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 201067010 NGC4507 188.90389 -39.9096 188.22871 -39.63425 205.6644 -32.77975 299.63991 22.86099 283.01684 60846.38894 2025-06-20 09:20:04 60849.08685 2025-06-23 02:05:04 118.557 100.000 118.557 109.499 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 109.499 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-07-15 02:03:24 2026-07-10 00:00:00 2025-07-05 08:11:26 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000013013 NCG 4507 is one of the X-ray brightest, but highly obscured, Seyfert 2 galaxies. It has been observed several times in the X-ray band, and it has always shown a strong iron K emission line. NCG 4507 is one of the few Compton thin AGN with a clear detection of the Ni Ka emission line. Iron K absorption lines have also been detected, suggesting the presence of an ionized absorber, possibly outflowing. The proposed 100 ksec XRISM observation will allow us to resolve with unprecedented precision the origin of the Fe K emission and absorption lines. Thanks to the high spectral resolution offered by Resolve any contribution from a BLR-Fe Ka will be fully revealed. NON-JET-DOMINATED AGN 2 B VALENTINA BRAITO YOSHIHIRO UEDA USJ 1 NOR THE ORIGIN OF THE FE KA LINE IN THE BRIGHT SEYFERT 2 NGC 4507 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201067010/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201067010'

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