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 902005010 HERCULES_X-1 254.45603 35.34288 254.00553 35.41851 245.99816 57.49405 58.14944 37.52434 89.57357 61119.55213 2026-03-20 13:15:04 61120.30630 2026-03-21 07:21:04 31.374 30.000 31.374 27.676 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 29.604 27.676 0.000 0.000 11110 313430 11310 PROCESSED 2026-03-26 05:49:00 2023-09-06 00:00:00 2026-03-27 05:49:00 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000029010 The precessing and distorted accretion disk of Hercules X-1 (Her X-1), a neutron star X-ray binary, may cause its 35-day cycle of high and low X-ray states. Since the last report of the extended low state in 2003, Her X-1 would enter a new state. XRISM is suitable for illustrating a high-resolution view of this state. The neutral absorber column density and the Compton shoulder will be examined by spectral curvature and Fe-K edge depth analysis. The narrow Fe I and several broad Fe K line fluxes may indicate the total brightness of Her X-1. We examine pulsations and analyse the influence of pulse phase on the spectrum. All these measurements will investigate which disk or accretion physics have been modified in the anomalous state. BH AND NS BINARIES 9 A XRISM Collaboration DDT 2 DDT-TOO DDT TOO REQUEST OF HERCULES X-1 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/9/902005010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '902005010'

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