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 300067010 Eta_Carinae 161.26326 -59.68439 160.77673 -59.42105 202.15378 -58.928 287.59609 -0.62983 267.00212 60470.01185 2024-06-09 00:17:04 60474.34310 2024-06-13 08:14:04 316.703 100.000 316.703 183.448 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 183.448 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2024-09-24 13:08:40 2025-08-31 00:00:00 2024-06-22 12:32:36 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000092 A massive mass-loss wind from the evolved supermassive star, eta Carinae, collides with a fast wind from its hidden companion and produces hot plasma at ~50 MK. The X-ray spectra show strong He-like iron K lines from the hot plasma and iron K fluorescence produced by absorption and reemission of the hard X-ray emission at the primary wind. These emission lines should hold crucial information on the shocked gas at the head-on collision, which would flow with a few hundred to thousand km s-1. The star is also surrounded by a ring-shaped diffuse soft X-ray nebula, whose emission lines may show Doppler broadening or shift if the nebula originates from a supernova imposter event in the 1840s. We aim to resolve these emission line features for the first time with XRISM/Resolve. STELLAR CORONAE, WINDS, AND YOUNG STARS 3 A XRISM Collaboration JAP 0 NOR DYNAMICS OF THE COLLISIONAL SHOCKS DRIVEN BY THE MASSIVE BINARY ETA CARINAE archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300067010/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '300067010'

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