开云体育

I personally don't imagine why CMOS observations must have a different weighting respect to CCD observations. Luca #204 [email protected]> ha scritto:

Hi all, I am currently working on fitting the orbits of some long-period comets based on data obtained from the MPC database. In assigning uncertainties to the data, my orbit fitting program follows

Dear Roberto, all, I was able to obtain a new set of images of this object last night via LCO-Tenerife. Both single and stacked images show a small condensed coma and a distinct, straight tail up to

Hi all, MPEC 2024-Y20 announced yesterday the discovery of the Jupiter-family comet C/2024 X1 (Fazekas). Its nominal orbital period (29.5 years) is surprisingly similar to that of Saturn (29.4 years;

Hi Jakub, 1. It is really the isue with the query looking from the comet center instead of the center of the image. If you have in the settings the option calculated comet pos. ON then the queries

Hello Jure, unfortunately this finds me in a time when I am heavy loaded with work and have no time to examine these things detailed. However answer to 1. question could be different obtaining of

Hi, I'm experiencing some strange behavior with KOPR. I have the stable version 0.83 installed as an compile executable. I also have the live version, which I run from a source with Python 3.10 I have

Hi Vladimir, I've been imaging this comet in the morning twilight using iTelescope T70 in Chile. This is a 135mm Samyang lens but it has the advantage of being able to get to the horizon. As of this

Hi All. Just for information - a recent bright comet C/2024 G3 (ATLAS) now is visible in the last SWAN images. X-Y position (0,0 - upper left) on 9/12 is 226-321. Comet`s UV singature is enough bright

Comet 333P/LINEAR made its close approach to Earth at 1014UT on the morning of 2024 December 9 as seen from Tucson, Arizona at a distance of 80,860,186 kilometers (50,254,932 miles). The comet was

We would like to invite everyone to a free Zoom webinar on *"The Importance of Preserving Astronomical History"* *by astronomy historian John W. Briggs this Saturday, December 14, at 8:30 p.m. EST

Hi everyone, we also tried to film the MOU0001 field and we did not detect anything in the field. Greetings Monte Viseggi Observatory 126 Associazione Astrofili Spezzini - APS Via delle Fornaci 1/A

Hi Maik, all, I’d still encourage anyone else to have a go at this. Theoretically, it could be “there” but faint, or several arcmin away from the ephemeris position and I somehow missed it, but

Alan, many thanks for this information. I really thought that the second tracklet was a good confirmation, and this was the reason for my message, but now it seems it might still be questionable. Maik

Hi Maik, all, I just took some images with LCO-Tenerife, and was unable to detect any moving objects down to magnitude ~19 within a 5x5 arcminute field centered on the predicted ephemeris position.

Hello all, I want to point out the object MOU0001 on the NEOCP. My parabolic solution looks very interesting - intrinsically faint but very close approach to Earth in January. Of course, this is based

Miki – this topic came up back in early September. See the messages starting with my #32535. Your browser may automatically be changing the link to https: – even if you manually type http:. Bill

I usually recommend use Aladin to open the FITS and find how many layers and what kind of images and data are in there. There are some FITS which have multiple slices. Some others are something called

Hi Roberto, Yes, I did. Sincerely, Alan Great that you confirmed. Did you send the observation with confirmation to the MPC? Regards, Roberto Haver On Mon, 09 Dec 2024 12:03:25 -0700 "Alan Hale"

Hello Miki, Maybe you should try to open it with Siril. At first level, just opening and looking at an image, it is quite simple to use. Christophe Envoyé avec la messagerie sécurisée [Proton