TCP J04291884+4354232 possible nova mag 10.2
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Re: TCP J04291884+4354232 possible nova mag 10.2
Merci Joan, c'est parfait!
Un câlin fort.
Umberto
Un câlin fort.
Umberto
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Re: TCP J04291884+4354232 possible nova mag 10.2
Bonsoir à tous, le profil de cette soirée 18/12/2020 et une comparaison avec la journée 16-12-2020 où une augmentation de l'OI-8446A est évidente. Un filtre rouge a été interposé.
Umberto Solllecchia
u]Comparison[/u]
Umberto Solllecchia
u]Comparison[/u]
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Re: TCP J04291884+4354232 possible nova mag 10.2
Here are two composite plots of spectra of Nova Per 2020 taken by ARAS observers using LISA spectroscopes which show its evolution during the 3 weeks since discovery. All spectra have been normalised to unity at 5500A, log-scaled and equally displaced vertically.
David
David
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Re: TCP J04291884+4354232 possible nova mag 10.2
Hi David,
Very interesting to see how it changed in the starting days and then more or less stabilized.
Thank you.
Very interesting to see how it changed in the starting days and then more or less stabilized.
Thank you.
regards Rainer____Observatorio Real de 14_____MÉXICO_____N 22° W 101°
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Re: TCP J04291884+4354232 possible nova mag 10.2
Bonsoir à tous. J'ai placé une comparaison séquentielle de mes observations dans l'IR
Umberto.
Umberto.
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Re: TCP J04291884+4354232 possible nova mag 10.2
Hello all,
A few nights with a clear sky allowed us to obtain the following spectra of the Nova Per 2020 with an Alpy 600.
The 17th of December at 20 h 17 TU (resolution of 520, JJ = 2459201.3451 and an acquisition time of 30 min) : The 18th of December at 23 h 04 TU (resolution of 521, JJ = 2459202.461 and an acquisition time of 70 min) : The relative intensities of the FeII lines as well as that of the [OI] line at 6300 A seem to have increased slightly in a few days... ...and the relative intensity of the Halpha line continues to increase : Clear skies,
Marion THOMAS et Christophe BOUSSIN
A few nights with a clear sky allowed us to obtain the following spectra of the Nova Per 2020 with an Alpy 600.
The 17th of December at 20 h 17 TU (resolution of 520, JJ = 2459201.3451 and an acquisition time of 30 min) : The 18th of December at 23 h 04 TU (resolution of 521, JJ = 2459202.461 and an acquisition time of 70 min) : The relative intensities of the FeII lines as well as that of the [OI] line at 6300 A seem to have increased slightly in a few days... ...and the relative intensity of the Halpha line continues to increase : Clear skies,
Marion THOMAS et Christophe BOUSSIN
CBO (Newton 200 F/5 / Alpy600 / Atik 314L+ / Atik Titan + Mewlon 180 F/12 / LHIRES III 2400 / Atik 460EX / Atik 314 L+) @ ARAS database
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Re: TCP J04291884+4354232 possible nova mag 10.2
Better late then never.....I've been taking Alpy600, LISA-IR, and LhiresIII data in Ha, Hb, & CaK.
First here is a stitched Alpy600+LISA-IR spectrum (Taken on the 4&5Dec20...I have more but wanted to do this pair first):

NOTE: All identified spectral lines are tenative.....I used a paper (Optical and near-infrared spectroscopy of nova V1494 Aquilae 1999 no. 2) to help identify the Ol lines in IR.
Here is an animation of the H-Alpha changes seen with my LhiresIII on 27Nov20, 11Dec20, 13Dec20, & 21Dec20:

NOTE: The 1st night (27Nov20) was slightly under-sampled, so I applied a low-pass gaussian filter. After this I increased my CCD cooling from -5 to -9 and increased
my sub-exposure duration from 2400 to 2700 seconds to get better SNR.
Here are two exposures in the H-Beta region with the LhiresIII (15Dec20 & 22Dec20):

Here is a single (set of 6 images, each 45min [2700sec] long) of the CaK region taken with the LhiresIII (16Dec20):

Hopefully this will stay above 11th magnitude for awhile longer....
James
First here is a stitched Alpy600+LISA-IR spectrum (Taken on the 4&5Dec20...I have more but wanted to do this pair first):

NOTE: All identified spectral lines are tenative.....I used a paper (Optical and near-infrared spectroscopy of nova V1494 Aquilae 1999 no. 2) to help identify the Ol lines in IR.
Here is an animation of the H-Alpha changes seen with my LhiresIII on 27Nov20, 11Dec20, 13Dec20, & 21Dec20:

NOTE: The 1st night (27Nov20) was slightly under-sampled, so I applied a low-pass gaussian filter. After this I increased my CCD cooling from -5 to -9 and increased
my sub-exposure duration from 2400 to 2700 seconds to get better SNR.
Here are two exposures in the H-Beta region with the LhiresIII (15Dec20 & 22Dec20):

Here is a single (set of 6 images, each 45min [2700sec] long) of the CaK region taken with the LhiresIII (16Dec20):

Hopefully this will stay above 11th magnitude for awhile longer....
James
James Foster
eShel2-Zwo ASI6200MM Pro
Lhires III (2400/1800/600 ln/mm Grat) Spectroscope
LISA IR/Visual Spectroscope (IR Configured)
Alpy 200/600 with Guide/Calibration modules and Photometric slit
Star Analyzer 200
eShel2-Zwo ASI6200MM Pro
Lhires III (2400/1800/600 ln/mm Grat) Spectroscope
LISA IR/Visual Spectroscope (IR Configured)
Alpy 200/600 with Guide/Calibration modules and Photometric slit
Star Analyzer 200
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Re: TCP J04291884+4354232 possible nova mag 10.2
Bonjour à tous, la nova va au repos. L'augmentation de l'intensité du CaII 8446A se poursuit.
Voici une comparaison entre le 21-12-2020 et le 27-12-2020.
Umberto Sollecchia
Voici une comparaison entre le 21-12-2020 et le 27-12-2020.
Umberto Sollecchia
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Re: TCP J04291884+4354232 possible nova mag 10.2
Bonjour Umberto
Super suivi de cette Nova.
Quelle est la configuration du materiel employé ?
Le 26/12 lors d'essais avec UVEX(4) j'ai choisi le champs autour du CA II.
La Nova etait une cible.
2 Pierre
Aspremont 06 (fr)
Super suivi de cette Nova.
Quelle est la configuration du materiel employé ?
Le 26/12 lors d'essais avec UVEX(4) j'ai choisi le champs autour du CA II.
La Nova etait une cible.
2 Pierre
Aspremont 06 (fr)
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Re: TCP J04291884+4354232 possible nova mag 10.2
The OI 8446 line at R~7000 (LHIRES 1200)
Robin
Robin
LHIRES III #29 ATIK314 ALPY 600/200 ATIK428 Star Analyser 100/200 C11 EQ6
http://www.threehillsobservatory.co.uk
http://www.threehillsobservatory.co.uk