David's Astronomy Pages
Images - Session 1198 (2024-03-15)

Objects Session Notes
Bullet 13P/Olbers - Comet
Bullet 62P/Tsuchinshan - Comet
Bullet 103P/Hartley - Comet
Bullet C/2022 E2 (ATLAS) - Comet
   
Bullet AT 2023tow - Nova Transient
Bullet AT 2023tsk - Type BL Transient
Bullet AT 2023txn - CV Type Transient
Bullet AT 2024crd - Type Nova? Transient
Bullet AT 2024dsj - CV Type Transient
   
Bullet IC 2190 - Spiral Galaxy with Type Ia Supernova 2024dhp
   
Bullet M101 - Spiral Galaxy with Type IIL Supernova 2023ixf
   
Bullet NGC 3206 - Spiral Galaxy with Type IIn Supernova 2024bch
Bullet NGC 3467 - Spiral Galaxy with Type MP Transient AT 2024dda
Bullet NGC 3690 - Spiral Galaxy with Type Ia Supernova 2023wrk
Bullet NGC 4619 - Spiral Galaxy with Type II Supernova 2024drt
Bullet NGC 4995 - Spiral Galaxy with Type II Supernova 2023gfo
Bullet NGC 5036 - Elliptical Galaxy with Type Ia Supernova 2024dop
Bullet NGC 6040 - Spiral Galaxy (ARP 122)
Bullet NGC 6745 - Spiral Galaxy with Type II Supernova 2023ucy
   
Bullet Segue 1 - Faint Dwarf Galaxy - 0.075mly
Bullet UGC 5886 - Spiral Galaxy with Type IIn Supernova 2024hw
Bullet UGC 8630 - Spiral Galaxy with Type II Supernova 2024drv
Bullet UGC 9002 - Spiral Galaxy with Type II Supernova 2023pls
Bullet UGC 9659 - Spiral Galaxy with Type Ia Supernova 2024ech
   
Bullet Variable Stars (photometric monitoring)
- YZ Cnc, BL Lac
    
Bullet Nearby Stars (astrometric monitoring)
- 61 Cyg
 
  
- All-Night Session (9.2 hrs)
   
- 12" LX200 + ST-10XME for imaging
- TS 80mm APO + ZWO ASI178MC for guiding & imaging
- Ambient Temperature: 2°C (min)
- CCD Temperature:   -20°/-25°C
- Notes from 2024-03-15 >>
   
-  
   

Observing Result

Image

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13P/Olbers - Comet

13P/Olbers - 2024-03-15
(passing through Cetus)
Sun Distance 1.93 AU (approaching)
Earth Distance 2.32 AU (347.1 million km)
   13P/Olbers - 2024-03-15 Detail
Autoguided on offset star using PHD2 with Lock Shift
set at the comet's rate of motion
(Ra 43.12 arcsec/hr, Dec 54.42 arcsec/hr)
Image   Image
Annotated CCD Image (50% size, square root scale)
3 x 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 20:00 UT (#1198007-09)
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)
10 x 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 20:05 UT (#1198007-16)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
     
Images of 13P/Olbers on Comets 2024 Page >>    

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62P/Tsuchinshan - Comet

62P/Tsuchinshan - 2024-03-16
(passing through Virgo)

Sun Distance 1.59 AU (receeding)
Earth Distance 0.60 AU (89.8 million km)
   62P/Tsuchinshan - 2024-03-16 Detail
Autoguided on offset star using PHD2 with Lock Shift
set at the comet's rate of motion
(Ra -33.87 arcsec/hr, Dec -1.78 arcsec/hr)
Image   Image
Annotated CCD Image (50% size, square root scale)
3 x 90s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 00:22 UT (#1198115-17)
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)
7 x 90s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 00:25 UT (#1198115-21)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
     
     62P/Tsuchinshan - 2024-03-16 Detail
Inverse Spectrum
    Image
    Annotated false-colour CCD Image (50% size, square root scale)
7 x 90s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 00:25 UT (#1198115-21)
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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103P/Hartley - Comet

103P/Hartley - 2024-03-15
(passing through Canis Minor)

Sun Distance 2.16 AU AU (receeding)
Earth Distance 1.43 AU (213.5 million km)
   103P/Hartley - 2024-03-15  Detail
Autoguided on offset star using PHD2 with Lock Shift
set at the comet's rate of motion
(Ra 19.43 arcsec/hr, Dec 25.07 arcsec/hr)
Image   Image
Annotated CCD Image (50% size, square root scale)
3 x 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 21:07 UT (#1198045-47)
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)
3 x 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 21:07 UT (#1198045-47)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
     
Images of 103P/Hartley on Comets 2023 Page >>    
Images of 103P/Hartley on Comets 2024 Page >>    

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C/2022 E2 (ATLAS) - Comet

C/2022 E2 (ATLAS) - 2024-03-15
(passing through Gemini)
Sun Distance 4.01  AU (approaching)
Earth Distance 3.55 AU (530.8 million km)
   C/2022 E2 (ATLAS) - 2024-03-15 Detail
Autoguided on offset star using PHD2 with Lock Shift
set at the comet's rate of motion
(Ra -40.78 arcsec/hr, Dec 19.35 arcsec/hr)
Image   Image
Annotated CCD Image (50% size, square root scale)
2 x 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 20:20 UT (#1198021-22)
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 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 20:21 UT (#1198019-25)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
     
 Images of C/2022 E2 (ATLAS) on Comets 2023 Page >>    
 Images of C/2022 E2 (ATLAS) on Comets 2024 Page >>    

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AT 2023tow - Nova Transient

AT 2023tow (Scutum)
AT 2023tow (Type: Nova) discovered 2023-09-20.778 UT by Gaia
Alias: Gaia23coj, ZTF23abceaws
Discovery Magnitude 12.26 (G-Gaia Filter) vs Historic Magnitude - None
Red bright Galactic plane transient
 ( TNS 2023tow | Gaia23coj )

 
AT 2023tow - 2024-03-16 (T+177.4d)
Image below (2024-03-16.174) was taken 177.4 days after discovery of 2023tow
Position of reported transient (faded & no longer visible) is shown by white cross-hairs
Non-Detection Limiting Mag +17.5 (Clear Filter)

Image

Annotated CCD Image (100% size, linear scale, cropped)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 04:20 UT (#1198203-07)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
AT 2023tow - Earlier Image, 2023-10-04 (T+14.1d)
Image below (2023-10-04.847) was taken 14.1 days after discovery of 2023tow
Position of reported transient (bright & distinct) is shown by white cross-hairs
Measured Magnitude +12.72 (Clear Filter)

Image

Annotated CCD Image (100% size, linear scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2023-10-04 20:28 UT (#1154004-08)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Images of AT 2023tow on Transients 2023 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 - 2024-03-16 (T+172.3d)
Image below (2024-03-16.104) was taken 172.3 days after discovery of 2023tsk
Position of reported transient (faint but distinct) is shown by white cross-hairs
Measured Magnitude +15.55 (Clear Filter)

Image

Annotated CCD Image (100% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 02:38 UT (#1198161-65)
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 2023txn - CV Type Transient

AT 2023txn (Cygnus)
AT 2023txn (Type: CV) discovered 2023-09-29.797 UT by Gaia
Alias: Gaia23cse
Discovery magnitude 11.83 (G-Gaia) vs Historic Mag 13.14
Red Galactic plane source brightens erratically by 2 mag & becomes bluer
 ( TNS 2023txn | Gaia23cse )
  
AT 2023txn - 2024-03-16 (T+168.3d)
Image below (2024-03-16.144) was taken 168.3 days after discovery of 2023txn
Position of reported transient (distinct but fading) is shown by white cross-hairs
Measured magntitude +12.84 (Clear Filter)
Image 
Annotated CCD Image (100% size, linear scale, cropped)
5 x 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 03:30 UT (#1198182-86)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of AT 2023txn on Transients 2023 Page >>

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AT 2024crd - Type Nova? Transient

AT 2024crd (Virgo)
AT 2024crd (Type: Nova?) discovered 2024-02-14.750 UT by Tadashi Kojima
Alias: TCP J13530185+0522000, Gaia24apm
Discovery Magnitude 13.2 (Clear Filter)
vs Prior Non-Detection Limiting Magnitude 15.2
Transient on faint blue PanSTARRS source
 ( TNS 2024crd | Gaia24apm )
 
AT 2024crd - 2024-03-16 (T+30.3d)
Image below (2024-03-16.056) was taken 30.3 days after discovery of 2024crd
Position of reported transient (fading) is shown by white cross-hairs 
Measured Magnitude +15.59 (Clear Filter)

Image

Annotated CCD Image (100% size, linear scale, cropped)
5 x 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 01:24 UT (#1198135-39)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Images of AT 2024crd on Transients 2024 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 - 2024-03-16 (T+16.3d)
Image below (2024-03-16.119) was taken 16.3 days after discovery of 2024dsj
Position of reported transient (faint) is shown by white cross-hairs
Measured Magnitude +14.44 (Clear Filter)
Image
Annotated CCD Image (100% size, linear scale, cropped)
4 x 60s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 02:55 UT (#1198168-72)
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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IC 2190 - Spiral Galaxy with Type Ia Supernova 2024dhp

IC 2190 with SN 2024dhp (Auriga)
SN 2024dhp (Type: Ia) discovered 2024-02-28.291 UT by ZTF
Alias: ZTF24aagirej
Discovery Magnitude 18.33 (r-ZTF Filter)
vs Prior Non-Detection Limiting Mag 16.0 (g-ZTF Filter)
 ( TNS 2024dhp )
 
 IC 2190 - Spiral Galaxy with SN 2024dhp (T+16.6d)
Image
Annotated CCD Image (50% size, square root scale)
2 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 20:51 UT (#1198038-42)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
IC 2190 with SN 2024dhp - 2024-03-15 (T+16.6d)
Image below (2024-03-15.864) was taken 16.6 days after discovery of 2024dhp
Position of reported SN (faint) is indicated by white cross-hairs.
Estimated Magnitude +17.6 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
2 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 20:51 UT (#1198038-42)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of SN 2024dhp (in IC 2190) on Supernova 2024 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 - 2024-03-15 (T+301.2d)
Image below (2024-03-15.920) was taken 301.2 days after discovery of 2023ixf
Position of supernova (faint) is shown by white cross-hairs
Measured Magnitude +15.67 (Clear Filter)
Image
Annotated CCD Image (100% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 22:14 UT (#1198072-76)
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 - 2024-03-16 (T+46.9d)
Image below (2024-03-16.126) was taken 46.9 days after discovery of 2024bch
Position of reported SN (distinct but fading slowly) is indicated by white cross-hairs.
Measured Magnitude +14.06 (Clear Filter)
Poor quality image (due to wind shake)
Image
Annotated CCD Image (125% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 03:11 UT (#1198175-79)
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 3467 - Spiral Galaxy with Type MP Transient AT 2024dda

NGC 3467 with AT 2024dda (Leo)
AT 2024dda (Type: MP) discovered 2024-02-20.987 UT by Italian Supernovae Search Project
Alias: MP (18961
Discovery Magnitude 17.94 (Clear Filter)
vs Prior Non-Detection Limiting Mag 19.0
 ( TNS 2024dda )
 
NGC 3467 - Spiral Galaxy
Image
Annotated CCD Image (50% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 21:31 UT (#1198056-60)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
NGC 3467 with AT 2024dda - 2024-03-15 (T+23.9d)
Image below (2024-03-15.891) was taken 23.9 days after discovery of 2024dda
Position of reported transient (not visible) is indicated by white cross-hairs.
Non-Detection Limiting Magnitude +17.6 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 21:31 UT (#1198056-60)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of SN 2024dda (in IC 2190) on Transients 2024 Page >>

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NGC 3690 - Spiral Galaxy with Type Ia Supernova 2023wrk

NGC 3690 with SN 2023wrk (Ursa Major)
SN 2023wrk (Type: Ia) discovered 2023-11-04.229 UT by GOTO
Alias: GOTO23bdo, ZTF23abpbdfm, ATLAS23vna
Discovery Magnitude 18.11 (L-GOTO filter)
 ( Rochester Supernova site ) ( TNS 2023wrk )
NGC 3690 with SN 2023wrk - 2024-03-15 (T+132.7d)
Image below (2024-03-15.906) was taken 132.7 days after discovery of 2023wrk
Position of SN (fading) is shown by white cross-hairs
Measured Magnitude +16.82 (C Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 21:54 UT (#1198064-68)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of SN 2023wrk (in NGC 3690) on Supernovae 2023 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 - Spiral Galaxy with SN 2024drt (T+13.5d)
Image
Annotated CCD Image (50% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 22:38 UT (#1198080-84)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
NGC 4619 with SN 2024drt - 2024-03-15 (T+13.5d)
Image below (2024-03-15.937) was taken 13.5 days after discovery of 2024drt
Position of reported SN (distinct) is indicated by white cross-hairs.
Estimated Magnitude +15.6 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 22:38 UT (#1198080-84)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
NGC 4619 with SN 2024drt - Detail 2024-03-15 (T+13.5d)
Image
Negative CCD Image (175% size, square root scale, cropped)
Image details as above
  
NGC 4619 - Earlier Image (2006)
Image
CCD Image
2 x 2 min exposure (average combine), 2x2 binning, C Filter 
2006-04-23 23:08h UT (#116105-06)
8" LX200 Classic + ST-7E
 
Images of SN 2024drt (in NGC 4619) on Supernova 2024 Page >>

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NGC 4995 - Spiral Galaxy with Type II Supernova 2023gfo

NGC 4995 with SN 2023gfo (Virgo)
SN 2023gfo (Type: II) discovered 2023-04-20.209 UT by ATLAS
Alias: ATLAS23ioa
Discovery Magnitude 16.19 (cyan-ATLAS Filter)
 ( TNS 2023gfo )

 
NGC 4995 with SN 2023gfo - 2024-03-16 (T+330.9d)
Image below (2024-03-16.073) was taken 330.9 days after discovery of 2023gfo
Position of reported SN (barely visible) is shown by white cross-hairs 

Image

Annotated CCD Image (125% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 01:53 UT (#1198147-51)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
NGC 4995 with AT 2023gfo - Earlier Image, 2023-04-21 (T+1.8d)
Image below (2023-04-21.965) was taken 1.8 days after discovery of 2023gfo
Position of reported SN (distinct) is shown by white cross-hairs 
Measured Magnitude +15.00

Image

Annotated CCD Image (125% size, square root scale, cropped)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter
2023-04-21 23:17 UT (#1117035-38)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Images of SN 2023gfo (NGC 4995) on Supernova 2023 Page >>

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NGC 5036 - Elliptical Galaxy with Type Ia Supernova 2024dop

NGC 5036 with SN 2024dop (Virgo)
SN 2024dop (Type: Ia) discovered 2024-03-02.390 UT by ASAS-SN
Alias: ASASSN-24bm
Discovery Magnitude 16.4 (g-SLOAN Filter)
vs Prior Non-Detection Limiting Mag 16.7
 ( TNS 2024dop )
 
NGC 5036 - Elliptical Galaxy with SN 2024dop (T+13.6d)
Image
Annotated CCD Image (50% size, square root scale)
2 x 180s exposure (average combine), 3x3 binning, C Filter
2024-03-16 00:38 UT (#1198124-25)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
NGC 5036 with SN 2024dop - 2024-03-16 (T+13.6d)
Image below (2024-03-16.024) was taken 13.6 days after discovery of 2024dop
Position of reported SN (faint but distinct) is indicated by white cross-hairs.
Measured Magnitude +16.00 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
2 x 180s exposure (average combine), 3x3 binning, C Filter
2024-03-16 00:38 UT (#1198124-25)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Images of SN 2024dop (in NGC 5036) on Supernova 2024 Page >>

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NGC 6040 - Spiral Galaxy (ARP 122)

ARP / NGC 6040 (Hercules)
Alias: ARP 122
NGC 6040 & PGC 59642. cf. Ast. Now Mar 2024, p9
[ ARP Galaxies ]
Glare in top right corner is from HIP 78690 (mag 6.75)
Image
Annotated CCD Image (50% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 03:57 UT (#1198196-200)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
ARP 122
NGC 6040 & PGC 56942
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
 
NGC 6040 & PGC 56942 and Adjacent Galaxies
including NGC 6041 and NGC 6042
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
 
 

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NGC 6745 - Spiral Galaxy with Type II Supernova 2023ucy

NGC 6745 with SN 2023ucy (Lyra)
SN 2023ucy (Type: II) discovered 2023-10-05.151 UT by ZTF
Alias: ZTF23abhzxwm
Discovery Mag +17.9 (r-ZTF filter) vs last non-detection image with 19.91 limiting mag
It is noted that SN 2022prr (19:01:41.897, +40:45:03.67) occurred in Jul 2022
at approximately the same location as this newly
reported transient 2023ucy (19:01:41.992, +40:45:05.89)
(are they possibly related ?)
 ( TNS 2023ucy ) ( TNS 2022prr )
 
NGC 6745 with SN 2023ucy - 2024-03-16 (T+163.0d)
Image below (2024-03-16.190) was taken 163.0 days after discovery of 2023ucy
Position of SN (brightening slightly ?) is shown by white cross-hairs
Measured magnitude +14.94 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 04:42 UT (#1198211-15)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of SN 2023ucy (NGC 6745) on Supernovae 2023 Page >>

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Segue 1 - Faint Dwarf Galaxy - 0.075 mly

Segue 1 (Leo)
Milky Way Dwarf Galaxy Satellite

Segue 1 is a dwarf spheroidal galaxy or globular cluster situated in the Leo constellation
and discovered in 2006 by Sloan Digital Sky Survey.
It is located at a distance of about 75,000 light years

Segue 1 is one of the smallest and faintest satellites of the Milky Way.
Its integrated luminosity is about 300 times that of the Sun which is
much smaller than the luminosity of a typical globular cluster.
Observations however indicate its mass is about 600,000 solar masses,
which suggest that it is dominated by dark matter.

In the image below the approximate area of Segue 1 dwarf galaxy
 is indicated by large white circle. By comparison with reference image
(Keck/Deimos image) the visible stars that are understood to
lie in Segue 1 are indicated by green circles
 [ Local Group Galaxies ]

Note: a longer exposure is required to detect more stars lying in the dwarf galaxy
Image 
Annotated CCD Image (70% size, square root scale)
12 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 23:34 UT (#1198094-105)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Segue 1 - Earlier Image (Feb 2020)
Image 
Annotated CCD Image (70% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, C Filter
2020-02-20 23:58 UT (#753140-44)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Segue 1 - Keck/Deimos Reference Image
Image 
Credit: Marla Geha  
Image has been rotated and resized to match own image
 
Segue 1 - Unannotated Images
Image 
Annotated CCD Image (70% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, C Filter
2020-02-20 23:58 UT (#753140-44)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Image 
Negative CCD Image (70% size, square root scale)
Image details as above
 

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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 - 2024-03-15 (T+70.6d)
Image below (2024-03-15.999) was taken 70.6 days after discovery of 2024hw
Position of reported transient (faint) is indicated by white cross-hairs.
Estimated Magnitude +16.8 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 00:07 UT (#1198108-12)
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 - Elliptical Galaxy with  SN 2024drv  (T+13.6d)
Image
Annotated CCD Image (50% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 02:16 UT (#1198154-58)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
UGC 8630 with SN 2024drv - 2024-03-16 (T+13.6d)
Image below (2024-03-16.088) was taken 13.6 days after discovery of 2024drv
Position of reported SN (distinct) is indicated by white cross-hairs.
Measured Magnitude +14.92 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 02:16 UT (#1198154-58)
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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UGC 9002 - Spiral Galaxy with Type II Supernova 2023pls

UGC 9002 with SN 2023pls (Bootes)
SN 2023pls (Type: II) discovered 2023-08-14.976 UT by ATLAS
Alias: ATLAS23red, Gaia23cbq
Discovery Magnitude 17.54 (cyan-ATLAS)
z (redshift) = 0.0136
 ( TNS 2023pls | Gaia23cbq )
 
UGC 9002 with SN 2023pls - 2024-03-15 (T+214.0d)
Image below (2024-03-15.952) was taken 214.0 days after discovery of 2023pls
Position of reported SN (very faint & fading) is indicated by white cross-hairs.
Measured Magnitude +17.51 (Clear Filter)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-15 23:00 UT (#1198087-91)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
  
Images of SN 2023pls (in UGC 9002) on Supernova 2023 Page >>
  

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UGC 9659 - Spiral Galaxy with Type Ia Supernova 2024ech

UGC 9659 with SN 2024ech (Virgo)
SN 2024ech (Type: Ia) discovered 2024-03-09.610 UT by ASAS-SN
Alias: ASASSN-24bv
Discovery Magnitude 17.2 (g-SLOAN Filter)
vs Prior Non-Detection Limiting Mag 18.0
 ( TNS 2024ech )
 
UGC 9659 - Spiral Galaxy
Alias: PGC 53675
Image
Annotated CCD Image (50% size, square root scale)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 01:06 UT (#1198128-32)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
UGC 9659 with SN 2024ech - 2024-03-16 (T+6.4d)
Image below (2024-03-16.040) was taken 6.4 days after discovery of 2024ech
Position of reported SN (not separately identifed) is indicated by white cross-hairs.
Measured Magnitude, Nucleus & SN  +15.65 (Clear Filter)
Bright star in FOV is GSC 342:839 (catalog mag +11.9)
Image
Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter
2024-03-16 01:06 UT (#1198128-32)
12" LX200R (at f/10.4) + ST-10XME
Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2
 
Images of SN 2024ech (in UGC 9659) on Supernova 2024 Page >>

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