NGC1068 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:53:10.787412 (UTC)

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Contents

Target info

This section gives some details of the APERO astrometric database used when processing this target (e.g. for BERV calculation). Any observation with a object name in the alias list will be associated with this “APERO target” i.e. DRSOBJN=NGC1068

Target Information

RA

40.66962153 [deg] (2020yCat.1350….0G)

Dec

-0.01329435839 [deg] (2020yCat.1350….0G)

Finder chart

[FINDER CHART]

Teff

nan [K] (None)

Spectral Type

None (None)

Proper Motion (RA)

nan [mas/yr] (None)

Proper Motion (Dec)

nan [mas/yr] (None)

Parallax

nan [mas/yr] (None)

Radial Velocity

0.00348372 [mas/yr] (2022ApJS..261….2K)

Aliases

M 77, APG 37, AT20G J024240-000046, 1AXG J024241-0000, BWE 0240-0013, 3C 71, 3C 71.0, 4C -00.13, 3CR 71, Cul 0240-002, DA 82, 6dFGS gJ024240.7-000048, 2E 649, 2E 0240.1-0013, 1ES 0240-00.2, 1FGL J0242.7+0007, 2FGL J0242.5+0006, 3FGL J0242.7-0001, 4FGL J0242.6-0000, 3FHL J0242.7-0002, FIRST J024240.7-000046, FL8Y J0242.6-0000, GLEAM J024240-000041, GRA B0240-00, HIPASS J0242+00, INTREF 128, IRAS 02401-0013, IRAS F02401-0013, ISOSS J02426-0000, 1Jy 0240-002, 1Jy 0240-00, KUG 0240-002, LEDA 10266, LHE 67, 2MASX J02424077-0000478, MCG+00-07-083, MITG J024240-0000, MRC 0240-002, MSH 02-0-14, NAICGB 0240-002, NAIC 0240-002, NGC 1068, NRAO 112, NVSS J024240-000047, OHIO D -067, PBC J0242.7-0000, PKS J0242-0000, PKS 0240-00, PKS 0240-002, PMN J0242-0000, PSCz Q02401-0013, QSO B0240-002, RAFGL 4220, RAFGL 4220S, RBS 348, 1RXP J024240.9-000042, RX J024239-00000, RX J0242.6+0000, 1RXS J024240.9-000046, S3 0240-00, SDSS J024240.70-000047.9, SINGG HIPASS J0242+00, SPASS J024245-000157, SWIFT J0242.6+0000, SWIFT J0242.9-0000, TC 656, TGSSADR J024240.7-000047, TXS 0240-002, UGC 2188, UZC J024240.7-000048, VLSSr J024240.8-000044, VLSS J0242.6-0000, WB 0240-0013, WISE J024240.69-000047.7, 2XMM J024240.7-000046, XSS J02445-0000, 9Y-MST J0242+0001, Z 388-98, Z 0240.1-0013, [CAB95] IRAS F02401-0013, [CHM2007] HDC 163 J024240.77-0000478, [CHM2007] LDC 174 J024240.77-0000478, [DML87] 57, [HB91] 0240-002, [KRL2007b] 25, [M98c] 024006.5-001332, [NKB95] N1068, [OKM2018] SWIFT J0242.6+0000, [SLK2004] 333, [VV2000c] J024240.7-000047, [VV2003c] J024240.7-000047, [VV2006c] J024240.7-000047, [VV2010c] J024240.7-000047, [VV98c] J024240.7-000047, AAVSO 0237-00, Gaia DR3 2498700788995507712, NGC_1068, M77, APG37, AT20GJ024240-000046, 1AXGJ024241-0000, BWE0240-0013, 3C71, 3C71.0, 4C-00.13, 3CR71, Cul0240-002, DA82, 6dFGSgJ024240.7-000048, 2E649, 2E0240.1-0013, 1ES0240-00.2, 1FGLJ0242.7+0007, 2FGLJ0242.5+0006, 3FGLJ0242.7-0001, 4FGLJ0242.6-0000, 3FHLJ0242.7-0002, FIRSTJ024240.7-000046, FL8YJ0242.6-0000, GLEAMJ024240-000041, GRAB0240-00, HIPASSJ0242+00, INTREF128, IRAS02401-0013, IRASF02401-0013, ISOSSJ02426-0000, 1Jy0240-002, 1Jy0240-00, KUG0240-002, LEDA10266, LHE67, 2MASXJ02424077-0000478, MCG+00-07-083, MITGJ024240-0000, MRC0240-002, MSH02-0-14, NAICGB0240-002, NAIC0240-002, NGC1068, NRAO112, NVSSJ024240-000047, OHIOD-067, PBCJ0242.7-0000, PKSJ0242-0000, PKS0240-00, PKS0240-002, PMNJ0242-0000, PSCzQ02401-0013, QSOB0240-002, RAFGL4220, RAFGL4220S, RBS348, 1RXPJ024240.9-000042, RXJ024239-00000, RXJ0242.6+0000, 1RXSJ024240.9-000046, S30240-00, SDSSJ024240.70-000047.9, SINGGHIPASSJ0242+00, SPASSJ024245-000157, SWIFTJ0242.6+0000, SWIFTJ0242.9-0000, TC656, TGSSADRJ024240.7-000047, TXS0240-002, UGC2188, UZCJ024240.7-000048, VLSSrJ024240.8-000044, VLSSJ0242.6-0000, WB0240-0013, WISEJ024240.69-000047.7, 2XMMJ024240.7-000046, XSSJ02445-0000, 9Y-MSTJ0242+0001, Z388-98, Z0240.1-0013, [CAB95]IRASF02401-0013, [CHM2007]HDC163J024240.77-0000478, [CHM2007]LDC174J024240.77-0000478, [DML87]57, [HB91]0240-002, [KRL2007b]25, [M98c]024006.5-001332, [NKB95]N1068, [OKM2018]SWIFTJ0242.6+0000, [SLK2004]333, [VV2000c]J024240.7-000047, [VV2003c]J024240.7-000047, [VV2006c]J024240.7-000047, [VV2010c]J024240.7-000047, [VV98c]J024240.7-000047, AAVSO0237-00, GaiaDR32498700788995507712, NGC1068

OBJECT name(s) in headers

NGC1068

PI name(s) in headers

Claire Moutou

Project/Run name(s) in headers

18BE99

Spectrum

This section presents the observation after extraction,with and without telluric correction.

LBL

No LBL reduction found

CCF

This section presents the APERO CCF results for this object.

../../../_images/ccf_plot_NGC1068_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

285742.12 \(\pm\) 11255.95 m/s

CCF FWHM

3572.09 \(\pm\) 1843.17 m/s

Number of CCF files Total

8

Number of CCF passed QC

8

Number CCF files failed QC

0

First ccf file [Mid exposure]

2018-09-25 12:13:54.794

Last ccf file [Mid exposure]

2018-09-25 12:55:03.510

Last processed [ccf]

2025-02-23 21:23:01.429

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_NGC1068_spirou_offline_udem_file_list.txt

2026-02-12 20:53:13.317

Time series

This section deals with providing the time series information for this object

Debug

This section has various debug plots from APERO products

Telluric map

../../../_images/debug_tcorr_map_plot_NGC1068_spirou_offline_udem.png

Telluric map of e2dsff_tcorr_A files.Files are low-passed and corrected for the stars motion. The QC is displayed to the right of the image - in purple are the files that passed, in orange the files that failed.

Maximum Saturation level plot

../../../_images/debug_extsmax_plot_NGC1068_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_NGC1068_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_NGC1068_spirou_offline_udem.png

Plotting the version and processed date from the header from APERO. Note that offline reductions should lead to a straight line, while online reductions should be roughly a one-to-one with the Date axis.

APERO Calibration times plot

../../../_images/debug_mjd_cdt_plot_NGC1068_spirou_offline_udem.png

Computed time between observation and calibration used. Some calibrations arereference calibrations (in purple) and thus diverge from the reference night, others should always be from the same night (orange) unless no calibration was taken that night in which case the closest calirbation in time should have been used.