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10P/Tempel - 2026-04-02 (passing through Serpens) Sun Distance 1.87 AU Earth Distance 1.45 AU (217.6 million km) |
10P/Tempel - 2026-04-02 Detail
Autoguided on offset star using PHD2 with Lock Shift set at the comet's rate of motion (Ra 72.2 arcsec/hr, Dec 6.5 arcsec/hr) Position of comet (not visible) is shown by white cross-hairs |
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Annotated CCD Image (50% size, square root scale)
2 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 03:01 UT (#1415139-41) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Annotated CCD Image (125% size, square root scale, cropped)
Image details as left |
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| Images of Comet_10P_Tempel on Comets 2026 Page >> | ||
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29P/Schwassmann-Wachmann - 2026-04-02 (passing through Leo) Sun Distance 6.31 AU Earth Distance 5.39 AU (806.0 million km) Poor quality image (bright moonlit sky background) |
29P/Schwassmann-Wachmann - 2026-04-02 Detail
Autoguided on offset star using PHD2 with Lock Shift set at the comet's rate of motion (Ra -13.7 arcsec/hr, Dec 5.7 arcsec/hr) Measured M2 Magnitude +16.10 (Clear Filter) |
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Annotated CCD Image (50% size, square root scale)
7 x 90s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 00:10 UT (#1415054-60) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Annotated CCD Image (125% size, square root scale, cropped)
Image details as above |
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| Images of Comet_29P_Schwassmann-Wachmann on Comets 2026 Page >> | ||
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240P/NEAT - 2026-04-01 (passing through Auriga) Sun Distance 2.27 AU Earth Distance 2.47 AU (369.0 million km) |
240P/NEAT - 2026-04-01 Detail
Autoguided on offset star using PHD2 with Lock Shift set at the comet's rate of motion (Ra 63.7 arcsec/hr, Dec 16.0 arcsec/hr) |
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Annotated CCD Image (50% size, square root scale)
3 x 60s exposure (average combine), 3x3 binning, Clear Filter 2026-04-01 22:51 UT (#1415015-17) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Annotated CCD Image (125% size, square root scale, cropped)
8 x 60s exposure (average combine), 3x3 binning, Clear Filter 2026-04-01 22:54 UT (#1415015-23) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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| Images of Comet_240P_NEAT on Comets 2026 Page >> | ||
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C/2022 N2 (PANSTARRS) - 2026-04-01 (passing through Taurus) Sun Distance 4.38 AU Earth Distance 4.88 AU (730.4 million km) |
C/2022 N2 (PANSTARRS) - 2026-04-01 Detail
Autoguided on offset star using PHD2 with Lock Shift set at the comet's rate of motion (Ra 37.3 arcsec/hr, Dec 4.4 arcsec/hr) |
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Annotated CCD Image (50% size, square root scale)
5 x 60s exposure (average combine), 3x3 binning, Clear Filter 2026-04-01 22:36 UT (#1415005-09) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Annotated CCD Image (125% size, square root scale, cropped)
5 x 60s exposure (average combine), 3x3 binning, Clear Filter 2026-04-01 22:36 UT (#1415005-09) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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| Images of C2022_N2_PANSTARRS on Comets 2026 Page >> | ||
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C/2025 R3 (PANSTARRS) - 2026-04-02 (passing through Pegasus) Sun Distance 0.65 AU Earth Distance 1.21 AU (181.0 million km) |
C/2025 R3 (PANSTARRS) - 2026-04-02 Detail
Autoguided on offset star using PHD2 with Lock Shift set at the comet's rate of motion (Ra 58.0 arcsec/hr, Dec 5.9 arcsec/hr) |
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Annotated CCD Image (50% size, log scale)
2 x 60s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 03:45 UT (#1415156-57) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
Annotated CCD Image (100% size, log scale, cropped)
7 x 60s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 03:48 UT (#1415156-63) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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| Images of C2025_R3_PANSTARRS on Comets 2026 Page >> | ||
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KIC 8462852 (Cygnus)
Alias: Tabby's Star, Boyajian's Star, WTF Star Star shows large irregular dimmings. 1470 ly. Mag +11.7 |
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KIC 8462852 (Cygnus)
Position of earlier transient (distinct) is shown by white cross-hairs Measured Magnitude +11.81 (Clear Filter) |
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Annotated CCD Image (100% size, linear scale, cropped)
3 x 60s exposure (average combine), 3x3 binning, V Filter 2026-04-02 03:14 UT (#1415144-46) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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AT 2026fkw (Libra)
AT 2026fkw (Type: CV) discovered 2026-03-12.881 UT by jiashuo Zhang Alias: STSP J154537.89-203632.8, LP 803-27 Discovery Magnitude 16.24 (Clear- Filter) vs Prior Non-Detection Limiting Magnitude ( Filter) Group reports the discovery of a candidate dwarf nova. ( TNS 2026fkw ) |
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AT 2026fkw - 2026-04-02 (T+20.2d)
Image below (2026-04-02.115) was taken 20.2 days after discovery of 2026fkw Position of earlier transient (faint) is shown by white cross-hairs Measured Magnitude +15.53 (Clear Filter) |
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Annotated CCD Image (100% size, linear scale, cropped)
4 x 60s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 02:47 UT (#1415130-33) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of AT 2026fkw on Transients 2026 Page >> |
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AT 2026hix (Canis Minor)
AT 2026hix (Type: CV?) discovered 2026-03-25.730 UT by XOSS Alias: KATS26F003 Discovery Magnitude 16.23 (Clear- Filter) vs Prior Non-Detection Limiting Magnitude ( Filter) Cataclysmic variable candidate classified by XOSS. Details can be found at http://xjltp.china-vo.org/kats26f003.html ( TNS 2026hix ) |
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AT 2026hix - 2026-04-01 (T+7.2d)
Image below (2026-04-01.973) was taken 7.2 days after discovery of 2026hix Position of earlier transient (not visible) is shown by white cross-hairs Non-Detection Limiting Magnitude +17.1 (Clear Filter) |
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Annotated CCD Image (100% size, linear scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-01 23:30 UT (#1415037-41) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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AT 2026hix - Earlier Image, 2026-03-31 (T+6.1d)
Image below (2026-03-31.858) was taken 6.1 days after discovery of 2026hix Position of earlier transient (very faint) is shown by white cross-hairs Measured Magnitude +17.16 (Clear Filter) |
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Annotated CCD Image (100% size, linear scale, cropped)
3 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-03-31 20:43 UT (#1414012-15) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of AT 2026hix on Transients 2026 Page >> |
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AT 2026hur (Serpens)
AT 2026hur (Type: CV?) discovered 2026-03-29.850 UT by XOSS Alias: KATS26F005 Discovery Magnitude 15.81 (Clear- Filter) vs Prior Non-Detection Limiting Magnitude ( Filter) Cataclysmic variable candidate classified by XOSS. Details can be found at http://xjltp.china-vo.org/kats26f005.html ( TNS 2026hur ) |
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AT 2026hur - 2026-04-02 (T+3.2d)
Image below (2026-04-02.084) was taken 3.2 days after discovery of 2026hur Position of earlier transient (faint) is shown by white cross-hairs Measured Magnitude +16.11 (Clear Filter) |
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Annotated CCD Image (100% size, linear scale, cropped)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 02:10 UT (#1415114-18) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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AT 2026hur - 2026-04-02 (T+3.2d)
Image below (2026-04-02.084) was taken 3.2 days after discovery of 2026hur Object shown by white cross-hairs is believed to be the reported transient, but is slightly offset from its reported coordinates Another transient is possibly present in image at position indicated by yellow cross-hair. Possibility is that the reported transient might have been an asterord, rather the dwarf nova suggested by the discoveries |
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Annotated CCD Image (175% size, linear scale, cropped)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 02:10 UT (#1415114-18) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of AT 2026hur on Transients 2026 Page >> |
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NGC 6070 with SN 2026ejy (Serpens)
SN 2026ejy (Type: II) discovered 2026-02-25.180 UT by ATLAS Alias: GOTO26bnq, ZTF26aaiedvz, ATLAS26coa, BGEM J161000.25+004220.7 Discovery Magnitude 18.55 (L-GOTO Filter) vs Prior Non-Detection Limiting Magnitude 20.4 (L-GOTO Filter) ( TNS 2026ejy ) |
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NGC 6070 with SN 2026ejy - 2026-04-02 (T+35.9d)
Image below (2026-04-02.053) was taken 35.9 days after discovery of 2026ejy Position of earlier supernova (faint) is shown by white cross-hairs Measured Magnitude +15.53 (Clear Filter) Poor quality image (due to bright moonlit sky background, single frame) |
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Annotated CCD Image (125% size, square root scale, cropped)
180s exposure (single frame), 3x3 binning, Clear Filter 2026-04-02 01:17 UT (#1415087) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of SN 2026ejy (in NGC 6070) on Supernovae 2026 Page >> |
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NGC 7292 with SN 2026fov (Pegasus)
SN 2026fov (Type: II) discovered 2026-03-14.851 UT by Koichi Itagaki Alias: ZTF26aaltzhc Discovery Magnitude 13.5 (Clear- Filter) vs Prior Non-Detection Limiting Magnitude ( Filter) 0.35-m F/11 + CCD (KAF-1001E) unfiltered ( TNS 2026fov ) [ Irregular Galaxies ] |
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NGC 7292 with SN 2026fov - 2026-04-02 (T+18.3d)
Image below (2026-04-02.141) was taken 18.3 days after discovery of 2026fov Position of earlier supernova (distinct) is shown by white cross-hairs Measured Magnitude +13.79 (Clear Filter) |
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Annotated CCD Image (125% size, square root scale, cropped)
3 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 03:28 UT (#1415149-51) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of SN 2026fov (in NGC 7292) on Supernovae 2026 Page >> |
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UGC 5381 with SN 2025ahep (Leo)
SN 2025ahep (Type: II) discovered 2025-12-17.443 UT by ATLAS Alias: ZTF25acinfdh Discovery Magnitude 17.506 (g-ZTF Filter) vs Prior Non-Detection Limiting Magnitude 21.0114 (g-ZTF Filter) Bright (m_peak <= 18.5) transient candidate identified autonomously by BTSbot (Rehemtulla et al. 2024; arXiv:2401.15167). ( TNS 2025ahep ) |
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UGC 5381 with SN 2025ahep - 2026-04-01 (T+105.5d)
Image below (2026-04-01.989) was taken 105.5 days after discovery of 2025ahep Position of earlier supernova (barely visible) is shown by white cross-hairs Limiting Magnitude +19.0 (Clear Filter) Poor quality image (poor transparency, uneven sky background) |
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Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-01 23:53 UT (#1415045-49) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of SN 2025ahep (in UGC 5381) on Supernovae 2025 Page >> |
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UGC 9533 with AT 2026hvo (Bootes)
AT 2026hvo (Type: unconf) discovered 2026-03-29.917 UT by Paolo Demaria Discovery Magnitude 15 (L- Filter) vs Prior Non-Detection Limiting Magnitude ( Filter) Captured with Seestar S50 during photometric session on EL Boo ( TNS 2026hvo ) |
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UGC 9533 with AT 2026hvo - 2026-04-02 (T+3.1d)
Image below (2026-04-02.031) was taken 3.1 days after discovery of 2026hvo Position of earlier transient (not visible) is shown by white cross-hairs Non-Detection Limiting Magnitude +18.2 (Clear Filter) |
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Annotated CCD Image (150% size, square root scale, cropped)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 00:51 UT (#1415076-79) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of AT 2026hvo on Transients 2026 Page >> |
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UGC 11058 with SN 2026ewd (Hercules)
SN 2026ewd (Type: Ia) discovered 2026-03-05.583 UT by ATLAS Alias: ATLAS26cph, GOTO26bqj, ZTF26aajugdc Discovery Magnitude 17.346 (orange-ATLAS Filter) vs Prior Non-Detection Limiting Magnitude 19.52 (cyan-ATLAS Filter) ( TNS 2026ewd ) |
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UGC 11058 with SN 2026ewd - 2026-04-02 (T+27.5d)
Image below (2026-04-02.099) was taken 27.5 days after discovery of 2026ewd Position of earlier supernova (faint but distinct, fading) is shown by white cross-hairs Measured Magnitude +15.48 (Clear Filter) |
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Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 02:32 UT (#1415121-25) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of SN 2026ewd (in UGC 11058) on Supernovae 2026 Page >> |
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UGC 9533 with AT 2026hvo (Bootes)
AT 2026hvo (Type: unconf) discovered 2026-03-29.917 UT by Paolo Demaria Discovery Magnitude 15 (L- Filter) vs Prior Non-Detection Limiting Magnitude ( Filter) Captured with Seestar S50 during photometric session on EL Boo ( TNS 2026hvo ) |
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UGC 9533 with AT 2026hvo - 2026-04-02 (T+3.1d)
Image below (2026-04-02.031) was taken 3.1 days after discovery of 2026hvo Position of earlier transient (not visible) is shown by white cross-hairs Non-Detection Limiting Magnitude +18.2 (Clear Filter) |
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Annotated CCD Image (150% size, square root scale, cropped)
4 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 00:51 UT (#1415076-79) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of AT 2026hvo on Transients 2026 Page >> |
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UGC 11058 with SN 2026ewd (Hercules)
SN 2026ewd (Type: Ia) discovered 2026-03-05.583 UT by ATLAS Alias: ATLAS26cph, GOTO26bqj, ZTF26aajugdc Discovery Magnitude 17.346 (orange-ATLAS Filter) vs Prior Non-Detection Limiting Magnitude 19.52 (cyan-ATLAS Filter) ( TNS 2026ewd ) |
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UGC 11058 with SN 2026ewd - 2026-04-02 (T+27.5d)
Image below (2026-04-02.099) was taken 27.5 days after discovery of 2026ewd Position of earlier supernova (faint but distinct, fading) is shown by white cross-hairs Measured Magnitude +15.48 (Clear Filter) |
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Annotated CCD Image (150% size, square root scale, cropped)
5 x 180s exposure (average combine), 3x3 binning, Clear Filter 2026-04-02 02:32 UT (#1415121-25) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
| Images of SN 2026ewd (in UGC 11058) on Supernovae 2026 Page >> |
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KIC 8462852 (Cygnus)
Alias: Tabby's Star, Boyajian's Star, WTF Star Star shows large irregular dimmings. 1470 ly. Mag +11.7 |
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KIC 8462852 (Cygnus)
Position of earlier transient (distinct) is shown by white cross-hairs Measured Magnitude +11.81 (Clear Filter) |
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Annotated CCD Image (100% size, linear scale, cropped)
3 x 60s exposure (average combine), 3x3 binning, V Filter 2026-04-02 03:14 UT (#1415144-46) 12" LX200R (at f/10.4) + ST-10XME Auto-guided using TS 80mm APO, ZWO ASI178MC & PHD2 |
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| This Web Page: | Images - Session 1415 (2026-04-01) |
| Last Updated : | 2026-05-22 |
| Site Owner : | David Richards |
| Home Page : | David's Astronomy Web Site |