Differences between revisions 1 and 5 (spanning 4 versions)
Revision 1 as of 2019-05-21 08:23:59
Size: 1656
Comment:
Revision 5 as of 2019-05-21 11:23:03
Size: 2012
Comment:
Deletions are marked like this. Additions are marked like this.
Line 29: Line 29:
eROSITA observations of the SNRs N132D and 1E0102-72
Line 33: Line 34:
Michael Freyberg, Manami Sasaki, Werner Becker, Frank Haberl, Konrad Dennerl Michael Freyberg, Manami Sasaki, Werner Becker, Frank Haberl, Konrad Dennerl (+ PhD Becker)
Line 40: Line 41:
 
Initially 1 year, with anticipated extension to
Line 42: Line 44:

==== Status ====

Approved within SNR/ISM WG (MF MS WB),

IEC membership recommended to start 05.08.2019 (45 days after launch, around first commissioning phase camera event data).

IEC membership also recommended by CAL WG (KD).

EroSnr EC Proposal 25

Proposal Date : 06-May-2019

External Collaborator

Name

First name

Institute

email

Plucinsky

Paul

CfA/Harvard

pplucinsky@cfa.harvard.edu

eROSITA_DE Proposing Member

Name

First name

Institute

email

Freyberg

Michael

MPE

mjf@mpe.mpg.de

Scientific Proposal

eROSITA observations of the SNRs N132D and 1E0102-72 Proposal

List of Potential Collaborators within eROSITA_DE

Michael Freyberg, Manami Sasaki, Werner Becker, Frank Haberl, Konrad Dennerl (+ PhD Becker)

Expected Outcome

* producing the highest quality calibration at low energies

Expected duration of the project

Initially 1 year, with anticipated extension to 4 years (Cal phase + 8 surveys with monitoring campaigns)

Status

Approved within SNR/ISM WG (MF MS WB),

IEC membership recommended to start 05.08.2019 (45 days after launch, around first commissioning phase camera event data).

IEC membership also recommended by CAL WG (KD).

EROSITAwiki: EroSnr/EcProposalPlucinsky (last edited 2019-05-21 11:23:03 by MichaelFreyberg)