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 201113010 ETA_CARINAE 161.26608 -59.68471 160.77953 -59.42137 202.15612 -58.92718 287.59749 -0.62945 285.00199 60841.73546 2025-06-15 17:39:04 60842.48130 2025-06-16 11:33:04 31.334 25.000 31.334 29.425 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 29.425 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-07-14 17:23:02 2026-06-25 00:00:00 2025-06-24 05:10:03 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000012213 We propose two XRISM observations of Eta Carinae, the closest most massive colliding wind binary during AO1, at a time when the two stars are approaching periastron passage and the X-ray flux is increasing. Our primary goal of measuring important changes in the iron K-line region in the Resolve spectra as the companion star moves towards superior conjunction. These observations will allow us to determine how much the shocked gas cools as the colliding wind shock moves into the acceleration zone of the companion star's wind; constrain the origin of the iron fluorescence line; constrain the Si/Fe ratio as an indicator of chemical abundance; and most importantly, determine the radial velocity shift of the Fe XXV line, which will provide our best measure of the mass of the companion star. STELLAR CORONAE, WINDS, AND YOUNG STARS 2 A MICHAEL CORCORAN USA 1 NOR ETA CARINAE: MINING THE IRON RANGE WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201113010/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201113010'

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