Archive for August, 2020

Preparing for MOS observations with the GTC

Posted August 18, 2020 By grigoris

The pandemic of Covid-19 has obviously affected our observing runs also. ESO is (still) totally shut down while GTC after some off period it seems that it is under some limited operation.

Our accepted observing program with GTC includes Mulit-Object Spectroscopic observations with the OSIRIS instrument. For this we need to prepare masks, i.e. metal plates on which a number of slits is cut to allow the light of specific targets to pass and acquire their spectrum. In order to optimize the positioning of those slits (and make sure that they are placed on the correct coordinates) we have asked for pre-imaging, e.g. the acquisition of short exposures of the FOVs we have requested (for all our targets). With these and the appropriate software (Mask Designer) it becomes easy to create the masks.

Some weeks ago we actually received (quite unexpectedly, given the pandemic status) a couple of images. That allowed us to prepare the corresponding masks (after resolving all technical difficulties and questions of course). An example of these masks is shown below for the galaxy IC 10. When creating the mask we have to avoid slits that result in overlapping spectra (because we will end up with useless data). That’s why we need to prioritize our targets and select the best combination which will allow for the maximum non-colliding number of targets to be observed, respecting all constraints imposed by the program and the instrument involved. Although mask designing with modern software tools can become easy it is still a time-consuming step that needs caution and accuracy.

Mask for multi-slit spectroscopic observations with OSIRIS GTC - Target galaxy IC 10

The image shows the mask designed for the galaxy IC 10. The small white line are the slits with the corresponding spectra visible as vertical thick green lines. Smaller lines correspond to fiducial stars, i.e. stars that help to the alignment of the mask. The yellow box corresponds to the physical limits of the maks. The background image is a short exposure of IC 10 in the r band.

So, the masks have been prepared, verified, constructed, … and now we wait for the real spectroscopic observations to be obtained! Fingers crossed!


note: the current article has been written originally for the ASSESS group.

 

Some 2020 Perseids observed …

Posted August 17, 2020 By grigoris

It has been many many years since my last visual observations of meteors (back in 2010…). Last week I found the opportunity to observe a bit the peak of the Perseid shower.

I observed for a couple of hours, just before the moon rise, from my place in the relatively light polluted Heraklion of Crete. I was a bit tired since I have waken up in the morning and didn’t manage to get any sleep so definitely I missed some fainter ones. But there were a few bright Perseids that I saw with a couple of them being kind of spectacular!

Although the total number recorded was low (7 Perseids and 5 Sporadics) I enjoyed the observation. Sitting relaxed in a chair and viewing the nigh sky feels nice, especially when the anticipation on the next bright meteor is added.

You can find the particular observation log as Session ID 80974 at IMO.