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I found one galaxy (low-mass AGN from Reines+2013) where the fit does not converge to a solution leading to wrong emission line fluxes. The fastspecfit-qa for this sources is as follows -
![image]…
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### Instrument
NIRSpec (Stages 1-3)
### What happened?
I am running
s3_spec, s3_meta = s3.reduce(eventlabel, ecf_path=ecf_path,
s2_meta=s2_meta)
at which po…
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These example cases are selected to have a good agreement between the **SDSS D4000_N** and the **DESI DN4000_MODEL** (within 0.03) but a large discrepancy between **DN4000** and **DN4000_MODEL** for D…
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### Instrument
_No response_
### What happened?
I'm trying to run Eureka on a relatively new Macbook Pro with an M1 chip, rather than Intel chip.
I followed all of the installation steps a…
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I got this error and I checked the header:
`CDELT1 = -0.00268754582783`
`CDELT2 = 0.00269177717671`
`CDELT3 = 0.20000000298`
Really, this is not `almost_equal`? Any idea for a work …
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We should double check we are consistent everywhere since in the 2d flm revisions we updated some of the healpix indexing to note that `lmax = L - 1`.
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On DiRAC's shared machine, a sample test orbit takes 95 seconds to return 27 matches in nearly 7 years of NSC observations (with profiling enabled). The profile indicates there are some low-hanging op…
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Brute-force attribution of (458508) finds 10 observations within 1 arcsecond in observations dated between August 30th, 2013 and September 30th, 2013.
The precovery code finds 2 observations, only…
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make_bin_map requires obs.pixel and obs.psi which are note defined properly.
Args:
obss (list of :class:`Observations`): observations to be mapped. They
are required to ha…
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implement simple monte carlo method: random uniform samples.
use geomstats or pytorchgeometric libraries