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 202084010 OAO1657-415 255.20245 -41.65561 254.32301 -41.58241 258.36975 -18.8119 344.36887 0.32019 95.16022 61103.78755 2026-03-04 18:54:04 61105.89935 2026-03-06 21:35:04 85.238 75.000 85.238 70.077 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 74.958 70.077 0.000 0.000 11110 313430 11310 PROCESSED 2026-03-11 10:41:51 2027-03-13 00:00:00 2026-03-12 10:41:51 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000023001 Our primary objective is to establish the first observational signature of the weak s-process, a key nucleosynthetic pathway responsible for producing lighter trans-iron elements such as Cu. We propose to search for the Cu Ka line as a probe of the weak s-process in the high-mass X-ray binary OAO 1657-415 during its eclipse phase. This system hosts a luminous blue variable (LBV) candidate and is the only viable target for this study. In a 75-ks Resolve observation, we expect to detect an enhanced Cu Ka line at a ~6 sigma significance level. With the measured Cu/Fe ratio and Fe spectral features, we will also investigate the internal and wind properties of the LBV, which attract interest in the context of stellar evolution and supernova mechanisms. BH AND NS BINARIES 2 A KAI MATSUNAGA PRAGATI PRADHAN JUS 2 NOR EXPLORING WEAK S-PROCESS AND STELLAR WIND PROPERTY IN THE HIGH MASS X-RAY BINARY OAO 1657-415 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202084010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202084010'

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