MWM Targeting Cartons

This page is a comprehensive list of cartons available up through data release 19. Each carton is associated with a well defined targeting generation. These generations were used at different points in the survey for plate designs or Robostrategy designs for the FPS. For a full description of the targeting generations see the List of Targeting Generations section on the BHM Targeting page. For more information about the targeting process see the MWM Targeting page.

Targeting Generation v0.plates: The Plate Era

When SDSS-V first began observing on sky, we continued to use the same type of aluminum plates and similar plate design code as in SDSS-IV. All of the cartons in the following table were created for use during the plate operations phase of SDSS-V. As a result, all of the cartons are from target selection plan 0.1.0 and targeting generation v0.plates.

Carton NamesSimplified Target SelectionInstrumentAvailable Targets1
mwm_cb_300pcCompact binaries within 300pc from Gaia+GALEXBOTH89492
mwm_cb_cvcandidatesCompact binaries from literature BOTH5167
mwm_cb_gaiagalexCompact binaries from Gaia+GALEXBOTH261570
mwm_gg_coreLuminous giants across the sky based on G-H color cutsAPOGEE5459267
mwm_halo_bbA sample of metal-poor giants selected based on optical and infrared photometryBOSS646940
mwm_halo_smA sample of metal-poor stars selected based on SkyMapper Ca K photometryBOSS138298
mwm_planet_tessTESS TOI and 2 minute Cadence Follow-up APOGEE177494
mwm_rv_long_bplatesShort Exposure Plate Radial Velocity Monitoring — Long Temporal BaselineAPOGEE6397
mwm_rv_long-bplatesShort Exposure Plate Radial Velocity Monitoring — Long Temporal BaselineAPOGEE4370
mwm_rv_long-fpsRadial Velocity Monitoring — Long Temporal BaselineAPOGEE111233
mwm_rv_long-rmRM Plate Radial Velocity Monitoring — Long Temporal BaselineAPOGEE1344
mwm_rv_short-bplatesShort Exposure Plate Radial Velocity Monitoring — Short Temporal BaselineAPOGEE50567
mwm_rv_short-fpsRadial Velocity Monitoring — Short Temporal BaselineAPOGEE6283604
mwm_rv_short-rmRM Plate Radial Velocity Monitoring — Short Temporal BaselineAPOGEE3855
mwm_snc_100pcVolume limited census of the solar neighborhoodBOTH322222
mwm_snc_250pcVolume limited census of the solar neighborhood, extension to earlier typesBOTH417431
mwm_tessrgb_coreTESS observed red giant asteroseismology follow-upAPOGEE1004714
mwm_wd_coreWhite dwarfs selected from Gaia + SDSS-V (Gentile Fusillo et al. 2019)BOSS192534
mwm_yso_clusterCandidates identified through phase space clustering, targeted with APOGEEBOTH45461
mwm_yso_cmzCandidates located in Central Molecular Zone+inner Galactic diskAPOGEE1282
mwm_yso_obSelection of the hottest and youngest OB starsBOTH8670
mwm_yso_s1Optically bright candidates identified through infrared excessBOTH28832
mwm_yso_s2Optically faint candidates identified through infrared excessAPOGEE11086
mwm_yso_s2-5Candidates found towards areas of high nebulosityAPOGEE1112
mwm_yso_s3Low mass candidates identified through Gaia variabilityBOTH52691
1Available targets is the number of targets that satisfy the carton selection function in the targeting database. The number of targets ultimately observed for each carton will be smaller than this value.

Targeting Generations v0.5.epsilon-7-core-0, v0.5.2, v0.5.3 and v0.5.5: The FPS Era

After the FPS was installed on the telescopes, there was a general redesign of the MWM targeting cartons. As time progressed, some cartons went through further changes which are recorded in different target selection plans. Any given target selection plan is associate with one or more targeting generations. In the carton table below, the Plan / Gen(s) column gives the targeting plan and targeting generations that plan appeared in associated with this carton. Cartons with multiple plans have multiple rows in this table. To save space in the carton table, the targeting geneartions will be referred to using a simple short hand:

Targeting GenerationShort hand for Plan/Gen(s) column
v0.5.epsilon-7-core-01
v0.5.2 2
v0.5.3 3
v0.5.54
CartonSimplified Target SelectionInstrumentAvailable Targets1Plan / Gen(s)2
manual_mwm_tess_obOB(AF)-type pulsating stars in eclipsing binaries (TESS Continuous Viewing Zones)APOGEE3640.5.13 / 3,4
manual_nsbh_apogeeCompact NS/BH binaries APOGEEAPOGEE750.5.3 / 1,2,3,4
manual_nsbh_bossCompact NS/BH binaries BOSSBOSS2490.5.3 / 1,2,3,4
manual_offset_mwmhalo _off00Offset Test CartonBOSS1330None
manual_offset_mwmhalo _off05Offset Test CartonBOSS1330None
manual_offset_mwmhalo _off10Offset Test CartonBOSS1330None
manual_offset_mwmhalo _off20Offset Test CartonBOSS1330None
manual_offset_mwmhalo _off30Offset Test CartonBOSS1330None
manual_offset_mwmhalo _offaOffset Test CartonBOSS1330None
manual_offset_mwmhalo _offbOffset Test CartonBOSS1330None
manual_validation_apogeeCalibration targets selected from a variety of surveys and catalogsAPOGEE245180.5.20 / 4
manual_validation_bossCalibration targets selected from a variety of surveys and catalogsBOSS1302180.5.20 / 4
mwm_cb_300pc_apogeeCompact binaries within 300pc from Gaia+GALEX G<16APOGEE173820.5.0 / 1
mwm_cb_300pc_apogeeCompact binaries within 300pc from Gaia+GALEX G<16APOGEE173820.5.19 / 2,3,4
mwm_cb_300pc_bossCompact binaries within 300pc from Gaia+GALEX G>=16BOSS522670.5.0 / 1
mwm_cb_300pc_bossCompact binaries within 300pc from Gaia+GALEX G>=16BOSS522670.5.19 / 2,3,4
mwm_cb_cvcandidates _apogeeCompact binaries from literature G<16APOGEE610.5.0 / 1,2,3,4
mwm_cb_cvcandidates _bossCompact binaries from literature G>=16BOSS51670.5.0 / 1,2,3,4
mwm_cb_gaiagalex_apogeeCompact binaries from Gaia+GALEX G<16APOGEE162870.5.0 / 1,2,3,4
mwm_cb_gaiagalex_bossCompact binaries from Gaia+GALEX G>=16BOSS2615700.5.0 / 1,2,3,4
mwm_cb_uvex1Compact binaries from Gaia+GALEX FUV+NUV for BOSS identificationBOSS1104470.5.0 / 1,2,3,4
mwm_cb_uvex2Compact binaries from Gaia+GALEX NUV only for BOSS identificationBOSS2789610.5.0 / 1,2,3,4
mwm_cb_uvex3Compact binaries from Gaia+XMM-Newton OM for BOSS identificationBOSS250320.5.0 / 1,2,3,4
mwm_cb_uvex4Compact binaries from Gaia+Swift UVOT for BOSS identificationBOSS210360.5.0 / 1,2,3,4
mwm_cb_uvex5Compact binaries from Gaia+GALEX RV for APOGEE identificatiomAPOGEE86410.5.0 / 1,2,3,4
mwm_dust_coreSample of bright, nearby, mid-plane giants complementary with Galactic GenesisAPOGEE619260.5.0 / 1,2,3,4
mwm_erosita_compact_geneROSITA/Gaia compact binary candidates for BOSS spectroscopyBOSS770380.5.2 / 1,2,3,4
mwm_erosita_compact_vareROSITA/Gaia compact binary candidates, Gaia variability, BOSS identificationBOSS168350.5.2 / 1,2,3,4
mwm_erosita_starseROSITA/Gaia coronal emittersBOSS899940.5.2 / 1,2,3,4
mwm_galactic_coreLuminous giants across the sky based on G-H color cutsAPOGEE54592670.5.0 / 1,2,3,4
mwm_halo_bb_bossHalo metal-poor star selection using “Best and Brightest” (Schlaufman & Casey 2014)BOSS6400580.5.1 / 1,2,3,4
mwm_halo_sm_bossHalo metal-poor star selection using Skymapper (Chiti et al. 2021)BOSS1382980.5.1 / 1,2,3,4
mwm_legacy_ir2optFollow-up of APOGEE-1/2 targets with BOSS — Filler CartonBOSS2098930.5.0 / 1,2,3,4
mwm_ob_cepheidsMWM – Cepheids from Inno et al. (2021) with BOSSBOSS23570.5.1 / 1,2,3,4
mwm_ob_coreMWM – OB(A) stars in the Milky Way and Magellanic clouds with BOSS BOSS6038540.5.1 / 1,2,3,4
mwm_rv_long_fpsFPS Radial Velocity Monitoring — Long Temporal BaselineAPOGEE1112330.5.0 / 1
mwm_rv_long_fpsFPS Radial Velocity Monitoring — Long Temporal BaselineAPOGEE1112330.5.18 / 2,3,4
mwm_rv_short_fpsFPS Radial Velocity Monitoring — Short Temporal BaselineAPOGEE62836040.5.0 / 1
mwm_rv_short_fpsFPS Radial Velocity Monitoring — Short Temporal BaselineAPOGEE62836040.5.18 / 2,3,4
mwm_snc_100pc_apogeeVolume limited census of the solar neighborhood G<16APOGEE1141730.5.0 / 1,2,3,4
mwm_snc_100pc_bossVolume limited census of the solar neighborhood G>=16BOSS3222220.5.0 / 1,2,3,4
mwm_snc_250pc_apogeeVolume limited census of the solar neighborhood, extension to earlier types G<16APOGEE4046180.5.0 / 1,2,3,4
mwm_snc_250pc_bossVolume limited census of the solar neighborhood, extension to earlier types G>=16BOSS4174310.5.0 / 1,2,3,4
mwm_tess_obPlaceholder targets for manual_mwm_tess_obAPOGEE7670.5.0 / 1
mwm_tess_obPlaceholder targets for manual_mwm_tess_obAPOGEE7670.5.11 / 2,3,4
mwm_tess_planetTESS TOI and 2 minute cadence follow-up APOGEE2237640.5.0 / 1,2,3,4
mwm_tessrgb_coreTESS observed red giant asteroseismology follow-upAPOGEE10047140.5.0 / 1,2,3,4
mwm_wd_coreWhite dwarfs selected from Gaia + SDSS-V (Gentile Fusillo et al. 2019)BOSS1925340.5.0 / 1,2,3,4
mwm_yso_cluster_apogeeCandidates identified through phase space clustering, targeted with APOGEEAPOGEE454610.5.0 / 1 
mwm_yso_cluster_apogeeCandidates identified through phase space clustering, targeted with APOGEEAPOGEE454610.5.17 / 2,3,4
mwm_yso_cluster_bossCandidates identified through phase space clustering, targeted with BOSSBOSS590650.5.0 / 1 
mwm_yso_cluster_bossCandidates identified through phase space clustering, targeted with BOSSBOSS590650.5.17 / 2,3,4
mwm_yso_cmz_apogeeCandidates located in Central Molecular Zone+inner Galactic disk, targeted with APOGEEAPOGEE131700.5.0 / 1 
mwm_yso_cmz_apogeeCandidates located in Central Molecular Zone+inner Galactic disk, targeted with APOGEEAPOGEE131700.5.17 / 2,3,4
mwm_yso_disk_apogeeOptically bright candidates identified through infrared excess, targeted with APOGEEAPOGEE288320.5.0 / 1 
mwm_yso_disk_apogeeOptically bright candidates identified through infrared excess, targeted with APOGEEAPOGEE288320.5.17 / 2,3,4
mwm_yso_disk_bossOptically bright candidates identified through infrared excess, targeted with BOSSBOSS374780.5.0 / 1 
mwm_yso_disk_bossOptically bright candidates identified through infrared excess, targeted with BOSSBOSS374780.5.17 / 2,3,4
mwm_yso_embedded_apogeeOptically faint candidates identified through infrared excess, targeted with APOGEEAPOGEE110860.5.0 / 1 
mwm_yso_embedded_apogeeOptically faint candidates identified through infrared excess, targeted with APOGEEAPOGEE110860.5.17 / 2,3,4
mwm_yso_nebula_apogeeCandidates found towards areas of high nebulosity, targeted with APOGEEAPOGEE11120.5.0 / 1 
mwm_yso_nebula_apogeeCandidates found towards areas of high nebulosity, targeted with APOGEEAPOGEE11120.5.17 / 2,3,4
mwm_yso_ob_apogeeSelection of the hottest and youngest OB stars, targeted with APOGEEAPOGEE86700.5.0 / 1,2,3,4
mwm_yso_ob_bossSelection of the hottest and youngest OB stars, targeted with BOSSBOSS86700.5.0 / 1,2,3,4
mwm_yso_pms_apogeeLow mass candidates located above main sequence on HR diagram, targeted with APOGEEAPOGEE763610.5.1 / 1,2,3,4
mwm_yso_pms_bossLow mass candidates located above main sequence on HR diagram, targeted with BOSSBOSS732140.5.1 / 1,2,3,4
mwm_yso_variable_apogeeLow mass candidates identified through Gaia variability, targeted with APOGEEAPOGEE526910.5.0 / 1 
mwm_yso_variable_apogeeLow mass candidates identified through Gaia variability, targeted with APOGEEAPOGEE526910.5.17 / 2,3,4
mwm_yso_variable_bossLow mass candidates identified through Gaia variability, targeted with BOSSBOSS477580.5.0 / 1 
mwm_yso_variable_bossLow mass candidates identified through Gaia variability, targeted with BOSSBOSS477580.5.17 / 2,3,4
1Available targets is the number of targets that satisfy the carton selection function in the targeting database. The number of targets ultimately observed for each carton will be smaller than this value.
2Plan / Gen(s) is the targeting plan and targeting generations that plan appeared in associated with this carton. Cartons with multiple plans, have multiple rows in this table. The generations have been simplified as follows: v0.5.epsilon-7-core-0 =1, v0.5.2 = 2, v0.5.3 = 3, and v0.5.5 = 4.

Technical Cartons

There are a few cartons that are not specifically for a science program, but were rather created for technical work. They are listed here.

manual_offset_mwmhalo

These cartons were used to develop methods for fiber positional offsetting to allow the observation of brighter stars than is generally possible with APOGEE and BOSS.

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