet and torus. Source and background observations are interspersed allowing for a rigorous background subtraction eliminating systematic effects. The polarization vector is found to be aligned with the spin axis of the pulsar for a polarization fraction, PF = (20.9 ± 5.0)%. Contrary to measurements at higher energies, no significant temporal evolution of phase-integrated polarisation parameters is observed. Through phase selections the off-pulse (OP) and pulsar (P1, P2) can be studied separately. The polarization properties of nebula dominated OP are compatible with the phase-integrated results. The polarization parameters for the pulsar itself (P2) are measured and are consistent with observations at optical wavelengths. Additionally, the instrument design and analysis methodology is detailed.
> 
> 
> 
> cheers
> 
> /Francesco
> -------------------------------------------
> Francesco Taddia
> Postdoctoral Researcher
> Department of Astronomy
> Stockholm University, Sweden
> ftadd at astro.su.se <mailto:ftadd at astro.su.se>
> 
> 
> 
> 
> 
> 
> 
> 
> 
>> On 31 Aug 2017, at 13:26, Francesco Taddia <francesco.taddia at astro.su.se <mailto:francesco.taddia at astro.su.se>> wrote:
>> 
>> Dear all,
>> 
>> it is time to restart our extreme object meetings after the summer break.
>> 
>> Mark these first three dates on your calendar:
>> 
>> 1) Next Thursday, 7/9, Federica Bianco (Center for Urban Science and Progress
>>  and NYU Center for Cosmology and Particle Physics) will talk about LSST and 
>> the recent adventures of an astrophysicist in urban science.
>> 
>> 2) On 28/9, we will have a talk titled "Shedding new light on the Crab with polarized X-rays" by the PoGo+ collaboration.
>> 
>> 3) On 12/10 we want to have another EO meeting, and
>> we kindly ask for volunteers to give a talk!
>> 
>> The meetings will be at 13:00-14:00, @ KTH meeting room on the 5th floor.
>> 
>> cheers
>> 
>> /Francesco
>> -------------------------------------------
>> Francesco Taddia
>> Postdoctoral Researcher
>> Department of Astronomy
>> Stockholm University, Sweden
>> ftadd at astro.su.se <mailto:ftadd at astro.su.se>
>> 
>> 
>> 
>> 
>> 
>> 
>> 
>> 
>> 
>> 
>> -------------------------------------------------
>> okc-wp4 at albanova.se <mailto:okc-wp4 at albanova.se> mailing list
> 
> 
> -------------------------------------------------
> okc-wp4 at albanova.se mailing list

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From ftadd at astro.su.se  Wed Oct 11 11:23:43 2017
From: ftadd at astro.su.se (Francesco Taddia)
Date: Wed, 11 Oct 2017 11:23:43 +0200
Subject: [Okc-wp4] No EO meeting tomorrow
Message-ID: <1B2D95BC-AF72-4709-BD73-985637081F48@astro.su.se>

Hi all,

we could not find a speaker, so no EO meeting tomorrow…

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se <mailto:ftadd at astro.su.se>









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From jesper at astro.su.se  Fri Oct 27 11:26:48 2017
From: jesper at astro.su.se (Jesper Sollerman)
Date: Fri, 27 Oct 2017 09:26:48 +0000
Subject: [Okc-wp4] Fw: [OKC-CosmologyGravity] C&G extra seminar - Nov 1 @
 13:15 in A5:003
In-Reply-To: <BF0F0AF9-1630-4BAE-90F2-A426259725FC@fysik.su.se>
References: <1509093808557.20274@fysik.su.se>,
 <BF0F0AF9-1630-4BAE-90F2-A426259725FC@fysik.su.se>
Message-ID: <1509096408780.72185@astro.su.se>

This could be of interest also for the EO-list ?




Begin forwarded message:


Subject: [OKC-CosmologyGravity] C&G extra seminar - Nov 1 @ 13:15 in A5:003

Dear all,

a kind reminder that we will have an extra Cosmology and Gravity meeting next week:

when: November 1
where: A5:003
what time: 13:15

Mikael Rigault, from CNRS/IN2P3, will talk about supernova cosmology and bias in measurements of H0.

Link to the Agenda:
http://agenda.albanova.se/conferenceDisplay.py?confId=6350




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From ftadd at astro.su.se  Sat Oct 28 17:46:03 2017
From: ftadd at astro.su.se (Francesco Taddia)
Date: Sat, 28 Oct 2017 17:46:03 +0200
Subject: [Okc-wp4] EO meeting on Nov. 2nd
Message-ID: <20C18F19-4F12-496E-8319-2E8D53CE3AEC@astro.su.se>

Hi all,

next EO meeting on Nov. 2nd, Josh Simon will talk about
optical observations of gravitational wave sources.
Usual place  (KTH meeting room, 5th floor) and time (13:00-14:00),

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se <mailto:ftadd at astro.su.se>









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From ariel at fysik.su.se  Thu Nov  2 12:46:22 2017
From: ariel at fysik.su.se (Ariel Goobar)
Date: Thu, 2 Nov 2017 11:46:22 +0000
Subject: [Okc-wp4] EO meeting on Nov. 2nd
In-Reply-To: <20C18F19-4F12-496E-8319-2E8D53CE3AEC@astro.su.se>
References: <20C18F19-4F12-496E-8319-2E8D53CE3AEC@astro.su.se>
Message-ID: <7BBF6AF4-FCD3-4FF9-AB40-56F6A977954C@fysik.su.se>

In 10 minutes!
___________________________________________________________________
Professor Ariel Goobar
The Oskar Klein Centre for Cosmoparticle Physics
Department of Physics, Stockholm University
AlbaNova University Center, SE-106 91 Stockholm, SWEDEN
tel:+46 8 55378659 fax:+46 8 55378601 web: www.fysik.su.se/~ariel<http://www.fysik.su.se/~ariel>

On 28 Oct 2017, at 17:46, Francesco Taddia <ftadd at astro.su.se<mailto:ftadd at astro.su.se>> wrote:

Hi all,

next EO meeting on Nov. 2nd, Josh Simon will talk about
optical observations of gravitational wave sources.
Usual place  (KTH meeting room, 5th floor) and time (13:00-14:00),

cheers

/Francesco
-------------------------------------------
Francesco Taddia
Postdoctoral Researcher
Department of Astronomy
Stockholm University, Sweden
ftadd at astro.su.se<mailto:ftadd at astro.su.se>











-------------------------------------------------
okc-wp4 at albanova.se<mailto:okc-wp4 at albanova.se> mailing list

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From ftadd at astro.su.se  Tue Nov 21 18:29:05 2017
From: ftadd at astro.su.se (Francesco Taddia)
Date: Tue, 21 Nov 2017 18:29:05 +0100
Subject: [Okc-wp4] EO meeting on Thursday
Message-ID: <1B2E5BCD-E3F4-4C47-A5E2-FEFDB2DF67BA@astro.su.se>

Hi all,

this Thursday (Nov 23rd) at our EO meeting we will have Christoffer Lundman talking about 
radiation mediated shocks (specifically in the GRB context). We will meet at 13:00 on the 5th floor, KTH meeting room as usual.
see you there,


/Francesco


From ftadd at astro.su.se  Thu Nov 23 10:30:00 2017
From: ftadd at astro.su.se (Francesco Taddia)
Date: Thu, 23 Nov 2017 10:30:00 +0100
Subject: [Okc-wp4] Reminder: EO meeting on Thursday
In-Reply-To: <1B2E5BCD-E3F4-4C47-A5E2-FEFDB2DF67BA@astro.su.se>
References: <1B2E5BCD-E3F4-4C47-A5E2-FEFDB2DF67BA@astro.su.se>
Message-ID: <322F14CB-1F3B-4DAD-9C77-06EC7D16988C@astro.su.se>


TODAY!!!

> On 21 Nov 2017, at 18:29, Francesco Taddia <ftadd at astro.su.se> wrote:
> 
> Hi all,
> 
> this Thursday (Nov 23rd) at our EO meeting we will have Christoffer Lundman talking about 
> radiation mediated shocks (specifically in the GRB context). We will meet at 13:00 on the 5th floor, KTH meeting room as usual.
> see you there,
> 
> 
> /Francesco
> 


From jesper at astro.su.se  Thu Nov 30 11:02:27 2017
From: jesper at astro.su.se (Jesper Sollerman)
Date: Thu, 30 Nov 2017 10:02:27 +0000
Subject: [Okc-wp4] EO
In-Reply-To: <1B2E5BCD-E3F4-4C47-A5E2-FEFDB2DF67BA@astro.su.se>
References: <1B2E5BCD-E3F4-4C47-A5E2-FEFDB2DF67BA@astro.su.se>
Message-ID: <1512036147004.77329@astro.su.se>

Thanks a lot for those that organized the OKC Bottle. Good work, Nice event! 
And thanks Fawad for the talk.
/Jesper