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 203151010 FAIRALL9 20.94252 -58.8075 20.46529 -59.06801 340.59053 -59.1463 295.07188 -57.82462 159.98782 61308.13963 2026-09-25 03:21:04 61312.48130 2026-09-29 11:33:04 179.898 150.000 179.898 138.612 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 148.266 138.612 0.000 0.000 11110 313430 11310 PROCESSED 2026-10-06 11:23:59 2099-12-31 00:00:00 2026-10-07 11:23:59 03.03.015.013 gen20241115_xtd20260315_rsl20260315 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000034024 We propose a 150ks snapshot of Fairall 9 with XRISM during our 34 orbit HST spectroscopic monitoring campaign (April-September 2026) to explore the structure of the BLR. A recent intensive monitoring campaign has given a unique insight into the structure of the inner flow. The missing piece is how the BLR structure links to this inner flow. HST gives the optical/UV spectra, allowing for a decomposition of the disc and BLR emission. But the optical/UV line-shapes are highly sensitive to radiative transfer effects, so not suitable for determining the BLR structure. The X-ray Fe-Ka line is a much more robust tracer of column-density. XRISM is uniquely able to resolve this line-shape, allowing us to model the BLR structure, giving a unique window into the link between the central flow and BLR. NON-JET-DOMINATED AGN 2 A SCOTT HAGEN EUR 3 NOR FAIRALL 9: UNTANGLING THE ORIGIN OF THE BLR WITH XRISM AND HST processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/203151010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '203151010'

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