Hi everybody !!! I have found an unidentified emission line in a Seyfert 2 spectra at 9625 angstroms. I've tried to reproduce it with cloudy, but I don't find...
That would be hard to answer like that - ie. it depends on relative line ratios, other lines present etc. But you will probably find the Atomic Line list a...
Thank you Jarle, but I used this Atomic Line list, and I have many candidates, as [Fe II], [P II] or He I. I tried to reproduce the spectrum then with cloudy...
... Cloudy may not be want you want to use if you are trying to identify an unknown line. The better approach would be to understand the line in the context...
You could perhaps compare the intensity of your unknown line to HeI 4471. If the ratio is close to 5d-3, it is an HeI line. You can cross check by looking for...
Note that if the line is indeed the HeI line, it is from an upper level that is not included by default in Cloudy's helium model. You will need to increase...
I'm doing a high-resolution Cloudy run (with "set continuum resolution 0.1") and I'm getting the following message on my output: NOTE OpacityCreate1Element...
Thanks Peter. I thought so. Actually, I've seen a subsequent and perhaps related problem that actually caused a thrown assert and crashed Cloudy. With the...
We were aware of this problem (although it looks like we neglected to document it anywhere). This will be fixed in the next major upgrade, with an expected...
Hi, We have been looking for the references of the transition probabilities used by Cloudy (c07.02.01) for different ions in the files "cool_*.cpp" and cannot...
... 5007A). ... The set in Osterbrock & Ferland, AGN3, should be up to date. The references were only entered in the code if the numbers were updated in the...
Hi Everyone, I have a question regarding the push pressure command. Could you please explain to me in more detail what interpretation does the (Pcorrect),...
... We are running simulations in which we want to measure the abundance discrepancy factor (ADF) from two multiplets of OII: M1 (4651A) and M10 (4075A). We...
... it would be helpful if you could post two very simple models that show the difference. One that works, and a similar one that does not. thanks, Gary...
Hi, an example of a model that runs correctly: table star wmbasic 41000 4 0 ionization parameter = -2.0 hden 2.48 sphere abundances HII region c print line...
Hi- I am trying to get output on all the level populations, line optical depths and intensities, etc, for OI (for a study of OI fluorescence lines). As an...
... L/4piR^2c? ... Pcorrect is the correct local pressure. this will equal the sum of Pin+Pinteg if the cloud is hydrostatic with only gas and radiation ...
Hi, is there a way to punch the local continuum, i.e. the continuum at a given depth? I've tried with the various punch continuum commands, but it seems to me...
Gary- I'm hesitant to jam up mailboxes with large files , so how about just a link: http://www.sal.wisc.edu/~khn/salt/Outgoing/cloudy/ This has the .in, .out,...
Hi, I'm having trouble understanding the normalization of the diffuse continuum (the 4th column of the punch continuum command). Specifically, it says in the ...
... continuum ... says in the ... one was ... factor of 0.2 ... the normalization ... I find the ... that I must not ... Hi Karen, I don't see a problem. when...
Greetings, The next major release of Cloudy, C08.02, will be posted within the next month or so. The Revision History page on the trac site lists changes that...
Hi, I've been running HII region models ionized by high-resolution continua (Delta lambda=0.3 Angstrom) in a region in which Cloudy's default resolution is 5...
... input script and the ... I need to reproduce the problem to fix it. how about pasting the contents of the input and the ini file into a posting? I don't...
