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 202099010 IGR_J16318-4848 247.95215 -48.81737 247.01795 -48.71072 253.95271 -26.599 335.61601 -0.44852 86.40831 61075.00977 2026-02-04 00:14:04 61077.18824 2026-02-06 04:31:04 143.470 100.000 143.470 136.172 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 136.172 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-02-12 05:29:19 2027-02-18 00:00:00 2026-02-13 05:29:19 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000026001 We propose to observe IGR J16318-4848, the most obscured X-ray source in our Galaxy, to study X-ray reflection in the Compton-thick regime. In this high-mass X-ray binary, XRISM will reveal detailed reflection features such as strong Fe Ka, Fe Kb, and Ni Ka lines with resolved line shapes, a structured Fe K-edge, and one of the best-resolved Compton shoulders, shedding light on the obscuring medium. Moreover, XRISM could confirm the tentative Ni overabundance and the unexpectedly low velocity broadening reported for this source, which would imply that the X-ray reprocessor is related to supernova ejecta rather than a dense stellar wind. More generally, this source will serve as a unique laboratory to study X-ray processes, and benchmark obscuration models for AGNs and XRBs. BH AND NS BINARIES 2 A BERT VANDER MEULEN PRAGATI PRADHAN EUS 2 NOR IGR J16318-4848: COMPTON-THICK REFLECTION INSIDE OUR GALAXY processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202099010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202099010'

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