Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731   9.95  07:31:59.59 -31:15:03.8
245.15063  -5.89028 galactic  Pup  Second-epoch detections are separated by 0.2" and 7.3 pix   
The object was found in VSX
 2"  ASAS J073200-3115.0           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    10.940   V       Y     0.530   V         2452043.20000         69.200000000000   M5                           
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:31:59.59 -31:15:03.8:  10.99 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:31:59.59 -31:15:03.8:  10.89 +/- 0.01  detection
Forced photometry reference-image weighted average:  10.94 +/- 0.01
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6568.95898 4833.20996 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 3043.61426 1525.86841 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6514.42627 4925.26221 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6511.96045 4932.09375 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 31 59.59 -31 15 03.8           9.9 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 31 59.60 -31 15 03.8           9.9 R      V36
     TAU0008  C2026 11 05.37339 07 31 59.58 -31 15 03.8          10.0 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 31 59.59 -31 15 03.8   9.9 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J073200-3115.0,2461349.8731,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J073200-3115.0 20261105.3731 9.95CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731   9.70  07:23:06.57 -29:22:22.4
242.57905  -6.70847 galactic  CMa  Second-epoch detections are separated by 0.0" and 7.1 pix   
The object was found in VSX
 2"  V0351 CMa                     
Type: SRA
#   Max.           Min./Amp.       JD0           Period
    10.700   V            12.500   V         2452785.00000        320.000000000000   M7                           
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:23:06.57 -29:22:22.4:  10.95 +/- 0.01  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:23:06.57 -29:22:22.4:  10.65 +/- 0.01  detection
Forced photometry reference-image weighted average:  10.76 +/- 0.01
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 5431.42383 5995.16846 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 4198.27783 379.11731 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 5343.93604 6043.39795 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 5341.47217 6050.09766 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 23 06.57 -29 22 22.4           9.7 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 23 06.57 -29 22 22.4           9.7 R      V36
     TAU0008  C2026 11 05.37339 07 23 06.57 -29 22 22.4           9.7 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 23 06.57 -29 22 22.4   9.7 U             CMa       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0351 CMa,2461349.8731,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0351 CMa 20261105.3731 9.70CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731   9.86  07:15:40.07 -31:32:06.3
243.79404  -9.11645 galactic  CMa  Second-epoch detections are separated by 1.4" and 7.0 pix   
The object was found in VSX
 2"  ASAS J071540-3132.1           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.370   V       Y     0.580   V         2451990.80000         68.000000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:15:40.07 -31:32:06.3:  11.16 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:15:40.07 -31:32:06.3:  10.80 +/- 0.01  detection
Forced photometry reference-image weighted average:  10.93 +/- 0.01
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 4458.37354 4684.27539 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 5152.82910 1704.49597 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 4417.69141 4704.64014 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 4415.27539 4711.18066 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 15 40.07 -31 32 06.3           9.9 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 15 40.02 -31 32 06.0           9.9 R      V36
     TAU0008  C2026 11 05.37339 07 15 40.12 -31 32 06.5           9.8 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 15 40.07 -31 32 06.3   9.9 U             CMa       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J071540-3132.1,2461349.8731,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J071540-3132.1 20261105.3731 9.86CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.58  07:50:27.36 -35:30:29.7
250.77047  -4.60786 galactic  Pup  Second-epoch detections are separated by 2.1" and 7.2 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
 online_id        | target                       | 07:50:27.36 -35:30:29.7 (user input)  | T                | P                    |  (position from user input)                                                  
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:50:27.36 -35:30:29.7:  12.52 +/- 0.06  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:50:27.36 -35:30:29.7:  12.71 +/- 0.08  detection
Forced photometry reference-image weighted average:  12.60 +/- 0.05
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits  wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 8795.90625 2313.78149 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 8793.47949 2320.55640 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 50 27.36 -35 30 29.7          11.6 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 50 27.44 -35 30 30.0          11.6 R      V36
     TAU0008  C2026 11 05.37339 07 50 27.28 -35 30 29.4          11.6 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 50 27.36 -35 30 29.7  11.6 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461349.8731,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261105.3731 11.58CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  12.97  07:51:46.18 -30:10:27.6
246.30890  -1.66083 galactic  Pup  Second-epoch detections are separated by 1.1" and 7.1 pix   
The object was found in VSX
 6"  GDS_J0751466-301027           
Type: VAR
#   Max.           Min./Amp.       JD0           Period
    14.540   r       Y     0.460   r                                                                              
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:51:46.18 -30:10:27.6:  14.39 +/- 0.35  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:51:46.18 -30:10:27.6:  14.07 +/- 0.28  detection
Forced photometry reference-image weighted average:  14.20 +/- 0.22
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits  wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 9122.48926 5539.98389 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 9120.45020 5546.81689 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 51 46.18 -30 10 27.6          13.0 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 51 46.15 -30 10 28.0          12.9 R      V36
     TAU0008  C2026 11 05.37339 07 51 46.21 -30 10 27.3          13.1 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 51 46.18 -30 10 27.6  13.0 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0751466-301027,2461349.8731,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0751466-301027 20261105.3731 12.97CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.69  07:45:26.24 -37:08:36.9
251.68886  -6.29905 galactic  Pup  Second-epoch detections are separated by 1.2" and 6.6 pix   
The object was found in VSX
 3"  ASASSN-V J074526.44-370838.4  
Type: M
#   Max.           Min./Amp.       JD0           Period
    15.500   g       Y     3.510   g         2459263.64400        207.000000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:45:26.24 -37:08:36.9:  12.89 +/- 0.10  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:45:26.24 -37:08:36.9:  13.46 +/- 0.17  detection
Forced photometry reference-image weighted average:  13.02 +/- 0.08
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 8087.33887 1184.14453 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 1474.22205 5155.84814 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 8138.64307 1350.18945 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 8136.74902 1356.55896 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 45 26.24 -37 08 36.9          11.7 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 45 26.20 -37 08 36.6          11.7 R      V36
     TAU0008  C2026 11 05.37339 07 45 26.29 -37 08 37.2          11.6 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 45 26.24 -37 08 36.9  11.7 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J074526.44-370838.4,2461349.8731,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J074526.44-370838.4 20261105.3731 11.69CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.38  07:54:18.41 -34:34:52.9
250.37264  -3.45772 galactic  Pup  Second-epoch detections are separated by 1.6" and 7.1 pix   
The object was found in VSX
 5"  GDS_J0754187-343452           
Type: VAR
#   Max.           Min./Amp.       JD0           Period
    12.880   r       Y     0.380   r                                                 M4:                          
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:54:18.41 -34:34:52.9:  12.44 +/- 0.06  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:54:18.41 -34:34:52.9:  12.70 +/- 0.09  detection
Forced photometry reference-image weighted average:  12.52 +/- 0.05
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 9307.29590 2652.34131 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 274.37930 3670.86255 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 9307.92480 2851.15552 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 9305.91113 2857.94824 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 54 18.41 -34 34 52.9          11.4 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 54 18.38 -34 34 53.5          11.4 R      V36
     TAU0008  C2026 11 05.37339 07 54 18.45 -34 34 52.2          11.3 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 54 18.41 -34 34 52.9  11.4 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0754187-343452,2461349.8731,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0754187-343452 20261105.3731 11.38CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  12.43  07:13:38.92 -33:42:29.6
245.58616 -10.45229 galactic  Pup  Second-epoch detections are separated by 1.2" and 6.8 pix   
The object was found in VSX
 0"  ASASSN-V J071338.89-334229.9  
Type: L
#   Max.           Min./Amp.       JD0           Period
    13.130   V            13.570   V                                                                              
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:13:38.92 -33:42:29.6:  13.30 +/- 0.10  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:13:38.92 -33:42:29.6:  13.35 +/- 0.11  detection
Forced photometry reference-image weighted average:  13.32 +/- 0.08
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 4214.48096 3369.54199 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 5377.90137 3023.15674 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 4217.65674 3387.43701 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 4215.30615 3393.76489 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 13 38.92 -33 42 29.6          12.4 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 13 38.92 -33 42 29.0          12.4 R      V36
     TAU0008  C2026 11 05.37339 07 13 38.91 -33 42 30.2          12.5 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 13 38.92 -33 42 29.6  12.4 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J071338.89-334229.9,2461349.8731,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J071338.89-334229.9 20261105.3731 12.43CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.34  07:48:07.22 -36:43:44.5
251.59356  -5.62801 galactic  Pup  Second-epoch detections are separated by 2.8" and 7.3 pix   
The object was found in VSX
 4"  ASASSN-V J074807.44-364347.0  
Type: SR
#   Max.           Min./Amp.       JD0           Period
    13.910   V            14.130   V         2458023.00000        148.000000000000   M9                           
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:48:07.22 -36:43:44.5:  12.97 +/- 0.10  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:48:07.22 -36:43:44.5:  13.29 +/- 0.15  detection
Forced photometry reference-image weighted average:  13.07 +/- 0.09
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 8433.74707 1415.00269 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 1131.38879 4920.26123 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 8475.16699 1588.10107 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 8473.12305 1595.08655 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 48 07.22 -36 43 44.5          11.3 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 48 07.25 -36 43 45.9          11.4 R      V36
     TAU0008  C2026 11 05.37339 07 48 07.19 -36 43 43.1          11.2 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 48 07.22 -36 43 44.5  11.3 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J074807.44-364347.0,2461349.8731,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J074807.44-364347.0 20261105.3731 11.34CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.28  07:44:10.83 -36:14:05.6
250.76823  -6.07215 galactic  Pup  Second-epoch detections are separated by 1.3" and 7.0 pix   
The object was found in VSX
 3"  ASAS J074411-3614.2           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
     9.131   Ic      Y     0.294   Ic        2452768.80000         96.000000000000   M8                           
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:44:10.83 -36:14:05.6:  12.36 +/- 0.05  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:44:10.83 -36:14:05.6:  13.08 +/- 0.11  detection
Forced photometry reference-image weighted average:  12.49 +/- 0.05
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 7967.28320 1746.32886 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 1601.84705 4595.41602 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 8002.74854 1903.85754 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 8000.75732 1910.53015 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 44 10.83 -36 14 05.6          11.3 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 44 10.79 -36 14 06.0          11.3 R      V36
     TAU0008  C2026 11 05.37339 07 44 10.87 -36 14 05.1          11.3 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 44 10.83 -36 14 05.6  11.3 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J074411-3614.2,2461349.8731,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J074411-3614.2 20261105.3731 11.28CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.10  06:59:34.40 -35:37:26.6
246.12982 -13.88180 galactic  Pup  Second-epoch detections are separated by 0.7" and 6.8 pix   
The object was found in VSX
 2"  ASAS J065934-3537.5           
Type: SR
#   Max.           Min./Amp.       JD0           Period
     8.877   Ic      Y     0.246   Ic        2453060.70000        315.000000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 06:59:34.40 -35:37:26.6:  12.35 +/- 0.05  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 06:59:34.40 -35:37:26.6:  12.13 +/- 0.04  detection
Forced photometry reference-image weighted average:  12.21 +/- 0.03
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 2496.30957 2159.31958 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 7078.66650 4257.43359 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 2546.63477 2123.61255 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 2544.39600 2130.06519 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 06 59 34.40 -35 37 26.6          11.1 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 06 59 34.37 -35 37 26.4          11.1 R      V36
     TAU0008  C2026 11 05.37339 06 59 34.42 -35 37 26.9          11.1 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  06 59 34.40 -35 37 26.6  11.1 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J065934-3537.5,2461349.8731,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J065934-3537.5 20261105.3731 11.10CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.34  07:51:09.29 -37:38:28.5
252.69104  -5.56172 galactic  Pup  Second-epoch detections are separated by 5.4" and 6.1 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
 online_id        | target                       | 07:51:09.29 -37:38:28.5 (user input)  | T                | P                    |  (position from user input)                                                  
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:51:09.29 -37:38:28.5:  12.43 +/- 0.07  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:51:09.29 -37:38:28.5:  12.78 +/- 0.10  detection
Forced photometry reference-image weighted average:  12.54 +/- 0.05
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 8764.32715 827.07422 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 793.02039 5503.96143 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 8821.25488 1019.61823 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 8818.91699 1025.23621 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 51 09.29 -37 38 28.5          11.3 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 51 09.37 -37 38 25.9          11.3 R      V36
     TAU0008  C2026 11 05.37339 07 51 09.22 -37 38 31.0          11.3 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 51 09.29 -37 38 28.5  11.3 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461349.8731,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261105.3731 11.34CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.16  07:07:40.70 -35:32:49.5
246.74976 -12.34665 galactic  Pup  Second-epoch detections are separated by 0.2" and 7.0 pix   
The object was found in VSX
 1"  ASAS J070740-3532.8           
Type: SRB
#   Max.           Min./Amp.       JD0           Period
    12.200   V            12.900   V         2458104.73000         68.200000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:07:40.70 -35:32:49.5:  12.28 +/- 0.04  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:07:40.70 -35:32:49.5:  12.13 +/- 0.04  detection
Forced photometry reference-image weighted average:  12.19 +/- 0.03
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 3493.69922 2244.87646 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 6082.32275 4157.74805 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 3536.55444 2242.99731 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 3534.28418 2249.61670 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 07 40.70 -35 32 49.5          11.2 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 07 40.69 -35 32 49.5          11.2 R      V36
     TAU0008  C2026 11 05.37339 07 07 40.71 -35 32 49.6          11.1 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 07 40.70 -35 32 49.5  11.2 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J070740-3532.8,2461349.8731,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J070740-3532.8 20261105.3731 11.16CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  12.20  07:38:48.75 -33:40:29.4
247.98175  -5.78651 galactic  Pup  Second-epoch detections are separated by 1.9" and 7.4 pix   
The object was found in VSX
 1"  ASASSN-V J073848.83-334028.5  
Type: L
#   Max.           Min./Amp.       JD0           Period
    13.530   V            14.030   V                                                                              
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:38:48.75 -33:40:29.4:  13.25 +/- 0.11  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:38:48.75 -33:40:29.4:  13.55 +/- 0.15  detection
Forced photometry reference-image weighted average:  13.35 +/- 0.09
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 7382.24414 3333.76831 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 2208.84888 3014.90210 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 7371.64209 3461.02808 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 7369.34473 3468.06909 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 38 48.75 -33 40 29.4          12.2 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 38 48.76 -33 40 30.3          12.2 R      V36
     TAU0008  C2026 11 05.37339 07 38 48.73 -33 40 28.5          12.2 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 38 48.75 -33 40 29.4  12.2 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J073848.83-334028.5,2461349.8731,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J073848.83-334028.5 20261105.3731 12.20CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  12.25  07:33:17.80 -33:38:49.6
247.40550  -6.78150 galactic  Pup  Second-epoch detections are separated by 2.1" and 6.6 pix   
The object was found in VSX
 2"  ASASSN-V J073317.89-333848.1  
Type: SR
#   Max.           Min./Amp.       JD0           Period
    15.480   g       Y     0.730   g         2459559.64500        493.000000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:33:17.80 -33:38:49.6:  13.17 +/- 0.10  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:33:17.80 -33:38:49.6:  13.36 +/- 0.12  detection
Forced photometry reference-image weighted average:  13.24 +/- 0.08
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6686.08252 3379.06909 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 2906.06860 2978.96802 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6677.27783 3482.37354 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6675.35498 3488.73779 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 33 17.80 -33 38 49.6          12.2 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 33 17.73 -33 38 48.9          12.3 R      V36
     TAU0008  C2026 11 05.37339 07 33 17.86 -33 38 50.3          12.2 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 33 17.80 -33 38 49.6  12.2 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J073317.89-333848.1,2461349.8731,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J073317.89-333848.1 20261105.3731 12.25CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.95  06:58:54.45 -31:10:26.9
241.90083 -12.19399 galactic  CMa  Second-epoch detections are separated by 0.5" and 7.0 pix   
The object was found in VSX
 2"  ASASSN-V J065854.35-311025.5  
Type: L
#   Max.           Min./Amp.       JD0           Period
    12.900   V            13.390   V                                                                              
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 06:58:54.45 -31:10:26.9:  13.13 +/- 0.10  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 06:58:54.45 -31:10:26.9:  12.74 +/- 0.07  detection
Forced photometry reference-image weighted average:  12.87 +/- 0.05
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 2282.73389 4847.34033 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 7331.34570 1572.11914 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 2246.46313 4792.40332 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 2243.93750 4798.87891 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 06 58 54.45 -31 10 26.9          11.9 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 06 58 54.45 -31 10 26.7          12.0 R      V36
     TAU0008  C2026 11 05.37339 06 58 54.45 -31 10 27.2          11.9 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  06 58 54.45 -31 10 26.9  11.9 U             CMa       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J065854.35-311025.5,2461349.8731,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J065854.35-311025.5 20261105.3731 11.95CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.03  07:38:15.61 -34:33:26.5
248.70389  -6.31209 galactic  Pup  Second-epoch detections are separated by 0.5" and 6.9 pix   
The object was found in VSX
 2"  ASAS J073816-3433.5           
Type: SR
#   Max.           Min./Amp.       JD0           Period
     8.915   Ic      Y     0.116   Ic        2452508.00000         58.900000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:38:15.61 -34:33:26.5:  12.03 +/- 0.04  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:38:15.61 -34:33:26.5:  12.32 +/- 0.05  detection
Forced photometry reference-image weighted average:  12.13 +/- 0.03
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 7287.25195 2803.73511 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 2296.79858 3546.14819 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 7293.68555 2930.75708 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 7291.45508 2937.31812 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 38 15.61 -34 33 26.5          11.0 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 38 15.61 -34 33 26.2          11.0 R      V36
     TAU0008  C2026 11 05.37339 07 38 15.61 -34 33 26.7          11.1 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 38 15.61 -34 33 26.5  11.0 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J073816-3433.5,2461349.8731,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J073816-3433.5 20261105.3731 11.03CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.99  07:30:35.04 -32:21:30.7
245.99118  -6.67646 galactic  Pup  Second-epoch detections are separated by 1.8" and 7.1 pix   
The object was found in VSX
 1"  ASAS J073035-3221.5           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.920   V       Y     0.440   V         2452091.00000         70.300000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:30:35.04 -32:21:30.7:  12.01 +/- 0.04  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:30:35.04 -32:21:30.7:  11.96 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.98 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6366.60303 4167.89062 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 3236.56250 2194.28320 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6334.31641 4256.32080 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6332.02148 4263.04102 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 30 35.04 -32 21 30.7          11.0 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 30 35.08 -32 21 31.5          11.0 R      V36
     TAU0008  C2026 11 05.37339 07 30 35.01 -32 21 29.9          11.0 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 30 35.04 -32 21 30.7  11.0 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J073035-3221.5,2461349.8731,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J073035-3221.5 20261105.3731 10.99CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.80  07:28:26.10 -36:45:49.8
249.72602  -9.10926 galactic  Pup  Second-epoch detections are separated by 0.5" and 6.9 pix   
The object was found in VSX
 2"  V0666 Pup                     
Type: SRB
#   Max.           Min./Amp.       JD0           Period
    12.700   V            14.000 : V                              125.000000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:28:26.10 -36:45:49.8:  11.89 +/- 0.03  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:28:26.10 -36:45:49.8:  12.13 +/- 0.04  detection
Forced photometry reference-image weighted average:  11.98 +/- 0.03
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6029.62061 1514.14209 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 3536.47998 4853.50000 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6082.82129 1604.74207 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6080.70215 1611.32507 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 28 26.10 -36 45 49.8          10.8 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 28 26.11 -36 45 50.1          10.8 R      V36
     TAU0008  C2026 11 05.37339 07 28 26.09 -36 45 49.6          10.8 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 28 26.10 -36 45 49.8  10.8 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0666 Pup,2461349.8731,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0666 Pup 20261105.3731 10.80CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.72  07:26:13.36 -29:51:38.8
243.32959  -6.33461 galactic  CMa  Second-epoch detections are separated by 3.2" and 7.2 pix   
The object was found in VSX
 3"  ASAS J072611-2951.5           
Type: SRB
#   Max.           Min./Amp.       JD0           Period
    11.500   V            12.500   V                                                 M7                           
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:26:13.36 -29:51:38.8:  11.87 +/- 0.03  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:26:13.36 -29:51:38.8:  11.68 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.77 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 5837.12891 5693.51367 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 3787.54541 675.54199 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 5758.14209 5756.60059 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 5755.29053 5763.25879 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 26 13.36 -29 51 38.8          10.7 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 26 13.48 -29 51 38.5          10.8 R      V36
     TAU0008  C2026 11 05.37339 07 26 13.24 -29 51 39.0          10.7 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 26 13.36 -29 51 38.8  10.7 U             CMa       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J072611-2951.5,2461349.8731,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J072611-2951.5 20261105.3731 10.72CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.79  07:23:58.97 -31:12:30.1
244.30868  -7.38516 galactic  CMa  Second-epoch detections are separated by 0.2" and 7.2 pix   
The object was found in VSX
 2"  ASAS J072359-3112.5           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    13.290   V       Y     1.250   V         2452346.60000        168.700000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:23:58.97 -31:12:30.1:  13.03 +/- 0.08  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:23:58.97 -31:12:30.1:  12.65 +/- 0.06  detection
Forced photometry reference-image weighted average:  12.78 +/- 0.05
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 5532.58398 4880.15771 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 4081.50879 1493.59863 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 5480.56934 4935.99170 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 5478.09326 4942.74609 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 23 58.97 -31 12 30.1          11.8 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 23 58.97 -31 12 30.0          11.8 R      V36
     TAU0008  C2026 11 05.37339 07 23 58.96 -31 12 30.1          11.8 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 23 58.97 -31 12 30.1  11.8 U             CMa       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J072359-3112.5,2461349.8731,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J072359-3112.5 20261105.3731 11.79CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.65  07:30:55.18 -31:03:26.4
244.86984  -6.00108 galactic  Pup  Second-epoch detections are separated by 0.4" and 7.1 pix   
The object was found in VSX
 1"  ASAS J073055-3103.4           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.690   V       Y     0.660   V         2452181.30000        248.000000000000   S                            
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:30:55.18 -31:03:26.4:  11.83 +/- 0.03  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:30:55.18 -31:03:26.4:  11.70 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.76 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6432.85498 4954.34668 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 3181.15918 1406.41052 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6375.40918 5041.27197 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6373.06982 5047.95605 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 30 55.18 -31 03 26.4          10.7 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 30 55.16 -31 03 26.2          10.7 R      V36
     TAU0008  C2026 11 05.37339 07 30 55.19 -31 03 26.5          10.6 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 30 55.18 -31 03 26.4  10.7 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J073055-3103.4,2461349.8731,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J073055-3103.4 20261105.3731 10.65CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.79  07:05:10.76 -36:54:44.3
247.81216 -13.36890 galactic  Pup  Second-epoch detections are separated by 0.6" and 6.8 pix   
The object was found in VSX
 1"  ASAS J070511-3654.7           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.730   V       Y     0.480   V         2452010.50000         63.800000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:05:10.76 -36:54:44.3:  11.81 +/- 0.03  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:05:10.76 -36:54:44.3:  11.66 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.72 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 3213.07422 1409.02185 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 6351.38428 4997.36523 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 3283.86914 1402.11584 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 3281.71240 1408.61023 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 05 10.76 -36 54 44.3          10.8 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 05 10.77 -36 54 44.6          10.8 R      V36
     TAU0008  C2026 11 05.37339 07 05 10.75 -36 54 44.0          10.8 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 05 10.76 -36 54 44.3  10.8 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J070511-3654.7,2461349.8731,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J070511-3654.7 20261105.3731 10.79CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.89  07:35:23.15 -35:55:34.8
249.63405  -7.48076 galactic  Pup  Second-epoch detections are separated by 0.9" and 6.9 pix   
The object was found in VSX
 2"  ASAS J073523-3555.6           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    12.010   V       Y     0.530   V         2452165.40000         91.500000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:35:23.15 -35:55:34.8:  11.80 +/- 0.03  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:35:23.15 -35:55:34.8:  12.09 +/- 0.04  detection
Forced photometry reference-image weighted average:  11.90 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6894.68213 1992.10596 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 2678.00757 4363.64697 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6928.35303 2110.14771 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6926.28467 2116.68799 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 35 23.15 -35 55 34.8          10.9 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 35 23.14 -35 55 34.4          10.9 R      V36
     TAU0008  C2026 11 05.37339 07 35 23.17 -35 55 35.2          10.9 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 35 23.15 -35 55 34.8  10.9 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J073523-3555.6,2461349.8731,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J073523-3555.6 20261105.3731 10.89CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.70  07:34:56.93 -36:25:20.8
250.03338  -7.79262 galactic  Pup  Second-epoch detections are separated by 0.6" and 6.8 pix   
The object was found in VSX
 3"  ASAS J073457-3625.4           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.780   V       Y     0.750   V         2452158.10000         99.800000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:34:56.93 -36:25:20.8:  11.77 +/- 0.03  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:34:56.93 -36:25:20.8:  12.16 +/- 0.04  detection
Forced photometry reference-image weighted average:  11.89 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6829.32715 1694.03577 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 2739.43994 4662.66357 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6872.62109 1811.88000 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6870.46582 1818.38135 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 34 56.93 -36 25 20.8          10.7 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 34 56.94 -36 25 20.5          10.7 R      V36
     TAU0008  C2026 11 05.37339 07 34 56.92 -36 25 21.0          10.7 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 34 56.93 -36 25 20.8  10.7 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J073457-3625.4,2461349.8731,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J073457-3625.4 20261105.3731 10.70CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.52  07:15:48.73 -36:00:37.0
247.89365 -11.04999 galactic  Pup  Second-epoch detections are separated by 0.3" and 6.9 pix   
The object was found in VSX
 2"  ASAS J071549-3600.6           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.760   V       Y     0.520   V         2452063.00000         69.500000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:15:48.73 -36:00:37.0:  11.65 +/- 0.03  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:15:48.73 -36:00:37.0:  11.65 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.65 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 4496.08838 1983.15527 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 5076.62939 4405.41064 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 4542.20215 2017.62146 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 4539.96680 2024.16174 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 15 48.73 -36 00 37.0          10.5 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 15 48.73 -36 00 36.8          10.5 R      V36
     TAU0008  C2026 11 05.37339 07 15 48.73 -36 00 37.1          10.5 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 15 48.73 -36 00 37.0  10.5 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J071549-3600.6,2461349.8731,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J071549-3600.6 20261105.3731 10.52CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.91  07:18:03.59 -38:08:54.2
250.05778 -11.56876 galactic  Pup  Second-epoch detections are separated by 1.2" and 6.6 pix   
The object was found in VSX
 1"  ASASSN-V J071803.66-380855.0  
Type: SR
#   Max.           Min./Amp.       JD0           Period
    13.410   V            13.970   V         2457784.60000         41.900000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:18:03.59 -38:08:54.2:  12.93 +/- 0.09  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:18:03.59 -38:08:54.2:  12.98 +/- 0.09  detection
Forced photometry reference-image weighted average:  12.95 +/- 0.06
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 4773.86816 689.68011 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 4780.65723 5695.15625 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 4859.16797 741.41260 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 4857.23389 747.76068 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 18 03.59 -38 08 54.2          11.9 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 18 03.56 -38 08 53.6          12.0 R      V36
     TAU0008  C2026 11 05.37339 07 18 03.62 -38 08 54.7          11.8 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 18 03.59 -38 08 54.2  11.9 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J071803.66-380855.0,2461349.8731,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J071803.66-380855.0 20261105.3731 11.91CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.18  07:11:20.80 -30:55:02.7
242.81972  -9.67402 galactic  CMa  Second-epoch detections are separated by 0.2" and 7.1 pix   
The object was found in VSX
 1"  ASAS J071121-3055.0           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.070   V       Y     0.440   V         2452713.10000        125.500000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:11:20.80 -30:55:02.7:  11.51 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:11:20.80 -30:55:02.7:  10.93 +/- 0.02  detection
Forced photometry reference-image weighted average:  11.16 +/- 0.01
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 3894.12061 5051.34863 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 5722.24805 1344.95435 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 3844.23560 5050.97266 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 3841.80444 5057.59277 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 11 20.80 -30 55 02.7          10.2 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 11 20.79 -30 55 02.7          10.2 R      V36
     TAU0008  C2026 11 05.37339 07 11 20.80 -30 55 02.6          10.2 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 11 20.80 -30 55 02.7  10.2 U             CMa       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J071121-3055.0,2461349.8731,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J071121-3055.0 20261105.3731 10.18CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.44  07:28:00.13 -32:26:32.0
245.80945  -7.19748 galactic  Pup  Second-epoch detections are separated by 0.5" and 7.1 pix   
The object was found in VSX
 1"  ASAS J072800-3226.5           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.280   V       Y     0.400   V         2452022.00000         67.900000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:28:00.13 -32:26:32.0:  11.45 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:28:00.13 -32:26:32.0:  11.39 +/- 0.02  detection
Forced photometry reference-image weighted average:  11.42 +/- 0.01
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6035.42920 4125.40332 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 3567.37061 2241.47925 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6005.84863 4202.44531 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6003.51953 4209.12012 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 28 00.13 -32 26 32.0          10.4 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 28 00.13 -32 26 32.2          10.4 R      V36
     TAU0008  C2026 11 05.37339 07 28 00.12 -32 26 31.7          10.4 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 28 00.13 -32 26 32.0  10.4 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J072800-3226.5,2461349.8731,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J072800-3226.5 20261105.3731 10.44CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.85  07:30:36.32 -35:34:00.8
248.85504  -8.16954 galactic  Pup  Second-epoch detections are separated by 4.3" and 7.0 pix   
The object was found in VSX
 9"  ASASSN-V J073036.06-353408.9  
Type: L
#   Max.           Min./Amp.       JD0           Period
    13.120   V            13.620   V                                                                              
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:30:36.32 -35:34:00.8:  13.08 +/- 0.09  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:30:36.32 -35:34:00.8:  13.27 +/- 0.11  detection
Forced photometry reference-image weighted average:  13.16 +/- 0.07
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6313.05615 2229.41040 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 3263.13208 4134.31641 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6342.48730 2326.01294 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6340.64697 2332.78564 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 30 36.32 -35 34 00.8          11.8 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 30 36.19 -35 34 02.3          11.8 R      V36
     TAU0008  C2026 11 05.37339 07 30 36.44 -35 33 59.3          11.9 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 30 36.32 -35 34 00.8  11.8 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J073036.06-353408.9,2461349.8731,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J073036.06-353408.9 20261105.3731 11.85CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.46  07:37:24.22 -36:05:38.1
249.97809  -7.20116 galactic  Pup  Second-epoch detections are separated by 0.4" and 6.8 pix   
The object was found in VSX
 2"  ASAS J073724-3605.7           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.800   V       Y     0.350   V         2451953.00000         33.430000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:37:24.22 -36:05:38.1:  11.36 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:37:24.22 -36:05:38.1:  11.70 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.47 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 7138.21875 1879.41321 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 2432.97021 4473.17139 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 7174.15771 2006.89099 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 7172.12598 2013.37085 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 37 24.22 -36 05 38.1          10.5 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 37 24.22 -36 05 37.9          10.5 R      V36
     TAU0008  C2026 11 05.37339 07 37 24.22 -36 05 38.3          10.4 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 37 24.22 -36 05 38.1  10.5 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J073724-3605.7,2461349.8731,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J073724-3605.7 20261105.3731 10.46CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.27  07:18:25.33 -38:04:08.2
250.01603 -11.47018 galactic  Pup  Second-epoch detections are separated by 0.9" and 6.7 pix   
The object was found in VSX
 3"  ASAS J071825-3804.1           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.210   V       Y     0.390   V         2452024.40000         60.800000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:18:25.33 -38:04:08.2:  11.36 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:18:25.33 -38:04:08.2:  11.52 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.43 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 4816.99463 737.92902 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 4738.11670 5646.11670 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 4900.56543 790.96960 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 4898.53418 797.35278 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 18 25.33 -38 04 08.2          10.3 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 18 25.32 -38 04 07.8          10.2 R      V36
     TAU0008  C2026 11 05.37339 07 18 25.33 -38 04 08.7          10.3 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 18 25.33 -38 04 08.2  10.3 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J071825-3804.1,2461349.8731,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J071825-3804.1 20261105.3731 10.27CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.29  07:12:52.42 -35:16:34.5
246.95640 -11.27288 galactic  Pup  Second-epoch detections are separated by 0.1" and 7.0 pix   
The object was found in VSX
 1"  ASAS J071252-3516.5           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.330   V       Y     0.490   V         2451989.70000         45.100000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:12:52.42 -35:16:34.5:  11.28 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:12:52.42 -35:16:34.5:  11.25 +/- 0.02  detection
Forced photometry reference-image weighted average:  11.26 +/- 0.01
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 4130.92627 2422.17798 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 5447.97119 3971.52954 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 4164.78809 2441.61597 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 4162.44531 2448.24805 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 12 52.42 -35 16 34.5          10.3 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 12 52.43 -35 16 34.5          10.3 R      V36
     TAU0008  C2026 11 05.37339 07 12 52.42 -35 16 34.6          10.3 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 12 52.42 -35 16 34.5  10.3 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J071252-3516.5,2461349.8731,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J071252-3516.5 20261105.3731 10.29CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.20  07:42:20.82 -36:21:21.7
250.69299  -6.45368 galactic  Pup  Second-epoch detections are separated by 0.9" and 6.9 pix   
The object was found in VSX
 4"  ASAS J074221-3621.4           
Type: SR
#   Max.           Min./Amp.       JD0           Period
     8.227   Ic      Y     0.091   Ic        2452515.00000         38.830000000000   M8                           
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:42:20.82 -36:21:21.7:  11.25 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:42:20.82 -36:21:21.7:  11.62 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.37 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 7737.72363 1687.62012 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 1830.80530 4656.64600 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 7776.25000 1837.23962 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 7774.20459 1843.82214 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 42 20.82 -36 21 21.7          10.2 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 42 20.79 -36 21 22.0          10.2 R      V36
     TAU0008  C2026 11 05.37339 07 42 20.85 -36 21 21.4          10.2 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 42 20.82 -36 21 21.7  10.2 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J074221-3621.4,2461349.8731,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J074221-3621.4 20261105.3731 10.20CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.29  07:48:53.08 -35:06:52.0
250.26721  -4.68680 galactic  Pup  Second-epoch detections are separated by 0.4" and 7.0 pix   
The object was found in VSX
 4"  V0481 Pup                     
Type: SR
#   Max.           Min./Amp.       JD0           Period
    12.000   V            13.000   V         2452960.00000        108.100000000000   S                            
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:48:53.08 -35:06:52.0:  11.23 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:48:53.08 -35:06:52.0:  11.65 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.35 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 8597.37500 2384.52930 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 981.02551 3947.94409 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 8610.16016 2560.08545 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 8607.93848 2566.75366 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 48 53.08 -35 06 52.0          10.3 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 48 53.09 -35 06 52.1          10.3 R      V36
     TAU0008  C2026 11 05.37339 07 48 53.07 -35 06 51.9          10.3 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 48 53.08 -35 06 52.0  10.3 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0481 Pup,2461349.8731,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0481 Pup 20261105.3731 10.29CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.01  07:05:36.50 -36:42:25.6
247.65575 -13.20671 galactic  Pup  Second-epoch detections are separated by 0.8" and 6.9 pix   
The object was found in VSX
 2"  ASAS J070537-3642.4           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.220   V       Y     0.490   V         2452160.40000         55.660000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:05:36.50 -36:42:25.6:  11.18 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:05:36.50 -36:42:25.6:  10.99 +/- 0.02  detection
Forced photometry reference-image weighted average:  11.07 +/- 0.01
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 3261.44043 1535.27747 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 6304.76416 4870.43750 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 3327.74536 1529.18005 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 3325.53833 1535.74890 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 05 36.50 -36 42 25.6          10.0 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 05 36.51 -36 42 26.0          10.0 R      V36
     TAU0008  C2026 11 05.37339 07 05 36.50 -36 42 25.2          10.0 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 05 36.50 -36 42 25.6  10.0 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J070537-3642.4,2461349.8731,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J070537-3642.4 20261105.3731 10.01CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.20  07:38:57.27 -33:29:27.6
247.83440  -5.67174 galactic  Pup  Second-epoch detections are separated by 0.5" and 7.2 pix   
The object was found in VSX
 2"  ASAS J073857-3329.4           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.390   V       Y     0.350   V         2451996.30000         85.000000000000   M5                           
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:38:57.27 -33:29:27.6:  11.12 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:38:57.27 -33:29:27.6:  11.34 +/- 0.02  detection
Forced photometry reference-image weighted average:  11.20 +/- 0.01
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 7405.06494 3444.08350 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 2187.78979 2904.11230 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 7390.99902 3571.84888 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 7388.67090 3578.62085 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 38 57.27 -33 29 27.6          10.2 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 38 57.28 -33 29 27.4          10.2 R      V36
     TAU0008  C2026 11 05.37339 07 38 57.27 -33 29 27.8          10.2 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 38 57.27 -33 29 27.6  10.2 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J073857-3329.4,2461349.8731,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J073857-3329.4 20261105.3731 10.20CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.05  07:47:14.67 -36:12:31.4
251.05206  -5.52185 galactic  Pup  Second-epoch detections are separated by 0.3" and 6.9 pix   
The object was found in VSX
 5"  ASAS J074715-3612.6           
Type: MISC
#   Max.           Min./Amp.       JD0           Period
    11.940   V       Y     1.060   V         2452243.20000         83.600000000000   M8                           
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:47:14.67 -36:12:31.4:  11.07 +/- 0.02  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:47:14.67 -36:12:31.4:  11.51 +/- 0.03  detection
Forced photometry reference-image weighted average:  11.20 +/- 0.02
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 8346.09375 1735.46924 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 1223.33704 4600.60449 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 8379.91992 1906.46985 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 8377.89551 1913.11743 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 47 14.67 -36 12 31.4          10.1 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 47 14.66 -36 12 31.4          10.1 R      V36
     TAU0008  C2026 11 05.37339 07 47 14.69 -36 12 31.5          10.0 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 47 14.67 -36 12 31.4  10.1 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J074715-3612.6,2461349.8731,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J074715-3612.6 20261105.3731 10.05CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.72  07:47:20.61 -35:07:27.6
250.11764  -4.96466 galactic  Pup  Second-epoch detections are separated by 0.5" and 6.9 pix   
The object was found in VSX
 3"  ASASSN-V J074720.83-350727.7  
Type: L
#   Max.           Min./Amp.       JD0           Period
    13.670   V            14.210   V                                                                              
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:47:20.61 -35:07:27.6:  12.81 +/- 0.09  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:47:20.61 -35:07:27.6:  13.37 +/- 0.15  detection
Forced photometry reference-image weighted average:  12.94 +/- 0.08
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 8403.86035 2392.38135 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 1173.86548 3942.89111 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 8417.31250 2561.39307 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 8415.23242 2567.94580 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 47 20.61 -35 07 27.6          11.7 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 47 20.60 -35 07 27.4          11.7 R      V36
     TAU0008  C2026 11 05.37339 07 47 20.63 -35 07 27.8          11.8 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 47 20.61 -35 07 27.6  11.7 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J074720.83-350727.7,2461349.8731,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J074720.83-350727.7 20261105.3731 11.72CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  10.06  07:28:45.19 -37:04:26.5
250.03495  -9.19434 galactic  Pup  Second-epoch detections are separated by 0.5" and 7.0 pix   
The object was found in VSX
 1"  ASASSN-V J072845.26-370427.3  
Type: SRS
#   Max.           Min./Amp.       JD0           Period
    11.490   V            11.620   V         2457447.58200         19.538000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:28:45.19 -37:04:26.5:  11.01 +/- 0.01  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:28:45.19 -37:04:26.5:  11.31 +/- 0.02  detection
Forced photometry reference-image weighted average:  11.12 +/- 0.01
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits -crosshair 6063.89746 1325.34668 image    wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits -crosshair 3499.72070 5041.71680 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits -crosshair 6122.76514 1418.26379 image    wcs_fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits -crosshair 6120.61719 1424.87805 image   

./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4/fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-05_CI_Pup-03-Q1b1x1_025821_TTUQ1b1x1_1169977_GdheU3n4

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 11 05.37312 07 28 45.19 -37 04 26.5          10.1 R      V36

Position measured on individual images:

     TAU0008  C2026 11 05.37285 07 28 45.19 -37 04 26.7          10.1 R      V36
     TAU0008  C2026 11 05.37339 07 28 45.19 -37 04 26.2          10.1 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 11 05.3731*  07 28 45.19 -37 04 26.5  10.1 U             Pup       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J072845.26-370427.3,2461349.8731,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J072845.26-370427.3 20261105.3731 10.06CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 11 05.3731  2461349.8731  11.88  07:48:21.14 -29:35:25.8
245.42934  -2.00247 galactic  Pup  Second-epoch detections are separated by 1.0" and 7.2 pix   
The object was found in VSX
 7"  GDS_J0748215-293521           
Type: VAR
#   Max.           Min./Amp.       JD0           Period
    12.990   r       Y     0.560   r                                                 M7                           
The object was not found in astcheck.
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits at 07:48:21.14 -29:35:25.8:  12.83 +/- 0.08  detection
Forced photometry on wcs_Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits at 07:48:21.14 -29:35:25.8:  12.93 +/- 0.10  detection
Forced photometry reference-image weighted average:  12.87 +/- 0.06
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Pup-03-Q1b1x1_2026-03-20_20-55-53_20.00sec_-15.00C_LIGHT_0008.fits


Pup-03-Q1b1x1_2026-03-25_21-01-13_20.00sec_-10.00C_LIGHT_0247.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-56-44_20.00sec_-0.00C_LIGHTs_0388.fits


fd_Pup-03-Q1b1x1_2026-11-05_02-57-31_20.00sec_0.00C_LIGHTs_0389.fits