Differences between revisions 1 and 2
Revision 1 as of 2024-08-27 08:56:44
Size: 2454
Editor: JanKurpas
Comment:
Revision 2 as of 2024-08-27 09:05:13
Size: 2216
Editor: JanKurpas
Comment:
Deletions are marked like this. Additions are marked like this.
Line 15: Line 15:
|| Anderson || Scott || see proposal pdf || anderson@astro.washington.edu||
|| Brandt || Niel || see proposal pdf || wnbrandt@gmail.com ||
|| Bauer || Franz || see proposal pdf || fbauer@astro.puc.cl||
|| Covey || Kevin || see proposal pdf || coveyk@wwu.edu ||
|| Demasi || Sebastian || see proposal pdf || demasi@uw.edu ||
|| Gaensicke || Boris || see proposal pdf || boris.gaensicke@gmail.com ||
|| Rodriguez || Antony || see proposal pdf ||acrodrig@astro.caltech.edu||
|| Stassun || Keivan || see proposal pdf || keivan.stassun@Vanderbilt.Edu||
|| Pan || Zhichen C. || see proposal pdf || panzc@bao.ac.cn ||
|| Zhang || Zhongli L. || see proposal pdf || zzl@shao.ac.cn ||
|| Qian || Lei || see proposal pdf || ||
|| Ji || Li || see proposal pdf || ji@pmo.ac.cn ||
Line 31: Line 27:
Joint eROSITA/SDSS project. Uses DL2 data from both collaborations. SDSS data meanwhile in the public area completely, some eROSITA data used still proprietary. No SDSS_only scientist has touched eROSITA data while preparing the manuscript. Follow-up project on an eROSITA discovered isolated neutron star. The collaborators helped to secure a follow-up observation with the FAST and conducted the analysis of the obtained radio data for the source. The paper does not include eROSITA data, but most of the follow-up observations (XMM-Newton, NICER, ESO-VLT), where proposed at the time when the eROSITA data of the target was not yet published. Non of the external collaborators has touched eROSITA data while preparing the manuscript.
Line 36: Line 32:
The list comprises the other co-authors on the paper (Schwope, AIP students, Dwelly, Salvato, Merloni, Maitra, Strong, Friedrich, Stelzer, Munoz-Giraldo). The list comprises the other co-authors on the paper (Schwope, Pires, Haberl, Traulsen).
Line 39: Line 35:
The expected outcome is a scientific paper describing the identification results of accreting compact white-dwarf binaries in eFEDS. The expected outcome is a scientific paper describing in more detail the properties of the pulsar, from radio to gamma-rays.
Line 42: Line 38:
Initially just for eropub #380, will be extended to full SDSS-V Just for eropub #704. The paper is expected to be submitted soon.

EroCompact EC Proposal 704

Proposal Date : 27-Aug-2024

  • Changed: 27-Aug-2024 by JanKurpas: Update [created page wrt to IEC proposal discussed in WG on Aug 24]

External Collaborator

Name

First name

Institute

email

Pan

Zhichen C.

see proposal pdf

panzc@bao.ac.cn

Zhang

Zhongli L.

see proposal pdf

zzl@shao.ac.cn

Qian

Lei

see proposal pdf

Ji

Li

see proposal pdf

ji@pmo.ac.cn

eROSITA_DE Proposing Member

Name

First name

Institute

email

Kurpas

jan

AIP

jkurpas@aip.de

Scientific Proposal

Follow-up project on an eROSITA discovered isolated neutron star. The collaborators helped to secure a follow-up observation with the FAST and conducted the analysis of the obtained radio data for the source. The paper does not include eROSITA data, but most of the follow-up observations (XMM-Newton, NICER, ESO-VLT), where proposed at the time when the eROSITA data of the target was not yet published. Non of the external collaborators has touched eROSITA data while preparing the manuscript.

The proposal for COA-IEC submitted Sep 23, 2023, is attached to this page.

List of Potential Collaborators within eROSITA_DE

The list comprises the other co-authors on the paper (Schwope, Pires, Haberl, Traulsen).

Expected Outcome

The expected outcome is a scientific paper describing in more detail the properties of the pulsar, from radio to gamma-rays.

Expected duration of the project

Just for eropub #704. The paper is expected to be submitted soon.

EROSITAwiki: EroCompact/EcProposalEropub704 (last edited 2024-08-27 13:54:48 by JanKurpas)