DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
observation_id
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
exposure
awarded_exposure
resolve_exposure
xtend_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
xtend_number_modes
xtend_dataclass_file1
xtend_dataclass_file2
xtend_window1_exposure
xtend_window2_exposure
xtend_window1_burst_exposure
xtend_window2_burst_exposure
xtend_code
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
xtend_data_mode1
xtend_data_mode2
processing_count
remarks
1 202054010 CYG_X-2 326.17165 38.3214 325.65371 38.09086 346.69932 47.95668 87.32829 -11.31646 251.76107 61002.03407 2025-11-23 00:49:04 61003.05560 2025-11-24 01:20:04 46.020 40.000 46.020 5.759 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31300010 320000A0 45.975 0.000 0.000 5.759 11110 313430 11310 PROCESSED 2025-11-28 09:02:49 2099-12-31 00:00:00 2025-11-29 09:02:49 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000021261 Cyg X-2 was observed as part of the XRISM in-flight calibration campaign for the Resolve point spread function. Although these data were not originally intended for spectroscopy---resulting in low signal-to-noise and several analytic uncertainties---we have nonetheless succeeded in resolving the complex Fe K-band emission-line components likely coming from the accretion disk corona. In this proposal, by achieving substantially higher S/N with an on-axis observation, we aim to reject models that remain viable with the current data, the disk line model. We also will compare it with other already-observed Z-track sources and establish a comprehensive picture of mass inflow and outflow in neutron star low-mass X-ray binaries, including Fe-K absorption lines by the ultrafast outflow (v/c=0.29). BH AND NS BINARIES 2 C MISAKI MIZUMOTO JAP 2 NOR CYG X-2: REVEALING ACCRETION AND OUTFLOWING IN THE Z-TRACK SOURCES processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202054010/ WINDOW2BURST WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202054010'

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