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 201086010 EF_ERI 48.55438 -22.59546 48.00064 -22.78078 38.27036 -38.8878 212.9381 -57.40602 58.1426 60867.46949 2025-07-11 11:16:04 60868.76741 2025-07-12 18:25:04 54.638 50.000 54.638 47.700 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 51.023 47.700 0.000 0.000 11110 313430 11310 PROCESSED 2025-07-18 07:21:09 2026-07-23 00:00:00 2025-07-19 07:21:09 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000012119 Polars represent a distinct class of highly magnetized CVs. Measuring their white dwarf (WD) masses is crucial to understanding the origin of WD magnetic fields and the mass evolution of CVs. By fully characterizing Fe K-shell lines with Resolve, we will perform the most detailed X-ray spectroscopic study for two polars (AM Her and EF Eri): (1) robustly testing the conventional Fe line flux ratio diagnostics, (2) detecting non-equilibrium plasma with differing ion and electron temperatures near the shock region, (3) applying new methods of determining WD masses through measuring shock velocities and gravitational redshifts, and (4) constraining the accretion geometry. The proposed observations will demonstrate the unique capabilities of XRISM to probe the fundamental CV astrophysics. ACCRETING WHITE DWARFS AND NOVAE 2 C KAYA MORI USA 1 NOR COMPLETE HIGH-RESOLUTION FE LINE DIAGNOSTICS OF POLARS WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201086010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201086010'

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