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12P/Pons-Brooks - 2024-01-17 (passing through Cygnus) Sun Distance 1.79 AU (approaching) Earth Distance 2.07 AU (310.3 million km) |
12P/Pons-Brooks - 2024-01-17 Detail Autoguided on offset star using PHD2 with Lock Shift set at the comet's rate of motion (Ra 128.53 arcsec/hr, Dec 3.51 arcsec/hr) |
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Annotated CCD Image (50% size, log scale) 90s exposure (single frame), 3x3 binning, Clear Filter 2024-01-17 05:52 UT (#1183129) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Annotated CCD Image (100% size, log root scale, cropped) 7 x 90s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 05:58 UT (#1183129-35) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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12P/Pons-Brooks - 2024-01-17 Detail | 12P/Pons-Brooks - 2024-01-17 Detail | |
Annotated false-colour CCD Image (50% size, log scale) 7 x 90s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 05:58 UT (#1183129-35) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Annotated false-colour CCD Image (100% size, log scale, cropped) Inverse Spectrum Image details as left |
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Images of 12P/Pons-Brooks on Comets 2023 Page >> | ||
Images of 12P/Pons-Brooks on Comets 2024 Page >> |
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62P/Tsuchinshan - 2024-01-17 (passing through Virgo) Sun Distance 1.29 AU (approaching) Earth Distance 0.50 AU (75.4 million km) |
62P/Tsuchinshan - 2024-01-17 Detail Autoguided on offset star using PHD2 with Lock Shift set at the comet's rate of motion (Ra 74.19 arcsec/hr, Dec -14.61 arcsec/hr) |
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Annotated CCD Image (50% size, square root scale) 2 x 90s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 02:40 UT (#1183051-52) 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 2024-01-17 02:38 UT (#1183047-53) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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62P/Tsuchinshan - 2024-01-17 Detail | 62P/Tsuchinshan - 2024-01-17 Detail | |
Annotated CCD Image (50% size, log scale) 7 x 90s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 02:38 UT (#1183047-53) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Annotated false-colour CCD Image (50% size, log scale) Inverse Spectrum Image details as left |
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Images of 62P/Tsuchinshan on Comets 2023 Page >> | ||
Images of 62P/Tsuchinshan on Comets 2024 Page >> |
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103P/Hartley - 2024-01-17 (passing through Puppis) Sun Distance 1.64 AU AU (receeding) Earth Distance 0.74 AU (110.3 million km) |
103P/Hartley - 2024-01-17 Detail Autoguided on offset star using PHD2 with Lock Shift set at the comet's rate of motion (Ra -47.78 arcsec/hr, Dec 23.89 arcsec/hr) |
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Annotated CCD Image (50% size, square root scale) 2 x 60s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 00:49 UT (#1183006-07) 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) 8 x 60s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 00:53 UT (#1183006-14) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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Images of 103P/Hartley on Comets 2023 Page >> | ||
Images of 103P/Hartley on Comets 2024 Page >> |
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Vega - TBA |
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AT 2024mu (Hercules) AT 2024mu (Type: CV) discovered 2024-01-04.095 UT by Gaia Alias: Gaia24adj Discovery magnitude 15.35 (G-Gaia Filter) vs Historic Magnitude 17.42 +/- 1.07 (SD) (Usual magnitude 19.0 +/- 0.8) Outburst in confirmed CV ASASSN-13bc ( TNS 2024mu | Gaia24adj ) |
AT 2024mu - 2024-01-17 (T+13.1d) Image below (2024-01-17.237) was taken 13.1 days after discovery of 2024mu Position of reported transient (very faint) is shown by white cross-hairs Estimated Magnitude +18.0 (Clear Filter) |
Annotated CCD Image (100% size, linear scale, cropped) 4 x 60s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 05:43 UT (#1183123-26) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Images of AT 2024mu on Transients 2024 Page >> |
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CGCG 160-062 with SN 2023ke (Coma Berenices) SN 2023ke (Type: Ia) discovered 2023-01-13.619 UT by ATLAS Alias: ATLAS23akr, ZTF18aahvkwq, PS23km Discovery Magnitude 15.96 (orange-ATLAS Filter) ( TNS 2023ke ) |
CGCG 160-062 / PGC 3073573 ? / PGC 44438- Galaxy |
CGCG 160-062 with SN 2023ke - 2024-01-17 (T+368.5d) Image below (2024-01-17.145) was taken 368.5 days after discovery of 2023ke Position of earlier SN (likely faded) is indicated by white cross-hairs. Light source visible at SN position is likely the nucleus of host galaxy Measured Magnitude ? (Clear Filter) |
Annotated CCD Image (125% size, square root scale, cropped) 2 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 03:32 UT (#1183081-82) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Images of SN 2023ke (in CGCG 160-062) on Supernova 2023 Page >> |
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IC 1125 with SN 2024jz (Serpens) SN 2024jz (Type: Ia) discovered 2024-01-05.641 UT by ATLAS Alias: ATLAS24ahj Discovery Magnitude 17.73 (orange-ATLAS Filter) ( TNS 2024jz ) |
IC 1125 with SN 2024jz - 2024-01-17 (T+11.6d) Image below (2024-01-17.222) was taken 11.6 days after discovery of 2024jz Position of reported supernova (distinct, brightening) is indicated by white cross-hairs. Measured Magnitude +14.87 (Clear Filter) |
Annotated CCD Image (150% size, square root scale, cropped) 4 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 05:26 UT (#1183116-19) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Images of SN 2024jz (in IC 1125) on Supernova 2024 Page >> |
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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 - 2024-01-17 (T+242.4d) Image below (2024-01-17.163) was taken 242.4 days after discovery of 2023ixf Position of supernova (fading) is shown by white cross-hairs Measured Magnitude +15.23 (Clear Filter) |
Annotated CCD Image (100% size, square root scale, cropped) 4 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 04:01 UT (#1183086-89) 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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MCG +9-27-70 with SN 2023acha (Draco) SN 2023acha (Type: Ia) discovered 2023-12-31.638 UT by ATLAS Alias: ATLAS23ych Discovery Magnitude 16.3 ( Clear Filter) ( TNS 2023acha ) |
MCG +9-27-70 with SN 2023acha - 2024-01-17 (T+16.6d) Image below (2024-01-17.264) was taken 16.6 days after discovery of 2023acha Position of reported SN (relatively distinct) is indicated by white cross-hairs. Estimated Magnitude +15.6 (Clear Filter) |
Annotated CCD Image (150% size, square root scale, cropped) 5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 06:29 UT (#1183143-47) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Images of SN 2023acha (in MCG +9-27-70) on Supernova 2023 Page >> |
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NGC 3893 with AT 2023uhx (Ursa Major) AT 2023uhx (Type: LRN) discovered 2023-10-07.816 UT by Koichi Itagaki Discovery magnitude 17.2 (Clear filter) vs DSS Archival Image Luminous Red Nova based on its peak luminosity, and narrow Balmer and Fe II emission lines. ( TNS 2023uhx) |
NGC 3893 with AT 2023uhx - 2024-01-17 (T+101.3d) Image below (2024-01-17.092) was taken 101.3 days after discovery of 2023uhx Position of reported transient (faint) is shown by white cross-hairs Measured Magnitude 17.56 (Clear Filter) |
Annotated CCD Image (125% size, square root scale, cropped) 5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 02:21 UT (#1183040-44) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Images of AT 2023uhx (NGC 3893) on Transients 2023 Page >> |
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NGC 4216 with SN 2024gy (Virgo) SN 2024gy (Type: Ia, z=0.001183) discovered 2024-01-04.678 UT by Koichi Itagaki Alias: AT2023acjv, AT2024ix, ASASSN-24ac, PSN J12155131+1306561 Discovery Magnitude 16.3 ( Clear Filter) ( TNS 2024gy ) |
NGC 4216 with SN 2024gy - 2024-01-17 (T+12.4d), Set 1 Image below (2024-01-17.069) was taken 12.4 days after discovery of 2024gy Position of reported SN (distinct, brightening) is indicated by white cross-hairs. Measured Magnitude +12.95 (Clear Filter) |
Annotated CCD Image (100% size, square root scale, cropped) 5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 01:47 UT (#1183028-32) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
NGC 4216 with SN 2024gy - 2024-01-17 (T+12.5d), Set 2 Image below (2024-01-17.130) was taken 12.5 days after discovery of 2024gy Position of reported SN (distinct, brightening) is indicated by white cross-hairs. Measured Magnitude +12.93 (Clear Filter) |
Annotated CCD Image (100% size, square root scale, cropped) 3 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 03:12 UT (#1183074-76) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
NGC 4216 with SN 2024gy - Spectral Image, 2024-01-17 (T+12.4d) |
Annotated Realtime CCD Image (35% size, linear scale) 180s exposure (single frame / unprocessed), 2x2 binning, Clear Filter 2024-01-17 01:25 UT (#1183023) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
SN 2024gy - Spectrum, 2024-01-17 (T+12.4d) |
Annotated CCD Image (100% size, square root scale, rotated, cropped) 5 x 180s exposure (average combine), 3x3 binning, S Filter (SA200) 2024-01-17 02:59 UT (#1183069-73) 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, rotated, cropped) 5 x 180s exposure (average combine), 3x3 binning, S Filter (SA200) 2024-01-17 02:59 UT (#1183069-73) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Spectra Chart 5 x 180s exposure (average combine), 3x3 binning, S Filter (SA200) 2024-01-17 02:59 UT (#1183069-73) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Spectra Chart 5 x 180s exposure (average combine), 2x2 binning, S Filter (SA200) 2024-01-17 01:31 UT (#1183023-27) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Generated using ExtractSpectra tool in AstroMain 3.71.12 which
includes new option to create spectra based on user entry of objects X/Y coordinates for an image that refuses to Image Link / Plate Solve |
Images of SN 2024gy (in NGC 4216) on Supernova 2024 Page >> |
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NGC 4415 with SN 2022pul (Virgo) SN 2022pul (Type: Ia) discovered 2022-07-26.730 UT by ASAS-SN Alias: ASASSN-22jp, ATLAS22zkt, TCP J12264894+0826566 Discovery Mag 15.9 (g-Sloan Filter) ( Rochester Supernova site | TNS 2022pul ) |
NGC 4415 with SN 2022pul - 2024-01-17 (T+539.4d) Image below (2024-01-17.175) was taken 539.4 days after discovery of 2022pul Position of SN (faded & no longer visible) is shown by white cross-hairs Non Detection, limiting magnitude +19.3 (Clear Filter) |
Annotated CCD Image (100% size, square root scale, cropped) 5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 04:21 UT (#1183094-98) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
NGC 4415 with SN 2022pul - Earlier Image, 2023-01-27 (T+184.4d) Image below (2023-01-27.140) was taken 184.4 days after discovery of 2022pul Position of SN (distinct) is shown by white cross-hairs Measured magnitude +15.85 |
Annotated CCD Image (100% size, square root scale, cropped) 4 x 180s exposure (average combine), 3x3 binning, Clear Filter 2023-01-27 03:30 UT (#1091123-27) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Images of SN 2022pul (NGC 4415) on Supernovae 2022 Page >> |
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NGC 5468 with SN 2023cj (Virgo) SN 2023cj (Type: Ic) discovered 2023-01-05.845 UT by Gaia Alias: Gaia23ada Discovery Mag 16.97 (G-Gaia Filter) ( TNS 2023cj | Gaia23ada ) |
NGC 5468 with SN 2023cj - 2024-01-17 (T+376.4d) Image below (2024-01-17.205) was taken 376.4 days after discovery of 2023cj Position of earlier supernova (no longer visible) is shown by white cross-hairs Non Detection, limiting magnitude +18.0 (Clear Filter) |
Annotated CCD Image (125% size, square root scale, cropped) 3 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 05:00 UT (#1183108-10) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
NGC 5468 with SN 2023cj - Earlier Image, 2023-01-12 (T+6.4d) Image below (2023-01-12.272) was taken 6.4 days after discovery of 2023cj Position of reported supernova (distinct) is shown by white cross-hairs Measured magnitude +15.74 |
Annotated CCD Image (125% size, square root scale, cropped) 5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2023-01-12 06:40 UT (#1085149-53) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Images of SN 2023cj (NGC 5468) on Supernova 2023 Page >> |
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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 - 2024-01-17 (T+104.1d) Image below (2024-01-17.279) was taken 104.1 days after discovery of 2023ucy Position of SN (fading) is shown by white cross-hairs Measured magnitude +15.13 (Clear Filter) |
Annotated CCD Image (150% size, square root scale, cropped) 5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 06:51 UT (#1183150-54) 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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UGCA 287 (Virgo) Alias: PGC 41743 (catalog mag +15.4) [ UGCA Galaxies ] Other faint galaxies in FOV include PGC 976158 (catalog mag +15.9), PGC 976178 (catalog mag +16.9), PGC 974560 (catalog mag +17.5) |
Annotated CCD Image (50% size, square root scale) 5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 04:41 UT (#1183101-05) 12" LX200R (at f/5.7) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
UGCA 287 - Detail |
Annotated CCD Image (125% size, square root scale, cropped) Image details as above |
Negative CCD Image (125% size, square root scale, cropped) Image details as above |
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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 - 2024-01-17 (T+11.7d) Image below (2024-01-17.082) was taken 11.7 days after discovery of 2024hw Position of reported transient (faint) is indicated by white cross-hairs. Estimated Magnitude +16.3 (Clear Filter) |
Annotated CCD Image (150% size, square root scale, cropped) 3 x 180s exposure (average combine), 3x3 binning, Clear Filter 2024-01-17 02:03 UT (#1183035-37) 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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This Web Page: | Images - Session 1183 (2024-01-16) |
Last Updated : | 2024-11-03 |
Site Owner : | David Richards |
Home Page : | David's Astronomy Web Site |