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 202090010 NGC2110 88.04762 -7.4565 87.44348 -7.46746 87.74422 -30.8805 212.92667 -16.54524 269.99888 61131.29310 2026-04-01 07:02:04 61133.56810 2026-04-03 13:38:04 93.070 80.000 93.070 77.698 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 83.110 77.698 0.000 0.000 11110 313430 11310 PROCESSED 2026-04-08 08:01:43 2027-04-11 00:00:00 2026-04-09 08:01:43 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000024013 We propose to observe the Seyfert 2 galaxy NGC 2110 with XRISM for 80 ks. We aim at studying its Fe K complex, which is the sum of two components: one constant and narrow (originating from the circumnuclear torus) and the other one broad and with intensity linearly correlated with the source flux (possibly arising from the Broad Line Region which is hidden in the optical: the HBLR). The source is one of the brightest AGN in the 3-10 keV band and it has shown a clear, double-peaked Ha line in the polarized optical spectra. The unprecedented XRISM Resolve spectral energy resolution will allow us to investigate in detail the Fe Ka doublet and the Fe Kb emission lines arising from distant material and the broad component from gas in motion close to the black hole. NON-JET-DOMINATED AGN 2 C ANDREA MARINUCCI EUR 2 NOR STUDYING THE INNERMOST REGIONS OF THE SEYFERT 2 GALAXY NGC 2110 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202090010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202090010'

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