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 201094010 NGC4945 196.36674 -49.46863 195.63672 -49.20094 217.02798 -38.64482 305.27355 13.33933 277.70966 60849.08685 2025-06-23 02:05:04 60854.12505 2025-06-28 03:00:04 291.188 200.000 291.188 278.282 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 278.282 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-07-13 09:35:54 2026-07-17 00:00:00 2025-07-05 12:17:14 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000012134 NGC 4945 is the brightest Seyfert 2 in hard X-rays, and the best example of only a few Compton-thick AGN known to vary strongly >10 keV. The strong hard X-ray variability implies the intrinsic flux is not smeared out by the obscurer, requiring an atypically low torus covering factor. The cause remains unknown, but may be related to outflows depleting the sub-pc reflecting gas. Chandra has also resolved part of the reflector directly on extended scales of ~30pc rather than a classical sub-pc torus. These ill-understood reflector properties make NGC 4945 an ideal target for XRISM. We propose a 200ks observation to constrain the location, density and clumpiness of the obscurer with Resolve, and understand implications for the wider population from this prototype variable Compton-thick AGN. NON-JET-DOMINATED AGN 2 B PETER BOORMAN USA 1 NOR THE NATURE OF THE CIRCUMNUCLEAR OBSCURING MEDIUM IN THE NEAREST VARIABLE COMPTON-THICK AGN NGC 4945 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201094010/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201094010'

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