David's Astronomy Pages
Images - Session 1201 (2024-03-27)

Objects Session Notes
Bullet 62P/Tsuchinshan - Comet
   
Bullet AT 2023tsk - Type BL Transient
Bullet AT 2024dsj - CV Type Transient
   
Bullet CGCG 217-021 - Spiral Galaxy with Type MP Transient AT 2023clc  (Attempt)
   
Bullet M101 - Spiral Galaxy with Type IIL Supernova 2023ixf
   
Bullet NGC 3206 - Spiral Galaxy with Type IIn Supernova 2024bch
Bullet NGC 3443 - Spiral Galaxy with Type II Supernova 2024ehs
Bullet NGC 4192A - Spiral Galaxy with Type II Supernova 2024exw
Bullet NGC 4619 - Spiral Galaxy with Type II Supernova 2024drt
Bullet NGC 6433 - Spiral Galaxy with Type Ia Supernova 2024efn
   
Bullet UGC 5886 - Spiral Galaxy with Type IIn Supernova 2024hw
Bullet UGC 8630 - Spiral Galaxy with Type II Supernova 2024drv
   
Bullet Variable Stars (photometric monitoring)
- R CrB, BL Lac
    
Bullet Nearby Stars (astrometric monitoring)
- Groombridge 34
 
  
- Attempted all-night Session (5.6 hrs) . Session started after early evening cloud had cleared.
   
- 12" LX200 + ST-10XME for imaging
- TS 80mm APO + ZWO ASI178MC for guiding & imaging
- Ambient Temperature: 5.5°C (min)
- CCD Temperature:   -15°/-20°C
- Notes from 2024-03-27 >>
   
-  
   

Observing Result

Image

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62P/Tsuchinshan - Comet

62P/Tsuchinshan - 2024-03-28
(passing through Virgo)

Sun Distance 1.67 AU (receeding)
Earth Distance 0.68 AU (101.7 million km)
   62P/Tsuchinshan - 2024-03-28 Detail
Autoguided on offset star using PHD2 with Lock Shift
set at the comet's rate of motion
(Ra -28.08 arcsec/hr, Dec -7.77 arcsec/hr)
Image   Image
Annotated CCD Image (50% size, square root scale)
2 x 90s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 00:08 UT (#1201027-28)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  Annotated CCD Image (100% size, square root scale, cropped)
6 x 90s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 00:12 UT (#1201027-32)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
     
Images of 62P/Tsuchinshan on Comets 2023 Page >>    
Images of 62P/Tsuchinshan on Comets 2024 Page >>    

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AT 2023tsk - Type BL Transient

AT 2023tsk (Bootes)
AT 2023tsk (Type: BL) discovered 2023-09-25.828 UT by Gaia
Alias: Gaia23cqg
Discovery Magnitude 14.76 (g-Gaia Filter)
vs Prior Non-Detection Limiting Magnitude 21.5 ?
vs Historic Magnitude 15.94 +/- 0.41 SD
Known BL Lac brightens by 2 mag in 45 months
Gaia, 2018-05-07 23:58, mag 15.01
Gaia, 2019-11-04 01:17, mag 16.99
Gaia, 2023-01-26 17:20, mag 15.50
Gaia, 2023-09-25 19:53, mag 14.76
Gaia, 2023-11-06 15:16, mag 15.51
Gaia, 2023-12-05 07:22, mag 15.30
Gaia, 2024-01-04 02:51, mag 15.54
 ( TNS 2023tsk | Gaia23cqg )

 
AT 2023tsk - 2024-03-27 (T+184.1d)
Image below (2024-03-27.962) was taken 184.1 days after discovery of 2023tsk
Position of reported transient (faint, fading again) is shown by white cross-hairs
Measured Magnitude +15.35 (Clear Filter)

Image

Annotated CCD Image (100% size, square root scale, cropped)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-27 23:12 UT (#1201005-08)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Images of AT 2023ati on Transients 2023 Page >>

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AT 2024dsj - CV Type Transient

AT 2024dsj (Cassiopeia)
AT 2024dsj (Type: CV) discovered 2024-02-28.787 UT by Gaia
Alias: Gaia24ath
Discovery Magnitude 15.25 (G-Gaia Filter)
vs Historic Magnitude 15.03 +/- 0.02 SD 
Gaia source fades by 0.2 mag
TNS discovery report on TNS says
Prior Non-Detection Limiting Mag 21.5 (2024-01-25 17:32)
but Gaia data for the same date gives mag 15.26)

 ( TNS 2024dsj | Gaia24ath )
 
AT 2024dsj - 2024-03-28 (T+28.3d)
Image below (2024-03-28.085) was taken 28.3 days after discovery of 2024dsj
Position of reported transient (faint) is shown by white cross-hairs
Measured Magnitude +14.46 (Clear Filter)
Image
Annotated CCD Image (100% size, linear scale, cropped)
4 x 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 02:05 UT (#1201069-72)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of AT 2024dsj on Transients 2024 Page >>

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CGCG 217-021 - Spiral Galaxy with Type MP Transient AT 2023clc (Attempt)

CGCG 217-021 with AT 2023clc (Canes Venatici)
AT 2023clc (Type: MP) discovered 2023-02-22.276 UT by ATLAS
Alias: ATLAS23cmd
Discovery Magnitude 15.68 (cyan-ATLAS Filter)
vs Prior Non-Detection Limiting Magnitude 19.06
 ( TNS 2023clc )
 
CGCG 217-021 / PGC 46002 - Spiral Galaxy
Alias : LEDA 46002
Image
Annotated CCD Image (50% size, square root scale)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 03:40 UT (#1201095-98)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
CGCG 217-021 / PGC 46002 - Detail
Image
Annotated CCD Image (150% size, square root scale, cropped)
Image details as above
  
Image
Negative CCD Image  (150% size, square root scale, cropped)
Image details as above
 
CGCG 217-021 with AT 2023clc - 2024-03-28 (T+399.9d)
Image below (2024-03-28.148) was taken 399.9 days after discovery of 2023clc
Position of earlier transient (likely faded & no longer visible) is shown by white cross-hairs
Image
Annotated CCD Image (150% size, square root scale, cropped)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 03:40 UT (#1201095-98)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of AT 2023clc (in CGCG 217-021) on Transients 2023 Page >>

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M101 - Spiral Galaxy with Type IIL Supernova 2023ixf

M101 with SN 2023ixf (Ursa Major)
SN 2023ixf (Type: IIL) discovered 2023-05-19.727 UT by Koichi Itagaki
Alias: ZTF23aaklqou, AT2023iyi, AT2023jgd, AT2023jfz, PSN J14033858+5418421, PS23dij
Discoverer Mag 14.9 (Clear filter)
 ( Rochester Supernova site | TNS 2023ixf )

SN 2023ixf (Type: IIL) discovered 2023-05-19.727 UT by Koichi Itagaki at Mag 14.9 is
located near M101's prominant star-forming region NGC 5461. 

The supernova resulted from a exploding red supergiant and lies just 21 million light years away.
 It's the closest core-collapse supernova to us since SN 1993J which lit up M81 (some 12 million ly away) in Spring 1993.
The SN is designated of type II-L (L for 'linear') , which is characterised by a rapid rise to maximum brightness
 followed by a slow and gradual decrease, that is thought to be brought about by ejection of the dead stars' outer hydrogen shell.
(from Article "Summer's Super Supernova", AstNow Magazine, Sep 2023, pp 36-39)
M101 with SN 2023ixf - 2024-03-28 (T+313.3d)
Image below (2024-03-28.030) was taken 313.3 days after discovery of 2023ixf
Position of supernova (faint) is shown by white cross-hairs
Measured Magnitude +15.93 (Clear Filter)
Image
Annotated CCD Image (100% size, square root scale, cropped)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 00:51 UT (#1201043-47)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of SN 2023ixf (M101) on Supernova 2023 Page

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NGC 3206 - Spiral Galaxy with Type IIn Supernova 2024bch

NGC 3206 with SN 2024bch (Ursa Major)
SN 2024bch (Type: IIn) discovered 2024-01-29.252 UT by Patrick Wiggins
Alias: ATLAS24bmx, PS24aap, GOTO24hm
Discovery Magnitude 15.5 ( Clear Filter)
 ( TNS 2024bch )
 
NGC 3206 with SN 2024bch - 2024-03-28 (T+58.9d)
Image below (2024-03-28.127) was taken 58.9 days after discovery of 2024bch
Position of reported SN (distinct but fading slowly) is indicated by white cross-hairs.
Measured Magnitude +14.23 (Clear Filter)
Image
Annotated CCD Image (125% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 03:12 UT (#1201079-83)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
   
Images of SN 2024bch (in NGC 3206) on Supernova 2024 Page >>

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NGC 3443 - Spiral Galaxy with Type II Supernova 2024ehs

NGC 3443 with SN 2024ehs (Leo)
SN 2024ehs (Type: II) discovered 2024-03-15.470 UT by ATLAS
Alias: ATLAS24dqq
Discovery Magnitude 18.10 (orange-ATLAS Filter)
vs Prior Non-Detection Limiting Magnitude 19.53 
 ( TNS 2024ehs )
 
NGC 3443 - Spiral Galaxy with SN 2024ehs (T+12.6d)
Image
Annotated CCD Image (50% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 01:36 UT (#1201057-61)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
NGC 3443 with SN 2024ehs - 2024-03-28 (T+12.6d)
Image below (2024-03-28.060) was taken 12.6 days after discovery of 2024ehs
Position of reported supernova (distinct) is shown by white cross-hairs
Measured Magnitude +14.89 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 01:36 UT (#1201057-61)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Image
Negative CCD Image  (150% size, square root scale, cropped)
Image details as above
 
Images of SN 2024ehs (in NGC 3443) on Supernova 2024 Page >>

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NGC 4192A - Spiral Galaxy with Type II Supernova 2024exw

NGC 4192A with SN 2024exw (Coma Berenices)
AT 2024exw (Type: II, z=0.007) discovered 2024-03-24.674 UT by Koichi Itagaki
Alias: ATLAS24ekc
Discovery Magnitude 15.9 (Clear Filter)
vs Prior Non-Detection in DSS Image
 ( TNS 2024exw )
 
NGC 4192A - Spiral Galaxy with SN 2024exw (T+3.3d)
Image
Annotated CCD Image (50% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-27 23:54 UT (#1201021-25)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
NGC 4192A with SN 2024exw - 2024-03-27 (T+3.3d)
Image below (2024-03-27.990) was taken 3.3 days after discovery of 2024exw
Position of reported supernova (distinct) is shown by white cross-hairs
Measured Magnitude +15.09 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-27 23:54 UT (#1201021-25)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of SN 2024exw (in NGC 4192A) on Supernova 2024 Page >>

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NGC 4619 - Spiral Galaxy with Type II Supernova 2024drt

NGC 4619 with SN 2024drt (Canes Venatici)
SN 2024drt (Type: II) discovered 2024-03-02.486 UT by ATLAS
Alias: ATLAS24dcr, ZTF24aagmhtq
Discovery Magnitude 17.93 (orange-ATLAS Filter)
vs Prior Non-Detection Limiting Mag 18.46 (g-ZTF Filter)
 ( TNS 2024drt )
 
NGC 4619 with SN 2024drt - 2024-03-28 (T+25.5d)
Image below (2024-03-28.016) was taken 25.5 days after discovery of 2024drt
Position of reported SN (fairly distinct but fading) is indicated by white cross-hairs.
Estimated Magnitude +15.8 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 00:32 UT (#1201036-40)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of SN 2024drt (in NGC 4619) on Supernova 2024 Page >>

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NGC 6433 - Spiral Galaxy with Type Ia Supernova 2024efn

NGC 6433 with SN 2024efn (Hercules)
SN 2024efn (Type: Ia) discovered 2024-03-12.496 UT by CRTS
Alias: SNhunt463
Discovery Magnitude 19.0 (V-crts-CRTS Filter)
vs Prior Non-Detection Limiting Magnitude 21.0
 ( TNS 2024efn )
 
NGC 6433 - Spiral Galaxy with SN 2024efn (T+15.5d)
Image
Annotated CCD Image (50% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-27 23:33 UT (#1201012-16)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
NGC 6433 with SN 2024efn - 2024-03-27 (T+15.5d)
Image below (2024-03-27.975) was taken 15.5 days after discovery of 2024efn
Position of reported supernova (faint but distinct) is shown by white cross-hairs
Measured Magnitude +15.70 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-27 23:33 UT (#1201012-16)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Images of SN 2024efn (in NGC 6433) on Supernova 2024 Page >>

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UGC 5886 - Spiral Galaxy with Type IIn Supernova 2024hw

UGC 5886 with AT 2024hw (Sextans)
AT 2024hw (Type: unk) discovered 2024-01-05.357 UT by ZTF
Alias: ZTF24aaaibep
Discovery Magnitude 17.394 (i-ZTF Filter)
 ( TNS 2024hw )
 
UGC 5886 with SN 2024hw - 2024-03-28 (T+82.7d)
Image below (2024-03-28.052) was taken 82.7 days after discovery of 2024hw
Position of reported transient (faint) is indicated by white cross-hairs.
Estimated Magnitude +17.0 (Clear Filter)
Poor quality image (poor sky transparency / bright background)
Image
Annotated CCD Image (150% size, square root scale, cropped)
3 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 01:20 UT (#1201052-54)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
   
Images of SN 2024hw (in UGC 5886) on Supernova 2024 Page >>

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UGC 8630 - Spiral Galaxy with Type II Supernova 2024drv

UGC 8630 with SN 2024drv (Canes Venatici)
SN 2024drv (Type: II) discovered 2024-03-02.513 UT by ATLAS
Alias: ATLAS24dct
Discovery Magnitude 16.56 (orange-ATLAS Filter)
vs Prior Non-Detection Limiting Mag 18.86
 ( TNS 2024drv )
 
UGC 8630 with SN 2024drv - 2024-03-28 (T+25.6d)
Image below (2024-03-28.163) was taken 25.6 days after discovery of 2024drv
Position of reported SN (distinct) is indicated by white cross-hairs.
Measured Magnitude +15.23 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-28 04:03 UT (#1201102-06)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Images of SN 2024drv (in UGC 8630) on Supernova 2024 Page >>

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