Closed cdeil closed 6 years ago
I figured out just now why the SkyCoord.from_name
calls for MSH 15-5-02
and MSH 15-52
give different results.
They always resolve to the same source in SIMBAD, the SNR: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=MSH%2015-52#lab_ident
But in NED MSH 15-52
resolves to the pulsar
http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=MSH%2015-52
which I think is an old pulsar position measurement, because it's different from the pulsar position on SIMBAD:
http://simbad.u-strasbg.fr/simbad/sim-id?Ident=PSR%201509-58
and MSH 15-5-02
doesn't resolve at all in NED.
SkyCoord.from_name
queries http://cds.u-strasbg.fr/cgi-bin/Sesame and I think the default "all" mode means NED first. That explains the positions obtained above.
That still leaves the question what position to put for this TeV source in gamma-cat. I think my preference would be to use the best-fit position from http://adsabs.harvard.edu/abs/2005A%26A...435L..17A and to leave comments explaining about the MSH names and positions.
I've made a commit with changes here: acf4947 I'm reasonably happy with this, so merging now. Discussion via email with Michelle, Yves and Konrad is still ongoing, if it concludes in a different way or someone else speaks up here we can always make another commit.
I did change the common_name
to "MSH 15-52", putting the previous "MSH 15-5-02" under other_names
. It seems that "MSH 15-52" is the "modern name" used in Fermi-LAT and HESS papers. From the original MSH catalog paper it isn't clear what the correct name should be, they do use "15-52" with an italic "2" sometimes, sometimes there is a space between the 5 and 2.
For the position, I did put the best-fit position from http://adsabs.harvard.edu/abs/2005A%26A...435L..17A , avoiding the issue concerning complex morphology / counterpart catalog positions for this source. I also checked the upcoming HGPS paper that contains a 3-Gauss morphology model. The centroid is almost identical with the one from 2005A%26A...435L..17A, i.e. what we have now in gamma-cat.
What we can't change is the CTA first data challenge, which used gamma-cat. It will forever have MSH 15-52 at ~0.1 offset from the true TeV source position. Oh well. :-) See here
I wonder if we have the correct position for the source that goes by the names of MSH 15-5-02, MSH 15-52, HESS J1514-591 in gamma-cat.
It's this one:
The current position we have is this:
The
ra/dec
comes from the SIMBAD position for MSH 15-5-02 from input/sources/tev-000079.yaml:The
pos_ra/pos_dec
comes from the HESS J1514-591 measurement in gamma-cat/input/data/2005/2005A%26A...435L..17A/tev-000079.yamlI double-checked the values in the paper. That is the correct base-fit position from the elongated Gaussian fit in http://adsabs.harvard.edu/abs/2005A%26A...435L..17A .
I'm aware the situation is complex and that there is https://arxiv.org/abs/1709.01422, but I still wonder if the positions we have now in
gamma-cat
, but also if the ones given in SIMBAD make sense or not.Here are all relevant positions:
The position of
HESS J1514-591
in the paper and in SIMBAD doesn't agree:The
hess_simbad
position matchesmsh1
andsnr
:The
hess_paper
position matchesmsh2
almost perfectly:The separation between those two positions is 0.13 deg:
As expected, neither coincides with the pulsar:
I'm not able to find the entry for
msh2
in SIMBAD directly, this resolves tomsh1
!? http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HESS+J1514-591Bottom line: I think we should consider changing common_name from
MSH 15-5-02
toMSH 15-52
in gamma-cat, or at least change the position ininput/sources/tev-000079.yaml
frommsh1
tomsh2
.Thoughts?